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Sine and cosine General information General definition Fields of application Trigonometry , Fourier series , Mathematical analysis .Domain, codomain and image Domain real number Image In mathematics , sine and cosine are trigonometric functions of an angle . The sine and cosine of an acute angle are defined in the context of a right triangle : for the specified angle, its sine is the ratio of the length of the side opposite that angle to the length of the longest side of the triangle (the hypotenuse ), and the cosine is the ratio of the length of the adjacent leg to that of the hypotenuse . For an angle , the sine and cosine functions are denoted as and . The definitions of sine and cosine have been extended to any real value in terms of the lengths of certain line segments in a unit circle . More modern definitions express the sine and cosine as infinite series , or as the solutions of certain differential equations , allowing their extension to arbitrary positive and negative values and even to complex numbers . The sine and cosine functions are commonly used to model periodic phenomena such as sound and light waves , the position and velocity of harmonic oscillators, sunlight intensity and day length, and average temperature variations throughout the year. They can be traced to the jyā and koṭi-jyā functions used in Indian astronomy during the Gupta period . Elementary descriptions [ edit ] Right-angled triangle definition [ edit ] For the angle α , the sine function gives the ratio of the length of the opposite side to the length of the hypotenuse. To define the sine and cosine of an acute angle , start with a right triangle that contains an angle of measure ; in the accompanying figure, angle in a right triangle is the angle of interest. The three sides of the triangle are named as follows: [ 1 ] Once such a triangle is chosen, the sine of the angle is equal to the length of the opposite side divided by the length of the hypotenuse, and the cosine of the angle is equal to the length of the adjacent side divided by the length of the hypotenuse: [ 1 ] The other trigonometric functions of the angle can be defined similarly; for example, the tangent is the ratio between the opposite and adjacent sides or equivalently the ratio between the sine and cosine functions. The reciprocal of sine is cosecant, which gives the ratio of the hypotenuse length to the length of the opposite side. Similarly, the reciprocal of cosine is secant, which gives the ratio of the hypotenuse length to that of the adjacent side. The cotangent function is the ratio between the adjacent and opposite sides, a reciprocal of a tangent function. These functions can be formulated as: [ 1 ] Special angle measures [ edit ] As stated, the values and appear to depend on the choice of a right triangle containing an angle of measure . However, this is not the case as all such triangles are similar , and so the ratios are the same for each of them. For example, each leg of the 45-45-90 right triangle is 1 unit, and its hypotenuse is ; therefore, . [ 2 ] The following table shows the special value of each input for both sine and cosine with the domain between . The input in this table provides various unit systems such as degree, radian, and so on. The angles other than those five can be obtained by using a calculator. [ 3 ] [ 4 ] Angle, x sin( x ) cos( x ) Degrees Radians Gradians Turns Exact Decimal Exact Decimal 0° 0 0 0 0 1 1 30° 0.5 0.866 45° 0.707 0.707 60° 0.866 0.5 90° 1 1 0 0 Law of sines and cosines' illustration The law of sines is useful for computing the lengths of the unknown sides in a triangle if two angles and one side are known. [ 5 ] Given a triangle with sides , , and , and angles opposite those sides , , and , the law states, This is equivalent to the equality of the first three expressions below: where is the triangle's circumradius . The law of cosines is useful for computing the length of an unknown side if two other sides and an angle are known. [ 5 ] The law states, In the case where from which , the resulting equation becomes the Pythagorean theorem . [ 6 ] The cross product and dot product are operations on two vectors in Euclidean vector space . The sine and cosine functions can be defined in terms of the cross product and dot product. If and are vectors, and is the angle between and , then sine and cosine can be defined as: [ 7 ] [ 8 ] Analytic descriptions [ edit ] Unit circle definition [ edit ] The sine and cosine functions may also be defined in a more general way by using unit circle , a circle of radius one centered at the origin , formulated as the equation of in the Cartesian coordinate system . Let a line through the origin intersect the unit circle, making an angle of with the positive half of the - axis. The - and - coordinates of this point of intersection are equal to and , respectively; that is, [ 9 ] This definition is consistent with the right-angled triangle definition of sine and cosine when because the length of the hypotenuse of the unit circle is always 1; mathematically speaking, the sine of an angle equals the opposite side of the triangle, which is simply the - coordinate. A similar argument can be made for the cosine function to show that the cosine of an angle when , even under the new definition using the unit circle. [ 10 ] [ 11 ] Graph of a function and its elementary properties [ edit ] Animation demonstrating how the sine function (in red) is graphed from the y - coordinate (red dot) of a point on the unit circle (in green), at an angle of θ . The cosine (in blue) is the x - coordinate. Using the unit circle definition has the advantage of drawing the graph of sine and cosine functions. This can be done by rotating counterclockwise a point along the circumference of a circle, depending on the input . In a sine function, if the input is , the point is rotated counterclockwise and stopped exactly on the - axis. If , the point is at the circle's halfway point. If , the point returns to its origin. This results in both sine and cosine functions having the range between . [ 12 ] Extending the angle to any real domain, the point rotated counterclockwise continuously. This can be done similarly for the cosine function as well, although the point is rotated initially from the - coordinate. In other words, both sine and cosine functions are periodic , meaning any angle added by the circle's circumference is the angle itself. Mathematically, [ 13 ] A function is said to be odd if , and is said to be even if . The sine function is odd, whereas the cosine function is even. [ 14 ] Both sine and cosine functions are similar, with their difference being shifted by . This phase shift can be expressed as or . This is distinct from the cofunction identities that follow below, which arise from right-triangle geometry and are not phase shifts: [ 15 ] The fixed point iteration x n +1  = cos( x n ) with initial value x 0  = −1 converges to the Dottie number. Zero is the only real fixed point of the sine function; in other words the only intersection of the sine function and the identity function is . The only real fixed point of the cosine function is called the Dottie number . The Dottie number is the unique real root of the equation . The decimal expansion of the Dottie number is approximately 0.739085. [ 16 ] Continuity and differentiation [ edit ] The quadrants of the unit circle and of sin( x ), using the Cartesian coordinate system The sine and cosine functions are infinitely differentiable. [ 17 ] The derivative of sine is cosine, and the derivative of cosine is negative sine: [ 18 ] Continuing the process in higher-order derivative results in the repeated same functions; the fourth derivative of a sine is the sine itself. [ 17 ] These derivatives can be applied to the first derivative test , according to which the monotonicity of a function can be defined as the inequality of function's first derivative greater or less than equal to zero. [ 19 ] It can also be applied to second derivative test , according to which the concavity of a function can be defined by applying the inequality of the function's second derivative greater or less than equal to zero. [ 20 ] The following table shows that both sine and cosine functions have concavity and monotonicity—the positive sign ( ) denotes a graph is increasing (going upward) and the negative sign ( ) is decreasing (going downward)—in certain intervals. [ 3 ] This information can be represented as a Cartesian coordinates system divided into four quadrants. Quadrant Angle Sine Cosine Degrees Radians Sign Monotony Convexity Sign Monotony Convexity 1st quadrant, I Increasing Concave Decreasing Concave 2nd quadrant, II Decreasing Concave Decreasing Convex 3rd quadrant, III Decreasing Convex Increasing Convex 4th quadrant, IV Increasing Convex Increasing Concave Both sine and cosine functions can be defined by using differential equations. The pair of is the solution to the two-dimensional system of differential equations and with the initial conditions and . One could interpret the unit circle in the above definitions as defining the phase space trajectory of the differential equation with the given initial conditions. It can be interpreted as a phase space trajectory of the system of differential equations and starting from the initial conditions and . [ citation needed ] Integral and the usage in mensuration [ edit ] Their area under a curve can be obtained by using the integral with a certain bounded interval. Their antiderivatives are: where denotes the constant of integration . [ 21 ] These antiderivatives may be applied to compute the mensuration properties of both sine and cosine functions' curves with a given interval. For example, the arc length of the sine curve between and is where is the incomplete elliptic integral of the second kind with modulus . It cannot be expressed using elementary functions . [ 22 ] In the case of a full period, its arc length is where is the gamma function and is the lemniscate constant . [ 23 ] [ 24 ] The usual principal values of the arcsin( x ) and arccos( x ) functions graphed on the Cartesian plane The functions and (as well as those functions with the same function rule and domain whose codomain is a subset of containing the interval ) are not bijective and therefore do not have inverse functions. For example, , but also , . Sine's "inverse", called arcsine, can then be described not as a function but a relation (for example, all integer multiples of would have an arcsine of zero). To define the inverse functions of sine and cosine, they must be restricted to their principal branches by restricting their domain and codomain; the standard functions used to define arcsine and arccosine are then and . [ 25 ] These are bijective and have inverses: and . Alternative notation is for arcsine and for arccosine. Using these definitions, one obtains the identity maps: and An acute angle is given by: where for some integer , By definition, both functions satisfy the equations: and According to Pythagorean theorem , the squared hypotenuse is the sum of two squared legs of a right triangle. Dividing the formula on both sides with squared hypotenuse resulting in the Pythagorean trigonometric identity , the sum of a squared sine and a squared cosine equals 1: [ 26 ] [ a ] Sine and cosine satisfy the following double-angle formulas: [ 27 ] Sine function in blue and sine squared function in red. The x - axis is in radians. The cosine double angle formula implies that sin 2 and cos 2 are, themselves, shifted and scaled sine waves. Specifically, [ 28 ] The graph shows both sine and sine squared functions, with the sine in blue and the sine squared in red. Both graphs have the same shape but with different ranges of values and different periods. Sine squared has only positive values, but twice the number of periods. [ citation needed ] Series and polynomials [ edit ] This animation shows how including more and more terms in the partial sum of its Taylor series approaches a sine curve. Both sine and cosine functions can be defined by using a Taylor series , a power series involving the higher-order derivatives. As mentioned in § Continuity and differentiation , the derivative of sine is cosine and the derivative of cosine is the negative of sine. This means the successive derivatives of are , , , , continuing to repeat those four functions. The - th derivative, evaluated at the point 0: where the superscript represents repeated differentiation. This implies the following Taylor series expansion at . One can then use the theory of Taylor series to show that the following identities hold for all real numbers —where is the angle in radians. [ 29 ] More generally, for all complex numbers : [ 30 ] Taking the derivative of each term gives the Taylor series for cosine: [ 29 ] [ 30 ] Both sine and cosine functions with multiple angles may appear as their linear combination , resulting in a polynomial. Such a polynomial is known as the trigonometric polynomial . The trigonometric polynomial's ample applications may be acquired in its interpolation , and its extension of a periodic function known as the Fourier series . Let and be any coefficients, then the trigonometric polynomial of a degree —denoted as —is defined as: [ 31 ] [ 32 ] The trigonometric series can be defined similarly analogous to the trigonometric polynomial, its infinite inversion. Let and be any coefficients, then the trigonometric series can be defined as: [ 33 ] In the case of a Fourier series with a given integrable function , the coefficients of a trigonometric series are: [ 34 ] Complex numbers relationship [ edit ] Complex exponential function definitions [ edit ] Both sine and cosine can be extended further via complex number , a set of numbers composed of both real and imaginary numbers . For real number , the definition of both sine and cosine functions can be extended in a complex plane in terms of an exponential function as follows: [ 35 ] Alternatively, both functions can be defined in terms of Euler's formula : [ 35 ] When plotted on the complex plane , the function for real values of traces out the unit circle in the complex plane. Both sine and cosine functions may be simplified to the imaginary and real parts of as: [ 36 ] When for real values and , where , both sine and cosine functions can be expressed in terms of real sines, cosines, and hyperbolic functions as: [ 37 ] Both functions and are the real and imaginary parts of . Sine and cosine are used to connect the real and imaginary parts of a complex number with its polar coordinates : and the real and imaginary parts are where and represent the magnitude and angle of the complex number . [ 38 ] For any real number , Euler's formula in terms of polar coordinates is stated as . [ 35 ] Domain coloring of sin( z ) in the complex plane. Brightness indicates absolute magnitude, hue represents complex argument. Vector field rendering of sin( z ) Applying the series definition of the sine and cosine to a complex argument, z , gives: where sinh and cosh are the hyperbolic sine and cosine . These are entire functions . It is also sometimes useful to express the complex sine and cosine functions in terms of the real and imaginary parts of its argument: Partial fraction and product expansions of complex sine [ edit ] Using the partial fraction expansion technique in complex analysis , one can find that the infinite series both converge and are equal to . Similarly, one can show that Using product expansion technique, one can derive Usage of complex sine [ edit ] sin( z ) is found in the functional equation for the Gamma function , which in turn is found in the functional equation for the Riemann zeta-function , As a holomorphic function , sin z is a 2D solution of Laplace's equation : The complex sine function is also related to the level curves of pendulums . [ how? ] [ 39 ] [ better source needed ] Sine function in the complex plane Real component Imaginary component Magnitude Arcsine function in the complex plane Real component Imaginary component Magnitude The word sine is derived, indirectly, from the Sanskrit word jyā 'bow-string' or more specifically its synonym jīvá (both adopted from Ancient Greek χορδή 'string; chord'), due to visual similarity between the arc of a circle with its corresponding chord and a bow with its string (see jyā, koti-jyā and utkrama-jyā ; sine and chord are closely related in a circle of unit diameter, see Ptolemy's Theorem ). This was transliterated in Arabic as jība , which is meaningless in that language and written as jb ( جب ). Since Arabic is written without short vowels, jb was interpreted as the homograph jayb ( جيب ), which means 'bosom', 'pocket', or 'fold'. [ 40 ] [ 41 ] When the Arabic texts of Al-Battani and al-Khwārizmī were translated into Medieval Latin in the 12th century by Gerard of Cremona , he used the Latin equivalent sinus (which also means 'bay' or 'fold', and more specifically 'the hanging fold of a toga over the breast'). [ 42 ] [ 43 ] [ 44 ] Gerard was probably not the first scholar to use this translation; Robert of Chester appears to have preceded him and there is evidence of even earlier usage. [ 45 ] [ 46 ] The English form sine was introduced in Thomas Fale 's 1593 Horologiographia . [ 47 ] The word cosine derives from an abbreviation of the Latin complementi sinus 'sine of the complementary angle ' as cosinus in Edmund Gunter 's Canon triangulorum (1620), which also includes a similar definition of cotangens . [ 48 ] Quadrant from 1840s Ottoman Turkey with axes for looking up the sine and versine of angles While the early study of trigonometry can be traced to antiquity, the trigonometric functions as they are in use today were developed in the medieval period. The chord function was discovered by Hipparchus of Nicaea (180–125 BCE) and Ptolemy of Roman Egypt (90–165 CE). [ 49 ] The sine and cosine functions are closely related to the jyā and koṭi-jyā functions used in Indian astronomy during the Gupta period ( Aryabhatiya and Surya Siddhanta ), via translation from Sanskrit to Arabic and then from Arabic to Latin. [ 42 ] [ 50 ] All six trigonometric functions in current use were known in Islamic mathematics by the 9th century, as was the law of sines , used in solving triangles . [ 51 ] Al-Khwārizmī (c. 780–850) produced tables of sines, cosines and tangents. [ 52 ] [ 53 ] Muhammad ibn Jābir al-Harrānī al-Battānī (853–929) discovered the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°. [ 53 ] In the early 17th-century, the French mathematician Albert Girard published the first use of the abbreviations sin , cos , and tan ; these were further promulgated by Euler (see below). The Opus palatinum de triangulis of Georg Joachim Rheticus , a student of Copernicus , was probably the first in Europe to define trigonometric functions directly in terms of right triangles instead of circles, with tables for all six trigonometric functions; this work was finished by Rheticus' student Valentin Otho in 1596. In a paper published in 1682, Leibniz proved that sin x is not an algebraic function of x . [ 54 ] Roger Cotes computed the derivative of sine in his Harmonia Mensurarum (1722). [ 55 ] Leonhard Euler 's Introductio in analysin infinitorum (1748) was mostly responsible for establishing the analytic treatment of trigonometric functions in Europe, also defining them as infinite series and presenting " Euler's formula ", as well as the near-modern abbreviations sin. , cos. , tang. , cot. , sec. , and cosec. [ 42 ] Software implementations [ edit ] There is no standard algorithm for calculating sine and cosine. IEEE 754 , the most widely used standard for the specification of reliable floating-point computation, does not address calculating trigonometric functions such as sine. The reason is that no efficient algorithm is known for computing sine and cosine with a specified accuracy, especially for large inputs. [ 56 ] Algorithms for calculating sine may be balanced for such constraints as speed, accuracy, portability, or range of input values accepted. This can lead to different results for different algorithms, especially for special circumstances such as very large inputs, e.g. sin(10 22 ) . A common programming optimization, used especially in 3D graphics, is to pre-calculate a table of sine values, for example one value per degree, then for values in-between pick the closest pre-calculated value, or linearly interpolate between the 2 closest values to approximate it. This allows results to be looked up from a table rather than being calculated in real time. With modern CPU architectures this method may offer no advantage. [ citation needed ] The CORDIC algorithm is commonly used in scientific calculators. The sine and cosine functions, along with other trigonometric functions, are widely available across programming languages and platforms. In computing, they are typically abbreviated to sin and cos . Some CPU architectures have a built-in instruction for sine, including the Intel x87 FPUs since the 80387. In programming languages, sin and cos are typically either a built-in function or found within the language's standard math library. For example, the C standard library defines sine functions within math.h : sin( double ) , sinf( float ) , and sinl( long double ) . The parameter of each is a floating point value, specifying the angle in radians. Each function returns the same data type as it accepts. Many other trigonometric functions are also defined in math.h , such as for cosine, arc sine, and hyperbolic sine (sinh). Similarly, Python defines math.sin(x) and math.cos(x) within the built-in math module. Complex sine and cosine functions are also available within the cmath module, e.g. cmath.sin(z) . CPython 's math functions call the C math library, and use a double-precision floating-point format . Turns based implementations [ edit ] "sinpi" redirects here. For the township in Pingtung County, Taiwan, see Xinpi . "cospi" redirects here. For the 17th-century Bolognese nobleman, see Ferdinando Cospi . Some software libraries provide implementations of sine and cosine using the input angle in half- turns , a half-turn being an angle of 180 degrees or radians. Representing angles in turns or half-turns has accuracy advantages and efficiency advantages in some cases. [ 57 ] [ 58 ] These functions are called sinpi and cospi in MATLAB, [ 57 ] OpenCL , [ 59 ] R, [ 58 ] Julia, [ 60 ] CUDA , [ 61 ] and ARM. [ 62 ] For example, sinpi(x) would evaluate to where x is expressed in half-turns, and consequently the final input to the function, πx can be interpreted in radians by sin . SciPy provides similar functions sindg and cosdg with input in degrees. [ 63 ] The accuracy advantage stems from the ability to perfectly represent key angles like full-turn, half-turn, and quarter-turn losslessly in binary floating-point or fixed-point. In contrast, representing , , and in binary floating-point or binary scaled fixed-point always involves a loss of accuracy since irrational numbers cannot be represented with finitely many binary digits. Turns also have an accuracy advantage and efficiency advantage for computing modulo to one period. Computing modulo 1 turn or modulo 2 half-turns can be losslessly and efficiently computed in both floating-point and fixed-point. For example, computing modulo 1 or modulo 2 for a binary point scaled fixed-point value requires only a bit shift or bitwise AND operation. In contrast, computing modulo involves inaccuracies in representing . For applications involving angle sensors, the sensor typically provides angle measurements in a form directly compatible with turns or half-turns. For example, an angle sensor may count from 0 to 4096 over one complete revolution. [ 64 ] If half-turns are used as the unit for angle, then the value provided by the sensor directly and losslessly maps to a fixed-point data type with 11 bits to the right of the binary point. In contrast, if radians are used as the unit for storing the angle, then the inaccuracies and cost of multiplying the raw sensor integer by an approximation to would be incurred. Āryabhaṭa's sine table Bhaskara I's sine approximation formula Discrete sine transform Dixon elliptic functions Euler's formula Generalized trigonometry Hyperbolic function Lemniscate elliptic functions Law of sines List of periodic functions List of trigonometric identities Madhava series Madhava's sine table Optical sine theorem Polar sine —a generalization to vertex angles Proofs of trigonometric identities Sinc function Sine and cosine transforms Sine integral Sine quadrant Sine wave Sine–Gordon equation Sinusoidal model SOH-CAH-TOA Trigonometric functions Trigonometric integral ^ a b c Young (2017) , p.  27 . ^ Young (2017) , p.  36 . ^ a b Varberg, Purcell & Rigdon (2007) , p. 42. ^ Young (2017) , p.  37 , 78 . ^ a b Axler (2012) , p.  634 . ^ Axler (2012) , p.  632 . ^ Weisstein, Eric W. "Cross Product" . MathWorld . Retrieved 5 June 2025 . ^ Weisstein, Eric W. "Dot Product" . MathWorld . Retrieved 5 June 2025 . ^ Varberg, Purcell & Rigdon (2007) , p. 41. ^ Young (2017) , p.  68 . ^ Varberg, Purcell & Rigdon (2007) , p. 47. ^ Varberg, Purcell & Rigdon (2007) , p. 41–42. ^ Varberg, Purcell & Rigdon (2007) , p. 41, 43. ^ Young (2012) , p.  165 . ^ Varberg, Purcell & Rigdon (2007) , p. 42, 47. ^ "OEIS A003957" . oeis.org . Retrieved 2019-05-26 . ^ a b Bourchtein & Bourchtein (2022) , p.  294 . ^ Varberg, Purcell & Rigdon (2007) , p. 115. ^ Varberg, Purcell & Rigdon (2007) , p. 155. ^ Varberg, Purcell & Rigdon (2007) , p. 157. ^ Varberg, Purcell & Rigdon (2007) , p. 199. ^ Vince (2023) , p.  162 . ^ Adlaj (2012) . ^ OEIS sequence A105419 (Decimal expansion of the arc length of the sine or cosine curve for one full period.) ^ Varberg, Purcell & Rigdon (2007) , p. 365. ^ Young (2017) , p.  99 . ^ Dennis G. Zill (2013). Precalculus with Calculus Previews . Jones & Bartlett Publishers. p. 238. ISBN   978-1-4496-4515-1 . Extract of page 238 ^ "Sine-squared function" . Retrieved August 9, 2019 . ^ a b Varberg, Purcell & Rigdon (2007) , p. 491–492. ^ a b Abramowitz & Stegun (1970) , p.  74 . ^ Powell (1981) , p. 150. ^ Rudin (1987) , p. 88. ^ Zygmund (1968) , p. 1. ^ Zygmund (1968) , p. 11. ^ a b c Howie (2003) , p.  24 . ^ Rudin (1987) , p. 2. ^ Brown, James Ward; Churchill, Ruel (2014). Complex Variables and Applications (9th ed.). McGraw-Hill . p. 105. ISBN   978-0-07-338317-0 . ^ Howie (2003) , p.  23–24 . ^ "Why are the phase portrait of the simple plane pendulum and a domain coloring of sin(z) so similar?" . math.stackexchange.com . Retrieved 2019-08-12 . ^ Plofker (2009) , p.  257 . ^ Maor (1998) , p.  35 . ^ a b c Merzbach & Boyer (2011) . ^ Maor (1998) , p. 35–36. ^ Katz (2008) , p. 253. ^ Smith (1958) , p. 202. ^ Various sources credit the first use of sinus to either Plato Tiburtinus 's 1116 translation of the Astronomy of Al-Battani Gerard of Cremona 's translation of the Algebra of al-Khwārizmī Robert of Chester 's 1145 translation of the tables of al-Khwārizmī See Merlet (2004) . See Maor (1998) , Chapter 3, for an earlier etymology crediting Gerard. See Katz (2008) , p. 210. ^ Fale's book alternately uses the spellings "sine", "signe", or "sign". Fale, Thomas (1593). Horologiographia. The Art of Dialling: Teaching, an Easie and Perfect Way to make all Kindes of Dials ... London: F. Kingston. p. 11, for example. ^ Gunter (1620) . ^ Brendan, T. (February 1965). "How Ptolemy constructed trigonometry tables". The Mathematics Teacher . 58 (2): 141– 149. doi : 10.5951/MT.58.2.0141 . JSTOR   27967990 . ^ Van Brummelen, Glen (2009). "India". The Mathematics of the Heavens and the Earth . Princeton University Press. Ch. 3, pp. 94–134. ISBN   978-0-691-12973-0 . ^ Gingerich, Owen (1986). "Islamic Astronomy" . Scientific American . Vol. 254. p. 74. Archived from the original on 2013-10-19 . Retrieved 2010-07-13 . ^ Jacques Sesiano, "Islamic mathematics", p. 157, in Selin, Helaine ; D'Ambrosio, Ubiratan , eds. (2000). Mathematics Across Cultures: The History of Non-western Mathematics . Springer Science+Business Media . ISBN   978-1-4020-0260-1 . ^ a b "trigonometry" . Encyclopedia Britannica. 17 June 2024. ^ Nicolás Bourbaki (1994). Elements of the History of Mathematics . Springer. ISBN   9783540647676 . ^ " Why the sine has a simple derivative Archived 2011-07-20 at the Wayback Machine ", in Historical Notes for Calculus Teachers Archived 2011-07-20 at the Wayback Machine by V. Frederick Rickey Archived 2011-07-20 at the Wayback Machine ^ Zimmermann (2006) . ^ a b "sinpi - Compute sin(X*pi) accurately" . www.mathworks.com . Archived from the original on 2025-11-23 . Retrieved 2026-01-08 . ^ a b "Trig function - RDocumentation" . www.rdocumentation.org . Retrieved 2026-02-17 . ^ "sin, sincos, sinh, sinpi" . registry.khronos.org . Retrieved 2026-02-17 . ^ "sinpi » Julia Functions" . www.jlhub.com . Retrieved 2026-02-17 . ^ "Double Precision Mathematical Functions" . docs.nvidia.com . Archived from the original on 2024-07-23 . Retrieved 2026-01-08 . ^ "Documentation – Arm Developer" . developer.arm.com . Retrieved 2026-02-17 . ^ "Special functions (scipy.special) — SciPy v1.17.0 Manual" . docs.scipy.org . Retrieved 25 February 2026 . ^ "AAS33051: Precision Angle Sensor IC with Incremental and Motor Commutation Outputs and On-Chip Linearization" . www.allegromicro.com . Archived from the original on 2019-04-17 . Retrieved 2026-02-17 . Abramowitz, Milton ; Stegun, Irene A. (1970), Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables , New York: Dover Publications , Ninth printing Adlaj, Semjon (2012), "An Eloquent Formula for the Perimeter of an Ellipse" (PDF) , American Mathematical Society , 59 (8): 1097 Axler, Sheldon (2012), Algebra and Trigonometry , John Wiley & Sons , ISBN   978-0470-58579-5 Bourchtein, Ludmila ; Bourchtein, Andrei (2022), Theory of Infinite Sequences and Series , Springer, doi : 10.1007/978-3-030-79431-6 , ISBN   978-3-030-79431-6 Gunter, Edmund (1620), Canon triangulorum Howie, John M. (2003), Complex Analysis , Springer Undergraduate Mathematics Series, Springer, doi : 10.1007/978-1-4471-0027-0 , ISBN   978-1-4471-0027-0 Traupman, Ph.D., John C. (1966), The New College Latin & English Dictionary , Toronto: Bantam, ISBN   0-553-27619-0 Katz, Victor J. (2008), A History of Mathematics (PDF) (3rd ed.), Boston: Addison-Wesley, The English word "sine" comes from a series of mistranslations of the Sanskrit jyā-ardha (chord-half). Āryabhaṭa frequently abbreviated this term to jyā or its synonym jīvá . When some of the Hindu works were later translated into Arabic, the word was simply transcribed phonetically into an otherwise meaningless Arabic word jiba . But since Arabic is written without vowels, later writers interpreted the consonants jb as jaib , which means bosom or breast. In the twelfth century, when an Arabic trigonometry work was translated into Latin, the translator used the equivalent Latin word sinus , which also meant bosom, and by extension, fold (as in a toga over a breast), or a bay or gulf. Maor, Eli (1998), Trigonometric Delights , Princeton University Press , ISBN   1-4008-4282-4 Merlet, Jean-Pierre (2004), "A Note on the History of the Trigonometric Functions", in Ceccarelli, Marco (ed.), International Symposium on History of Machines and Mechanisms , Springer, doi : 10.1007/1-4020-2204-2 , ISBN   978-1-4020-2203-6 Merzbach, Uta C. ; Boyer, Carl B. (2011), A History of Mathematics (3rd ed.), John Wiley & Sons , It was Robert of Chester's translation from Arabic that resulted in our word "sine". The Hindus had given the name jiva to the half-chord in trigonometry, and the Arabs had taken this over as jiba. In the Arabic language, there is also the word jaib meaning "bay" or "inlet". When Robert of Chester came to translate the technical word jiba, he seems to have confused this with the word jaib (perhaps because vowels were omitted); hence, he used the word sinus, the Latin word for "bay" or "inlet". Plofker (2009), Mathematics in India , Princeton University Press Powell, Michael J. D. (1981), Approximation Theory and Methods , Cambridge University Press , ISBN   978-0-521-29514-7 Rudin, Walter (1987), Real and complex analysis (3rd ed.), New York: McGraw-Hill , ISBN   978-0-07-054234-1 , MR   0924157 Smith, D. E. (1958) [1925], History of Mathematics , vol. I, Dover Publications , ISBN   0-486-20429-4 Varberg, Dale E.; Purcell, Edwin J.; Rigdon, Steven E. (2007), Calculus (9th ed.), Pearson Prentice Hall , ISBN   978-0131469686 Vince, John (2023), Calculus for Computer Graphics , Springer, doi : 10.1007/978-3-031-28117-4 , ISBN   978-3-031-28117-4 Young, Cynthia (2012), Trigonometry (3rd ed.), John Wiley & Sons, ISBN   978-1-119-32113-2 ——— (2017), Trigonometry (4th ed.), John Wiley & Sons, ISBN   978-1-119-32113-2 Zimmermann, Paul (2006), "Can we trust floating-point numbers?", Grand Challenges of Informatics (PDF) , p. 14/31 Zygmund, Antoni (1968), Trigonometric Series (2nd, reprinted ed.), Cambridge University Press , MR   0236587 Look up sine in Wiktionary, the free dictionary. Media related to Sine function at Wikimedia Commons
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[Jump to content](https://en.wikipedia.org/wiki/Sine_and_cosine#bodyContent) Main menu Main menu move to sidebar hide Navigation - [Main page](https://en.wikipedia.org/wiki/Main_Page "Visit the main page [z]") - [Contents](https://en.wikipedia.org/wiki/Wikipedia:Contents "Guides to browsing Wikipedia") - [Current events](https://en.wikipedia.org/wiki/Portal:Current_events "Articles related to current events") - [Random article](https://en.wikipedia.org/wiki/Special:Random "Visit a randomly selected article [x]") - [About Wikipedia](https://en.wikipedia.org/wiki/Wikipedia:About "Learn about Wikipedia and how it works") - [Contact us](https://en.wikipedia.org/wiki/Wikipedia:Contact_us "How to contact Wikipedia") Contribute - [Help](https://en.wikipedia.org/wiki/Help:Contents "Guidance on how to use and edit Wikipedia") - [Learn to edit](https://en.wikipedia.org/wiki/Help:Introduction "Learn how to edit Wikipedia") - [Community portal](https://en.wikipedia.org/wiki/Wikipedia:Community_portal "The hub for editors") - [Recent changes](https://en.wikipedia.org/wiki/Special:RecentChanges "A list of recent changes to Wikipedia [r]") - [Upload file](https://en.wikipedia.org/wiki/Wikipedia:File_upload_wizard "Add images or other media for use on Wikipedia") - [Special pages](https://en.wikipedia.org/wiki/Special:SpecialPages "A list of all special pages [q]") [![](https://en.wikipedia.org/static/images/icons/enwiki-25.svg) ![Wikipedia](https://en.wikipedia.org/static/images/mobile/copyright/wikipedia-wordmark-en-25.svg) ![The Free Encyclopedia](https://en.wikipedia.org/static/images/mobile/copyright/wikipedia-tagline-en-25.svg)](https://en.wikipedia.org/wiki/Main_Page) [Search](https://en.wikipedia.org/wiki/Special:Search "Search Wikipedia [f]") Appearance - [Donate](https://donate.wikimedia.org/?wmf_source=donate&wmf_medium=sidebar&wmf_campaign=en.wikipedia.org&uselang=en) - [Create account](https://en.wikipedia.org/w/index.php?title=Special:CreateAccount&returnto=Sine+and+cosine "You are encouraged to create an account and log in; however, it is not mandatory") - [Log in](https://en.wikipedia.org/w/index.php?title=Special:UserLogin&returnto=Sine+and+cosine "You're encouraged to log in; however, it's not mandatory. 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[o]") ## Contents move to sidebar hide - [(Top)](https://en.wikipedia.org/wiki/Sine_and_cosine) - [1 Elementary descriptions](https://en.wikipedia.org/wiki/Sine_and_cosine#Elementary_descriptions) Toggle Elementary descriptions subsection - [1\.1 Right-angled triangle definition](https://en.wikipedia.org/wiki/Sine_and_cosine#Right-angled_triangle_definition) - [1\.2 Special angle measures](https://en.wikipedia.org/wiki/Sine_and_cosine#Special_angle_measures) - [1\.3 Laws](https://en.wikipedia.org/wiki/Sine_and_cosine#Laws) - [1\.4 Vector definition](https://en.wikipedia.org/wiki/Sine_and_cosine#Vector_definition) - [2 Analytic descriptions](https://en.wikipedia.org/wiki/Sine_and_cosine#Analytic_descriptions) Toggle Analytic descriptions subsection - [2\.1 Unit circle definition](https://en.wikipedia.org/wiki/Sine_and_cosine#Unit_circle_definition) - [2\.1.1 Graph of a function and its elementary properties](https://en.wikipedia.org/wiki/Sine_and_cosine#Graph_of_a_function_and_its_elementary_properties) - [2\.1.2 Continuity and differentiation](https://en.wikipedia.org/wiki/Sine_and_cosine#Continuity_and_differentiation) - [2\.1.3 Integral and the usage in mensuration](https://en.wikipedia.org/wiki/Sine_and_cosine#Integral_and_the_usage_in_mensuration) - [2\.1.4 Inverse functions](https://en.wikipedia.org/wiki/Sine_and_cosine#Inverse_functions) - [2\.1.5 Other identities](https://en.wikipedia.org/wiki/Sine_and_cosine#Other_identities) - [2\.2 Series and polynomials](https://en.wikipedia.org/wiki/Sine_and_cosine#Series_and_polynomials) - [3 Complex numbers relationship](https://en.wikipedia.org/wiki/Sine_and_cosine#Complex_numbers_relationship) Toggle Complex numbers relationship subsection - [3\.1 Complex exponential function definitions](https://en.wikipedia.org/wiki/Sine_and_cosine#Complex_exponential_function_definitions) - [3\.2 Polar coordinates](https://en.wikipedia.org/wiki/Sine_and_cosine#Polar_coordinates) - [3\.3 Complex arguments](https://en.wikipedia.org/wiki/Sine_and_cosine#Complex_arguments) - [3\.3.1 Partial fraction and product expansions of complex sine](https://en.wikipedia.org/wiki/Sine_and_cosine#Partial_fraction_and_product_expansions_of_complex_sine) - [3\.3.2 Usage of complex sine](https://en.wikipedia.org/wiki/Sine_and_cosine#Usage_of_complex_sine) - [3\.4 Complex graphs](https://en.wikipedia.org/wiki/Sine_and_cosine#Complex_graphs) - [4 Background](https://en.wikipedia.org/wiki/Sine_and_cosine#Background) Toggle Background subsection - [4\.1 Etymology](https://en.wikipedia.org/wiki/Sine_and_cosine#Etymology) - [4\.2 History](https://en.wikipedia.org/wiki/Sine_and_cosine#History) - [5 Software implementations](https://en.wikipedia.org/wiki/Sine_and_cosine#Software_implementations) Toggle Software implementations subsection - [5\.1 Turns based implementations](https://en.wikipedia.org/wiki/Sine_and_cosine#Turns_based_implementations) - [6 See also](https://en.wikipedia.org/wiki/Sine_and_cosine#See_also) - [7 References](https://en.wikipedia.org/wiki/Sine_and_cosine#References) Toggle References subsection - [7\.1 Footnotes](https://en.wikipedia.org/wiki/Sine_and_cosine#Footnotes) - [7\.2 Citations](https://en.wikipedia.org/wiki/Sine_and_cosine#Citations) - [7\.3 Works cited](https://en.wikipedia.org/wiki/Sine_and_cosine#Works_cited) - [8 External links](https://en.wikipedia.org/wiki/Sine_and_cosine#External_links) Toggle the table of contents # Sine and cosine 10 languages - [বাংলা](https://bn.wikipedia.org/wiki/%E0%A6%B8%E0%A6%BE%E0%A6%87%E0%A6%A8_%E0%A6%93_%E0%A6%95%E0%A7%8B%E0%A6%B8%E0%A6%BE%E0%A6%87%E0%A6%A8 "সাইন ও কোসাইন – Bangla") - [Deutsch](https://de.wikipedia.org/wiki/Sinus_und_Kosinus "Sinus und Kosinus – German") - [Galego](https://gl.wikipedia.org/wiki/Seno_e_coseno "Seno e coseno – Galician") - [Bahasa Indonesia](https://id.wikipedia.org/wiki/Sinus_dan_kosinus "Sinus dan kosinus – Indonesian") - [ქართული](https://ka.wikipedia.org/wiki/%E1%83%A1%E1%83%98%E1%83%9C%E1%83%A3%E1%83%A1%E1%83%98_%E1%83%93%E1%83%90_%E1%83%99%E1%83%9D%E1%83%A1%E1%83%98%E1%83%9C%E1%83%A3%E1%83%A1%E1%83%98 "სინუსი და კოსინუსი – Georgian") - [Nederlands](https://nl.wikipedia.org/wiki/Sinus_en_cosinus "Sinus en cosinus – Dutch") - [Norsk bokmål](https://no.wikipedia.org/wiki/Trigonometriske_funksjoner#Sinus,_cosinus_og_tangens "Trigonometriske funksjoner – Norwegian Bokmål") - [Kiswahili](https://sw.wikipedia.org/wiki/Sini,_kosini_na_tanjenti "Sini, kosini na tanjenti – Swahili") - [Українська](https://uk.wikipedia.org/wiki/%D0%A1%D0%B8%D0%BD%D1%83%D1%81_%D1%82%D0%B0_%D0%BA%D0%BE%D1%81%D0%B8%D0%BD%D1%83%D1%81 "Синус та косинус – Ukrainian") - [中文](https://zh.wikipedia.org/wiki/%E6%AD%A3%E5%BC%A6%E5%92%8C%E4%BD%99%E5%BC%A6 "正弦和余弦 – Chinese") [Edit links](https://www.wikidata.org/wiki/Special:EntityPage/Q13647261#sitelinks-wikipedia "Edit interlanguage links") - [Article](https://en.wikipedia.org/wiki/Sine_and_cosine "View the content page [c]") - [Talk](https://en.wikipedia.org/wiki/Talk:Sine_and_cosine "Discuss improvements to the content page [t]") English - [Read](https://en.wikipedia.org/wiki/Sine_and_cosine) - [Edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit "Edit this page [e]") - 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[Cite this page](https://en.wikipedia.org/w/index.php?title=Special:CiteThisPage&page=Sine_and_cosine&id=1346396571&wpFormIdentifier=titleform "Information on how to cite this page") - [Get shortened URL](https://en.wikipedia.org/w/index.php?title=Special:UrlShortener&url=https%3A%2F%2Fen.wikipedia.org%2Fwiki%2FSine_and_cosine) Print/export - [Download as PDF](https://en.wikipedia.org/w/index.php?title=Special:DownloadAsPdf&page=Sine_and_cosine&action=show-download-screen "Download this page as a PDF file") - [Printable version](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&printable=yes "Printable version of this page [p]") In other projects - [Wikibooks](https://en.wikibooks.org/wiki/Trigonometry/Cosine_and_Sine) - [Wikidata item](https://www.wikidata.org/wiki/Special:EntityPage/Q13647261 "Structured data on this page hosted by Wikidata [g]") Appearance move to sidebar hide From Wikipedia, the free encyclopedia Fundamental trigonometric functions "Sine" and "Cosine" redirect here. For other uses, see [Sine (disambiguation)](https://en.wikipedia.org/wiki/Sine_\(disambiguation\) "Sine (disambiguation)") and [Cosine (disambiguation)](https://en.wikipedia.org/wiki/Cosine_\(disambiguation\) "Cosine (disambiguation)"). "Sine" is not to be confused with [Sign](https://en.wikipedia.org/wiki/Sign "Sign"), [Sign (mathematics)](https://en.wikipedia.org/wiki/Sign_\(mathematics\) "Sign (mathematics)") or the [sign function](https://en.wikipedia.org/wiki/Sign_function "Sign function"). | Sine and cosine | | |---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/7/71/Sine_cosine_one_period.svg/250px-Sine_cosine_one_period.svg.png)](https://en.wikipedia.org/wiki/File:Sine_cosine_one_period.svg) | | | General information | | | General definition | sin ⁡ ( θ ) \= opposite hypotenuse cos ⁡ ( θ ) \= adjacent hypotenuse {\\displaystyle {\\begin{aligned}&\\sin(\\theta )={\\frac {\\textrm {opposite}}{\\textrm {hypotenuse}}}\\\\\[8pt\]&\\cos(\\theta )={\\frac {\\textrm {adjacent}}{\\textrm {hypotenuse}}}\\\\\[8pt\]\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}&\\sin(\\theta )={\\frac {\\textrm {opposite}}{\\textrm {hypotenuse}}}\\\\\[8pt\]&\\cos(\\theta )={\\frac {\\textrm {adjacent}}{\\textrm {hypotenuse}}}\\\\\[8pt\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/52374fd3474dfab1331993d6c170e9cac82f4a4a) | In [mathematics](https://en.wikipedia.org/wiki/Mathematics "Mathematics"), **sine** and **cosine** are [trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") of an [angle](https://en.wikipedia.org/wiki/Angle "Angle"). The sine and cosine of an [acute angle](https://en.wikipedia.org/wiki/Acute_angle "Acute angle") are defined in the context of a [right triangle](https://en.wikipedia.org/wiki/Right_triangle "Right triangle"): for the specified angle, its sine is the ratio of the length of the side opposite that angle to the length of the longest side of the [triangle](https://en.wikipedia.org/wiki/Triangle "Triangle") (the [hypotenuse](https://en.wikipedia.org/wiki/Hypotenuse "Hypotenuse")), and the cosine is the [ratio](https://en.wikipedia.org/wiki/Ratio "Ratio") of the length of the adjacent leg to that of the [hypotenuse](https://en.wikipedia.org/wiki/Hypotenuse "Hypotenuse"). For an angle θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), the sine and cosine functions are denoted as sin ⁡ ( θ ) {\\displaystyle \\sin(\\theta )} ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948) and cos ⁡ ( θ ) {\\displaystyle \\cos(\\theta )} ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd). The definitions of sine and cosine have been extended to any [real](https://en.wikipedia.org/wiki/Real_number "Real number") value in terms of the lengths of certain line segments in a [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle"). More modern definitions express the sine and cosine as [infinite series](https://en.wikipedia.org/wiki/Series_\(mathematics\) "Series (mathematics)"), or as the solutions of certain [differential equations](https://en.wikipedia.org/wiki/Differential_equation "Differential equation"), allowing their extension to arbitrary positive and negative values and even to [complex numbers](https://en.wikipedia.org/wiki/Complex_number "Complex number"). The sine and cosine functions are commonly used to model [periodic](https://en.wikipedia.org/wiki/Periodic_function "Periodic function") phenomena such as [sound](https://en.wikipedia.org/wiki/Sound "Sound") and [light waves](https://en.wikipedia.org/wiki/Light_waves "Light waves"), the position and velocity of harmonic oscillators, sunlight intensity and day length, and average temperature variations throughout the year. They can be traced to the [*jyā* and *koṭi-jyā*](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā") functions used in [Indian astronomy](https://en.wikipedia.org/wiki/Indian_astronomy "Indian astronomy") during the [Gupta period](https://en.wikipedia.org/wiki/Gupta_period "Gupta period"). ## Elementary descriptions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=1 "Edit section: Elementary descriptions")\] ### Right-angled triangle definition \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=2 "Edit section: Right-angled triangle definition")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ed/Trigono_sine_en2.svg/250px-Trigono_sine_en2.svg.png)](https://en.wikipedia.org/wiki/File:Trigono_sine_en2.svg) For the angle *α*, the sine function gives the ratio of the length of the opposite side to the length of the hypotenuse. To define the sine and cosine of an acute angle α {\\displaystyle \\alpha } ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3), start with a [right triangle](https://en.wikipedia.org/wiki/Right_triangle "Right triangle") that contains an angle of measure α {\\displaystyle \\alpha } ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3); in the accompanying figure, angle α {\\displaystyle \\alpha } ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3) in a right triangle A B C {\\displaystyle ABC} ![{\\displaystyle ABC}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5e55b44cfd965fbdc7a328d5db8a35a619db0971) is the angle of interest. The three sides of the triangle are named as follows:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) - The *opposite side* is the side opposite to the angle of interest; in this case, it is a {\\displaystyle a} ![{\\displaystyle a}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ffd2487510aa438433a2579450ab2b3d557e5edc) . - The *hypotenuse* is the side opposite the right angle; in this case, it is h {\\displaystyle h} ![{\\displaystyle h}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b26be3e694314bc90c3215047e4a2010c6ee184a) . The hypotenuse is always the longest side of a right-angled triangle. - The *adjacent side* is the remaining side; in this case, it is b {\\displaystyle b} ![{\\displaystyle b}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f11423fbb2e967f986e36804a8ae4271734917c3) . It forms a side of (and is adjacent to) both the angle of interest and the right angle. Once such a triangle is chosen, the sine of the angle is equal to the length of the opposite side divided by the length of the hypotenuse, and the cosine of the angle is equal to the length of the adjacent side divided by the length of the hypotenuse:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) sin ⁡ ( α ) \= opposite hypotenuse , cos ⁡ ( α ) \= adjacent hypotenuse . {\\displaystyle \\sin(\\alpha )={\\frac {\\text{opposite}}{\\text{hypotenuse}}},\\qquad \\cos(\\alpha )={\\frac {\\text{adjacent}}{\\text{hypotenuse}}}.} ![{\\displaystyle \\sin(\\alpha )={\\frac {\\text{opposite}}{\\text{hypotenuse}}},\\qquad \\cos(\\alpha )={\\frac {\\text{adjacent}}{\\text{hypotenuse}}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f0cbaaff1eba0ec735281921a03965ab3a36763b) The other trigonometric functions of the angle can be defined similarly; for example, the [tangent](https://en.wikipedia.org/wiki/Trigonometric_functions#Right-angled_triangle_definitions "Trigonometric functions") is the ratio between the opposite and adjacent sides or equivalently the ratio between the sine and cosine functions. The [reciprocal](https://en.wikipedia.org/wiki/Multiplicative_inverse "Multiplicative inverse") of sine is cosecant, which gives the ratio of the hypotenuse length to the length of the opposite side. Similarly, the reciprocal of cosine is secant, which gives the ratio of the hypotenuse length to that of the adjacent side. The cotangent function is the ratio between the adjacent and opposite sides, a reciprocal of a tangent function. These functions can be formulated as:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) tan ⁡ ( θ ) \= sin ⁡ ( θ ) cos ⁡ ( θ ) \= opposite adjacent , cot ⁡ ( θ ) \= 1 tan ⁡ ( θ ) \= adjacent opposite , csc ⁡ ( θ ) \= 1 sin ⁡ ( θ ) \= hypotenuse opposite , sec ⁡ ( θ ) \= 1 cos ⁡ ( θ ) \= hypotenuse adjacent . {\\displaystyle {\\begin{aligned}\\tan(\\theta )&={\\frac {\\sin(\\theta )}{\\cos(\\theta )}}={\\frac {\\text{opposite}}{\\text{adjacent}}},\\\\\\cot(\\theta )&={\\frac {1}{\\tan(\\theta )}}={\\frac {\\text{adjacent}}{\\text{opposite}}},\\\\\\csc(\\theta )&={\\frac {1}{\\sin(\\theta )}}={\\frac {\\text{hypotenuse}}{\\text{opposite}}},\\\\\\sec(\\theta )&={\\frac {1}{\\cos(\\theta )}}={\\frac {\\textrm {hypotenuse}}{\\textrm {adjacent}}}.\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\tan(\\theta )&={\\frac {\\sin(\\theta )}{\\cos(\\theta )}}={\\frac {\\text{opposite}}{\\text{adjacent}}},\\\\\\cot(\\theta )&={\\frac {1}{\\tan(\\theta )}}={\\frac {\\text{adjacent}}{\\text{opposite}}},\\\\\\csc(\\theta )&={\\frac {1}{\\sin(\\theta )}}={\\frac {\\text{hypotenuse}}{\\text{opposite}}},\\\\\\sec(\\theta )&={\\frac {1}{\\cos(\\theta )}}={\\frac {\\textrm {hypotenuse}}{\\textrm {adjacent}}}.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a6a3c9e1e99b68fbda583330226dc87136a62315) ### Special angle measures \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=3 "Edit section: Special angle measures")\] As stated, the values sin ⁡ ( α ) {\\displaystyle \\sin(\\alpha )} ![{\\displaystyle \\sin(\\alpha )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/95a2a215bb78a456fe5662229c73775521b95299) and cos ⁡ ( α ) {\\displaystyle \\cos(\\alpha )} ![{\\displaystyle \\cos(\\alpha )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8323c66f99d1f3b7e0858fb92b0644fb0b8fba8a) appear to depend on the choice of a right triangle containing an angle of measure α {\\displaystyle \\alpha } ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3). However, this is not the case as all such triangles are [similar](https://en.wikipedia.org/wiki/Similarity_\(geometry\) "Similarity (geometry)"), and so the ratios are the same for each of them. For example, each [leg](https://en.wikipedia.org/wiki/Catheti "Catheti") of the 45-45-90 right triangle is 1 unit, and its hypotenuse is 2 {\\displaystyle {\\sqrt {2}}} ![{\\displaystyle {\\sqrt {2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b4afc1e27d418021bf10898eb44a7f5f315735ff); therefore, sin ⁡ 45 ∘ \= cos ⁡ 45 ∘ \= 2 2 {\\textstyle \\sin 45^{\\circ }=\\cos 45^{\\circ }={\\frac {\\sqrt {2}}{2}}} ![{\\textstyle \\sin 45^{\\circ }=\\cos 45^{\\circ }={\\frac {\\sqrt {2}}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/35373a42f10dc6f660ac17f1243294010fea43fc).[\[2\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA36_36]-2) The following table shows the special value of each input for both sine and cosine with the domain between 0 \< α \< π 2 {\\textstyle 0\<\\alpha \<{\\frac {\\pi }{2}}} ![{\\textstyle 0\<\\alpha \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d878d68144536cb7db4805f440b6cf3e0b82825b). The input in this table provides various unit systems such as degree, radian, and so on. The angles other than those five can be obtained by using a calculator.[\[3\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742-3)[\[4\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA37_37],_[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA78_78]-4) | Angle, x | sin(*x*) | cos(*x*) | | | | | | |---|---|---|---|---|---|---|---| | [Degrees](https://en.wikipedia.org/wiki/Degree_\(angle\) "Degree (angle)") | [Radians](https://en.wikipedia.org/wiki/Radian "Radian") | [Gradians](https://en.wikipedia.org/wiki/Gradian "Gradian") | [Turns](https://en.wikipedia.org/wiki/Turn_\(geometry\) "Turn (geometry)") | Exact | Decimal | Exact | Decimal | | 0° | 0 | 0 g {\\displaystyle 0^{g}} ![{\\displaystyle 0^{g}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ec8a3ac7e88cac5b0efbd0ccee88f8fb38ddf6d2) | | | | | | ### Laws \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=4 "Edit section: Laws")\] Main articles: [Law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines") and [Law of cosines](https://en.wikipedia.org/wiki/Law_of_cosines "Law of cosines") [![](https://upload.wikimedia.org/wikipedia/commons/thumb/a/a5/Law_of_sines_%28simple%29.svg/250px-Law_of_sines_%28simple%29.svg.png)](https://en.wikipedia.org/wiki/File:Law_of_sines_\(simple\).svg) Law of sines and cosines' illustration The [law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines") is useful for computing the lengths of the unknown sides in a triangle if two angles and one side are known.[\[5\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]-5) Given a triangle A B C {\\displaystyle ABC} ![{\\displaystyle ABC}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5e55b44cfd965fbdc7a328d5db8a35a619db0971) with sides a {\\displaystyle a} ![{\\displaystyle a}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ffd2487510aa438433a2579450ab2b3d557e5edc), b {\\displaystyle b} ![{\\displaystyle b}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f11423fbb2e967f986e36804a8ae4271734917c3), and c {\\displaystyle c} ![{\\displaystyle c}](https://wikimedia.org/api/rest_v1/media/math/render/svg/86a67b81c2de995bd608d5b2df50cd8cd7d92455), and angles opposite those sides α {\\displaystyle \\alpha } ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3), β {\\displaystyle \\beta } ![{\\displaystyle \\beta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/7ed48a5e36207156fb792fa79d29925d2f7901e8), and γ {\\displaystyle \\gamma } ![{\\displaystyle \\gamma }](https://wikimedia.org/api/rest_v1/media/math/render/svg/a223c880b0ce3da8f64ee33c4f0010beee400b1a), the law states, sin ⁡ α a \= sin ⁡ β b \= sin ⁡ γ c . {\\displaystyle {\\frac {\\sin \\alpha }{a}}={\\frac {\\sin \\beta }{b}}={\\frac {\\sin \\gamma }{c}}.} ![{\\displaystyle {\\frac {\\sin \\alpha }{a}}={\\frac {\\sin \\beta }{b}}={\\frac {\\sin \\gamma }{c}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/08ea457459d16cc937492f939b8e40e543078680) This is equivalent to the equality of the first three expressions below: a sin ⁡ α \= b sin ⁡ β \= c sin ⁡ γ \= 2 R , {\\displaystyle {\\frac {a}{\\sin \\alpha }}={\\frac {b}{\\sin \\beta }}={\\frac {c}{\\sin \\gamma }}=2R,} ![{\\displaystyle {\\frac {a}{\\sin \\alpha }}={\\frac {b}{\\sin \\beta }}={\\frac {c}{\\sin \\gamma }}=2R,}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0db5ccda5a3e2e9a89f282c1fc4ef0ace7014bcc) where R {\\displaystyle R} ![{\\displaystyle R}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4b0bfb3769bf24d80e15374dc37b0441e2616e33) is the triangle's [circumradius](https://en.wikipedia.org/wiki/Circumcircle "Circumcircle"). The [law of cosines](https://en.wikipedia.org/wiki/Law_of_cosines "Law of cosines") is useful for computing the length of an unknown side if two other sides and an angle are known.[\[5\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]-5) The law states, a 2 \+ b 2 − 2 a b cos ⁡ ( γ ) \= c 2 {\\displaystyle a^{2}+b^{2}-2ab\\cos(\\gamma )=c^{2}} ![{\\displaystyle a^{2}+b^{2}-2ab\\cos(\\gamma )=c^{2}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f30e796ac2afe7443a406b49fa5a718eae315275) In the case where γ \= π / 2 {\\displaystyle \\gamma =\\pi /2} ![{\\displaystyle \\gamma =\\pi /2}](https://wikimedia.org/api/rest_v1/media/math/render/svg/982a2789fde8a2fa65fd04c5e1bfec4dfecffc73) from which cos ⁡ ( γ ) \= 0 {\\displaystyle \\cos(\\gamma )=0} ![{\\displaystyle \\cos(\\gamma )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/04328c6895a6a1741585425ddb9474ea27e5ea0b), the resulting equation becomes the [Pythagorean theorem](https://en.wikipedia.org/wiki/Pythagorean_theorem "Pythagorean theorem").[\[6\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA632_632]-6) ### Vector definition \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=5 "Edit section: Vector definition")\] The [cross product](https://en.wikipedia.org/wiki/Cross_product "Cross product") and [dot product](https://en.wikipedia.org/wiki/Dot_product "Dot product") are operations on two [vectors](https://en.wikipedia.org/wiki/Vector_\(mathematics_and_physics\) "Vector (mathematics and physics)") in [Euclidean vector space](https://en.wikipedia.org/wiki/Euclidean_vector_space "Euclidean vector space"). The sine and cosine functions can be defined in terms of the cross product and dot product. If a {\\displaystyle \\mathbf {a} } ![{\\displaystyle \\mathbf {a} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/1a957216653a9ee0d0133dcefd13fb75e36b8b9d) and b {\\displaystyle \\mathbf {b} } ![{\\displaystyle \\mathbf {b} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/13ebf4628a1adf07133a6009e4a78bdd990c6eb9) are vectors, and θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) is the angle between a {\\displaystyle \\mathbf {a} } ![{\\displaystyle \\mathbf {a} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/1a957216653a9ee0d0133dcefd13fb75e36b8b9d) and b {\\displaystyle \\mathbf {b} } ![{\\displaystyle \\mathbf {b} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/13ebf4628a1adf07133a6009e4a78bdd990c6eb9), then sine and cosine can be defined as:[\[7\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-7)[\[8\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-8) sin ⁡ ( θ ) \= \| a × b \| \| a \| \| b \| , cos ⁡ ( θ ) \= a ⋅ b \| a \| \| b \| . {\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {\|\\mathbf {a} \\times \\mathbf {b} \|}{\|\\mathbf {a} \|\|\\mathbf {b} \|}},\\\\\\cos(\\theta )&={\\frac {\\mathbf {a} \\cdot \\mathbf {b} }{\|\\mathbf {a} \|\|\\mathbf {b} \|}}.\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {\|\\mathbf {a} \\times \\mathbf {b} \|}{\|\\mathbf {a} \|\|\\mathbf {b} \|}},\\\\\\cos(\\theta )&={\\frac {\\mathbf {a} \\cdot \\mathbf {b} }{\|\\mathbf {a} \|\|\\mathbf {b} \|}}.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6b60441dd703c8b6b683a4cf5a5258824b704875) ## Analytic descriptions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=6 "Edit section: Analytic descriptions")\] ### Unit circle definition \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=7 "Edit section: Unit circle definition")\] The sine and cosine functions may also be defined in a more general way by using [unit circle](https://en.wikipedia.org/wiki/Unit_circle#Trigonometric_functions_on_the_unit_circle "Unit circle"), a circle of radius one centered at the origin ( 0 , 0 ) {\\displaystyle (0,0)} ![{\\displaystyle (0,0)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5d630d3e781a53b0a3559ae7e5b45f9479a3141a), formulated as the equation of x 2 \+ y 2 \= 1 {\\displaystyle x^{2}+y^{2}=1} ![{\\displaystyle x^{2}+y^{2}=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ec84b90236512e8d27ff1a8f7707b60b63327de1) in the [Cartesian coordinate system](https://en.wikipedia.org/wiki/Cartesian_coordinate_system "Cartesian coordinate system"). Let a line through the origin intersect the unit circle, making an angle of θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) with the positive half of the x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) \-axis. The x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) \- and y {\\displaystyle y} ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d) \-coordinates of this point of intersection are equal to cos ⁡ ( θ ) {\\displaystyle \\cos(\\theta )} ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd) and sin ⁡ ( θ ) {\\displaystyle \\sin(\\theta )} ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948), respectively; that is,[\[9\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741-9) sin ⁡ ( θ ) \= y , cos ⁡ ( θ ) \= x . {\\displaystyle \\sin(\\theta )=y,\\qquad \\cos(\\theta )=x.} ![{\\displaystyle \\sin(\\theta )=y,\\qquad \\cos(\\theta )=x.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9e7decc76049a9174f255e3491d6e58bab1d4740) This definition is consistent with the right-angled triangle definition of sine and cosine when 0 \< θ \< π 2 {\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}} ![{\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ef78a27752a1f9a51d3b66c7863740f477aa4756) because the length of the hypotenuse of the unit circle is always 1; mathematically speaking, the sine of an angle equals the opposite side of the triangle, which is simply the y {\\displaystyle y} ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d) \-coordinate. A similar argument can be made for the cosine function to show that the cosine of an angle when 0 \< θ \< π 2 {\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}} ![{\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ef78a27752a1f9a51d3b66c7863740f477aa4756), even under the new definition using the unit circle.[\[10\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA68_68]-10)[\[11\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200747-11) #### Graph of a function and its elementary properties \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=8 "Edit section: Graph of a function and its elementary properties")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/3/3b/Circle_cos_sin.gif/500px-Circle_cos_sin.gif)](https://en.wikipedia.org/wiki/File:Circle_cos_sin.gif) Animation demonstrating how the sine function (in red) is graphed from the *y*\-coordinate (red dot) of a point on the [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle") (in green), at an angle of *θ*. The cosine (in blue) is the *x*\-coordinate. Using the unit circle definition has the advantage of drawing the graph of sine and cosine functions. This can be done by rotating counterclockwise a point along the circumference of a circle, depending on the input θ \> 0 {\\displaystyle \\theta \>0} ![{\\displaystyle \\theta \>0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0b0ac07626379d065418cc158ce6be9aeccf33b9). In a sine function, if the input is θ \= π 2 {\\textstyle \\theta ={\\frac {\\pi }{2}}} ![{\\textstyle \\theta ={\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e6095ebb8d0b6505f453ae2da2fbd3477ecd3a1), the point is rotated counterclockwise and stopped exactly on the y {\\displaystyle y} ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d) \-axis. If θ \= π {\\displaystyle \\theta =\\pi } ![{\\displaystyle \\theta =\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/ab4db588619489e27efb50a1d0d5aa016c49ce15), the point is at the circle's halfway point. If θ \= 2 π {\\displaystyle \\theta =2\\pi } ![{\\displaystyle \\theta =2\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/af3479f95999b7e195e5ecc2ee808bf02286332e), the point returns to its origin. This results in both sine and cosine functions having the [range](https://en.wikipedia.org/wiki/Range_of_a_function "Range of a function") between − 1 ≤ y ≤ 1 {\\displaystyle -1\\leq y\\leq 1} ![{\\displaystyle -1\\leq y\\leq 1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/29d02e9a39a0ad4594157a2f8b82ad89863543c9).[\[12\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741&ndash;42-12) Extending the angle to any real domain, the point rotated counterclockwise continuously. This can be done similarly for the cosine function as well, although the point is rotated initially from the y {\\displaystyle y} ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d) \-coordinate. In other words, both sine and cosine functions are [periodic](https://en.wikipedia.org/wiki/Periodic_function "Periodic function"), meaning any angle added by the circle's circumference is the angle itself. Mathematically,[\[13\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741,_43-13) sin ⁡ ( θ \+ 2 π ) \= sin ⁡ ( θ ) , cos ⁡ ( θ \+ 2 π ) \= cos ⁡ ( θ ) . {\\displaystyle \\sin(\\theta +2\\pi )=\\sin(\\theta ),\\qquad \\cos(\\theta +2\\pi )=\\cos(\\theta ).} ![{\\displaystyle \\sin(\\theta +2\\pi )=\\sin(\\theta ),\\qquad \\cos(\\theta +2\\pi )=\\cos(\\theta ).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d22ad562f48059fa7b33be5b34f0b0ca1979cd0d) A function f {\\displaystyle f} ![{\\displaystyle f}](https://wikimedia.org/api/rest_v1/media/math/render/svg/132e57acb643253e7810ee9702d9581f159a1c61) is said to be [odd](https://en.wikipedia.org/wiki/Odd_function "Odd function") if f ( − x ) \= − f ( x ) {\\displaystyle f(-x)=-f(x)} ![{\\displaystyle f(-x)=-f(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b022ffe516cf5bc26a68fd954753aa2bddf508f1), and is said to be [even](https://en.wikipedia.org/wiki/Even_function "Even function") if f ( − x ) \= f ( x ) {\\displaystyle f(-x)=f(x)} ![{\\displaystyle f(-x)=f(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/185fd2e78903788bc5756b067d0ac6aae1846724). The sine function is odd, whereas the cosine function is even.[\[14\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2012[httpsbooksgooglecombooksidOMrcN0a3LxICpgRA1-PA165_165]-14) Both sine and cosine functions are similar, with their difference being [shifted](https://en.wikipedia.org/wiki/Translation_\(geometry\) "Translation (geometry)") by π 2 {\\textstyle {\\frac {\\pi }{2}}} ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae). This phase shift can be expressed as cos ⁡ ( θ ) \= sin ⁡ ( θ \+ π 2 ) {\\textstyle \\cos(\\theta )=\\sin \\left(\\theta +{\\frac {\\pi }{2}}\\right)} ![{\\textstyle \\cos(\\theta )=\\sin \\left(\\theta +{\\frac {\\pi }{2}}\\right)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/16e716cd4b5339b573745c33edcc769226903a9b) or sin ⁡ ( θ ) \= cos ⁡ ( θ − π 2 ) {\\textstyle \\sin(\\theta )=\\cos \\left(\\theta -{\\frac {\\pi }{2}}\\right)} ![{\\textstyle \\sin(\\theta )=\\cos \\left(\\theta -{\\frac {\\pi }{2}}\\right)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ea80145f070fac0e114bd339dac33c3aa4286cda). This is distinct from the cofunction identities that follow below, which arise from right-triangle geometry and are not phase shifts: [\[15\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742,_47-15) sin ⁡ ( θ ) \= cos ⁡ ( π 2 − θ ) , cos ⁡ ( θ ) \= sin ⁡ ( π 2 − θ ) . {\\displaystyle {\\begin{aligned}\\sin(\\theta )&=\\cos \\left({\\frac {\\pi }{2}}-\\theta \\right),\\\\\\cos(\\theta )&=\\sin \\left({\\frac {\\pi }{2}}-\\theta \\right).\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&=\\cos \\left({\\frac {\\pi }{2}}-\\theta \\right),\\\\\\cos(\\theta )&=\\sin \\left({\\frac {\\pi }{2}}-\\theta \\right).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d4998408fbf02a4669c3e151a840a7bc314101ef) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Cosine_fixed_point.svg/250px-Cosine_fixed_point.svg.png)](https://en.wikipedia.org/wiki/File:Cosine_fixed_point.svg) The fixed point iteration *x**n*\+1 = cos(*xn*) with initial value *x*0 = −1 converges to the Dottie number. Zero is the only real [fixed point](https://en.wikipedia.org/wiki/Fixed_point_\(mathematics\) "Fixed point (mathematics)") of the sine function; in other words the only intersection of the sine function and the [identity function](https://en.wikipedia.org/wiki/Identity_function "Identity function") is sin ⁡ ( 0 ) \= 0 {\\displaystyle \\sin(0)=0} ![{\\displaystyle \\sin(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ecb40badcf53b50e5d03c49c7a5e1977e3ff262e). The only real fixed point of the cosine function is called the [Dottie number](https://en.wikipedia.org/wiki/Dottie_number "Dottie number"). The Dottie number is the unique real root of the equation cos ⁡ ( x ) \= x {\\displaystyle \\cos(x)=x} ![{\\displaystyle \\cos(x)=x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3cf8688ffc25998040ed8bf59f0a6298233a143c). The decimal expansion of the Dottie number is approximately 0.739085.[\[16\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-16) #### Continuity and differentiation \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=9 "Edit section: Continuity and differentiation")\] Main article: [Differentiation of trigonometric functions](https://en.wikipedia.org/wiki/Differentiation_of_trigonometric_functions "Differentiation of trigonometric functions") [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Sine_quads_01_Pengo.svg/500px-Sine_quads_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Sine_quads_01_Pengo.svg) The quadrants of the unit circle and of sin(*x*), using the [Cartesian coordinate system](https://en.wikipedia.org/wiki/Cartesian_coordinate_system "Cartesian coordinate system") The sine and cosine functions are infinitely differentiable.[\[17\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]-17) The derivative of sine is cosine, and the derivative of cosine is negative sine:[\[18\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007115-18) d d x sin ⁡ ( x ) \= cos ⁡ ( x ) , d d x cos ⁡ ( x ) \= − sin ⁡ ( x ) . {\\displaystyle {\\frac {d}{dx}}\\sin(x)=\\cos(x),\\qquad {\\frac {d}{dx}}\\cos(x)=-\\sin(x).} ![{\\displaystyle {\\frac {d}{dx}}\\sin(x)=\\cos(x),\\qquad {\\frac {d}{dx}}\\cos(x)=-\\sin(x).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3ae62cb5b610f8b5309ca193d299662fb18d4099) Continuing the process in higher-order derivative results in the repeated same functions; the fourth derivative of a sine is the sine itself.[\[17\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]-17) These derivatives can be applied to the [first derivative test](https://en.wikipedia.org/wiki/First_derivative_test "First derivative test"), according to which the [monotonicity](https://en.wikipedia.org/wiki/Monotone_function "Monotone function") of a function can be defined as the inequality of function's first derivative greater or less than equal to zero.[\[19\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007155-19) It can also be applied to [second derivative test](https://en.wikipedia.org/wiki/Second_derivative_test "Second derivative test"), according to which the [concavity](https://en.wikipedia.org/wiki/Concave_function "Concave function") of a function can be defined by applying the inequality of the function's second derivative greater or less than equal to zero.[\[20\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007157-20) The following table shows that both sine and cosine functions have concavity and monotonicity—the positive sign (\+ {\\displaystyle +} ![{\\displaystyle +}](https://wikimedia.org/api/rest_v1/media/math/render/svg/fe6ef363cd19902d1a7a71fb1c8b21e8ede52406)) denotes a graph is increasing (going upward) and the negative sign (− {\\displaystyle -} ![{\\displaystyle -}](https://wikimedia.org/api/rest_v1/media/math/render/svg/04bd52ce670743d3b61bec928a7ec9f47309eb36)) is decreasing (going downward)—in certain intervals.[\[3\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742-3) This information can be represented as a Cartesian coordinates system divided into four quadrants. | [Quadrant](https://en.wikipedia.org/wiki/Cartesian_coordinate_system#Quadrants_and_octants "Cartesian coordinate system") | Angle | Sine | Cosine | | | | | |---|---|---|---|---|---|---|---| | [Degrees](https://en.wikipedia.org/wiki/Degree_\(angle\) "Degree (angle)") | [Radians](https://en.wikipedia.org/wiki/Radian "Radian") | [Sign](https://en.wikipedia.org/wiki/Sign_\(mathematics\) "Sign (mathematics)") | [Monotony](https://en.wikipedia.org/wiki/Monotonic_function "Monotonic function") | [Convexity](https://en.wikipedia.org/wiki/Convex_function "Convex function") | [Sign](https://en.wikipedia.org/wiki/Sign_\(mathematics\) "Sign (mathematics)") | [Monotony](https://en.wikipedia.org/wiki/Monotonic_function "Monotonic function") | [Convexity](https://en.wikipedia.org/wiki/Convex_function "Convex function") | | 1st quadrant, I | 0 ∘ \< x \< 90 ∘ {\\displaystyle 0^{\\circ }\<x\<90^{\\circ }} ![{\\displaystyle 0^{\\circ }\<x\<90^{\\circ }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3cd94c157a7ab3ac44ece2b4a7e2a805c5e3774b) | | | | | | | Both sine and cosine functions can be defined by using differential equations. The pair of ( cos ⁡ θ , sin ⁡ θ ) {\\displaystyle (\\cos \\theta ,\\sin \\theta )} ![{\\displaystyle (\\cos \\theta ,\\sin \\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/591da286444bb19845241d047707dd8793d4b143) is the solution ( x ( θ ) , y ( θ ) ) {\\displaystyle (x(\\theta ),y(\\theta ))} ![{\\displaystyle (x(\\theta ),y(\\theta ))}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3761d6e3635ea327a1fea316311a9974ba2a2898) to the two-dimensional system of [differential equations](https://en.wikipedia.org/wiki/Differential_equation "Differential equation") y ′ ( θ ) \= x ( θ ) {\\displaystyle y'(\\theta )=x(\\theta )} ![{\\displaystyle y'(\\theta )=x(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e24c7568490cc0b2b359757eab6411e071ea5a4e) and x ′ ( θ ) \= − y ( θ ) {\\displaystyle x'(\\theta )=-y(\\theta )} ![{\\displaystyle x'(\\theta )=-y(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8d2efd00b2708f705444970234d98bb745c37b4c) with the [initial conditions](https://en.wikipedia.org/wiki/Initial_conditions "Initial conditions") y ( 0 ) \= 0 {\\displaystyle y(0)=0} ![{\\displaystyle y(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/343c32f38bb379b4b208477b130d8f522d3f0788) and x ( 0 ) \= 1 {\\displaystyle x(0)=1} ![{\\displaystyle x(0)=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e502f85fa127369616c9d6cce7b0cfdfad2abbc1). One could interpret the unit circle in the above definitions as defining the [phase space trajectory](https://en.wikipedia.org/wiki/Phase_space_trajectory "Phase space trajectory") of the differential equation with the given initial conditions. It can be interpreted as a phase space trajectory of the system of differential equations y ′ ( θ ) \= x ( θ ) {\\displaystyle y'(\\theta )=x(\\theta )} ![{\\displaystyle y'(\\theta )=x(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e24c7568490cc0b2b359757eab6411e071ea5a4e) and x ′ ( θ ) \= − y ( θ ) {\\displaystyle x'(\\theta )=-y(\\theta )} ![{\\displaystyle x'(\\theta )=-y(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8d2efd00b2708f705444970234d98bb745c37b4c) starting from the initial conditions y ( 0 ) \= 0 {\\displaystyle y(0)=0} ![{\\displaystyle y(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/343c32f38bb379b4b208477b130d8f522d3f0788) and x ( 0 ) \= 1 {\\displaystyle x(0)=1} ![{\\displaystyle x(0)=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e502f85fa127369616c9d6cce7b0cfdfad2abbc1).\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] #### Integral and the usage in mensuration \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=10 "Edit section: Integral and the usage in mensuration")\] Main article: [List of integrals of trigonometric functions](https://en.wikipedia.org/wiki/List_of_integrals_of_trigonometric_functions "List of integrals of trigonometric functions") Their area under a curve can be obtained by using the [integral](https://en.wikipedia.org/wiki/Integral "Integral") with a certain bounded interval. Their antiderivatives are: ∫ sin ⁡ ( x ) d x \= − cos ⁡ ( x ) \+ C ∫ cos ⁡ ( x ) d x \= sin ⁡ ( x ) \+ C , {\\displaystyle \\int \\sin(x)\\,dx=-\\cos(x)+C\\qquad \\int \\cos(x)\\,dx=\\sin(x)+C,} ![{\\displaystyle \\int \\sin(x)\\,dx=-\\cos(x)+C\\qquad \\int \\cos(x)\\,dx=\\sin(x)+C,}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2e14210f7e049e74d1153559c98ea8fd4fb5efa0) where C {\\displaystyle C} ![{\\displaystyle C}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4fc55753007cd3c18576f7933f6f089196732029) denotes the [constant of integration](https://en.wikipedia.org/wiki/Constant_of_integration "Constant of integration").[\[21\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007199-21) These antiderivatives may be applied to compute the mensuration properties of both sine and cosine functions' curves with a given interval. For example, the [arc length](https://en.wikipedia.org/wiki/Arc_length "Arc length") of the sine curve between 0 {\\displaystyle 0} ![{\\displaystyle 0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2aae8864a3c1fec9585261791a809ddec1489950) and t {\\displaystyle t} ![{\\displaystyle t}](https://wikimedia.org/api/rest_v1/media/math/render/svg/65658b7b223af9e1acc877d848888ecdb4466560) is ∫ 0 t 1 \+ cos 2 ⁡ ( x ) d x \= 2 E ⁡ ( t , 1 2 ) , {\\displaystyle \\int \_{0}^{t}\\!{\\sqrt {1+\\cos ^{2}(x)}}\\,dx={\\sqrt {2}}\\operatorname {E} \\left(t,{\\frac {1}{\\sqrt {2}}}\\right),} ![{\\displaystyle \\int \_{0}^{t}\\!{\\sqrt {1+\\cos ^{2}(x)}}\\,dx={\\sqrt {2}}\\operatorname {E} \\left(t,{\\frac {1}{\\sqrt {2}}}\\right),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a4e732378f19b126018432e28c062594d9538420) where E ⁡ ( φ , k ) {\\displaystyle \\operatorname {E} (\\varphi ,k)} ![{\\displaystyle \\operatorname {E} (\\varphi ,k)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c1520125a116a29984e7bca67df1f10ef35292b0) is the [incomplete elliptic integral of the second kind](https://en.wikipedia.org/wiki/Elliptic_integral#Incomplete_elliptic_integral_of_the_second_kind "Elliptic integral") with modulus k {\\displaystyle k} ![{\\displaystyle k}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c3c9a2c7b599b37105512c5d570edc034056dd40). It cannot be expressed using [elementary functions](https://en.wikipedia.org/wiki/Elementary_function "Elementary function").[\[22\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVince2023[httpsbooksgooglecombooksidGnW6EAAAQBAJpgPA162_162]-22) In the case of a full period, its arc length is L \= 4 2 π 3 Γ ( 1 / 4 ) 2 \+ Γ ( 1 / 4 ) 2 2 π \= 2 π ϖ \+ 2 ϖ ≈ 7\.6404 {\\displaystyle L={\\frac {4{\\sqrt {2\\pi ^{3}}}}{\\Gamma (1/4)^{2}}}+{\\frac {\\Gamma (1/4)^{2}}{\\sqrt {2\\pi }}}={\\frac {2\\pi }{\\varpi }}+2\\varpi \\approx 7.6404} ![{\\displaystyle L={\\frac {4{\\sqrt {2\\pi ^{3}}}}{\\Gamma (1/4)^{2}}}+{\\frac {\\Gamma (1/4)^{2}}{\\sqrt {2\\pi }}}={\\frac {2\\pi }{\\varpi }}+2\\varpi \\approx 7.6404}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7a6d9ffe117d665d73ef4788658c5b5cfd8cae33) where Γ {\\displaystyle \\Gamma } ![{\\displaystyle \\Gamma }](https://wikimedia.org/api/rest_v1/media/math/render/svg/4cfde86a3f7ec967af9955d0988592f0693d2b19) is the [gamma function](https://en.wikipedia.org/wiki/Gamma_function "Gamma function") and ϖ {\\displaystyle \\varpi } ![{\\displaystyle \\varpi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/e50d258418b5fa150a86b58f8d5eb40613e3ebf7) is the [lemniscate constant](https://en.wikipedia.org/wiki/Lemniscate_constant "Lemniscate constant").[\[23\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAdlaj2012-23)[\[24\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-24) #### Inverse functions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=11 "Edit section: Inverse functions")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b4/Arcsine_Arccosine.svg/250px-Arcsine_Arccosine.svg.png)](https://en.wikipedia.org/wiki/File:Arcsine_Arccosine.svg) The usual principal values of the arcsin(*x*) and arccos(*x*) functions graphed on the Cartesian plane The functions sin : R → R {\\textstyle \\sin :\\mathbb {R} \\to \\mathbb {R} } ![{\\textstyle \\sin :\\mathbb {R} \\to \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/5b76babd4c66e7d6257658191c1e4b6dd443412d) and cos : R → R {\\displaystyle \\cos :\\mathbb {R} \\to \\mathbb {R} } ![{\\displaystyle \\cos :\\mathbb {R} \\to \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/490d5f0e2fdc2b561101f411ecea9e3f98e468d9) (as well as those functions with the same function rule and domain whose codomain is a subset of R {\\displaystyle \\mathbb {R} } ![{\\displaystyle \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/786849c765da7a84dbc3cce43e96aad58a5868dc) containing the interval \[ − 1 , 1 \] {\\displaystyle \\left\[-1,1\\right\]} ![{\\displaystyle \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/79566f857ac1fcd0ef0f62226298a4ed15b796ad)) are not bijective and therefore do not have inverse functions. For example, sin ⁡ ( 0 ) \= 0 {\\displaystyle \\sin(0)=0} ![{\\displaystyle \\sin(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ecb40badcf53b50e5d03c49c7a5e1977e3ff262e), but also sin ⁡ ( π ) \= 0 {\\displaystyle \\sin(\\pi )=0} ![{\\displaystyle \\sin(\\pi )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f6e7e3130a6ba2043ae878c9b1dc7aa7998afb8c), sin ⁡ ( 2 π ) \= 0 {\\displaystyle \\sin(2\\pi )=0} ![{\\displaystyle \\sin(2\\pi )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/55c160c102e7cd62b4a03d1df4761601235a2b3d). Sine's "inverse", called arcsine, can then be described not as a function but a relation (for example, all integer multiples of π {\\displaystyle \\pi } ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a) would have an arcsine of zero). To define the inverse functions of sine and cosine, they must be restricted to their [principal branches](https://en.wikipedia.org/wiki/Principal_branch "Principal branch") by restricting their domain and codomain; the standard functions used to define arcsine and arccosine are then sin : \[ − π / 2 , π / 2 \] → \[ − 1 , 1 \] {\\displaystyle \\sin :\\left\[-\\pi /2,\\pi /2\\right\]\\to \\left\[-1,1\\right\]} ![{\\displaystyle \\sin :\\left\[-\\pi /2,\\pi /2\\right\]\\to \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/34676d3cc30ba3520fb506118910a65ae45fe25f) and cos : \[ 0 , π \] → \[ − 1 , 1 \] {\\displaystyle \\cos :\\left\[0,\\pi \\right\]\\to \\left\[-1,1\\right\]} ![{\\displaystyle \\cos :\\left\[0,\\pi \\right\]\\to \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4a2864b5c77dc4b8af5111e9d4e78e9ea9a876b7).[\[25\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007365-25) These are bijective and have inverses: arcsin : \[ − 1 , 1 \] → \[ − π / 2 , π / 2 \] {\\displaystyle \\arcsin :\\left\[-1,1\\right\]\\to \\left\[-\\pi /2,\\pi /2\\right\]} ![{\\displaystyle \\arcsin :\\left\[-1,1\\right\]\\to \\left\[-\\pi /2,\\pi /2\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/024a4d91e022705b40fb40e554d294bdd9e2eea4) and arccos : \[ − 1 , 1 \] → \[ 0 , π \] {\\displaystyle \\arccos :\\left\[-1,1\\right\]\\to \\left\[0,\\pi \\right\]} ![{\\displaystyle \\arccos :\\left\[-1,1\\right\]\\to \\left\[0,\\pi \\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e1126b78ee63338e44c6a25dae46d50fdad0b5c1). Alternative notation is sin − 1 {\\displaystyle \\sin ^{-1}} ![{\\displaystyle \\sin ^{-1}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/21bc4ca64ac415c9ae60fb4e60fe4bddee17b8ef) for arcsine and cos − 1 {\\displaystyle \\cos ^{-1}} ![{\\displaystyle \\cos ^{-1}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7eabf706b4642d521c6279a2f07ac9715c7679a7) for arccosine. Using these definitions, one obtains the identity maps: sin ∘ arcsin ( x ) \= x x ∈ \[ − 1 , 1 \] arcsin ∘ sin ( x ) \= x x ∈ \[ − π / 2 , π / 2 \] {\\displaystyle {\\begin{aligned}\\sin \\circ \\arcsin \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arcsin \\circ \\sin \\,(x)&=x\\qquad x\\in \\left\[-\\pi /2,\\pi /2\\right\]\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin \\circ \\arcsin \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arcsin \\circ \\sin \\,(x)&=x\\qquad x\\in \\left\[-\\pi /2,\\pi /2\\right\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/631b526ef79de3155b8c652483e136009c87f6ef)and cos ∘ arccos ( x ) \= x x ∈ \[ − 1 , 1 \] arccos ∘ cos ( x ) \= x x ∈ \[ 0 , π \] {\\displaystyle {\\begin{aligned}\\cos \\circ \\arccos \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arccos \\circ \\cos \\,(x)&=x\\qquad x\\in \\left\[0,\\pi \\right\]\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\cos \\circ \\arccos \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arccos \\circ \\cos \\,(x)&=x\\qquad x\\in \\left\[0,\\pi \\right\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/81aa8f5001ec127005efd5c2508631440ff6ab8d) An acute angle θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) is given by: θ \= arcsin ⁡ ( opposite hypotenuse ) \= arccos ⁡ ( adjacent hypotenuse ) , {\\displaystyle \\theta =\\arcsin \\left({\\frac {\\text{opposite}}{\\text{hypotenuse}}}\\right)=\\arccos \\left({\\frac {\\text{adjacent}}{\\text{hypotenuse}}}\\right),} ![{\\displaystyle \\theta =\\arcsin \\left({\\frac {\\text{opposite}}{\\text{hypotenuse}}}\\right)=\\arccos \\left({\\frac {\\text{adjacent}}{\\text{hypotenuse}}}\\right),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6a7fb2ae2f0c2ec3085667df4d1e54d48d67cd7a) where for some integer k {\\displaystyle k} ![{\\displaystyle k}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c3c9a2c7b599b37105512c5d570edc034056dd40), sin ⁡ ( y ) \= x ⟺ y \= arcsin ⁡ ( x ) \+ 2 π k , or y \= π − arcsin ⁡ ( x ) \+ 2 π k cos ⁡ ( y ) \= x ⟺ y \= arccos ⁡ ( x ) \+ 2 π k , or y \= − arccos ⁡ ( x ) \+ 2 π k {\\displaystyle {\\begin{aligned}\\sin(y)=x\\iff \&y=\\arcsin(x)+2\\pi k,{\\text{ or }}\\\\\&y=\\pi -\\arcsin(x)+2\\pi k\\\\\\cos(y)=x\\iff \&y=\\arccos(x)+2\\pi k,{\\text{ or }}\\\\\&y=-\\arccos(x)+2\\pi k\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(y)=x\\iff \&y=\\arcsin(x)+2\\pi k,{\\text{ or }}\\\\\&y=\\pi -\\arcsin(x)+2\\pi k\\\\\\cos(y)=x\\iff \&y=\\arccos(x)+2\\pi k,{\\text{ or }}\\\\\&y=-\\arccos(x)+2\\pi k\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/da20b32e7b46d5ccdf3f058b812c8ad9768fa678) By definition, both functions satisfy the equations: sin ⁡ ( arcsin ⁡ ( x ) ) \= x cos ⁡ ( arccos ⁡ ( x ) ) \= x {\\displaystyle \\sin(\\arcsin(x))=x\\qquad \\cos(\\arccos(x))=x} ![{\\displaystyle \\sin(\\arcsin(x))=x\\qquad \\cos(\\arccos(x))=x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/25b4ef466eeb61838eb9b7b8692bebf636a9423f) and arcsin ⁡ ( sin ⁡ ( θ ) ) \= θ for − π 2 ≤ θ ≤ π 2 arccos ⁡ ( cos ⁡ ( θ ) ) \= θ for 0 ≤ θ ≤ π {\\displaystyle {\\begin{aligned}\\arcsin(\\sin(\\theta ))=\\theta \\quad &{\\text{for}}\\quad -{\\frac {\\pi }{2}}\\leq \\theta \\leq {\\frac {\\pi }{2}}\\\\\\arccos(\\cos(\\theta ))=\\theta \\quad &{\\text{for}}\\quad 0\\leq \\theta \\leq \\pi \\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\arcsin(\\sin(\\theta ))=\\theta \\quad &{\\text{for}}\\quad -{\\frac {\\pi }{2}}\\leq \\theta \\leq {\\frac {\\pi }{2}}\\\\\\arccos(\\cos(\\theta ))=\\theta \\quad &{\\text{for}}\\quad 0\\leq \\theta \\leq \\pi \\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/11a64d948fdadfaf9eeb77c6fcd8c3f646f46cee) #### Other identities \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=12 "Edit section: Other identities")\] Main article: [List of trigonometric identities](https://en.wikipedia.org/wiki/List_of_trigonometric_identities "List of trigonometric identities") According to [Pythagorean theorem](https://en.wikipedia.org/wiki/Pythagorean_theorem "Pythagorean theorem"), the squared hypotenuse is the sum of two squared legs of a right triangle. Dividing the formula on both sides with squared hypotenuse resulting in the [Pythagorean trigonometric identity](https://en.wikipedia.org/wiki/Pythagorean_trigonometric_identity "Pythagorean trigonometric identity"), the sum of a squared sine and a squared cosine equals 1:[\[26\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA99_99]-26)[\[a\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-27) sin 2 ⁡ ( θ ) \+ cos 2 ⁡ ( θ ) \= 1\. {\\displaystyle \\sin ^{2}(\\theta )+\\cos ^{2}(\\theta )=1.} ![{\\displaystyle \\sin ^{2}(\\theta )+\\cos ^{2}(\\theta )=1.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8c2fa6795bad3d685ca0704a63f5771bda27d5ac) Sine and cosine satisfy the following double-angle formulas:[\[27\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-28) sin ⁡ ( 2 θ ) \= 2 sin ⁡ ( θ ) cos ⁡ ( θ ) , cos ⁡ ( 2 θ ) \= cos 2 ⁡ ( θ ) − sin 2 ⁡ ( θ ) \= 2 cos 2 ⁡ ( θ ) − 1 \= 1 − 2 sin 2 ⁡ ( θ ) {\\displaystyle {\\begin{aligned}\\sin(2\\theta )&=2\\sin(\\theta )\\cos(\\theta ),\\\\\\cos(2\\theta )&=\\cos ^{2}(\\theta )-\\sin ^{2}(\\theta )\\\\&=2\\cos ^{2}(\\theta )-1\\\\&=1-2\\sin ^{2}(\\theta )\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(2\\theta )&=2\\sin(\\theta )\\cos(\\theta ),\\\\\\cos(2\\theta )&=\\cos ^{2}(\\theta )-\\sin ^{2}(\\theta )\\\\&=2\\cos ^{2}(\\theta )-1\\\\&=1-2\\sin ^{2}(\\theta )\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/497be0073c63433342edee671020c7aa109e0e6e) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c9/SinSquared.png/250px-SinSquared.png)](https://en.wikipedia.org/wiki/File:SinSquared.png) Sine function in blue and sine squared function in red. The *x*\-axis is in radians. The cosine double angle formula implies that sin2 and cos2 are, themselves, shifted and scaled sine waves. Specifically,[\[28\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-29) sin 2 ⁡ ( θ ) \= 1 − cos ⁡ ( 2 θ ) 2 cos 2 ⁡ ( θ ) \= 1 \+ cos ⁡ ( 2 θ ) 2 {\\displaystyle \\sin ^{2}(\\theta )={\\frac {1-\\cos(2\\theta )}{2}}\\qquad \\cos ^{2}(\\theta )={\\frac {1+\\cos(2\\theta )}{2}}} ![{\\displaystyle \\sin ^{2}(\\theta )={\\frac {1-\\cos(2\\theta )}{2}}\\qquad \\cos ^{2}(\\theta )={\\frac {1+\\cos(2\\theta )}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4dc6bb37905a99fd21458b0011b90ebfcf6e9092) The graph shows both sine and sine squared functions, with the sine in blue and the sine squared in red. Both graphs have the same shape but with different ranges of values and different periods. Sine squared has only positive values, but twice the number of periods.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] ### Series and polynomials \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=13 "Edit section: Series and polynomials")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Sine.gif/250px-Sine.gif)](https://en.wikipedia.org/wiki/File:Sine.gif) This animation shows how including more and more terms in the partial sum of its Taylor series approaches a sine curve. Both sine and cosine functions can be defined by using a [Taylor series](https://en.wikipedia.org/wiki/Taylor_series "Taylor series"), a [power series](https://en.wikipedia.org/wiki/Power_series "Power series") involving the higher-order derivatives. As mentioned in [§ Continuity and differentiation](https://en.wikipedia.org/wiki/Sine_and_cosine#Continuity_and_differentiation), the [derivative](https://en.wikipedia.org/wiki/Derivative "Derivative") of sine is cosine and the derivative of cosine is the negative of sine. This means the successive derivatives of sin ⁡ ( x ) {\\displaystyle \\sin(x)} ![{\\displaystyle \\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3a990a5545cac26c1c6821dca95d898bc80fe3a8) are cos ⁡ ( x ) {\\displaystyle \\cos(x)} ![{\\displaystyle \\cos(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/eb9af7ed6f44822021b74bb82b431022c7fd66b3), − sin ⁡ ( x ) {\\displaystyle -\\sin(x)} ![{\\displaystyle -\\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a7326163fe774b61667587334208ecaef5798056), − cos ⁡ ( x ) {\\displaystyle -\\cos(x)} ![{\\displaystyle -\\cos(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3f5dca2087cf314bb30116832bea1df5e00086be), sin ⁡ ( x ) {\\displaystyle \\sin(x)} ![{\\displaystyle \\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3a990a5545cac26c1c6821dca95d898bc80fe3a8), continuing to repeat those four functions. The ( 4 n \+ k ) {\\displaystyle (4n+k)} ![{\\displaystyle (4n+k)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d6d26c80aefe4f8e27c3b52e0b0375980f8addba) \-th derivative, evaluated at the point 0: sin ( 4 n \+ k ) ⁡ ( 0 ) \= { 0 when k \= 0 1 when k \= 1 0 when k \= 2 − 1 when k \= 3 {\\displaystyle \\sin ^{(4n+k)}(0)={\\begin{cases}0&{\\text{when }}k=0\\\\1&{\\text{when }}k=1\\\\0&{\\text{when }}k=2\\\\-1&{\\text{when }}k=3\\end{cases}}} ![{\\displaystyle \\sin ^{(4n+k)}(0)={\\begin{cases}0&{\\text{when }}k=0\\\\1&{\\text{when }}k=1\\\\0&{\\text{when }}k=2\\\\-1&{\\text{when }}k=3\\end{cases}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d46c038e501fe9a5f4ca170b57667a244b9b77b2) where the superscript represents repeated differentiation. This implies the following Taylor series expansion at x \= 0 {\\displaystyle x=0} ![{\\displaystyle x=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/953917eaf52f2e1baad54c8c9e3d6f9bb3710cdc). One can then use the theory of [Taylor series](https://en.wikipedia.org/wiki/Taylor_series "Taylor series") to show that the following identities hold for all [real numbers](https://en.wikipedia.org/wiki/Real_number "Real number") x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4)—where x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) is the angle in radians.[\[29\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492-30) More generally, for all [complex numbers](https://en.wikipedia.org/wiki/Complex_number "Complex number"):[\[30\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]-31) sin ⁡ ( x ) \= x − x 3 3 \! \+ x 5 5 \! − x 7 7 \! \+ ⋯ \= ∑ n \= 0 ∞ ( − 1 ) n ( 2 n \+ 1 ) \! x 2 n \+ 1 {\\displaystyle {\\begin{aligned}\\sin(x)&=x-{\\frac {x^{3}}{3!}}+{\\frac {x^{5}}{5!}}-{\\frac {x^{7}}{7!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}x^{2n+1}\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(x)&=x-{\\frac {x^{3}}{3!}}+{\\frac {x^{5}}{5!}}-{\\frac {x^{7}}{7!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}x^{2n+1}\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f13ee50efedabff2d208516e6a31ea495a9c843d) Taking the derivative of each term gives the Taylor series for cosine:[\[29\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492-30)[\[30\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]-31) cos ⁡ ( x ) \= 1 − x 2 2 \! \+ x 4 4 \! − x 6 6 \! \+ ⋯ \= ∑ n \= 0 ∞ ( − 1 ) n ( 2 n ) \! x 2 n {\\displaystyle {\\begin{aligned}\\cos(x)&=1-{\\frac {x^{2}}{2!}}+{\\frac {x^{4}}{4!}}-{\\frac {x^{6}}{6!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}x^{2n}\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\cos(x)&=1-{\\frac {x^{2}}{2!}}+{\\frac {x^{4}}{4!}}-{\\frac {x^{6}}{6!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}x^{2n}\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/742bd8177eff1a0186a49c19c6a0c626c7fe3563) Both sine and cosine functions with multiple angles may appear as their [linear combination](https://en.wikipedia.org/wiki/Linear_combination "Linear combination"), resulting in a polynomial. Such a polynomial is known as the [trigonometric polynomial](https://en.wikipedia.org/wiki/Trigonometric_polynomial "Trigonometric polynomial"). The trigonometric polynomial's ample applications may be acquired in [its interpolation](https://en.wikipedia.org/wiki/Trigonometric_interpolation "Trigonometric interpolation"), and its extension of a periodic function known as the [Fourier series](https://en.wikipedia.org/wiki/Fourier_series "Fourier series"). Let a n {\\displaystyle a\_{n}} ![{\\displaystyle a\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/790f9209748c2dca7ed7b81932c37c02af1dbc31) and b n {\\displaystyle b\_{n}} ![{\\displaystyle b\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/28e2d72f6dd9375c8f1f59f1effd9b4e5492ac97) be any coefficients, then the trigonometric polynomial of a degree N {\\displaystyle N} ![{\\displaystyle N}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f5e3890c981ae85503089652feb48b191b57aae3)—denoted as T ( x ) {\\displaystyle T(x)} ![{\\displaystyle T(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/1171c29b4c2b5575f50a4ea9313f90448a2cbe05)—is defined as:[\[31\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEPowell1981150-32)[\[32\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTERudin198788-33) T ( x ) \= a 0 \+ ∑ n \= 1 N a n cos ⁡ ( n x ) \+ ∑ n \= 1 N b n sin ⁡ ( n x ) . {\\displaystyle T(x)=a\_{0}+\\sum \_{n=1}^{N}a\_{n}\\cos(nx)+\\sum \_{n=1}^{N}b\_{n}\\sin(nx).} ![{\\displaystyle T(x)=a\_{0}+\\sum \_{n=1}^{N}a\_{n}\\cos(nx)+\\sum \_{n=1}^{N}b\_{n}\\sin(nx).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0d91df6657ed384066a15aee6f8f0ef01c9a0787) The [trigonometric series](https://en.wikipedia.org/wiki/Trigonometric_series "Trigonometric series") can be defined similarly analogous to the trigonometric polynomial, its infinite inversion. Let A n {\\displaystyle A\_{n}} ![{\\displaystyle A\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/730f6906700685b6d52f3958b1c2ae659d2d97d2) and B n {\\displaystyle B\_{n}} ![{\\displaystyle B\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2f568bf6d34e97b9fdda0dc7e276d6c4501d2045) be any coefficients, then the trigonometric series can be defined as:[\[33\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZygmund19681-34) 1 2 A 0 \+ ∑ n \= 1 ∞ A n cos ⁡ ( n x ) \+ B n sin ⁡ ( n x ) . {\\displaystyle {\\frac {1}{2}}A\_{0}+\\sum \_{n=1}^{\\infty }A\_{n}\\cos(nx)+B\_{n}\\sin(nx).} ![{\\displaystyle {\\frac {1}{2}}A\_{0}+\\sum \_{n=1}^{\\infty }A\_{n}\\cos(nx)+B\_{n}\\sin(nx).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a20bbca53c25bda2d3a375f83924db3637e013b7) In the case of a Fourier series with a given integrable function f {\\displaystyle f} ![{\\displaystyle f}](https://wikimedia.org/api/rest_v1/media/math/render/svg/132e57acb643253e7810ee9702d9581f159a1c61), the coefficients of a trigonometric series are:[\[34\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZygmund196811-35) A n \= 1 π ∫ 0 2 π f ( x ) cos ⁡ ( n x ) d x , B n \= 1 π ∫ 0 2 π f ( x ) sin ⁡ ( n x ) d x . {\\displaystyle {\\begin{aligned}A\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\cos(nx)\\,dx,\\\\B\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\sin(nx)\\,dx.\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}A\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\cos(nx)\\,dx,\\\\B\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\sin(nx)\\,dx.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/71e46a4445a4bb3a0d5933f7f542c39673dafef1) ## Complex numbers relationship \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=14 "Edit section: Complex numbers relationship")\] | | | |---|---| | [![icon](https://upload.wikimedia.org/wikipedia/en/thumb/9/99/Question_book-new.svg/60px-Question_book-new.svg.png)](https://en.wikipedia.org/wiki/File:Question_book-new.svg) | This section **needs additional citations for [verification](https://en.wikipedia.org/wiki/Wikipedia:Verifiability "Wikipedia:Verifiability")**. Please help [improve this article](https://en.wikipedia.org/wiki/Special:EditPage/Sine_and_cosine "Special:EditPage/Sine and cosine") by [adding citations to reliable sources](https://en.wikipedia.org/wiki/Help:Referencing_for_beginners "Help:Referencing for beginners") in this section. Unsourced material may be challenged and removed. *(August 2024)* *([Learn how and when to remove this message](https://en.wikipedia.org/wiki/Help:Maintenance_template_removal "Help:Maintenance template removal"))* | ### Complex exponential function definitions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=15 "Edit section: Complex exponential function definitions")\] Both sine and cosine can be extended further via [complex number](https://en.wikipedia.org/wiki/Complex_number "Complex number"), a set of numbers composed of both [real](https://en.wikipedia.org/wiki/Real_number "Real number") and [imaginary numbers](https://en.wikipedia.org/wiki/Imaginary_number "Imaginary number"). For real number θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), the definition of both sine and cosine functions can be extended in a [complex plane](https://en.wikipedia.org/wiki/Complex_plane "Complex plane") in terms of an [exponential function](https://en.wikipedia.org/wiki/Exponential_function "Exponential function") as follows:[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) sin ⁡ ( θ ) \= e i θ − e − i θ 2 i , cos ⁡ ( θ ) \= e i θ \+ e − i θ 2 , {\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {e^{i\\theta }-e^{-i\\theta }}{2i}},\\\\\\cos(\\theta )&={\\frac {e^{i\\theta }+e^{-i\\theta }}{2}},\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {e^{i\\theta }-e^{-i\\theta }}{2i}},\\\\\\cos(\\theta )&={\\frac {e^{i\\theta }+e^{-i\\theta }}{2}},\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/725f29f76be948091e80a1467b067a8ca9e9dbd3) Alternatively, both functions can be defined in terms of [Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula"):[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) e i θ \= cos ⁡ ( θ ) \+ i sin ⁡ ( θ ) , e − i θ \= cos ⁡ ( θ ) − i sin ⁡ ( θ ) . {\\displaystyle {\\begin{aligned}e^{i\\theta }&=\\cos(\\theta )+i\\sin(\\theta ),\\\\e^{-i\\theta }&=\\cos(\\theta )-i\\sin(\\theta ).\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}e^{i\\theta }&=\\cos(\\theta )+i\\sin(\\theta ),\\\\e^{-i\\theta }&=\\cos(\\theta )-i\\sin(\\theta ).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/77db983756d03fe6b65cfb8af534812004ebfbbb) When plotted on the [complex plane](https://en.wikipedia.org/wiki/Complex_plane "Complex plane"), the function e i x {\\displaystyle e^{ix}} ![{\\displaystyle e^{ix}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5271aa5bef13f6bd715afeda45bc59ae37d7c6d4) for real values of x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) traces out the [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle") in the complex plane. Both sine and cosine functions may be simplified to the imaginary and real parts of e i θ {\\displaystyle e^{i\\theta }} ![{\\displaystyle e^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7b4b8e67ee479d68e0e5040aaf87eff99214c90f) as:[\[36\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTERudin19872-37) sin ⁡ θ \= Im ⁡ ( e i θ ) , cos ⁡ θ \= Re ⁡ ( e i θ ) . {\\displaystyle {\\begin{aligned}\\sin \\theta &=\\operatorname {Im} (e^{i\\theta }),\\\\\\cos \\theta &=\\operatorname {Re} (e^{i\\theta }).\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin \\theta &=\\operatorname {Im} (e^{i\\theta }),\\\\\\cos \\theta &=\\operatorname {Re} (e^{i\\theta }).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/646f096950ba96ce2f21de18bfa047b6421b21e0) When z \= x \+ i y {\\displaystyle z=x+iy} ![{\\displaystyle z=x+iy}](https://wikimedia.org/api/rest_v1/media/math/render/svg/08e90bb6b36fef59c6113eed2a08f10d77240741) for real values x {\\displaystyle x} ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) and y {\\displaystyle y} ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d), where i \= − 1 {\\displaystyle i={\\sqrt {-1}}} ![{\\displaystyle i={\\sqrt {-1}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/370c8cebe9634fbfc84c29ea61680b0ad4a1ae0d), both sine and cosine functions can be expressed in terms of real sines, cosines, and [hyperbolic functions](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function") as:[\[37\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-38) sin ⁡ z \= sin ⁡ x cosh ⁡ y \+ i cos ⁡ x sinh ⁡ y , cos ⁡ z \= cos ⁡ x cosh ⁡ y − i sin ⁡ x sinh ⁡ y . {\\displaystyle {\\begin{aligned}\\sin z&=\\sin x\\cosh y+i\\cos x\\sinh y,\\\\\\cos z&=\\cos x\\cosh y-i\\sin x\\sinh y.\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin z&=\\sin x\\cosh y+i\\cos x\\sinh y,\\\\\\cos z&=\\cos x\\cosh y-i\\sin x\\sinh y.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/47251493866932a39ed455153827afe21a781596) ### Polar coordinates \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=16 "Edit section: Polar coordinates")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/8/8d/Sinus_und_Kosinus_am_Einheitskreis_3.svg/250px-Sinus_und_Kosinus_am_Einheitskreis_3.svg.png)](https://en.wikipedia.org/wiki/File:Sinus_und_Kosinus_am_Einheitskreis_3.svg) Both functions cos ⁡ ( θ ) {\\displaystyle \\cos(\\theta )} ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd) and sin ⁡ ( θ ) {\\displaystyle \\sin(\\theta )} ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948) are the real and imaginary parts of e i θ {\\displaystyle e^{i\\theta }} ![{\\displaystyle e^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7b4b8e67ee479d68e0e5040aaf87eff99214c90f) . Sine and cosine are used to connect the real and imaginary parts of a [complex number](https://en.wikipedia.org/wiki/Complex_number "Complex number") with its [polar coordinates](https://en.wikipedia.org/wiki/Polar_coordinates "Polar coordinates") ( r , θ ) {\\displaystyle (r,\\theta )} ![{\\displaystyle (r,\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ed8396fdc359fb06c93722137c959e7496e47ed6): z \= r ( cos ⁡ ( θ ) \+ i sin ⁡ ( θ ) ) \= r cos ⁡ ( θ ) \+ i r sin ⁡ ( θ ) , {\\displaystyle z=r(\\cos(\\theta )+i\\sin(\\theta ))=r\\cos(\\theta )+ir\\sin(\\theta ),} ![{\\displaystyle z=r(\\cos(\\theta )+i\\sin(\\theta ))=r\\cos(\\theta )+ir\\sin(\\theta ),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/250e8c59ae404db0bbf52c140bd7b9d7ac8387b2) and the real and imaginary parts are Re ⁡ ( z ) \= r cos ⁡ ( θ ) , Im ⁡ ( z ) \= r sin ⁡ ( θ ) , {\\displaystyle {\\begin{aligned}\\operatorname {Re} (z)&=r\\cos(\\theta ),\\\\\\operatorname {Im} (z)&=r\\sin(\\theta ),\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\operatorname {Re} (z)&=r\\cos(\\theta ),\\\\\\operatorname {Im} (z)&=r\\sin(\\theta ),\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/abf44a594aabf7817998c91793f805ecdb366282) where r {\\displaystyle r} ![{\\displaystyle r}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0d1ecb613aa2984f0576f70f86650b7c2a132538) and θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) represent the magnitude and angle of the complex number z {\\displaystyle z} ![{\\displaystyle z}](https://wikimedia.org/api/rest_v1/media/math/render/svg/bf368e72c009decd9b6686ee84a375632e11de98).[\[38\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_23&ndash;24]-39) For any real number θ {\\displaystyle \\theta } ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), Euler's formula in terms of polar coordinates is stated as z \= r e i θ {\\textstyle z=re^{i\\theta }} ![{\\textstyle z=re^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/95946f451434232fc04452bd3b3e4251de1a9d13).[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) ### Complex arguments \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=17 "Edit section: Complex arguments")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/4/45/Complex_sin.jpg/250px-Complex_sin.jpg)](https://en.wikipedia.org/wiki/File:Complex_sin.jpg) [Domain coloring](https://en.wikipedia.org/wiki/Domain_coloring "Domain coloring") of sin(*z*) in the complex plane. Brightness indicates absolute magnitude, hue represents complex argument. [![](https://upload.wikimedia.org/wikipedia/commons/thumb/9/96/Sin_z_vector_field_02_Pengo.svg/250px-Sin_z_vector_field_02_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Sin_z_vector_field_02_Pengo.svg) Vector field rendering of sin(*z*) Applying the series definition of the sine and cosine to a complex argument, *z*, gives: sin ⁡ ( z ) \= ∑ n \= 0 ∞ ( − 1 ) n ( 2 n \+ 1 ) \! z 2 n \+ 1 \= e i z − e − i z 2 i \= sinh ⁡ ( i z ) i \= − i sinh ⁡ ( i z ) cos ⁡ ( z ) \= ∑ n \= 0 ∞ ( − 1 ) n ( 2 n ) \! z 2 n \= e i z \+ e − i z 2 \= cosh ⁡ ( i z ) {\\displaystyle {\\begin{aligned}\\sin(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}z^{2n+1}\\\\&={\\frac {e^{iz}-e^{-iz}}{2i}}\\\\&={\\frac {\\sinh \\left(iz\\right)}{i}}\\\\&=-i\\sinh \\left(iz\\right)\\\\\\cos(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}z^{2n}\\\\&={\\frac {e^{iz}+e^{-iz}}{2}}\\\\&=\\cosh(iz)\\\\\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}z^{2n+1}\\\\&={\\frac {e^{iz}-e^{-iz}}{2i}}\\\\&={\\frac {\\sinh \\left(iz\\right)}{i}}\\\\&=-i\\sinh \\left(iz\\right)\\\\\\cos(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}z^{2n}\\\\&={\\frac {e^{iz}+e^{-iz}}{2}}\\\\&=\\cosh(iz)\\\\\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/77ff8035628f5a90a7aced4bb8fb5b4a2b0c3a52) where sinh and cosh are the [hyperbolic sine and cosine](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function"). These are [entire functions](https://en.wikipedia.org/wiki/Entire_function "Entire function"). It is also sometimes useful to express the complex sine and cosine functions in terms of the real and imaginary parts of its argument: sin ⁡ ( x \+ i y ) \= sin ⁡ ( x ) cos ⁡ ( i y ) \+ cos ⁡ ( x ) sin ⁡ ( i y ) \= sin ⁡ ( x ) cosh ⁡ ( y ) \+ i cos ⁡ ( x ) sinh ⁡ ( y ) cos ⁡ ( x \+ i y ) \= cos ⁡ ( x ) cos ⁡ ( i y ) − sin ⁡ ( x ) sin ⁡ ( i y ) \= cos ⁡ ( x ) cosh ⁡ ( y ) − i sin ⁡ ( x ) sinh ⁡ ( y ) {\\displaystyle {\\begin{aligned}\\sin(x+iy)&=\\sin(x)\\cos(iy)+\\cos(x)\\sin(iy)\\\\&=\\sin(x)\\cosh(y)+i\\cos(x)\\sinh(y)\\\\\\cos(x+iy)&=\\cos(x)\\cos(iy)-\\sin(x)\\sin(iy)\\\\&=\\cos(x)\\cosh(y)-i\\sin(x)\\sinh(y)\\\\\\end{aligned}}} ![{\\displaystyle {\\begin{aligned}\\sin(x+iy)&=\\sin(x)\\cos(iy)+\\cos(x)\\sin(iy)\\\\&=\\sin(x)\\cosh(y)+i\\cos(x)\\sinh(y)\\\\\\cos(x+iy)&=\\cos(x)\\cos(iy)-\\sin(x)\\sin(iy)\\\\&=\\cos(x)\\cosh(y)-i\\sin(x)\\sinh(y)\\\\\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/22162f3c99776ef5203c9c7fc8d418162bdcfd99) #### Partial fraction and product expansions of complex sine \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=18 "Edit section: Partial fraction and product expansions of complex sine")\] Using the partial fraction expansion technique in [complex analysis](https://en.wikipedia.org/wiki/Complex_analysis "Complex analysis"), one can find that the infinite series ∑ n \= − ∞ ∞ ( − 1 ) n z − n \= 1 z − 2 z ∑ n \= 1 ∞ ( − 1 ) n n 2 − z 2 {\\displaystyle \\sum \_{n=-\\infty }^{\\infty }{\\frac {(-1)^{n}}{z-n}}={\\frac {1}{z}}-2z\\sum \_{n=1}^{\\infty }{\\frac {(-1)^{n}}{n^{2}-z^{2}}}} ![{\\displaystyle \\sum \_{n=-\\infty }^{\\infty }{\\frac {(-1)^{n}}{z-n}}={\\frac {1}{z}}-2z\\sum \_{n=1}^{\\infty }{\\frac {(-1)^{n}}{n^{2}-z^{2}}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/767d43fdad5d7a47e46f1433d20d909d91af8883) both converge and are equal to π sin ⁡ ( π z ) {\\textstyle {\\frac {\\pi }{\\sin(\\pi z)}}} ![{\\textstyle {\\frac {\\pi }{\\sin(\\pi z)}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/02adeb7acbfc515905a0c72f7130ae5d2589df72). Similarly, one can show that π 2 sin 2 ⁡ ( π z ) \= ∑ n \= − ∞ ∞ 1 ( z − n ) 2 . {\\displaystyle {\\frac {\\pi ^{2}}{\\sin ^{2}(\\pi z)}}=\\sum \_{n=-\\infty }^{\\infty }{\\frac {1}{(z-n)^{2}}}.} ![{\\displaystyle {\\frac {\\pi ^{2}}{\\sin ^{2}(\\pi z)}}=\\sum \_{n=-\\infty }^{\\infty }{\\frac {1}{(z-n)^{2}}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/76b4bc619e6aa45ebdcdb9e88551598f69931529) Using product expansion technique, one can derive sin ⁡ ( π z ) \= π z ∏ n \= 1 ∞ ( 1 − z 2 n 2 ) . {\\displaystyle \\sin(\\pi z)=\\pi z\\prod \_{n=1}^{\\infty }\\left(1-{\\frac {z^{2}}{n^{2}}}\\right).} ![{\\displaystyle \\sin(\\pi z)=\\pi z\\prod \_{n=1}^{\\infty }\\left(1-{\\frac {z^{2}}{n^{2}}}\\right).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/17ce4c82316483de357bac1133ac3d7af0092707) #### Usage of complex sine \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=19 "Edit section: Usage of complex sine")\] sin(*z*) is found in the [functional equation](https://en.wikipedia.org/wiki/Functional_equation "Functional equation") for the [Gamma function](https://en.wikipedia.org/wiki/Gamma_function "Gamma function"), Γ ( s ) Γ ( 1 − s ) \= π sin ⁡ ( π s ) , {\\displaystyle \\Gamma (s)\\Gamma (1-s)={\\pi \\over \\sin(\\pi s)},} ![{\\displaystyle \\Gamma (s)\\Gamma (1-s)={\\pi \\over \\sin(\\pi s)},}](https://wikimedia.org/api/rest_v1/media/math/render/svg/07f53255b83f8d3db49cf23173da760f7048b689) which in turn is found in the [functional equation](https://en.wikipedia.org/wiki/Functional_equation "Functional equation") for the [Riemann zeta-function](https://en.wikipedia.org/wiki/Riemann_zeta-function "Riemann zeta-function"), ζ ( s ) \= 2 ( 2 π ) s − 1 Γ ( 1 − s ) sin ⁡ ( π 2 s ) ζ ( 1 − s ) . {\\displaystyle \\zeta (s)=2(2\\pi )^{s-1}\\Gamma (1-s)\\sin \\left({\\frac {\\pi }{2}}s\\right)\\zeta (1-s).} ![{\\displaystyle \\zeta (s)=2(2\\pi )^{s-1}\\Gamma (1-s)\\sin \\left({\\frac {\\pi }{2}}s\\right)\\zeta (1-s).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f170929c08858f62da589f8fccb2565c43c769a8) As a [holomorphic function](https://en.wikipedia.org/wiki/Holomorphic_function "Holomorphic function"), sin *z* is a 2D solution of [Laplace's equation](https://en.wikipedia.org/wiki/Laplace%27s_equation "Laplace's equation"): Δ u ( x 1 , x 2 ) \= 0\. {\\displaystyle \\Delta u(x\_{1},x\_{2})=0.} ![{\\displaystyle \\Delta u(x\_{1},x\_{2})=0.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/cdaaf4948b285dfd3deb916716fc5daa6d9d3d22) The complex sine function is also related to the level curves of [pendulums](https://en.wikipedia.org/wiki/Pendulums "Pendulums").\[*[how?](https://en.wikipedia.org/wiki/Wikipedia:Please_clarify "Wikipedia:Please clarify")*\][\[39\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-40)\[*[better source needed](https://en.wikipedia.org/wiki/Wikipedia:Verifiability#Questionable_sources "Wikipedia:Verifiability")*\] ### Complex graphs \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=20 "Edit section: Complex graphs")\] | | | | |---|---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f4/Complex_sin_real_01_Pengo.svg/250px-Complex_sin_real_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_real_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Complex_sin_imag_01_Pengo.svg/250px-Complex_sin_imag_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_imag_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/9/9e/Complex_sin_abs_01_Pengo.svg/250px-Complex_sin_abs_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_abs_01_Pengo.svg) | | Real component | Imaginary component | Magnitude | | | | | |---|---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b3/Complex_arcsin_real_01_Pengo.svg/250px-Complex_arcsin_real_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_real_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f1/Complex_arcsin_imag_01_Pengo.svg/250px-Complex_arcsin_imag_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_imag_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/1/1f/Complex_arcsin_abs_01_Pengo.svg/250px-Complex_arcsin_abs_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_abs_01_Pengo.svg) | | Real component | Imaginary component | Magnitude | ## Background \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=21 "Edit section: Background")\] ### Etymology \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=22 "Edit section: Etymology")\] Main article: [History of trigonometry § Etymology](https://en.wikipedia.org/wiki/History_of_trigonometry#Etymology "History of trigonometry") The word *sine* is derived, indirectly, from the [Sanskrit](https://en.wikipedia.org/wiki/Sanskrit "Sanskrit") word *jyā* 'bow-string' or more specifically its synonym *jīvá* (both adopted from [Ancient Greek](https://en.wikipedia.org/wiki/Ancient_Greek_language "Ancient Greek language") χορδή 'string; chord'), due to visual similarity between the arc of a circle with its corresponding chord and a bow with its string (see [jyā, koti-jyā and utkrama-jyā](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā"); *sine* and *chord* are closely related in a circle of unit diameter, see [Ptolemy's Theorem](https://en.wikipedia.org/wiki/Ptolemy%27s_theorem#Corollaries "Ptolemy's theorem")). This was [transliterated](https://en.wikipedia.org/wiki/Transliteration "Transliteration") in [Arabic](https://en.wikipedia.org/wiki/Arabic_language "Arabic language") as *jība*, which is meaningless in that language and written as *jb* (جب). Since Arabic is written without short vowels, *jb* was interpreted as the [homograph](https://en.wikipedia.org/wiki/Homograph "Homograph") *jayb* ([جيب](https://en.wiktionary.org/wiki/%D8%AC%D9%8A%D8%A8 "wikt:جيب")), which means 'bosom', 'pocket', or 'fold'.[\[40\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEPlofker2009[httpsbooksgooglecombooksidDHvThPNp9yMCpgPA257_257]-41)[\[41\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMaor1998[httpsbooksgooglecombooksidr9aMrneWFpUCpgPA35_35]-42) When the Arabic texts of [Al-Battani](https://en.wikipedia.org/wiki/Al-Battani "Al-Battani") and [al-Khwārizmī](https://en.wikipedia.org/wiki/Mu%E1%B8%A5ammad_ibn_M%C5%ABs%C4%81_al-Khw%C4%81rizm%C4%AB "Muḥammad ibn Mūsā al-Khwārizmī") were translated into [Medieval Latin](https://en.wikipedia.org/wiki/Medieval_Latin "Medieval Latin") in the 12th century by [Gerard of Cremona](https://en.wikipedia.org/wiki/Gerard_of_Cremona "Gerard of Cremona"), he used the Latin equivalent [*sinus*](https://en.wiktionary.org/wiki/sinus "wikt:sinus") (which also means 'bay' or 'fold', and more specifically 'the hanging fold of a [toga](https://en.wikipedia.org/wiki/Toga "Toga") over the breast').[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43)[\[43\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMaor199835&ndash;36-44)[\[44\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEKatz2008253-45) Gerard was probably not the first scholar to use this translation; Robert of Chester appears to have preceded him and there is evidence of even earlier usage.[\[45\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTESmith1958202-46)[\[46\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-47) The English form *sine* was introduced in [Thomas Fale](https://en.wikipedia.org/wiki/Thomas_Fale "Thomas Fale")'s 1593 *Horologiographia*.[\[47\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-48) The word *cosine* derives from an abbreviation of the Latin *complementi sinus* 'sine of the [complementary angle](https://en.wikipedia.org/wiki/Complementary_angle "Complementary angle")' as *cosinus* in [Edmund Gunter](https://en.wikipedia.org/wiki/Edmund_Gunter "Edmund Gunter")'s *Canon triangulorum* (1620), which also includes a similar definition of *cotangens*.[\[48\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEGunter1620-49) ### History \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=23 "Edit section: History")\] Main article: [History of trigonometry](https://en.wikipedia.org/wiki/History_of_trigonometry "History of trigonometry") [![](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg/250px-Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg)](https://en.wikipedia.org/wiki/File:Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg) Quadrant from 1840s [Ottoman Turkey](https://en.wikipedia.org/wiki/Ottoman_Empire "Ottoman Empire") with axes for looking up the sine and [versine](https://en.wikipedia.org/wiki/Versine "Versine") of angles While the early study of trigonometry can be traced to antiquity, the [trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") as they are in use today were developed in the medieval period. The [chord](https://en.wikipedia.org/wiki/Chord_\(geometry\) "Chord (geometry)") function was discovered by [Hipparchus](https://en.wikipedia.org/wiki/Hipparchus "Hipparchus") of [Nicaea](https://en.wikipedia.org/wiki/%C4%B0znik "İznik") (180–125 BCE) and [Ptolemy](https://en.wikipedia.org/wiki/Ptolemy "Ptolemy") of [Roman Egypt](https://en.wikipedia.org/wiki/Egypt_\(Roman_province\) "Egypt (Roman province)") (90–165 CE).[\[49\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-50) The sine and cosine functions are closely related to the [*jyā* and *koṭi-jyā*](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā") functions used in [Indian astronomy](https://en.wikipedia.org/wiki/Indian_astronomy "Indian astronomy") during the [Gupta period](https://en.wikipedia.org/wiki/Gupta_period "Gupta period") (*[Aryabhatiya](https://en.wikipedia.org/wiki/Aryabhatiya "Aryabhatiya")* and *[Surya Siddhanta](https://en.wikipedia.org/wiki/Surya_Siddhanta "Surya Siddhanta")*), via translation from Sanskrit to Arabic and then from Arabic to Latin.[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43)[\[50\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-51) All six trigonometric functions in current use were known in [Islamic mathematics](https://en.wikipedia.org/wiki/Islamic_mathematics "Islamic mathematics") by the 9th century, as was the [law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines"), used in [solving triangles](https://en.wikipedia.org/wiki/Solving_triangles "Solving triangles").[\[51\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Gingerich_1986-52) [Al-Khwārizmī](https://en.wikipedia.org/wiki/Al-Khw%C4%81rizm%C4%AB "Al-Khwārizmī") (c. 780–850) produced tables of sines, cosines and tangents.[\[52\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Sesiano-53)[\[53\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Britannica-54) [Muhammad ibn Jābir al-Harrānī al-Battānī](https://en.wikipedia.org/wiki/Muhammad_ibn_J%C4%81bir_al-Harr%C4%81n%C4%AB_al-Batt%C4%81n%C4%AB "Muhammad ibn Jābir al-Harrānī al-Battānī") (853–929) discovered the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.[\[53\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Britannica-54) In the early 17th-century, the French mathematician [Albert Girard](https://en.wikipedia.org/wiki/Albert_Girard "Albert Girard") published the first use of the abbreviations *sin*, *cos*, and *tan*; these were further promulgated by Euler (see below). The *Opus palatinum de triangulis* of [Georg Joachim Rheticus](https://en.wikipedia.org/wiki/Georg_Joachim_Rheticus "Georg Joachim Rheticus"), a student of [Copernicus](https://en.wikipedia.org/wiki/Copernicus "Copernicus"), was probably the first in Europe to define trigonometric functions directly in terms of right triangles instead of circles, with tables for all six trigonometric functions; this work was finished by Rheticus' student Valentin Otho in 1596. In a paper published in 1682, [Leibniz](https://en.wikipedia.org/wiki/Gottfried_Leibniz "Gottfried Leibniz") proved that sin *x* is not an [algebraic function](https://en.wikipedia.org/wiki/Algebraic_function "Algebraic function") of *x*.[\[54\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-55) [Roger Cotes](https://en.wikipedia.org/wiki/Roger_Cotes "Roger Cotes") computed the derivative of sine in his *Harmonia Mensurarum* (1722).[\[55\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-56) [Leonhard Euler](https://en.wikipedia.org/wiki/Leonhard_Euler "Leonhard Euler")'s *Introductio in analysin infinitorum* (1748) was mostly responsible for establishing the analytic treatment of trigonometric functions in Europe, also defining them as infinite series and presenting "[Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula")", as well as the near-modern abbreviations *sin.*, *cos.*, *tang.*, *cot.*, *sec.*, and *cosec.*[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43) ## Software implementations \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=24 "Edit section: Software implementations")\] | | | |---|---| | [![icon](https://upload.wikimedia.org/wikipedia/en/thumb/9/99/Question_book-new.svg/60px-Question_book-new.svg.png)](https://en.wikipedia.org/wiki/File:Question_book-new.svg) | This section **needs additional citations for [verification](https://en.wikipedia.org/wiki/Wikipedia:Verifiability "Wikipedia:Verifiability")**. Please help [improve this article](https://en.wikipedia.org/wiki/Special:EditPage/Sine_and_cosine "Special:EditPage/Sine and cosine") by [adding citations to reliable sources](https://en.wikipedia.org/wiki/Help:Referencing_for_beginners "Help:Referencing for beginners") in this section. Unsourced material may be challenged and removed. *(August 2024)* *([Learn how and when to remove this message](https://en.wikipedia.org/wiki/Help:Maintenance_template_removal "Help:Maintenance template removal"))* | See also: [Lookup table § Computing sines](https://en.wikipedia.org/wiki/Lookup_table#Computing_sines "Lookup table") There is no standard algorithm for calculating sine and cosine. [IEEE 754](https://en.wikipedia.org/wiki/IEEE_754 "IEEE 754"), the most widely used standard for the specification of reliable floating-point computation, does not address calculating trigonometric functions such as sine. The reason is that no efficient algorithm is known for computing sine and cosine with a specified accuracy, especially for large inputs.[\[56\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZimmermann2006-57) Algorithms for calculating sine may be balanced for such constraints as speed, accuracy, portability, or range of input values accepted. This can lead to different results for different algorithms, especially for special circumstances such as very large inputs, e.g. `sin(1022)`. A common programming optimization, used especially in 3D graphics, is to pre-calculate a table of sine values, for example one value per degree, then for values in-between pick the closest pre-calculated value, or [linearly interpolate](https://en.wikipedia.org/wiki/Linear_interpolation "Linear interpolation") between the 2 closest values to approximate it. This allows results to be looked up from a table rather than being calculated in real time. With modern CPU architectures this method may offer no advantage.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] The [CORDIC](https://en.wikipedia.org/wiki/CORDIC "CORDIC") algorithm is commonly used in scientific calculators. The sine and cosine functions, along with other trigonometric functions, are widely available across programming languages and platforms. In computing, they are typically abbreviated to `sin` and `cos`. Some CPU architectures have a built-in instruction for sine, including the Intel [x87](https://en.wikipedia.org/wiki/X87 "X87") FPUs since the 80387. In programming languages, `sin` and `cos` are typically either a built-in function or found within the language's standard math library. For example, the [C standard library](https://en.wikipedia.org/wiki/C_standard_library "C standard library") defines sine functions within [math.h](https://en.wikipedia.org/wiki/C_mathematical_functions "C mathematical functions"): `sin(double)`, `sinf(float)`, and `sinl(long double)`. The parameter of each is a [floating point](https://en.wikipedia.org/wiki/Floating_point "Floating point") value, specifying the angle in radians. Each function returns the same [data type](https://en.wikipedia.org/wiki/Data_type "Data type") as it accepts. Many other trigonometric functions are also defined in [math.h](https://en.wikipedia.org/wiki/C_mathematical_functions "C mathematical functions"), such as for cosine, arc sine, and hyperbolic sine (sinh). Similarly, [Python](https://en.wikipedia.org/wiki/Python_\(programming_language\) "Python (programming language)") defines `math.sin(x)` and `math.cos(x)` within the built-in `math` module. Complex sine and cosine functions are also available within the `cmath` module, e.g. `cmath.sin(z)`. [CPython](https://en.wikipedia.org/wiki/CPython "CPython")'s math functions call the [C](https://en.wikipedia.org/wiki/C_\(programming_language\) "C (programming language)") `math` library, and use a [double-precision floating-point format](https://en.wikipedia.org/wiki/Double-precision_floating-point_format "Double-precision floating-point format"). ### Turns based implementations \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=25 "Edit section: Turns based implementations")\] "sinpi" redirects here. For the township in Pingtung County, Taiwan, see [Xinpi](https://en.wikipedia.org/wiki/Xinpi "Xinpi"). "cospi" redirects here. For the 17th-century Bolognese nobleman, see [Ferdinando Cospi](https://en.wikipedia.org/wiki/Ferdinando_Cospi "Ferdinando Cospi"). Some software libraries provide implementations of sine and cosine using the input angle in half-[turns](https://en.wikipedia.org/wiki/Turn_\(angle\) "Turn (angle)"), a half-turn being an angle of 180 degrees or π {\\displaystyle \\pi } ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a) radians. Representing angles in turns or half-turns has accuracy advantages and efficiency advantages in some cases.[\[57\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-matlab-58)[\[58\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-r-59) These functions are called `sinpi` and `cospi` in MATLAB,[\[57\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-matlab-58) [OpenCL](https://en.wikipedia.org/wiki/OpenCL "OpenCL"),[\[59\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-60) R,[\[58\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-r-59) Julia,[\[60\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-61) [CUDA](https://en.wikipedia.org/wiki/CUDA "CUDA"),[\[61\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-62) and ARM.[\[62\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-63) For example, `sinpi(x)` would evaluate to sin ⁡ ( π x ) , {\\displaystyle \\sin(\\pi x),} ![{\\displaystyle \\sin(\\pi x),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f4f4681ee034a3d894ce28068c5f6bacfa86e8c5) where *x* is expressed in half-turns, and consequently the final input to the function, *πx* can be interpreted in radians by sin. [SciPy](https://en.wikipedia.org/wiki/SciPy "SciPy") provides similar functions `sindg` and `cosdg` with input in degrees.[\[63\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-64) The accuracy advantage stems from the ability to perfectly represent key angles like full-turn, half-turn, and quarter-turn losslessly in binary floating-point or fixed-point. In contrast, representing 2 π {\\displaystyle 2\\pi } ![{\\displaystyle 2\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/73efd1f6493490b058097060a572606d2c550a06), π {\\displaystyle \\pi } ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a), and π 2 {\\textstyle {\\frac {\\pi }{2}}} ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae) in binary floating-point or binary scaled fixed-point always involves a loss of accuracy since irrational numbers cannot be represented with finitely many binary digits. Turns also have an accuracy advantage and efficiency advantage for computing modulo to one period. Computing modulo 1 turn or modulo 2 half-turns can be losslessly and efficiently computed in both floating-point and fixed-point. For example, computing modulo 1 or modulo 2 for a binary point scaled fixed-point value requires only a bit shift or bitwise AND operation. In contrast, computing modulo π 2 {\\textstyle {\\frac {\\pi }{2}}} ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae) involves inaccuracies in representing π 2 {\\textstyle {\\frac {\\pi }{2}}} ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae). For applications involving angle sensors, the sensor typically provides angle measurements in a form directly compatible with turns or half-turns. For example, an angle sensor may count from 0 to 4096 over one complete revolution.[\[64\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-65) If half-turns are used as the unit for angle, then the value provided by the sensor directly and losslessly maps to a fixed-point data type with 11 bits to the right of the binary point. In contrast, if radians are used as the unit for storing the angle, then the inaccuracies and cost of multiplying the raw sensor integer by an approximation to π 2048 {\\textstyle {\\frac {\\pi }{2048}}} ![{\\textstyle {\\frac {\\pi }{2048}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/af6a95707656082f4af5a498fb84cd8a03827286) would be incurred. ## See also \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=26 "Edit section: See also")\] - [Āryabhaṭa's sine table](https://en.wikipedia.org/wiki/%C4%80ryabha%E1%B9%ADa%27s_sine_table "Āryabhaṭa's sine table") - [Bhaskara I's sine approximation formula](https://en.wikipedia.org/wiki/Bhaskara_I%27s_sine_approximation_formula "Bhaskara I's sine approximation formula") - [Discrete sine transform](https://en.wikipedia.org/wiki/Discrete_sine_transform "Discrete sine transform") - [Dixon elliptic functions](https://en.wikipedia.org/wiki/Dixon_elliptic_functions "Dixon elliptic functions") - [Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula") - [Generalized trigonometry](https://en.wikipedia.org/wiki/Generalized_trigonometry "Generalized trigonometry") - [Hyperbolic function](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function") - [Lemniscate elliptic functions](https://en.wikipedia.org/wiki/Lemniscate_elliptic_functions "Lemniscate elliptic functions") - [Law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines") - [List of periodic functions](https://en.wikipedia.org/wiki/List_of_periodic_functions "List of periodic functions") - [List of trigonometric identities](https://en.wikipedia.org/wiki/List_of_trigonometric_identities "List of trigonometric identities") - [Madhava series](https://en.wikipedia.org/wiki/Madhava_series "Madhava series") - [Madhava's sine table](https://en.wikipedia.org/wiki/Madhava%27s_sine_table "Madhava's sine table") - [Optical sine theorem](https://en.wikipedia.org/wiki/Optical_sine_theorem "Optical sine theorem") - [Polar sine](https://en.wikipedia.org/wiki/Polar_sine "Polar sine")—a generalization to vertex angles - [Proofs of trigonometric identities](https://en.wikipedia.org/wiki/Proofs_of_trigonometric_identities "Proofs of trigonometric identities") - [Sinc function](https://en.wikipedia.org/wiki/Sinc_function "Sinc function") - [Sine and cosine transforms](https://en.wikipedia.org/wiki/Sine_and_cosine_transforms "Sine and cosine transforms") - [Sine integral](https://en.wikipedia.org/wiki/Sine_integral "Sine integral") - [Sine quadrant](https://en.wikipedia.org/wiki/Sine_quadrant "Sine quadrant") - [Sine wave](https://en.wikipedia.org/wiki/Sine_wave "Sine wave") - [Sine–Gordon equation](https://en.wikipedia.org/wiki/Sine%E2%80%93Gordon_equation "Sine–Gordon equation") - [Sinusoidal model](https://en.wikipedia.org/wiki/Sinusoidal_model "Sinusoidal model") - [SOH-CAH-TOA](https://en.wikipedia.org/wiki/Mnemonics_in_trigonometry#SOH-CAH-TOA "Mnemonics in trigonometry") - [Trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") - [Trigonometric integral](https://en.wikipedia.org/wiki/Trigonometric_integral "Trigonometric integral") ## References \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=27 "Edit section: References")\] ### Footnotes \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=28 "Edit section: Footnotes")\] 1. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-27)** Here, sin 2 ⁡ ( x ) {\\displaystyle \\sin ^{2}(x)} ![{\\displaystyle \\sin ^{2}(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/53a0a5d7313c2ee4d060de4479eb4d418ce73310) means the squared sine function sin ⁡ ( x ) ⋅ sin ⁡ ( x ) {\\displaystyle \\sin(x)\\cdot \\sin(x)} ![{\\displaystyle \\sin(x)\\cdot \\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c6abd8bbecb1c69b243659fadd4125845de237b5) . ### Citations \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=29 "Edit section: Citations")\] 1. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-2) [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [27](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA27). 2. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA36_36]_2-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [36](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA36). 3. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742_3-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742_3-1) [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 42. 4. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA37_37],_[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA78_78]_4-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [37](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA37), [78](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA78). 5. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]_5-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]_5-1) [Axler (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAxler2012), p. [634](https://books.google.com/books?id=B5RxDwAAQBAJ&pg=PA634). 6. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA632_632]_6-0)** [Axler (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAxler2012), p. [632](https://books.google.com/books?id=B5RxDwAAQBAJ&pg=PA632). 7. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-7)** [Weisstein, Eric W.](https://en.wikipedia.org/wiki/Eric_W._Weisstein "Eric W. Weisstein") ["Cross Product"](https://mathworld.wolfram.com/CrossProduct.html). *[MathWorld](https://en.wikipedia.org/wiki/MathWorld "MathWorld")*. Retrieved 5 June 2025. 8. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-8)** [Weisstein, Eric W.](https://en.wikipedia.org/wiki/Eric_W._Weisstein "Eric W. Weisstein") ["Dot Product"](https://mathworld.wolfram.com/DotProduct.html). *[MathWorld](https://en.wikipedia.org/wiki/MathWorld "MathWorld")*. Retrieved 5 June 2025. 9. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741_9-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41. 10. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA68_68]_10-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [68](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA68). 11. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200747_11-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 47. 12. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741&ndash;42_12-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41–42. 13. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741,_43_13-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41, 43. 14. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2012[httpsbooksgooglecombooksidOMrcN0a3LxICpgRA1-PA165_165]_14-0)** [Young (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2012), p. [165](https://books.google.com/books?id=OMrcN0a3LxIC&pg=RA1-PA165). 15. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742,_47_15-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 42, 47. 16. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-16)** ["OEIS A003957"](https://oeis.org/A003957). *oeis.org*. Retrieved 2019-05-26. 17. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]_17-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]_17-1) [Bourchtein & Bourchtein (2022)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFBourchteinBourchtein2022), p. [294](https://books.google.com/books?id=nGxOEAAAQBAJ&pg=PA294). 18. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007115_18-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 115. 19. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007155_19-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 155. 20. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007157_20-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 157. 21. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007199_21-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 199. 22. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVince2023[httpsbooksgooglecombooksidGnW6EAAAQBAJpgPA162_162]_22-0)** [Vince (2023)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVince2023), p. [162](https://books.google.com/books?id=GnW6EAAAQBAJ&pg=PA162). 23. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAdlaj2012_23-0)** [Adlaj (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAdlaj2012). 24. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-24)** OEIS [sequence A105419 (Decimal expansion of the arc length of the sine or cosine curve for one full period.)](https://oeis.org/A105419) 25. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007365_25-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 365. 26. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA99_99]_26-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [99](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA99). 27. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-28)** Dennis G. Zill (2013). *Precalculus with Calculus Previews*. Jones & Bartlett Publishers. p. 238. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4496-4515-1](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4496-4515-1 "Special:BookSources/978-1-4496-4515-1") . [Extract of page 238](https://books.google.com/books?id=dtS5M4lx7scC&pg=PA238) 28. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-29)** ["Sine-squared function"](https://calculus.subwiki.org/wiki/Sine-squared_function#Identities). Retrieved August 9, 2019. 29. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492_30-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492_30-1) [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 491–492. 30. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]_31-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]_31-1) [Abramowitz & Stegun (1970)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAbramowitzStegun1970), p. [74](https://books.google.com/books?id=MtU8uP7XMvoC&pg=PA74). 31. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEPowell1981150_32-0)** [Powell (1981)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFPowell1981), p. 150. 32. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTERudin198788_33-0)** [Rudin (1987)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFRudin1987), p. 88. 33. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEZygmund19681_34-0)** [Zygmund (1968)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFZygmund1968), p. 1. 34. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEZygmund196811_35-0)** [Zygmund (1968)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFZygmund1968), p. 11. 35. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-2) [Howie (2003)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFHowie2003), p. [24](https://books.google.com/books?id=0FZDBAAAQBAJ&pg=PA24). 36. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTERudin19872_37-0)** [Rudin (1987)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFRudin1987), p. 2. 37. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-38)** Brown, James Ward; [Churchill, Ruel](https://en.wikipedia.org/wiki/Ruel_Vance_Churchill "Ruel Vance Churchill") (2014). *Complex Variables and Applications* (9th ed.). [McGraw-Hill](https://en.wikipedia.org/wiki/McGraw-Hill "McGraw-Hill"). p. 105. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-07-338317-0](https://en.wikipedia.org/wiki/Special:BookSources/978-0-07-338317-0 "Special:BookSources/978-0-07-338317-0") . 38. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_23&ndash;24]_39-0)** [Howie (2003)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFHowie2003), p. [23–24](https://books.google.com/books?id=0FZDBAAAQBAJ&pg=PA24). 39. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-40)** ["Why are the phase portrait of the simple plane pendulum and a domain coloring of sin(z) so similar?"](https://math.stackexchange.com/q/220418). *math.stackexchange.com*. Retrieved 2019-08-12. 40. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEPlofker2009[httpsbooksgooglecombooksidDHvThPNp9yMCpgPA257_257]_41-0)** [Plofker (2009)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFPlofker2009), p. [257](https://books.google.com/books?id=DHvThPNp9yMC&pg=PA257). 41. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMaor1998[httpsbooksgooglecombooksidr9aMrneWFpUCpgPA35_35]_42-0)** [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), p. [35](https://books.google.com/books?id=r9aMrneWFpUC&pg=PA35). 42. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-2) [Merzbach & Boyer (2011)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMerzbachBoyer2011). 43. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMaor199835&ndash;36_44-0)** [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), p. 35–36. 44. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEKatz2008253_45-0)** [Katz (2008)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFKatz2008), p. 253. 45. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTESmith1958202_46-0)** [Smith (1958)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFSmith1958), p. 202. 46. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-47)** Various sources credit the first use of *sinus* to either - [Plato Tiburtinus](https://en.wikipedia.org/wiki/Plato_Tiburtinus "Plato Tiburtinus")'s 1116 translation of the *Astronomy* of [Al-Battani](https://en.wikipedia.org/wiki/Al-Battani "Al-Battani") - [Gerard of Cremona](https://en.wikipedia.org/wiki/Gerard_of_Cremona "Gerard of Cremona")'s translation of the *Algebra* of [al-Khwārizmī](https://en.wikipedia.org/wiki/Mu%E1%B8%A5ammad_ibn_M%C5%ABs%C4%81_al-Khw%C4%81rizm%C4%AB "Muḥammad ibn Mūsā al-Khwārizmī") - [Robert of Chester](https://en.wikipedia.org/wiki/Robert_of_Chester "Robert of Chester")'s 1145 translation of the tables of al-Khwārizmī See [Merlet (2004)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMerlet2004). See [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), Chapter 3, for an earlier etymology crediting Gerard. See [Katz (2008)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFKatz2008), p. 210. 47. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-48)** Fale's book alternately uses the spellings "sine", "signe", or "sign". Fale, Thomas (1593). [*Horologiographia. The Art of Dialling: Teaching, an Easie and Perfect Way to make all Kindes of Dials ...*](https://archive.org/details/b30333106/page/19/mode/1up) London: F. Kingston. p. 11, for example. 48. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEGunter1620_49-0)** [Gunter (1620)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFGunter1620). 49. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-50)** Brendan, T. (February 1965). "How Ptolemy constructed trigonometry tables". *The Mathematics Teacher*. **58** (2): 141–149\. [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.5951/MT.58.2.0141](https://doi.org/10.5951%2FMT.58.2.0141). [JSTOR](https://en.wikipedia.org/wiki/JSTOR_\(identifier\) "JSTOR (identifier)") [27967990](https://www.jstor.org/stable/27967990). 50. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-51)** [Van Brummelen, Glen](https://en.wikipedia.org/wiki/Glen_Van_Brummelen "Glen Van Brummelen") (2009). "India". *The Mathematics of the Heavens and the Earth*. Princeton University Press. Ch. 3, pp. 94–134. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-691-12973-0](https://en.wikipedia.org/wiki/Special:BookSources/978-0-691-12973-0 "Special:BookSources/978-0-691-12973-0") . 51. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Gingerich_1986_52-0)** Gingerich, Owen (1986). ["Islamic Astronomy"](https://web.archive.org/web/20131019140821/http://faculty.kfupm.edu.sa/PHYS/alshukri/PHYS215/Islamic_astronomy.htm). *[Scientific American](https://en.wikipedia.org/wiki/Scientific_American "Scientific American")*. Vol. 254. p. 74. Archived from [the original](http://faculty.kfupm.edu.sa/PHYS/alshukri/PHYS215/Islamic_astronomy.htm) on 2013-10-19. Retrieved 2010-07-13. 52. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Sesiano_53-0)** Jacques Sesiano, "Islamic mathematics", p. 157, in [Selin, Helaine](https://en.wikipedia.org/wiki/Helaine_Selin "Helaine Selin"); [D'Ambrosio, Ubiratan](https://en.wikipedia.org/wiki/Ubiratan_D%27Ambrosio "Ubiratan D'Ambrosio"), eds. (2000). *Mathematics Across Cultures: The History of Non-western Mathematics*. [Springer Science+Business Media](https://en.wikipedia.org/wiki/Springer_Science%2BBusiness_Media "Springer Science+Business Media"). [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4020-0260-1](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4020-0260-1 "Special:BookSources/978-1-4020-0260-1") . 53. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Britannica_54-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Britannica_54-1) ["trigonometry"](http://www.britannica.com/EBchecked/topic/605281/trigonometry). Encyclopedia Britannica. 17 June 2024. 54. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-55)** Nicolás Bourbaki (1994). [*Elements of the History of Mathematics*](https://archive.org/details/elementsofhistor0000bour). Springer. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [9783540647676](https://en.wikipedia.org/wiki/Special:BookSources/9783540647676 "Special:BookSources/9783540647676") . 55. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-56)** "[Why the sine has a simple derivative](http://www.math.usma.edu/people/rickey/hm/CalcNotes/Sine-Deriv.pdf) [Archived](https://web.archive.org/web/20110720102700/http://www.math.usma.edu/people/rickey/hm/CalcNotes/Sine-Deriv.pdf) 2011-07-20 at the [Wayback Machine](https://en.wikipedia.org/wiki/Wayback_Machine "Wayback Machine")", in *[Historical Notes for Calculus Teachers](http://www.math.usma.edu/people/rickey/hm/CalcNotes/default.htm) [Archived](https://web.archive.org/web/20110720102613/http://www.math.usma.edu/people/rickey/hm/CalcNotes/default.htm) 2011-07-20 at the [Wayback Machine](https://en.wikipedia.org/wiki/Wayback_Machine "Wayback Machine")* by [V. 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Retrieved 2026-01-08. 58. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-r_59-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-r_59-1) ["Trig function - RDocumentation"](https://www.rdocumentation.org/packages/base/versions/3.5.3/topics/Trig). *www.rdocumentation.org*. Retrieved 2026-02-17. 59. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-60)** ["sin, sincos, sinh, sinpi"](https://registry.khronos.org/OpenCL/sdk/1.0/docs/man/xhtml/sin.html). *registry.khronos.org*. Retrieved 2026-02-17. 60. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-61)** ["sinpi » Julia Functions"](http://www.jlhub.com/julia/manual/en/function/sinpi). *www.jlhub.com*. Retrieved 2026-02-17. 61. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-62)** ["Double Precision Mathematical Functions"](http://web.archive.org/web/20240723062728/https://docs.nvidia.com/cuda/cuda-math-api/group__CUDA__MATH__DOUBLE.html). *docs.nvidia.com*. Archived from [the original](https://docs.nvidia.com/cuda/cuda-math-api/group__CUDA__MATH__DOUBLE.html) on 2024-07-23. Retrieved 2026-01-08. 62. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-63)** ["Documentation – Arm Developer"](https://developer.arm.com/documentation/100614/latest/b-opencl-built-in-functions/b2-math-functions). *developer.arm.com*. Retrieved 2026-02-17. 63. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-64)** ["Special functions (scipy.special) — SciPy v1.17.0 Manual"](https://docs.scipy.org/doc/scipy/reference/special.html#convenience-functions). *docs.scipy.org*. Retrieved 25 February 2026. 64. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-65)** ["AAS33051: Precision Angle Sensor IC with Incremental and Motor Commutation Outputs and On-Chip Linearization"](http://web.archive.org/web/20190417143715/https://www.allegromicro.com/en/Products/Magnetic-Linear-And-Angular-Position-Sensor-ICs/Angular-Position-Sensor-ICs/AAS33051.aspx). *www.allegromicro.com*. Archived from [the original](https://www.allegromicro.com/en/Products/Magnetic-Linear-And-Angular-Position-Sensor-ICs/Angular-Position-Sensor-ICs/AAS33051.aspx) on 2019-04-17. Retrieved 2026-02-17. ### Works cited \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=30 "Edit section: Works cited")\] - [Abramowitz, Milton](https://en.wikipedia.org/wiki/Milton_Abramowitz "Milton Abramowitz"); [Stegun, Irene A.](https://en.wikipedia.org/wiki/Irene_Stegun "Irene Stegun") (1970), *[Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables](https://en.wikipedia.org/wiki/Abramowitz_and_Stegun "Abramowitz and Stegun")*, New York: [Dover Publications](https://en.wikipedia.org/wiki/Dover_Publications "Dover Publications"), Ninth printing - Adlaj, Semjon (2012), ["An Eloquent Formula for the Perimeter of an Ellipse"](https://www.ams.org/notices/201208/rtx120801094p.pdf) (PDF), *American Mathematical Society*, **59** (8): 1097 - Axler, Sheldon (2012), *Algebra and Trigonometry*, [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0470-58579-5](https://en.wikipedia.org/wiki/Special:BookSources/978-0470-58579-5 "Special:BookSources/978-0470-58579-5") - [Bourchtein, Ludmila](https://en.wikipedia.org/wiki/Ludmila_Bourchtein "Ludmila Bourchtein"); Bourchtein, Andrei (2022), *Theory of Infinite Sequences and Series*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-3-030-79431-6](https://doi.org/10.1007%2F978-3-030-79431-6), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-3-030-79431-6](https://en.wikipedia.org/wiki/Special:BookSources/978-3-030-79431-6 "Special:BookSources/978-3-030-79431-6") - [Gunter, Edmund](https://en.wikipedia.org/wiki/Edmund_Gunter "Edmund Gunter") (1620), *Canon triangulorum* - Howie, John M. (2003), *Complex Analysis*, Springer Undergraduate Mathematics Series, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-1-4471-0027-0](https://doi.org/10.1007%2F978-1-4471-0027-0), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4471-0027-0](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4471-0027-0 "Special:BookSources/978-1-4471-0027-0") - Traupman, Ph.D., John C. (1966), [*The New College Latin & English Dictionary*](https://archive.org/details/boysgirlsbookabo00gard_0), Toronto: Bantam, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [0-553-27619-0](https://en.wikipedia.org/wiki/Special:BookSources/0-553-27619-0 "Special:BookSources/0-553-27619-0") - Katz, Victor J. (2008), [*A History of Mathematics*](http://deti-bilingual.com/wp-content/uploads/2014/06/3rd-Edition-Victor-J.-Katz-A-History-of-Mathematics-Pearson-2008.pdf) (PDF) (3rd ed.), Boston: Addison-Wesley, "The English word "sine" comes from a series of mistranslations of the Sanskrit *jyā-ardha* (chord-half). Āryabhaṭa frequently abbreviated this term to *jyā* or its synonym *jīvá*. When some of the Hindu works were later translated into Arabic, the word was simply transcribed phonetically into an otherwise meaningless Arabic word *jiba*. But since Arabic is written without vowels, later writers interpreted the consonants *jb* as *jaib*, which means bosom or breast. In the twelfth century, when an Arabic trigonometry work was translated into Latin, the translator used the equivalent Latin word *sinus*, which also meant bosom, and by extension, fold (as in a toga over a breast), or a bay or gulf." - Maor, Eli (1998), *Trigonometric Delights*, [Princeton University Press](https://en.wikipedia.org/wiki/Princeton_University_Press "Princeton University Press"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [1-4008-4282-4](https://en.wikipedia.org/wiki/Special:BookSources/1-4008-4282-4 "Special:BookSources/1-4008-4282-4") - Merlet, Jean-Pierre (2004), "A Note on the History of the Trigonometric Functions", in Ceccarelli, Marco (ed.), *International Symposium on History of Machines and Mechanisms*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/1-4020-2204-2](https://doi.org/10.1007%2F1-4020-2204-2), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4020-2203-6](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4020-2203-6 "Special:BookSources/978-1-4020-2203-6") - [Merzbach, Uta C.](https://en.wikipedia.org/wiki/Uta_Merzbach "Uta Merzbach"); [Boyer, Carl B.](https://en.wikipedia.org/wiki/Carl_B._Boyer "Carl B. Boyer") (2011), *A History of Mathematics* (3rd ed.), [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"), "It was Robert of Chester's translation from Arabic that resulted in our word "sine". The Hindus had given the name jiva to the half-chord in trigonometry, and the Arabs had taken this over as jiba. In the Arabic language, there is also the word jaib meaning "bay" or "inlet". When Robert of Chester came to translate the technical word jiba, he seems to have confused this with the word jaib (perhaps because vowels were omitted); hence, he used the word sinus, the Latin word for "bay" or "inlet"." - Plofker (2009), [*Mathematics in India*](https://en.wikipedia.org/wiki/Mathematics_in_India_\(book\) "Mathematics in India (book)"), [Princeton University Press](https://en.wikipedia.org/wiki/Princeton_University_Press "Princeton University Press") - [Powell, Michael J. D.](https://en.wikipedia.org/wiki/Michael_J._D._Powell "Michael J. D. Powell") (1981), *Approximation Theory and Methods*, [Cambridge University Press](https://en.wikipedia.org/wiki/Cambridge_University_Press "Cambridge University Press"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-521-29514-7](https://en.wikipedia.org/wiki/Special:BookSources/978-0-521-29514-7 "Special:BookSources/978-0-521-29514-7") - [Rudin, Walter](https://en.wikipedia.org/wiki/Walter_Rudin "Walter Rudin") (1987), *Real and complex analysis* (3rd ed.), New York: [McGraw-Hill](https://en.wikipedia.org/wiki/McGraw-Hill "McGraw-Hill"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-07-054234-1](https://en.wikipedia.org/wiki/Special:BookSources/978-0-07-054234-1 "Special:BookSources/978-0-07-054234-1") , [MR](https://en.wikipedia.org/wiki/MR_\(identifier\) "MR (identifier)") [0924157](https://mathscinet.ams.org/mathscinet-getitem?mr=0924157) - Smith, D. E. (1958) \[1925\], *History of Mathematics*, vol. I, [Dover Publications](https://en.wikipedia.org/wiki/Dover_Publications "Dover Publications"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [0-486-20429-4](https://en.wikipedia.org/wiki/Special:BookSources/0-486-20429-4 "Special:BookSources/0-486-20429-4") `{{citation}}`: ISBN / Date incompatibility ([help](https://en.wikipedia.org/wiki/Help:CS1_errors#invalid_isbn_date "Help:CS1 errors")) - Varberg, Dale E.; Purcell, Edwin J.; Rigdon, Steven E. (2007), [*Calculus*](https://archive.org/details/matematika-a-purcell-calculus-9th-ed/mode/2up) (9th ed.), [Pearson Prentice Hall](https://en.wikipedia.org/wiki/Pearson_Prentice_Hall "Pearson Prentice Hall"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0131469686](https://en.wikipedia.org/wiki/Special:BookSources/978-0131469686 "Special:BookSources/978-0131469686") - Vince, John (2023), *Calculus for Computer Graphics*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-3-031-28117-4](https://doi.org/10.1007%2F978-3-031-28117-4), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-3-031-28117-4](https://en.wikipedia.org/wiki/Special:BookSources/978-3-031-28117-4 "Special:BookSources/978-3-031-28117-4") - [Young, Cynthia](https://en.wikipedia.org/wiki/Cynthia_Y._Young "Cynthia Y. Young") (2012), *Trigonometry* (3rd ed.), John Wiley & Sons, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-119-32113-2](https://en.wikipedia.org/wiki/Special:BookSources/978-1-119-32113-2 "Special:BookSources/978-1-119-32113-2") - ——— (2017), *Trigonometry* (4th ed.), John Wiley & Sons, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-119-32113-2](https://en.wikipedia.org/wiki/Special:BookSources/978-1-119-32113-2 "Special:BookSources/978-1-119-32113-2") - Zimmermann, Paul (2006), "Can we trust floating-point numbers?", [*Grand Challenges of Informatics*](http://www.jaist.ac.jp/~bjorner/ae-is-budapest/talks/Sept20pm2_Zimmermann.pdf) (PDF), p. 14/31 - [Zygmund, Antoni](https://en.wikipedia.org/wiki/Antoni_Zygmund "Antoni Zygmund") (1968), [*Trigonometric Series*](https://archive.org/details/trigonometricser0012azyg/) (2nd, reprinted ed.), [Cambridge University Press](https://en.wikipedia.org/wiki/Cambridge_University_Press "Cambridge University Press"), [MR](https://en.wikipedia.org/wiki/MR_\(identifier\) "MR (identifier)") [0236587](https://mathscinet.ams.org/mathscinet-getitem?mr=0236587) ## External links \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=31 "Edit section: External links")\] [![Wiktionary logo](https://upload.wikimedia.org/wikipedia/commons/thumb/9/99/Wiktionary-logo-en-v2.svg/40px-Wiktionary-logo-en-v2.svg.png)](https://en.wikipedia.org/wiki/File:Wiktionary-logo-en-v2.svg) Look up ***[sine](https://en.wiktionary.org/wiki/sine "wiktionary:sine")*** in Wiktionary, the free dictionary. - [![Wikimedia Commons logo](https://upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/20px-Commons-logo.svg.png)](https://en.wikipedia.org/wiki/File:Commons-logo.svg) Media related to [Sine function](https://commons.wikimedia.org/wiki/Category:Sine_function "commons:Category:Sine function") at Wikimedia Commons [![Wiktionary logo](https://upload.wikimedia.org/wikipedia/commons/thumb/9/99/Wiktionary-logo-en-v2.svg/40px-Wiktionary-logo-en-v2.svg.png)](https://en.wikipedia.org/wiki/File:Wiktionary-logo-en-v2.svg) Look up ***[sine and cosine](https://en.wiktionary.org/wiki/Special:Search/sine_and_cosine "wiktionary:Special:Search/sine and cosine")*** in Wiktionary, the free dictionary. | [v](https://en.wikipedia.org/wiki/Template:Trigonometric_and_hyperbolic_functions "Template:Trigonometric and hyperbolic functions") [t](https://en.wikipedia.org/wiki/Template_talk:Trigonometric_and_hyperbolic_functions "Template talk:Trigonometric and hyperbolic functions") [e](https://en.wikipedia.org/wiki/Special:EditPage/Template:Trigonometric_and_hyperbolic_functions "Special:EditPage/Template:Trigonometric and hyperbolic functions")Trigonometric and hyperbolic functions | | |---|---| | Groups | [Trigonometric](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") [Sine and cosine]() [Inverse trigonometric](https://en.wikipedia.org/wiki/Inverse_trigonometric_functions "Inverse trigonometric functions") [Hyperbolic](https://en.wikipedia.org/wiki/Hyperbolic_functions "Hyperbolic functions") [Inverse hyperbolic](https://en.wikipedia.org/wiki/Inverse_hyperbolic_functions "Inverse hyperbolic functions") | | Other | [Versine](https://en.wikipedia.org/wiki/Versine "Versine") [Exsecant](https://en.wikipedia.org/wiki/Exsecant "Exsecant") [Jyā, koti-jyā and utkrama-jyā](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā") [atan2](https://en.wikipedia.org/wiki/Atan2 "Atan2") | ![](https://en.wikipedia.org/wiki/Special:CentralAutoLogin/start?useformat=desktop&type=1x1&usesul3=1) Retrieved from "<https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&oldid=1346396571>" [Categories](https://en.wikipedia.org/wiki/Help:Category "Help:Category"): - 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| Sine and cosine | | |---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/7/71/Sine_cosine_one_period.svg/250px-Sine_cosine_one_period.svg.png)](https://en.wikipedia.org/wiki/File:Sine_cosine_one_period.svg) | | | General information | | | General definition | ![{\\displaystyle {\\begin{aligned}&\\sin(\\theta )={\\frac {\\textrm {opposite}}{\\textrm {hypotenuse}}}\\\\\[8pt\]&\\cos(\\theta )={\\frac {\\textrm {adjacent}}{\\textrm {hypotenuse}}}\\\\\[8pt\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/52374fd3474dfab1331993d6c170e9cac82f4a4a) | In [mathematics](https://en.wikipedia.org/wiki/Mathematics "Mathematics"), **sine** and **cosine** are [trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") of an [angle](https://en.wikipedia.org/wiki/Angle "Angle"). The sine and cosine of an [acute angle](https://en.wikipedia.org/wiki/Acute_angle "Acute angle") are defined in the context of a [right triangle](https://en.wikipedia.org/wiki/Right_triangle "Right triangle"): for the specified angle, its sine is the ratio of the length of the side opposite that angle to the length of the longest side of the [triangle](https://en.wikipedia.org/wiki/Triangle "Triangle") (the [hypotenuse](https://en.wikipedia.org/wiki/Hypotenuse "Hypotenuse")), and the cosine is the [ratio](https://en.wikipedia.org/wiki/Ratio "Ratio") of the length of the adjacent leg to that of the [hypotenuse](https://en.wikipedia.org/wiki/Hypotenuse "Hypotenuse"). For an angle ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), the sine and cosine functions are denoted as ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948) and ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd). The definitions of sine and cosine have been extended to any [real](https://en.wikipedia.org/wiki/Real_number "Real number") value in terms of the lengths of certain line segments in a [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle"). More modern definitions express the sine and cosine as [infinite series](https://en.wikipedia.org/wiki/Series_\(mathematics\) "Series (mathematics)"), or as the solutions of certain [differential equations](https://en.wikipedia.org/wiki/Differential_equation "Differential equation"), allowing their extension to arbitrary positive and negative values and even to [complex numbers](https://en.wikipedia.org/wiki/Complex_number "Complex number"). The sine and cosine functions are commonly used to model [periodic](https://en.wikipedia.org/wiki/Periodic_function "Periodic function") phenomena such as [sound](https://en.wikipedia.org/wiki/Sound "Sound") and [light waves](https://en.wikipedia.org/wiki/Light_waves "Light waves"), the position and velocity of harmonic oscillators, sunlight intensity and day length, and average temperature variations throughout the year. They can be traced to the [*jyā* and *koṭi-jyā*](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā") functions used in [Indian astronomy](https://en.wikipedia.org/wiki/Indian_astronomy "Indian astronomy") during the [Gupta period](https://en.wikipedia.org/wiki/Gupta_period "Gupta period"). ## Elementary descriptions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=1 "Edit section: Elementary descriptions")\] ### Right-angled triangle definition \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=2 "Edit section: Right-angled triangle definition")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ed/Trigono_sine_en2.svg/250px-Trigono_sine_en2.svg.png)](https://en.wikipedia.org/wiki/File:Trigono_sine_en2.svg) For the angle *α*, the sine function gives the ratio of the length of the opposite side to the length of the hypotenuse. To define the sine and cosine of an acute angle ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3), start with a [right triangle](https://en.wikipedia.org/wiki/Right_triangle "Right triangle") that contains an angle of measure ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3); in the accompanying figure, angle ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3) in a right triangle ![{\\displaystyle ABC}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5e55b44cfd965fbdc7a328d5db8a35a619db0971) is the angle of interest. The three sides of the triangle are named as follows:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) Once such a triangle is chosen, the sine of the angle is equal to the length of the opposite side divided by the length of the hypotenuse, and the cosine of the angle is equal to the length of the adjacent side divided by the length of the hypotenuse:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) ![{\\displaystyle \\sin(\\alpha )={\\frac {\\text{opposite}}{\\text{hypotenuse}}},\\qquad \\cos(\\alpha )={\\frac {\\text{adjacent}}{\\text{hypotenuse}}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f0cbaaff1eba0ec735281921a03965ab3a36763b) The other trigonometric functions of the angle can be defined similarly; for example, the [tangent](https://en.wikipedia.org/wiki/Trigonometric_functions#Right-angled_triangle_definitions "Trigonometric functions") is the ratio between the opposite and adjacent sides or equivalently the ratio between the sine and cosine functions. The [reciprocal](https://en.wikipedia.org/wiki/Multiplicative_inverse "Multiplicative inverse") of sine is cosecant, which gives the ratio of the hypotenuse length to the length of the opposite side. Similarly, the reciprocal of cosine is secant, which gives the ratio of the hypotenuse length to that of the adjacent side. The cotangent function is the ratio between the adjacent and opposite sides, a reciprocal of a tangent function. These functions can be formulated as:[\[1\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]-1) ![{\\displaystyle {\\begin{aligned}\\tan(\\theta )&={\\frac {\\sin(\\theta )}{\\cos(\\theta )}}={\\frac {\\text{opposite}}{\\text{adjacent}}},\\\\\\cot(\\theta )&={\\frac {1}{\\tan(\\theta )}}={\\frac {\\text{adjacent}}{\\text{opposite}}},\\\\\\csc(\\theta )&={\\frac {1}{\\sin(\\theta )}}={\\frac {\\text{hypotenuse}}{\\text{opposite}}},\\\\\\sec(\\theta )&={\\frac {1}{\\cos(\\theta )}}={\\frac {\\textrm {hypotenuse}}{\\textrm {adjacent}}}.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a6a3c9e1e99b68fbda583330226dc87136a62315) ### Special angle measures \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=3 "Edit section: Special angle measures")\] As stated, the values ![{\\displaystyle \\sin(\\alpha )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/95a2a215bb78a456fe5662229c73775521b95299) and ![{\\displaystyle \\cos(\\alpha )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8323c66f99d1f3b7e0858fb92b0644fb0b8fba8a) appear to depend on the choice of a right triangle containing an angle of measure ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3). However, this is not the case as all such triangles are [similar](https://en.wikipedia.org/wiki/Similarity_\(geometry\) "Similarity (geometry)"), and so the ratios are the same for each of them. For example, each [leg](https://en.wikipedia.org/wiki/Catheti "Catheti") of the 45-45-90 right triangle is 1 unit, and its hypotenuse is ![{\\displaystyle {\\sqrt {2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b4afc1e27d418021bf10898eb44a7f5f315735ff); therefore, ![{\\textstyle \\sin 45^{\\circ }=\\cos 45^{\\circ }={\\frac {\\sqrt {2}}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/35373a42f10dc6f660ac17f1243294010fea43fc).[\[2\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA36_36]-2) The following table shows the special value of each input for both sine and cosine with the domain between ![{\\textstyle 0\<\\alpha \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d878d68144536cb7db4805f440b6cf3e0b82825b). The input in this table provides various unit systems such as degree, radian, and so on. The angles other than those five can be obtained by using a calculator.[\[3\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742-3)[\[4\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA37_37],_[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA78_78]-4) | Angle, x | sin(*x*) | cos(*x*) | | | | | | |---|---|---|---|---|---|---|---| | [Degrees](https://en.wikipedia.org/wiki/Degree_\(angle\) "Degree (angle)") | [Radians](https://en.wikipedia.org/wiki/Radian "Radian") | [Gradians](https://en.wikipedia.org/wiki/Gradian "Gradian") | [Turns](https://en.wikipedia.org/wiki/Turn_\(geometry\) "Turn (geometry)") | Exact | Decimal | Exact | Decimal | | 0° | 0 | ![{\\displaystyle 0^{g}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ec8a3ac7e88cac5b0efbd0ccee88f8fb38ddf6d2) | | | | | | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/a/a5/Law_of_sines_%28simple%29.svg/250px-Law_of_sines_%28simple%29.svg.png)](https://en.wikipedia.org/wiki/File:Law_of_sines_\(simple\).svg) Law of sines and cosines' illustration The [law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines") is useful for computing the lengths of the unknown sides in a triangle if two angles and one side are known.[\[5\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]-5) Given a triangle ![{\\displaystyle ABC}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5e55b44cfd965fbdc7a328d5db8a35a619db0971) with sides ![{\\displaystyle a}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ffd2487510aa438433a2579450ab2b3d557e5edc), ![{\\displaystyle b}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f11423fbb2e967f986e36804a8ae4271734917c3), and ![{\\displaystyle c}](https://wikimedia.org/api/rest_v1/media/math/render/svg/86a67b81c2de995bd608d5b2df50cd8cd7d92455), and angles opposite those sides ![{\\displaystyle \\alpha }](https://wikimedia.org/api/rest_v1/media/math/render/svg/b79333175c8b3f0840bfb4ec41b8072c83ea88d3), ![{\\displaystyle \\beta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/7ed48a5e36207156fb792fa79d29925d2f7901e8), and ![{\\displaystyle \\gamma }](https://wikimedia.org/api/rest_v1/media/math/render/svg/a223c880b0ce3da8f64ee33c4f0010beee400b1a), the law states, ![{\\displaystyle {\\frac {\\sin \\alpha }{a}}={\\frac {\\sin \\beta }{b}}={\\frac {\\sin \\gamma }{c}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/08ea457459d16cc937492f939b8e40e543078680) This is equivalent to the equality of the first three expressions below: ![{\\displaystyle {\\frac {a}{\\sin \\alpha }}={\\frac {b}{\\sin \\beta }}={\\frac {c}{\\sin \\gamma }}=2R,}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0db5ccda5a3e2e9a89f282c1fc4ef0ace7014bcc) where ![{\\displaystyle R}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4b0bfb3769bf24d80e15374dc37b0441e2616e33) is the triangle's [circumradius](https://en.wikipedia.org/wiki/Circumcircle "Circumcircle"). The [law of cosines](https://en.wikipedia.org/wiki/Law_of_cosines "Law of cosines") is useful for computing the length of an unknown side if two other sides and an angle are known.[\[5\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]-5) The law states, ![{\\displaystyle a^{2}+b^{2}-2ab\\cos(\\gamma )=c^{2}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f30e796ac2afe7443a406b49fa5a718eae315275) In the case where ![{\\displaystyle \\gamma =\\pi /2}](https://wikimedia.org/api/rest_v1/media/math/render/svg/982a2789fde8a2fa65fd04c5e1bfec4dfecffc73) from which ![{\\displaystyle \\cos(\\gamma )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/04328c6895a6a1741585425ddb9474ea27e5ea0b), the resulting equation becomes the [Pythagorean theorem](https://en.wikipedia.org/wiki/Pythagorean_theorem "Pythagorean theorem").[\[6\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA632_632]-6) The [cross product](https://en.wikipedia.org/wiki/Cross_product "Cross product") and [dot product](https://en.wikipedia.org/wiki/Dot_product "Dot product") are operations on two [vectors](https://en.wikipedia.org/wiki/Vector_\(mathematics_and_physics\) "Vector (mathematics and physics)") in [Euclidean vector space](https://en.wikipedia.org/wiki/Euclidean_vector_space "Euclidean vector space"). The sine and cosine functions can be defined in terms of the cross product and dot product. If ![{\\displaystyle \\mathbf {a} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/1a957216653a9ee0d0133dcefd13fb75e36b8b9d) and ![{\\displaystyle \\mathbf {b} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/13ebf4628a1adf07133a6009e4a78bdd990c6eb9) are vectors, and ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) is the angle between ![{\\displaystyle \\mathbf {a} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/1a957216653a9ee0d0133dcefd13fb75e36b8b9d) and ![{\\displaystyle \\mathbf {b} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/13ebf4628a1adf07133a6009e4a78bdd990c6eb9), then sine and cosine can be defined as:[\[7\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-7)[\[8\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-8) ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {\|\\mathbf {a} \\times \\mathbf {b} \|}{\|\\mathbf {a} \|\|\\mathbf {b} \|}},\\\\\\cos(\\theta )&={\\frac {\\mathbf {a} \\cdot \\mathbf {b} }{\|\\mathbf {a} \|\|\\mathbf {b} \|}}.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6b60441dd703c8b6b683a4cf5a5258824b704875) ## Analytic descriptions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=6 "Edit section: Analytic descriptions")\] ### Unit circle definition \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=7 "Edit section: Unit circle definition")\] The sine and cosine functions may also be defined in a more general way by using [unit circle](https://en.wikipedia.org/wiki/Unit_circle#Trigonometric_functions_on_the_unit_circle "Unit circle"), a circle of radius one centered at the origin ![{\\displaystyle (0,0)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5d630d3e781a53b0a3559ae7e5b45f9479a3141a), formulated as the equation of ![{\\displaystyle x^{2}+y^{2}=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ec84b90236512e8d27ff1a8f7707b60b63327de1) in the [Cartesian coordinate system](https://en.wikipedia.org/wiki/Cartesian_coordinate_system "Cartesian coordinate system"). Let a line through the origin intersect the unit circle, making an angle of ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) with the positive half of the ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4)\-axis. The ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4)\- and ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d)\-coordinates of this point of intersection are equal to ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd) and ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948), respectively; that is,[\[9\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741-9) ![{\\displaystyle \\sin(\\theta )=y,\\qquad \\cos(\\theta )=x.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9e7decc76049a9174f255e3491d6e58bab1d4740) This definition is consistent with the right-angled triangle definition of sine and cosine when ![{\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ef78a27752a1f9a51d3b66c7863740f477aa4756) because the length of the hypotenuse of the unit circle is always 1; mathematically speaking, the sine of an angle equals the opposite side of the triangle, which is simply the ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d)\-coordinate. A similar argument can be made for the cosine function to show that the cosine of an angle when ![{\\textstyle 0\<\\theta \<{\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ef78a27752a1f9a51d3b66c7863740f477aa4756), even under the new definition using the unit circle.[\[10\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA68_68]-10)[\[11\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200747-11) #### Graph of a function and its elementary properties \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=8 "Edit section: Graph of a function and its elementary properties")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/3/3b/Circle_cos_sin.gif/500px-Circle_cos_sin.gif)](https://en.wikipedia.org/wiki/File:Circle_cos_sin.gif) Animation demonstrating how the sine function (in red) is graphed from the *y*\-coordinate (red dot) of a point on the [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle") (in green), at an angle of *θ*. The cosine (in blue) is the *x*\-coordinate. Using the unit circle definition has the advantage of drawing the graph of sine and cosine functions. This can be done by rotating counterclockwise a point along the circumference of a circle, depending on the input ![{\\displaystyle \\theta \>0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0b0ac07626379d065418cc158ce6be9aeccf33b9). In a sine function, if the input is ![{\\textstyle \\theta ={\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e6095ebb8d0b6505f453ae2da2fbd3477ecd3a1), the point is rotated counterclockwise and stopped exactly on the ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d)\-axis. If ![{\\displaystyle \\theta =\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/ab4db588619489e27efb50a1d0d5aa016c49ce15), the point is at the circle's halfway point. If ![{\\displaystyle \\theta =2\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/af3479f95999b7e195e5ecc2ee808bf02286332e), the point returns to its origin. This results in both sine and cosine functions having the [range](https://en.wikipedia.org/wiki/Range_of_a_function "Range of a function") between ![{\\displaystyle -1\\leq y\\leq 1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/29d02e9a39a0ad4594157a2f8b82ad89863543c9).[\[12\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741&ndash;42-12) Extending the angle to any real domain, the point rotated counterclockwise continuously. This can be done similarly for the cosine function as well, although the point is rotated initially from the ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d)\-coordinate. In other words, both sine and cosine functions are [periodic](https://en.wikipedia.org/wiki/Periodic_function "Periodic function"), meaning any angle added by the circle's circumference is the angle itself. Mathematically,[\[13\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200741,_43-13) ![{\\displaystyle \\sin(\\theta +2\\pi )=\\sin(\\theta ),\\qquad \\cos(\\theta +2\\pi )=\\cos(\\theta ).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d22ad562f48059fa7b33be5b34f0b0ca1979cd0d) A function ![{\\displaystyle f}](https://wikimedia.org/api/rest_v1/media/math/render/svg/132e57acb643253e7810ee9702d9581f159a1c61) is said to be [odd](https://en.wikipedia.org/wiki/Odd_function "Odd function") if ![{\\displaystyle f(-x)=-f(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b022ffe516cf5bc26a68fd954753aa2bddf508f1), and is said to be [even](https://en.wikipedia.org/wiki/Even_function "Even function") if ![{\\displaystyle f(-x)=f(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/185fd2e78903788bc5756b067d0ac6aae1846724). The sine function is odd, whereas the cosine function is even.[\[14\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2012[httpsbooksgooglecombooksidOMrcN0a3LxICpgRA1-PA165_165]-14) Both sine and cosine functions are similar, with their difference being [shifted](https://en.wikipedia.org/wiki/Translation_\(geometry\) "Translation (geometry)") by ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae). This phase shift can be expressed as ![{\\textstyle \\cos(\\theta )=\\sin \\left(\\theta +{\\frac {\\pi }{2}}\\right)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/16e716cd4b5339b573745c33edcc769226903a9b) or ![{\\textstyle \\sin(\\theta )=\\cos \\left(\\theta -{\\frac {\\pi }{2}}\\right)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ea80145f070fac0e114bd339dac33c3aa4286cda). This is distinct from the cofunction identities that follow below, which arise from right-triangle geometry and are not phase shifts: [\[15\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742,_47-15) ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&=\\cos \\left({\\frac {\\pi }{2}}-\\theta \\right),\\\\\\cos(\\theta )&=\\sin \\left({\\frac {\\pi }{2}}-\\theta \\right).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d4998408fbf02a4669c3e151a840a7bc314101ef) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Cosine_fixed_point.svg/250px-Cosine_fixed_point.svg.png)](https://en.wikipedia.org/wiki/File:Cosine_fixed_point.svg) The fixed point iteration *x**n*\+1 = cos(*xn*) with initial value *x*0 = −1 converges to the Dottie number. Zero is the only real [fixed point](https://en.wikipedia.org/wiki/Fixed_point_\(mathematics\) "Fixed point (mathematics)") of the sine function; in other words the only intersection of the sine function and the [identity function](https://en.wikipedia.org/wiki/Identity_function "Identity function") is ![{\\displaystyle \\sin(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ecb40badcf53b50e5d03c49c7a5e1977e3ff262e). The only real fixed point of the cosine function is called the [Dottie number](https://en.wikipedia.org/wiki/Dottie_number "Dottie number"). The Dottie number is the unique real root of the equation ![{\\displaystyle \\cos(x)=x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3cf8688ffc25998040ed8bf59f0a6298233a143c). The decimal expansion of the Dottie number is approximately 0.739085.[\[16\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-16) #### Continuity and differentiation \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=9 "Edit section: Continuity and differentiation")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Sine_quads_01_Pengo.svg/500px-Sine_quads_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Sine_quads_01_Pengo.svg) The quadrants of the unit circle and of sin(*x*), using the [Cartesian coordinate system](https://en.wikipedia.org/wiki/Cartesian_coordinate_system "Cartesian coordinate system") The sine and cosine functions are infinitely differentiable.[\[17\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]-17) The derivative of sine is cosine, and the derivative of cosine is negative sine:[\[18\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007115-18) ![{\\displaystyle {\\frac {d}{dx}}\\sin(x)=\\cos(x),\\qquad {\\frac {d}{dx}}\\cos(x)=-\\sin(x).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3ae62cb5b610f8b5309ca193d299662fb18d4099) Continuing the process in higher-order derivative results in the repeated same functions; the fourth derivative of a sine is the sine itself.[\[17\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]-17) These derivatives can be applied to the [first derivative test](https://en.wikipedia.org/wiki/First_derivative_test "First derivative test"), according to which the [monotonicity](https://en.wikipedia.org/wiki/Monotone_function "Monotone function") of a function can be defined as the inequality of function's first derivative greater or less than equal to zero.[\[19\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007155-19) It can also be applied to [second derivative test](https://en.wikipedia.org/wiki/Second_derivative_test "Second derivative test"), according to which the [concavity](https://en.wikipedia.org/wiki/Concave_function "Concave function") of a function can be defined by applying the inequality of the function's second derivative greater or less than equal to zero.[\[20\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007157-20) The following table shows that both sine and cosine functions have concavity and monotonicity—the positive sign (![{\\displaystyle +}](https://wikimedia.org/api/rest_v1/media/math/render/svg/fe6ef363cd19902d1a7a71fb1c8b21e8ede52406)) denotes a graph is increasing (going upward) and the negative sign (![{\\displaystyle -}](https://wikimedia.org/api/rest_v1/media/math/render/svg/04bd52ce670743d3b61bec928a7ec9f47309eb36)) is decreasing (going downward)—in certain intervals.[\[3\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon200742-3) This information can be represented as a Cartesian coordinates system divided into four quadrants. | [Quadrant](https://en.wikipedia.org/wiki/Cartesian_coordinate_system#Quadrants_and_octants "Cartesian coordinate system") | Angle | Sine | Cosine | | | | | |---|---|---|---|---|---|---|---| | [Degrees](https://en.wikipedia.org/wiki/Degree_\(angle\) "Degree (angle)") | [Radians](https://en.wikipedia.org/wiki/Radian "Radian") | [Sign](https://en.wikipedia.org/wiki/Sign_\(mathematics\) "Sign (mathematics)") | [Monotony](https://en.wikipedia.org/wiki/Monotonic_function "Monotonic function") | [Convexity](https://en.wikipedia.org/wiki/Convex_function "Convex function") | [Sign](https://en.wikipedia.org/wiki/Sign_\(mathematics\) "Sign (mathematics)") | [Monotony](https://en.wikipedia.org/wiki/Monotonic_function "Monotonic function") | [Convexity](https://en.wikipedia.org/wiki/Convex_function "Convex function") | | 1st quadrant, I | ![{\\displaystyle 0^{\\circ }\<x\<90^{\\circ }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3cd94c157a7ab3ac44ece2b4a7e2a805c5e3774b) | | | | | | | Both sine and cosine functions can be defined by using differential equations. The pair of ![{\\displaystyle (\\cos \\theta ,\\sin \\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/591da286444bb19845241d047707dd8793d4b143) is the solution ![{\\displaystyle (x(\\theta ),y(\\theta ))}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3761d6e3635ea327a1fea316311a9974ba2a2898) to the two-dimensional system of [differential equations](https://en.wikipedia.org/wiki/Differential_equation "Differential equation") ![{\\displaystyle y'(\\theta )=x(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e24c7568490cc0b2b359757eab6411e071ea5a4e) and ![{\\displaystyle x'(\\theta )=-y(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8d2efd00b2708f705444970234d98bb745c37b4c) with the [initial conditions](https://en.wikipedia.org/wiki/Initial_conditions "Initial conditions") ![{\\displaystyle y(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/343c32f38bb379b4b208477b130d8f522d3f0788) and ![{\\displaystyle x(0)=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e502f85fa127369616c9d6cce7b0cfdfad2abbc1). One could interpret the unit circle in the above definitions as defining the [phase space trajectory](https://en.wikipedia.org/wiki/Phase_space_trajectory "Phase space trajectory") of the differential equation with the given initial conditions. It can be interpreted as a phase space trajectory of the system of differential equations ![{\\displaystyle y'(\\theta )=x(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e24c7568490cc0b2b359757eab6411e071ea5a4e) and ![{\\displaystyle x'(\\theta )=-y(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8d2efd00b2708f705444970234d98bb745c37b4c) starting from the initial conditions ![{\\displaystyle y(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/343c32f38bb379b4b208477b130d8f522d3f0788) and ![{\\displaystyle x(0)=1}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e502f85fa127369616c9d6cce7b0cfdfad2abbc1).\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] #### Integral and the usage in mensuration \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=10 "Edit section: Integral and the usage in mensuration")\] Their area under a curve can be obtained by using the [integral](https://en.wikipedia.org/wiki/Integral "Integral") with a certain bounded interval. Their antiderivatives are: ![{\\displaystyle \\int \\sin(x)\\,dx=-\\cos(x)+C\\qquad \\int \\cos(x)\\,dx=\\sin(x)+C,}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2e14210f7e049e74d1153559c98ea8fd4fb5efa0) where ![{\\displaystyle C}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4fc55753007cd3c18576f7933f6f089196732029) denotes the [constant of integration](https://en.wikipedia.org/wiki/Constant_of_integration "Constant of integration").[\[21\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007199-21) These antiderivatives may be applied to compute the mensuration properties of both sine and cosine functions' curves with a given interval. For example, the [arc length](https://en.wikipedia.org/wiki/Arc_length "Arc length") of the sine curve between ![{\\displaystyle 0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2aae8864a3c1fec9585261791a809ddec1489950) and ![{\\displaystyle t}](https://wikimedia.org/api/rest_v1/media/math/render/svg/65658b7b223af9e1acc877d848888ecdb4466560) is ![{\\displaystyle \\int \_{0}^{t}\\!{\\sqrt {1+\\cos ^{2}(x)}}\\,dx={\\sqrt {2}}\\operatorname {E} \\left(t,{\\frac {1}{\\sqrt {2}}}\\right),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a4e732378f19b126018432e28c062594d9538420) where ![{\\displaystyle \\operatorname {E} (\\varphi ,k)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c1520125a116a29984e7bca67df1f10ef35292b0) is the [incomplete elliptic integral of the second kind](https://en.wikipedia.org/wiki/Elliptic_integral#Incomplete_elliptic_integral_of_the_second_kind "Elliptic integral") with modulus ![{\\displaystyle k}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c3c9a2c7b599b37105512c5d570edc034056dd40). It cannot be expressed using [elementary functions](https://en.wikipedia.org/wiki/Elementary_function "Elementary function").[\[22\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVince2023[httpsbooksgooglecombooksidGnW6EAAAQBAJpgPA162_162]-22) In the case of a full period, its arc length is ![{\\displaystyle L={\\frac {4{\\sqrt {2\\pi ^{3}}}}{\\Gamma (1/4)^{2}}}+{\\frac {\\Gamma (1/4)^{2}}{\\sqrt {2\\pi }}}={\\frac {2\\pi }{\\varpi }}+2\\varpi \\approx 7.6404}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7a6d9ffe117d665d73ef4788658c5b5cfd8cae33) where ![{\\displaystyle \\Gamma }](https://wikimedia.org/api/rest_v1/media/math/render/svg/4cfde86a3f7ec967af9955d0988592f0693d2b19) is the [gamma function](https://en.wikipedia.org/wiki/Gamma_function "Gamma function") and ![{\\displaystyle \\varpi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/e50d258418b5fa150a86b58f8d5eb40613e3ebf7) is the [lemniscate constant](https://en.wikipedia.org/wiki/Lemniscate_constant "Lemniscate constant").[\[23\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAdlaj2012-23)[\[24\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-24) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b4/Arcsine_Arccosine.svg/250px-Arcsine_Arccosine.svg.png)](https://en.wikipedia.org/wiki/File:Arcsine_Arccosine.svg) The usual principal values of the arcsin(*x*) and arccos(*x*) functions graphed on the Cartesian plane The functions ![{\\textstyle \\sin :\\mathbb {R} \\to \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/5b76babd4c66e7d6257658191c1e4b6dd443412d) and ![{\\displaystyle \\cos :\\mathbb {R} \\to \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/490d5f0e2fdc2b561101f411ecea9e3f98e468d9) (as well as those functions with the same function rule and domain whose codomain is a subset of ![{\\displaystyle \\mathbb {R} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/786849c765da7a84dbc3cce43e96aad58a5868dc) containing the interval ![{\\displaystyle \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/79566f857ac1fcd0ef0f62226298a4ed15b796ad)) are not bijective and therefore do not have inverse functions. For example, ![{\\displaystyle \\sin(0)=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ecb40badcf53b50e5d03c49c7a5e1977e3ff262e), but also ![{\\displaystyle \\sin(\\pi )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f6e7e3130a6ba2043ae878c9b1dc7aa7998afb8c), ![{\\displaystyle \\sin(2\\pi )=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/55c160c102e7cd62b4a03d1df4761601235a2b3d). Sine's "inverse", called arcsine, can then be described not as a function but a relation (for example, all integer multiples of ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a) would have an arcsine of zero). To define the inverse functions of sine and cosine, they must be restricted to their [principal branches](https://en.wikipedia.org/wiki/Principal_branch "Principal branch") by restricting their domain and codomain; the standard functions used to define arcsine and arccosine are then ![{\\displaystyle \\sin :\\left\[-\\pi /2,\\pi /2\\right\]\\to \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/34676d3cc30ba3520fb506118910a65ae45fe25f) and ![{\\displaystyle \\cos :\\left\[0,\\pi \\right\]\\to \\left\[-1,1\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4a2864b5c77dc4b8af5111e9d4e78e9ea9a876b7).[\[25\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007365-25) These are bijective and have inverses: ![{\\displaystyle \\arcsin :\\left\[-1,1\\right\]\\to \\left\[-\\pi /2,\\pi /2\\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/024a4d91e022705b40fb40e554d294bdd9e2eea4) and ![{\\displaystyle \\arccos :\\left\[-1,1\\right\]\\to \\left\[0,\\pi \\right\]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e1126b78ee63338e44c6a25dae46d50fdad0b5c1). Alternative notation is ![{\\displaystyle \\sin ^{-1}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/21bc4ca64ac415c9ae60fb4e60fe4bddee17b8ef) for arcsine and ![{\\displaystyle \\cos ^{-1}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7eabf706b4642d521c6279a2f07ac9715c7679a7) for arccosine. Using these definitions, one obtains the identity maps: ![{\\displaystyle {\\begin{aligned}\\sin \\circ \\arcsin \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arcsin \\circ \\sin \\,(x)&=x\\qquad x\\in \\left\[-\\pi /2,\\pi /2\\right\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/631b526ef79de3155b8c652483e136009c87f6ef)and ![{\\displaystyle {\\begin{aligned}\\cos \\circ \\arccos \\,(x)&=x\\qquad x\\in \\left\[-1,1\\right\]\\\\\\arccos \\circ \\cos \\,(x)&=x\\qquad x\\in \\left\[0,\\pi \\right\]\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/81aa8f5001ec127005efd5c2508631440ff6ab8d) An acute angle ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) is given by: ![{\\displaystyle \\theta =\\arcsin \\left({\\frac {\\text{opposite}}{\\text{hypotenuse}}}\\right)=\\arccos \\left({\\frac {\\text{adjacent}}{\\text{hypotenuse}}}\\right),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6a7fb2ae2f0c2ec3085667df4d1e54d48d67cd7a) where for some integer ![{\\displaystyle k}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c3c9a2c7b599b37105512c5d570edc034056dd40), ![{\\displaystyle {\\begin{aligned}\\sin(y)=x\\iff \&y=\\arcsin(x)+2\\pi k,{\\text{ or }}\\\\\&y=\\pi -\\arcsin(x)+2\\pi k\\\\\\cos(y)=x\\iff \&y=\\arccos(x)+2\\pi k,{\\text{ or }}\\\\\&y=-\\arccos(x)+2\\pi k\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/da20b32e7b46d5ccdf3f058b812c8ad9768fa678) By definition, both functions satisfy the equations: ![{\\displaystyle \\sin(\\arcsin(x))=x\\qquad \\cos(\\arccos(x))=x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/25b4ef466eeb61838eb9b7b8692bebf636a9423f) and ![{\\displaystyle {\\begin{aligned}\\arcsin(\\sin(\\theta ))=\\theta \\quad &{\\text{for}}\\quad -{\\frac {\\pi }{2}}\\leq \\theta \\leq {\\frac {\\pi }{2}}\\\\\\arccos(\\cos(\\theta ))=\\theta \\quad &{\\text{for}}\\quad 0\\leq \\theta \\leq \\pi \\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/11a64d948fdadfaf9eeb77c6fcd8c3f646f46cee) According to [Pythagorean theorem](https://en.wikipedia.org/wiki/Pythagorean_theorem "Pythagorean theorem"), the squared hypotenuse is the sum of two squared legs of a right triangle. Dividing the formula on both sides with squared hypotenuse resulting in the [Pythagorean trigonometric identity](https://en.wikipedia.org/wiki/Pythagorean_trigonometric_identity "Pythagorean trigonometric identity"), the sum of a squared sine and a squared cosine equals 1:[\[26\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA99_99]-26)[\[a\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-27) ![{\\displaystyle \\sin ^{2}(\\theta )+\\cos ^{2}(\\theta )=1.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8c2fa6795bad3d685ca0704a63f5771bda27d5ac) Sine and cosine satisfy the following double-angle formulas:[\[27\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-28) ![{\\displaystyle {\\begin{aligned}\\sin(2\\theta )&=2\\sin(\\theta )\\cos(\\theta ),\\\\\\cos(2\\theta )&=\\cos ^{2}(\\theta )-\\sin ^{2}(\\theta )\\\\&=2\\cos ^{2}(\\theta )-1\\\\&=1-2\\sin ^{2}(\\theta )\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/497be0073c63433342edee671020c7aa109e0e6e) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c9/SinSquared.png/250px-SinSquared.png)](https://en.wikipedia.org/wiki/File:SinSquared.png) Sine function in blue and sine squared function in red. The *x*\-axis is in radians. The cosine double angle formula implies that sin2 and cos2 are, themselves, shifted and scaled sine waves. Specifically,[\[28\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-29) ![{\\displaystyle \\sin ^{2}(\\theta )={\\frac {1-\\cos(2\\theta )}{2}}\\qquad \\cos ^{2}(\\theta )={\\frac {1+\\cos(2\\theta )}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4dc6bb37905a99fd21458b0011b90ebfcf6e9092) The graph shows both sine and sine squared functions, with the sine in blue and the sine squared in red. Both graphs have the same shape but with different ranges of values and different periods. Sine squared has only positive values, but twice the number of periods.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] ### Series and polynomials \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=13 "Edit section: Series and polynomials")\] [![](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Sine.gif/250px-Sine.gif)](https://en.wikipedia.org/wiki/File:Sine.gif) This animation shows how including more and more terms in the partial sum of its Taylor series approaches a sine curve. Both sine and cosine functions can be defined by using a [Taylor series](https://en.wikipedia.org/wiki/Taylor_series "Taylor series"), a [power series](https://en.wikipedia.org/wiki/Power_series "Power series") involving the higher-order derivatives. As mentioned in [§ Continuity and differentiation](https://en.wikipedia.org/wiki/Sine_and_cosine#Continuity_and_differentiation), the [derivative](https://en.wikipedia.org/wiki/Derivative "Derivative") of sine is cosine and the derivative of cosine is the negative of sine. This means the successive derivatives of ![{\\displaystyle \\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3a990a5545cac26c1c6821dca95d898bc80fe3a8) are ![{\\displaystyle \\cos(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/eb9af7ed6f44822021b74bb82b431022c7fd66b3), ![{\\displaystyle -\\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a7326163fe774b61667587334208ecaef5798056), ![{\\displaystyle -\\cos(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3f5dca2087cf314bb30116832bea1df5e00086be), ![{\\displaystyle \\sin(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3a990a5545cac26c1c6821dca95d898bc80fe3a8), continuing to repeat those four functions. The ![{\\displaystyle (4n+k)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d6d26c80aefe4f8e27c3b52e0b0375980f8addba)\-th derivative, evaluated at the point 0: ![{\\displaystyle \\sin ^{(4n+k)}(0)={\\begin{cases}0&{\\text{when }}k=0\\\\1&{\\text{when }}k=1\\\\0&{\\text{when }}k=2\\\\-1&{\\text{when }}k=3\\end{cases}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d46c038e501fe9a5f4ca170b57667a244b9b77b2) where the superscript represents repeated differentiation. This implies the following Taylor series expansion at ![{\\displaystyle x=0}](https://wikimedia.org/api/rest_v1/media/math/render/svg/953917eaf52f2e1baad54c8c9e3d6f9bb3710cdc). One can then use the theory of [Taylor series](https://en.wikipedia.org/wiki/Taylor_series "Taylor series") to show that the following identities hold for all [real numbers](https://en.wikipedia.org/wiki/Real_number "Real number") ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4)—where ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) is the angle in radians.[\[29\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492-30) More generally, for all [complex numbers](https://en.wikipedia.org/wiki/Complex_number "Complex number"):[\[30\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]-31) ![{\\displaystyle {\\begin{aligned}\\sin(x)&=x-{\\frac {x^{3}}{3!}}+{\\frac {x^{5}}{5!}}-{\\frac {x^{7}}{7!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}x^{2n+1}\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f13ee50efedabff2d208516e6a31ea495a9c843d) Taking the derivative of each term gives the Taylor series for cosine:[\[29\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492-30)[\[30\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]-31) ![{\\displaystyle {\\begin{aligned}\\cos(x)&=1-{\\frac {x^{2}}{2!}}+{\\frac {x^{4}}{4!}}-{\\frac {x^{6}}{6!}}+\\cdots \\\\&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}x^{2n}\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/742bd8177eff1a0186a49c19c6a0c626c7fe3563) Both sine and cosine functions with multiple angles may appear as their [linear combination](https://en.wikipedia.org/wiki/Linear_combination "Linear combination"), resulting in a polynomial. Such a polynomial is known as the [trigonometric polynomial](https://en.wikipedia.org/wiki/Trigonometric_polynomial "Trigonometric polynomial"). The trigonometric polynomial's ample applications may be acquired in [its interpolation](https://en.wikipedia.org/wiki/Trigonometric_interpolation "Trigonometric interpolation"), and its extension of a periodic function known as the [Fourier series](https://en.wikipedia.org/wiki/Fourier_series "Fourier series"). Let ![{\\displaystyle a\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/790f9209748c2dca7ed7b81932c37c02af1dbc31) and ![{\\displaystyle b\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/28e2d72f6dd9375c8f1f59f1effd9b4e5492ac97) be any coefficients, then the trigonometric polynomial of a degree ![{\\displaystyle N}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f5e3890c981ae85503089652feb48b191b57aae3)—denoted as ![{\\displaystyle T(x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/1171c29b4c2b5575f50a4ea9313f90448a2cbe05)—is defined as:[\[31\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEPowell1981150-32)[\[32\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTERudin198788-33) ![{\\displaystyle T(x)=a\_{0}+\\sum \_{n=1}^{N}a\_{n}\\cos(nx)+\\sum \_{n=1}^{N}b\_{n}\\sin(nx).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0d91df6657ed384066a15aee6f8f0ef01c9a0787) The [trigonometric series](https://en.wikipedia.org/wiki/Trigonometric_series "Trigonometric series") can be defined similarly analogous to the trigonometric polynomial, its infinite inversion. Let ![{\\displaystyle A\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/730f6906700685b6d52f3958b1c2ae659d2d97d2) and ![{\\displaystyle B\_{n}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2f568bf6d34e97b9fdda0dc7e276d6c4501d2045) be any coefficients, then the trigonometric series can be defined as:[\[33\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZygmund19681-34) ![{\\displaystyle {\\frac {1}{2}}A\_{0}+\\sum \_{n=1}^{\\infty }A\_{n}\\cos(nx)+B\_{n}\\sin(nx).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a20bbca53c25bda2d3a375f83924db3637e013b7) In the case of a Fourier series with a given integrable function ![{\\displaystyle f}](https://wikimedia.org/api/rest_v1/media/math/render/svg/132e57acb643253e7810ee9702d9581f159a1c61), the coefficients of a trigonometric series are:[\[34\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZygmund196811-35) ![{\\displaystyle {\\begin{aligned}A\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\cos(nx)\\,dx,\\\\B\_{n}&={\\frac {1}{\\pi }}\\int \_{0}^{2\\pi }f(x)\\sin(nx)\\,dx.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/71e46a4445a4bb3a0d5933f7f542c39673dafef1) ## Complex numbers relationship \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=14 "Edit section: Complex numbers relationship")\] ### Complex exponential function definitions \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=15 "Edit section: Complex exponential function definitions")\] Both sine and cosine can be extended further via [complex number](https://en.wikipedia.org/wiki/Complex_number "Complex number"), a set of numbers composed of both [real](https://en.wikipedia.org/wiki/Real_number "Real number") and [imaginary numbers](https://en.wikipedia.org/wiki/Imaginary_number "Imaginary number"). For real number ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), the definition of both sine and cosine functions can be extended in a [complex plane](https://en.wikipedia.org/wiki/Complex_plane "Complex plane") in terms of an [exponential function](https://en.wikipedia.org/wiki/Exponential_function "Exponential function") as follows:[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) ![{\\displaystyle {\\begin{aligned}\\sin(\\theta )&={\\frac {e^{i\\theta }-e^{-i\\theta }}{2i}},\\\\\\cos(\\theta )&={\\frac {e^{i\\theta }+e^{-i\\theta }}{2}},\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/725f29f76be948091e80a1467b067a8ca9e9dbd3) Alternatively, both functions can be defined in terms of [Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula"):[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) ![{\\displaystyle {\\begin{aligned}e^{i\\theta }&=\\cos(\\theta )+i\\sin(\\theta ),\\\\e^{-i\\theta }&=\\cos(\\theta )-i\\sin(\\theta ).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/77db983756d03fe6b65cfb8af534812004ebfbbb) When plotted on the [complex plane](https://en.wikipedia.org/wiki/Complex_plane "Complex plane"), the function ![{\\displaystyle e^{ix}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5271aa5bef13f6bd715afeda45bc59ae37d7c6d4) for real values of ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) traces out the [unit circle](https://en.wikipedia.org/wiki/Unit_circle "Unit circle") in the complex plane. Both sine and cosine functions may be simplified to the imaginary and real parts of ![{\\displaystyle e^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7b4b8e67ee479d68e0e5040aaf87eff99214c90f) as:[\[36\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTERudin19872-37) ![{\\displaystyle {\\begin{aligned}\\sin \\theta &=\\operatorname {Im} (e^{i\\theta }),\\\\\\cos \\theta &=\\operatorname {Re} (e^{i\\theta }).\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/646f096950ba96ce2f21de18bfa047b6421b21e0) When ![{\\displaystyle z=x+iy}](https://wikimedia.org/api/rest_v1/media/math/render/svg/08e90bb6b36fef59c6113eed2a08f10d77240741) for real values ![{\\displaystyle x}](https://wikimedia.org/api/rest_v1/media/math/render/svg/87f9e315fd7e2ba406057a97300593c4802b53e4) and ![{\\displaystyle y}](https://wikimedia.org/api/rest_v1/media/math/render/svg/b8a6208ec717213d4317e666f1ae872e00620a0d), where ![{\\displaystyle i={\\sqrt {-1}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/370c8cebe9634fbfc84c29ea61680b0ad4a1ae0d), both sine and cosine functions can be expressed in terms of real sines, cosines, and [hyperbolic functions](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function") as:[\[37\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-38) ![{\\displaystyle {\\begin{aligned}\\sin z&=\\sin x\\cosh y+i\\cos x\\sinh y,\\\\\\cos z&=\\cos x\\cosh y-i\\sin x\\sinh y.\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/47251493866932a39ed455153827afe21a781596) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/8/8d/Sinus_und_Kosinus_am_Einheitskreis_3.svg/250px-Sinus_und_Kosinus_am_Einheitskreis_3.svg.png)](https://en.wikipedia.org/wiki/File:Sinus_und_Kosinus_am_Einheitskreis_3.svg) Both functions ![{\\displaystyle \\cos(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aaac7b75cda6d5570780075aa2622d27b21117cd) and ![{\\displaystyle \\sin(\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/acafc444aea85d63a40dabf84f035a6b4955a948) are the real and imaginary parts of ![{\\displaystyle e^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7b4b8e67ee479d68e0e5040aaf87eff99214c90f). Sine and cosine are used to connect the real and imaginary parts of a [complex number](https://en.wikipedia.org/wiki/Complex_number "Complex number") with its [polar coordinates](https://en.wikipedia.org/wiki/Polar_coordinates "Polar coordinates") ![{\\displaystyle (r,\\theta )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ed8396fdc359fb06c93722137c959e7496e47ed6): ![{\\displaystyle z=r(\\cos(\\theta )+i\\sin(\\theta ))=r\\cos(\\theta )+ir\\sin(\\theta ),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/250e8c59ae404db0bbf52c140bd7b9d7ac8387b2) and the real and imaginary parts are ![{\\displaystyle {\\begin{aligned}\\operatorname {Re} (z)&=r\\cos(\\theta ),\\\\\\operatorname {Im} (z)&=r\\sin(\\theta ),\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/abf44a594aabf7817998c91793f805ecdb366282) where ![{\\displaystyle r}](https://wikimedia.org/api/rest_v1/media/math/render/svg/0d1ecb613aa2984f0576f70f86650b7c2a132538) and ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af) represent the magnitude and angle of the complex number ![{\\displaystyle z}](https://wikimedia.org/api/rest_v1/media/math/render/svg/bf368e72c009decd9b6686ee84a375632e11de98).[\[38\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_23&ndash;24]-39) For any real number ![{\\displaystyle \\theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/6e5ab2664b422d53eb0c7df3b87e1360d75ad9af), Euler's formula in terms of polar coordinates is stated as ![{\\textstyle z=re^{i\\theta }}](https://wikimedia.org/api/rest_v1/media/math/render/svg/95946f451434232fc04452bd3b3e4251de1a9d13).[\[35\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]-36) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/4/45/Complex_sin.jpg/250px-Complex_sin.jpg)](https://en.wikipedia.org/wiki/File:Complex_sin.jpg) [Domain coloring](https://en.wikipedia.org/wiki/Domain_coloring "Domain coloring") of sin(*z*) in the complex plane. Brightness indicates absolute magnitude, hue represents complex argument. [![](https://upload.wikimedia.org/wikipedia/commons/thumb/9/96/Sin_z_vector_field_02_Pengo.svg/250px-Sin_z_vector_field_02_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Sin_z_vector_field_02_Pengo.svg) Vector field rendering of sin(*z*) Applying the series definition of the sine and cosine to a complex argument, *z*, gives: ![{\\displaystyle {\\begin{aligned}\\sin(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n+1)!}}z^{2n+1}\\\\&={\\frac {e^{iz}-e^{-iz}}{2i}}\\\\&={\\frac {\\sinh \\left(iz\\right)}{i}}\\\\&=-i\\sinh \\left(iz\\right)\\\\\\cos(z)&=\\sum \_{n=0}^{\\infty }{\\frac {(-1)^{n}}{(2n)!}}z^{2n}\\\\&={\\frac {e^{iz}+e^{-iz}}{2}}\\\\&=\\cosh(iz)\\\\\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/77ff8035628f5a90a7aced4bb8fb5b4a2b0c3a52) where sinh and cosh are the [hyperbolic sine and cosine](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function"). These are [entire functions](https://en.wikipedia.org/wiki/Entire_function "Entire function"). It is also sometimes useful to express the complex sine and cosine functions in terms of the real and imaginary parts of its argument: ![{\\displaystyle {\\begin{aligned}\\sin(x+iy)&=\\sin(x)\\cos(iy)+\\cos(x)\\sin(iy)\\\\&=\\sin(x)\\cosh(y)+i\\cos(x)\\sinh(y)\\\\\\cos(x+iy)&=\\cos(x)\\cos(iy)-\\sin(x)\\sin(iy)\\\\&=\\cos(x)\\cosh(y)-i\\sin(x)\\sinh(y)\\\\\\end{aligned}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/22162f3c99776ef5203c9c7fc8d418162bdcfd99) #### Partial fraction and product expansions of complex sine \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=18 "Edit section: Partial fraction and product expansions of complex sine")\] Using the partial fraction expansion technique in [complex analysis](https://en.wikipedia.org/wiki/Complex_analysis "Complex analysis"), one can find that the infinite series ![{\\displaystyle \\sum \_{n=-\\infty }^{\\infty }{\\frac {(-1)^{n}}{z-n}}={\\frac {1}{z}}-2z\\sum \_{n=1}^{\\infty }{\\frac {(-1)^{n}}{n^{2}-z^{2}}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/767d43fdad5d7a47e46f1433d20d909d91af8883) both converge and are equal to ![{\\textstyle {\\frac {\\pi }{\\sin(\\pi z)}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/02adeb7acbfc515905a0c72f7130ae5d2589df72). Similarly, one can show that ![{\\displaystyle {\\frac {\\pi ^{2}}{\\sin ^{2}(\\pi z)}}=\\sum \_{n=-\\infty }^{\\infty }{\\frac {1}{(z-n)^{2}}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/76b4bc619e6aa45ebdcdb9e88551598f69931529) Using product expansion technique, one can derive ![{\\displaystyle \\sin(\\pi z)=\\pi z\\prod \_{n=1}^{\\infty }\\left(1-{\\frac {z^{2}}{n^{2}}}\\right).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/17ce4c82316483de357bac1133ac3d7af0092707) #### Usage of complex sine \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=19 "Edit section: Usage of complex sine")\] sin(*z*) is found in the [functional equation](https://en.wikipedia.org/wiki/Functional_equation "Functional equation") for the [Gamma function](https://en.wikipedia.org/wiki/Gamma_function "Gamma function"), ![{\\displaystyle \\Gamma (s)\\Gamma (1-s)={\\pi \\over \\sin(\\pi s)},}](https://wikimedia.org/api/rest_v1/media/math/render/svg/07f53255b83f8d3db49cf23173da760f7048b689) which in turn is found in the [functional equation](https://en.wikipedia.org/wiki/Functional_equation "Functional equation") for the [Riemann zeta-function](https://en.wikipedia.org/wiki/Riemann_zeta-function "Riemann zeta-function"), ![{\\displaystyle \\zeta (s)=2(2\\pi )^{s-1}\\Gamma (1-s)\\sin \\left({\\frac {\\pi }{2}}s\\right)\\zeta (1-s).}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f170929c08858f62da589f8fccb2565c43c769a8) As a [holomorphic function](https://en.wikipedia.org/wiki/Holomorphic_function "Holomorphic function"), sin *z* is a 2D solution of [Laplace's equation](https://en.wikipedia.org/wiki/Laplace%27s_equation "Laplace's equation"): ![{\\displaystyle \\Delta u(x\_{1},x\_{2})=0.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/cdaaf4948b285dfd3deb916716fc5daa6d9d3d22) The complex sine function is also related to the level curves of [pendulums](https://en.wikipedia.org/wiki/Pendulums "Pendulums").\[*[how?](https://en.wikipedia.org/wiki/Wikipedia:Please_clarify "Wikipedia:Please clarify")*\][\[39\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-40)\[*[better source needed](https://en.wikipedia.org/wiki/Wikipedia:Verifiability#Questionable_sources "Wikipedia:Verifiability")*\] | | | | |---|---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f4/Complex_sin_real_01_Pengo.svg/250px-Complex_sin_real_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_real_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Complex_sin_imag_01_Pengo.svg/250px-Complex_sin_imag_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_imag_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/9/9e/Complex_sin_abs_01_Pengo.svg/250px-Complex_sin_abs_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_sin_abs_01_Pengo.svg) | | Real component | Imaginary component | Magnitude | | | | | |---|---|---| | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b3/Complex_arcsin_real_01_Pengo.svg/250px-Complex_arcsin_real_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_real_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/f/f1/Complex_arcsin_imag_01_Pengo.svg/250px-Complex_arcsin_imag_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_imag_01_Pengo.svg) | [![](https://upload.wikimedia.org/wikipedia/commons/thumb/1/1f/Complex_arcsin_abs_01_Pengo.svg/250px-Complex_arcsin_abs_01_Pengo.svg.png)](https://en.wikipedia.org/wiki/File:Complex_arcsin_abs_01_Pengo.svg) | | Real component | Imaginary component | Magnitude | The word *sine* is derived, indirectly, from the [Sanskrit](https://en.wikipedia.org/wiki/Sanskrit "Sanskrit") word *jyā* 'bow-string' or more specifically its synonym *jīvá* (both adopted from [Ancient Greek](https://en.wikipedia.org/wiki/Ancient_Greek_language "Ancient Greek language") χορδή 'string; chord'), due to visual similarity between the arc of a circle with its corresponding chord and a bow with its string (see [jyā, koti-jyā and utkrama-jyā](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā"); *sine* and *chord* are closely related in a circle of unit diameter, see [Ptolemy's Theorem](https://en.wikipedia.org/wiki/Ptolemy%27s_theorem#Corollaries "Ptolemy's theorem")). This was [transliterated](https://en.wikipedia.org/wiki/Transliteration "Transliteration") in [Arabic](https://en.wikipedia.org/wiki/Arabic_language "Arabic language") as *jība*, which is meaningless in that language and written as *jb* (جب). Since Arabic is written without short vowels, *jb* was interpreted as the [homograph](https://en.wikipedia.org/wiki/Homograph "Homograph") *jayb* ([جيب](https://en.wiktionary.org/wiki/%D8%AC%D9%8A%D8%A8 "wikt:جيب")), which means 'bosom', 'pocket', or 'fold'.[\[40\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEPlofker2009[httpsbooksgooglecombooksidDHvThPNp9yMCpgPA257_257]-41)[\[41\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMaor1998[httpsbooksgooglecombooksidr9aMrneWFpUCpgPA35_35]-42) When the Arabic texts of [Al-Battani](https://en.wikipedia.org/wiki/Al-Battani "Al-Battani") and [al-Khwārizmī](https://en.wikipedia.org/wiki/Mu%E1%B8%A5ammad_ibn_M%C5%ABs%C4%81_al-Khw%C4%81rizm%C4%AB "Muḥammad ibn Mūsā al-Khwārizmī") were translated into [Medieval Latin](https://en.wikipedia.org/wiki/Medieval_Latin "Medieval Latin") in the 12th century by [Gerard of Cremona](https://en.wikipedia.org/wiki/Gerard_of_Cremona "Gerard of Cremona"), he used the Latin equivalent [*sinus*](https://en.wiktionary.org/wiki/sinus "wikt:sinus") (which also means 'bay' or 'fold', and more specifically 'the hanging fold of a [toga](https://en.wikipedia.org/wiki/Toga "Toga") over the breast').[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43)[\[43\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMaor199835&ndash;36-44)[\[44\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEKatz2008253-45) Gerard was probably not the first scholar to use this translation; Robert of Chester appears to have preceded him and there is evidence of even earlier usage.[\[45\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTESmith1958202-46)[\[46\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-47) The English form *sine* was introduced in [Thomas Fale](https://en.wikipedia.org/wiki/Thomas_Fale "Thomas Fale")'s 1593 *Horologiographia*.[\[47\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-48) The word *cosine* derives from an abbreviation of the Latin *complementi sinus* 'sine of the [complementary angle](https://en.wikipedia.org/wiki/Complementary_angle "Complementary angle")' as *cosinus* in [Edmund Gunter](https://en.wikipedia.org/wiki/Edmund_Gunter "Edmund Gunter")'s *Canon triangulorum* (1620), which also includes a similar definition of *cotangens*.[\[48\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEGunter1620-49) [![](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg/250px-Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg)](https://en.wikipedia.org/wiki/File:Khalili_Collection_Islamic_Art_sci_0040.1_CROP.jpg) Quadrant from 1840s [Ottoman Turkey](https://en.wikipedia.org/wiki/Ottoman_Empire "Ottoman Empire") with axes for looking up the sine and [versine](https://en.wikipedia.org/wiki/Versine "Versine") of angles While the early study of trigonometry can be traced to antiquity, the [trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") as they are in use today were developed in the medieval period. The [chord](https://en.wikipedia.org/wiki/Chord_\(geometry\) "Chord (geometry)") function was discovered by [Hipparchus](https://en.wikipedia.org/wiki/Hipparchus "Hipparchus") of [Nicaea](https://en.wikipedia.org/wiki/%C4%B0znik "İznik") (180–125 BCE) and [Ptolemy](https://en.wikipedia.org/wiki/Ptolemy "Ptolemy") of [Roman Egypt](https://en.wikipedia.org/wiki/Egypt_\(Roman_province\) "Egypt (Roman province)") (90–165 CE).[\[49\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-50) The sine and cosine functions are closely related to the [*jyā* and *koṭi-jyā*](https://en.wikipedia.org/wiki/Jy%C4%81,_koti-jy%C4%81_and_utkrama-jy%C4%81 "Jyā, koti-jyā and utkrama-jyā") functions used in [Indian astronomy](https://en.wikipedia.org/wiki/Indian_astronomy "Indian astronomy") during the [Gupta period](https://en.wikipedia.org/wiki/Gupta_period "Gupta period") (*[Aryabhatiya](https://en.wikipedia.org/wiki/Aryabhatiya "Aryabhatiya")* and *[Surya Siddhanta](https://en.wikipedia.org/wiki/Surya_Siddhanta "Surya Siddhanta")*), via translation from Sanskrit to Arabic and then from Arabic to Latin.[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43)[\[50\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-51) All six trigonometric functions in current use were known in [Islamic mathematics](https://en.wikipedia.org/wiki/Islamic_mathematics "Islamic mathematics") by the 9th century, as was the [law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines"), used in [solving triangles](https://en.wikipedia.org/wiki/Solving_triangles "Solving triangles").[\[51\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Gingerich_1986-52) [Al-Khwārizmī](https://en.wikipedia.org/wiki/Al-Khw%C4%81rizm%C4%AB "Al-Khwārizmī") (c. 780–850) produced tables of sines, cosines and tangents.[\[52\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Sesiano-53)[\[53\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Britannica-54) [Muhammad ibn Jābir al-Harrānī al-Battānī](https://en.wikipedia.org/wiki/Muhammad_ibn_J%C4%81bir_al-Harr%C4%81n%C4%AB_al-Batt%C4%81n%C4%AB "Muhammad ibn Jābir al-Harrānī al-Battānī") (853–929) discovered the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.[\[53\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-Britannica-54) In the early 17th-century, the French mathematician [Albert Girard](https://en.wikipedia.org/wiki/Albert_Girard "Albert Girard") published the first use of the abbreviations *sin*, *cos*, and *tan*; these were further promulgated by Euler (see below). The *Opus palatinum de triangulis* of [Georg Joachim Rheticus](https://en.wikipedia.org/wiki/Georg_Joachim_Rheticus "Georg Joachim Rheticus"), a student of [Copernicus](https://en.wikipedia.org/wiki/Copernicus "Copernicus"), was probably the first in Europe to define trigonometric functions directly in terms of right triangles instead of circles, with tables for all six trigonometric functions; this work was finished by Rheticus' student Valentin Otho in 1596. In a paper published in 1682, [Leibniz](https://en.wikipedia.org/wiki/Gottfried_Leibniz "Gottfried Leibniz") proved that sin *x* is not an [algebraic function](https://en.wikipedia.org/wiki/Algebraic_function "Algebraic function") of *x*.[\[54\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-55) [Roger Cotes](https://en.wikipedia.org/wiki/Roger_Cotes "Roger Cotes") computed the derivative of sine in his *Harmonia Mensurarum* (1722).[\[55\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-56) [Leonhard Euler](https://en.wikipedia.org/wiki/Leonhard_Euler "Leonhard Euler")'s *Introductio in analysin infinitorum* (1748) was mostly responsible for establishing the analytic treatment of trigonometric functions in Europe, also defining them as infinite series and presenting "[Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula")", as well as the near-modern abbreviations *sin.*, *cos.*, *tang.*, *cot.*, *sec.*, and *cosec.*[\[42\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEMerzbachBoyer2011-43) ## Software implementations \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=24 "Edit section: Software implementations")\] There is no standard algorithm for calculating sine and cosine. [IEEE 754](https://en.wikipedia.org/wiki/IEEE_754 "IEEE 754"), the most widely used standard for the specification of reliable floating-point computation, does not address calculating trigonometric functions such as sine. The reason is that no efficient algorithm is known for computing sine and cosine with a specified accuracy, especially for large inputs.[\[56\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-FOOTNOTEZimmermann2006-57) Algorithms for calculating sine may be balanced for such constraints as speed, accuracy, portability, or range of input values accepted. This can lead to different results for different algorithms, especially for special circumstances such as very large inputs, e.g. `sin(1022)`. A common programming optimization, used especially in 3D graphics, is to pre-calculate a table of sine values, for example one value per degree, then for values in-between pick the closest pre-calculated value, or [linearly interpolate](https://en.wikipedia.org/wiki/Linear_interpolation "Linear interpolation") between the 2 closest values to approximate it. This allows results to be looked up from a table rather than being calculated in real time. With modern CPU architectures this method may offer no advantage.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\] The [CORDIC](https://en.wikipedia.org/wiki/CORDIC "CORDIC") algorithm is commonly used in scientific calculators. The sine and cosine functions, along with other trigonometric functions, are widely available across programming languages and platforms. In computing, they are typically abbreviated to `sin` and `cos`. Some CPU architectures have a built-in instruction for sine, including the Intel [x87](https://en.wikipedia.org/wiki/X87 "X87") FPUs since the 80387. In programming languages, `sin` and `cos` are typically either a built-in function or found within the language's standard math library. For example, the [C standard library](https://en.wikipedia.org/wiki/C_standard_library "C standard library") defines sine functions within [math.h](https://en.wikipedia.org/wiki/C_mathematical_functions "C mathematical functions"): `sin(double)`, `sinf(float)`, and `sinl(long double)`. The parameter of each is a [floating point](https://en.wikipedia.org/wiki/Floating_point "Floating point") value, specifying the angle in radians. Each function returns the same [data type](https://en.wikipedia.org/wiki/Data_type "Data type") as it accepts. Many other trigonometric functions are also defined in [math.h](https://en.wikipedia.org/wiki/C_mathematical_functions "C mathematical functions"), such as for cosine, arc sine, and hyperbolic sine (sinh). Similarly, [Python](https://en.wikipedia.org/wiki/Python_\(programming_language\) "Python (programming language)") defines `math.sin(x)` and `math.cos(x)` within the built-in `math` module. Complex sine and cosine functions are also available within the `cmath` module, e.g. `cmath.sin(z)`. [CPython](https://en.wikipedia.org/wiki/CPython "CPython")'s math functions call the [C](https://en.wikipedia.org/wiki/C_\(programming_language\) "C (programming language)") `math` library, and use a [double-precision floating-point format](https://en.wikipedia.org/wiki/Double-precision_floating-point_format "Double-precision floating-point format"). ### Turns based implementations \[[edit](https://en.wikipedia.org/w/index.php?title=Sine_and_cosine&action=edit&section=25 "Edit section: Turns based implementations")\] "sinpi" redirects here. For the township in Pingtung County, Taiwan, see [Xinpi](https://en.wikipedia.org/wiki/Xinpi "Xinpi"). "cospi" redirects here. For the 17th-century Bolognese nobleman, see [Ferdinando Cospi](https://en.wikipedia.org/wiki/Ferdinando_Cospi "Ferdinando Cospi"). Some software libraries provide implementations of sine and cosine using the input angle in half-[turns](https://en.wikipedia.org/wiki/Turn_\(angle\) "Turn (angle)"), a half-turn being an angle of 180 degrees or ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a) radians. Representing angles in turns or half-turns has accuracy advantages and efficiency advantages in some cases.[\[57\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-matlab-58)[\[58\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-r-59) These functions are called `sinpi` and `cospi` in MATLAB,[\[57\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-matlab-58) [OpenCL](https://en.wikipedia.org/wiki/OpenCL "OpenCL"),[\[59\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-60) R,[\[58\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-r-59) Julia,[\[60\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-61) [CUDA](https://en.wikipedia.org/wiki/CUDA "CUDA"),[\[61\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-62) and ARM.[\[62\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-63) For example, `sinpi(x)` would evaluate to ![{\\displaystyle \\sin(\\pi x),}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f4f4681ee034a3d894ce28068c5f6bacfa86e8c5) where *x* is expressed in half-turns, and consequently the final input to the function, *πx* can be interpreted in radians by sin. [SciPy](https://en.wikipedia.org/wiki/SciPy "SciPy") provides similar functions `sindg` and `cosdg` with input in degrees.[\[63\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-64) The accuracy advantage stems from the ability to perfectly represent key angles like full-turn, half-turn, and quarter-turn losslessly in binary floating-point or fixed-point. In contrast, representing ![{\\displaystyle 2\\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/73efd1f6493490b058097060a572606d2c550a06), ![{\\displaystyle \\pi }](https://wikimedia.org/api/rest_v1/media/math/render/svg/9be4ba0bb8df3af72e90a0535fabcc17431e540a), and ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae) in binary floating-point or binary scaled fixed-point always involves a loss of accuracy since irrational numbers cannot be represented with finitely many binary digits. Turns also have an accuracy advantage and efficiency advantage for computing modulo to one period. Computing modulo 1 turn or modulo 2 half-turns can be losslessly and efficiently computed in both floating-point and fixed-point. For example, computing modulo 1 or modulo 2 for a binary point scaled fixed-point value requires only a bit shift or bitwise AND operation. In contrast, computing modulo ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae) involves inaccuracies in representing ![{\\textstyle {\\frac {\\pi }{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/313947d4107765408f902d3eaee6a719e7f01dae). For applications involving angle sensors, the sensor typically provides angle measurements in a form directly compatible with turns or half-turns. For example, an angle sensor may count from 0 to 4096 over one complete revolution.[\[64\]](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_note-65) If half-turns are used as the unit for angle, then the value provided by the sensor directly and losslessly maps to a fixed-point data type with 11 bits to the right of the binary point. In contrast, if radians are used as the unit for storing the angle, then the inaccuracies and cost of multiplying the raw sensor integer by an approximation to ![{\\textstyle {\\frac {\\pi }{2048}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/af6a95707656082f4af5a498fb84cd8a03827286) would be incurred. - [Āryabhaṭa's sine table](https://en.wikipedia.org/wiki/%C4%80ryabha%E1%B9%ADa%27s_sine_table "Āryabhaṭa's sine table") - [Bhaskara I's sine approximation formula](https://en.wikipedia.org/wiki/Bhaskara_I%27s_sine_approximation_formula "Bhaskara I's sine approximation formula") - [Discrete sine transform](https://en.wikipedia.org/wiki/Discrete_sine_transform "Discrete sine transform") - [Dixon elliptic functions](https://en.wikipedia.org/wiki/Dixon_elliptic_functions "Dixon elliptic functions") - [Euler's formula](https://en.wikipedia.org/wiki/Euler%27s_formula "Euler's formula") - [Generalized trigonometry](https://en.wikipedia.org/wiki/Generalized_trigonometry "Generalized trigonometry") - [Hyperbolic function](https://en.wikipedia.org/wiki/Hyperbolic_function "Hyperbolic function") - [Lemniscate elliptic functions](https://en.wikipedia.org/wiki/Lemniscate_elliptic_functions "Lemniscate elliptic functions") - [Law of sines](https://en.wikipedia.org/wiki/Law_of_sines "Law of sines") - [List of periodic functions](https://en.wikipedia.org/wiki/List_of_periodic_functions "List of periodic functions") - [List of trigonometric identities](https://en.wikipedia.org/wiki/List_of_trigonometric_identities "List of trigonometric identities") - [Madhava series](https://en.wikipedia.org/wiki/Madhava_series "Madhava series") - [Madhava's sine table](https://en.wikipedia.org/wiki/Madhava%27s_sine_table "Madhava's sine table") - [Optical sine theorem](https://en.wikipedia.org/wiki/Optical_sine_theorem "Optical sine theorem") - [Polar sine](https://en.wikipedia.org/wiki/Polar_sine "Polar sine")—a generalization to vertex angles - [Proofs of trigonometric identities](https://en.wikipedia.org/wiki/Proofs_of_trigonometric_identities "Proofs of trigonometric identities") - [Sinc function](https://en.wikipedia.org/wiki/Sinc_function "Sinc function") - [Sine and cosine transforms](https://en.wikipedia.org/wiki/Sine_and_cosine_transforms "Sine and cosine transforms") - [Sine integral](https://en.wikipedia.org/wiki/Sine_integral "Sine integral") - [Sine quadrant](https://en.wikipedia.org/wiki/Sine_quadrant "Sine quadrant") - [Sine wave](https://en.wikipedia.org/wiki/Sine_wave "Sine wave") - [Sine–Gordon equation](https://en.wikipedia.org/wiki/Sine%E2%80%93Gordon_equation "Sine–Gordon equation") - [Sinusoidal model](https://en.wikipedia.org/wiki/Sinusoidal_model "Sinusoidal model") - [SOH-CAH-TOA](https://en.wikipedia.org/wiki/Mnemonics_in_trigonometry#SOH-CAH-TOA "Mnemonics in trigonometry") - [Trigonometric functions](https://en.wikipedia.org/wiki/Trigonometric_functions "Trigonometric functions") - [Trigonometric integral](https://en.wikipedia.org/wiki/Trigonometric_integral "Trigonometric integral") 1. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA27_27]_1-2) [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [27](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA27). 2. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA36_36]_2-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [36](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA36). 3. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742_3-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742_3-1) [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 42. 4. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA37_37],_[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA78_78]_4-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [37](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA37), [78](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA78). 5. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]_5-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA634_634]_5-1) [Axler (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAxler2012), p. [634](https://books.google.com/books?id=B5RxDwAAQBAJ&pg=PA634). 6. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAxler2012[httpsbooksgooglecombooksidB5RxDwAAQBAJpgPA632_632]_6-0)** [Axler (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAxler2012), p. [632](https://books.google.com/books?id=B5RxDwAAQBAJ&pg=PA632). 7. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-7)** [Weisstein, Eric W.](https://en.wikipedia.org/wiki/Eric_W._Weisstein "Eric W. Weisstein") ["Cross Product"](https://mathworld.wolfram.com/CrossProduct.html). *[MathWorld](https://en.wikipedia.org/wiki/MathWorld "MathWorld")*. Retrieved 5 June 2025. 8. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-8)** [Weisstein, Eric W.](https://en.wikipedia.org/wiki/Eric_W._Weisstein "Eric W. Weisstein") ["Dot Product"](https://mathworld.wolfram.com/DotProduct.html). *[MathWorld](https://en.wikipedia.org/wiki/MathWorld "MathWorld")*. Retrieved 5 June 2025. 9. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741_9-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41. 10. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA68_68]_10-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [68](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA68). 11. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200747_11-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 47. 12. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741&ndash;42_12-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41–42. 13. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200741,_43_13-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 41, 43. 14. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2012[httpsbooksgooglecombooksidOMrcN0a3LxICpgRA1-PA165_165]_14-0)** [Young (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2012), p. [165](https://books.google.com/books?id=OMrcN0a3LxIC&pg=RA1-PA165). 15. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon200742,_47_15-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 42, 47. 16. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-16)** ["OEIS A003957"](https://oeis.org/A003957). *oeis.org*. Retrieved 2019-05-26. 17. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]_17-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEBourchteinBourchtein2022[httpsbooksgooglecombooksidnGxOEAAAQBAJpgPA294_294]_17-1) [Bourchtein & Bourchtein (2022)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFBourchteinBourchtein2022), p. [294](https://books.google.com/books?id=nGxOEAAAQBAJ&pg=PA294). 18. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007115_18-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 115. 19. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007155_19-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 155. 20. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007157_20-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 157. 21. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007199_21-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 199. 22. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVince2023[httpsbooksgooglecombooksidGnW6EAAAQBAJpgPA162_162]_22-0)** [Vince (2023)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVince2023), p. [162](https://books.google.com/books?id=GnW6EAAAQBAJ&pg=PA162). 23. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAdlaj2012_23-0)** [Adlaj (2012)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAdlaj2012). 24. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-24)** OEIS [sequence A105419 (Decimal expansion of the arc length of the sine or cosine curve for one full period.)](https://oeis.org/A105419) 25. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007365_25-0)** [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 365. 26. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEYoung2017[httpsbooksgooglecombooksid476ZDwAAQBAJpgPA99_99]_26-0)** [Young (2017)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFYoung2017), p. [99](https://books.google.com/books?id=476ZDwAAQBAJ&pg=PA99). 27. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-28)** Dennis G. Zill (2013). *Precalculus with Calculus Previews*. Jones & Bartlett Publishers. p. 238. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4496-4515-1](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4496-4515-1 "Special:BookSources/978-1-4496-4515-1") . [Extract of page 238](https://books.google.com/books?id=dtS5M4lx7scC&pg=PA238) 28. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-29)** ["Sine-squared function"](https://calculus.subwiki.org/wiki/Sine-squared_function#Identities). Retrieved August 9, 2019. 29. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492_30-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEVarbergPurcellRigdon2007491&ndash;492_30-1) [Varberg, Purcell & Rigdon (2007)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFVarbergPurcellRigdon2007), p. 491–492. 30. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]_31-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEAbramowitzStegun1970[httpsbooksgooglecombooksidMtU8uP7XMvoCpgPA74_74]_31-1) [Abramowitz & Stegun (1970)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFAbramowitzStegun1970), p. [74](https://books.google.com/books?id=MtU8uP7XMvoC&pg=PA74). 31. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEPowell1981150_32-0)** [Powell (1981)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFPowell1981), p. 150. 32. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTERudin198788_33-0)** [Rudin (1987)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFRudin1987), p. 88. 33. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEZygmund19681_34-0)** [Zygmund (1968)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFZygmund1968), p. 1. 34. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEZygmund196811_35-0)** [Zygmund (1968)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFZygmund1968), p. 11. 35. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_24]_36-2) [Howie (2003)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFHowie2003), p. [24](https://books.google.com/books?id=0FZDBAAAQBAJ&pg=PA24). 36. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTERudin19872_37-0)** [Rudin (1987)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFRudin1987), p. 2. 37. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-38)** Brown, James Ward; [Churchill, Ruel](https://en.wikipedia.org/wiki/Ruel_Vance_Churchill "Ruel Vance Churchill") (2014). *Complex Variables and Applications* (9th ed.). [McGraw-Hill](https://en.wikipedia.org/wiki/McGraw-Hill "McGraw-Hill"). p. 105. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-07-338317-0](https://en.wikipedia.org/wiki/Special:BookSources/978-0-07-338317-0 "Special:BookSources/978-0-07-338317-0") . 38. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEHowie2003[httpsbooksgooglecombooksid0FZDBAAAQBAJpgPA24_23&ndash;24]_39-0)** [Howie (2003)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFHowie2003), p. [23–24](https://books.google.com/books?id=0FZDBAAAQBAJ&pg=PA24). 39. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-40)** ["Why are the phase portrait of the simple plane pendulum and a domain coloring of sin(z) so similar?"](https://math.stackexchange.com/q/220418). *math.stackexchange.com*. Retrieved 2019-08-12. 40. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEPlofker2009[httpsbooksgooglecombooksidDHvThPNp9yMCpgPA257_257]_41-0)** [Plofker (2009)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFPlofker2009), p. [257](https://books.google.com/books?id=DHvThPNp9yMC&pg=PA257). 41. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMaor1998[httpsbooksgooglecombooksidr9aMrneWFpUCpgPA35_35]_42-0)** [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), p. [35](https://books.google.com/books?id=r9aMrneWFpUC&pg=PA35). 42. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-1) [***c***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMerzbachBoyer2011_43-2) [Merzbach & Boyer (2011)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMerzbachBoyer2011). 43. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEMaor199835&ndash;36_44-0)** [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), p. 35–36. 44. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEKatz2008253_45-0)** [Katz (2008)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFKatz2008), p. 253. 45. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTESmith1958202_46-0)** [Smith (1958)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFSmith1958), p. 202. 46. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-47)** Various sources credit the first use of *sinus* to either - [Plato Tiburtinus](https://en.wikipedia.org/wiki/Plato_Tiburtinus "Plato Tiburtinus")'s 1116 translation of the *Astronomy* of [Al-Battani](https://en.wikipedia.org/wiki/Al-Battani "Al-Battani") - [Gerard of Cremona](https://en.wikipedia.org/wiki/Gerard_of_Cremona "Gerard of Cremona")'s translation of the *Algebra* of [al-Khwārizmī](https://en.wikipedia.org/wiki/Mu%E1%B8%A5ammad_ibn_M%C5%ABs%C4%81_al-Khw%C4%81rizm%C4%AB "Muḥammad ibn Mūsā al-Khwārizmī") - [Robert of Chester](https://en.wikipedia.org/wiki/Robert_of_Chester "Robert of Chester")'s 1145 translation of the tables of al-Khwārizmī See [Merlet (2004)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMerlet2004). See [Maor (1998)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFMaor1998), Chapter 3, for an earlier etymology crediting Gerard. See [Katz (2008)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFKatz2008), p. 210. 47. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-48)** Fale's book alternately uses the spellings "sine", "signe", or "sign". Fale, Thomas (1593). [*Horologiographia. The Art of Dialling: Teaching, an Easie and Perfect Way to make all Kindes of Dials ...*](https://archive.org/details/b30333106/page/19/mode/1up) London: F. Kingston. p. 11, for example. 48. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEGunter1620_49-0)** [Gunter (1620)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFGunter1620). 49. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-50)** Brendan, T. (February 1965). "How Ptolemy constructed trigonometry tables". *The Mathematics Teacher*. **58** (2): 141–149\. [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.5951/MT.58.2.0141](https://doi.org/10.5951%2FMT.58.2.0141). [JSTOR](https://en.wikipedia.org/wiki/JSTOR_\(identifier\) "JSTOR (identifier)") [27967990](https://www.jstor.org/stable/27967990). 50. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-51)** [Van Brummelen, Glen](https://en.wikipedia.org/wiki/Glen_Van_Brummelen "Glen Van Brummelen") (2009). "India". *The Mathematics of the Heavens and the Earth*. Princeton University Press. Ch. 3, pp. 94–134. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-691-12973-0](https://en.wikipedia.org/wiki/Special:BookSources/978-0-691-12973-0 "Special:BookSources/978-0-691-12973-0") . 51. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Gingerich_1986_52-0)** Gingerich, Owen (1986). ["Islamic Astronomy"](https://web.archive.org/web/20131019140821/http://faculty.kfupm.edu.sa/PHYS/alshukri/PHYS215/Islamic_astronomy.htm). *[Scientific American](https://en.wikipedia.org/wiki/Scientific_American "Scientific American")*. Vol. 254. p. 74. Archived from [the original](http://faculty.kfupm.edu.sa/PHYS/alshukri/PHYS215/Islamic_astronomy.htm) on 2013-10-19. Retrieved 2010-07-13. 52. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Sesiano_53-0)** Jacques Sesiano, "Islamic mathematics", p. 157, in [Selin, Helaine](https://en.wikipedia.org/wiki/Helaine_Selin "Helaine Selin"); [D'Ambrosio, Ubiratan](https://en.wikipedia.org/wiki/Ubiratan_D%27Ambrosio "Ubiratan D'Ambrosio"), eds. (2000). *Mathematics Across Cultures: The History of Non-western Mathematics*. [Springer Science+Business Media](https://en.wikipedia.org/wiki/Springer_Science%2BBusiness_Media "Springer Science+Business Media"). [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4020-0260-1](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4020-0260-1 "Special:BookSources/978-1-4020-0260-1") . 53. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Britannica_54-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-Britannica_54-1) ["trigonometry"](http://www.britannica.com/EBchecked/topic/605281/trigonometry). Encyclopedia Britannica. 17 June 2024. 54. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-55)** Nicolás Bourbaki (1994). [*Elements of the History of Mathematics*](https://archive.org/details/elementsofhistor0000bour). Springer. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [9783540647676](https://en.wikipedia.org/wiki/Special:BookSources/9783540647676 "Special:BookSources/9783540647676") . 55. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-56)** "[Why the sine has a simple derivative](http://www.math.usma.edu/people/rickey/hm/CalcNotes/Sine-Deriv.pdf) [Archived](https://web.archive.org/web/20110720102700/http://www.math.usma.edu/people/rickey/hm/CalcNotes/Sine-Deriv.pdf) 2011-07-20 at the [Wayback Machine](https://en.wikipedia.org/wiki/Wayback_Machine "Wayback Machine")", in *[Historical Notes for Calculus Teachers](http://www.math.usma.edu/people/rickey/hm/CalcNotes/default.htm) [Archived](https://web.archive.org/web/20110720102613/http://www.math.usma.edu/people/rickey/hm/CalcNotes/default.htm) 2011-07-20 at the [Wayback Machine](https://en.wikipedia.org/wiki/Wayback_Machine "Wayback Machine")* by [V. Frederick Rickey](http://www.math.usma.edu/people/rickey/) [Archived](https://web.archive.org/web/20110720102654/http://www.math.usma.edu/people/rickey/) 2011-07-20 at the [Wayback Machine](https://en.wikipedia.org/wiki/Wayback_Machine "Wayback Machine") 56. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-FOOTNOTEZimmermann2006_57-0)** [Zimmermann (2006)](https://en.wikipedia.org/wiki/Sine_and_cosine#CITEREFZimmermann2006). 57. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-matlab_58-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-matlab_58-1) ["sinpi - Compute sin(X\*pi) accurately"](https://www.mathworks.com/help/matlab/ref/double.sinpi.html). *www.mathworks.com*. [Archived](http://web.archive.org/web/20251123002724/https://www.mathworks.com/help/matlab/ref/double.sinpi.html) from the original on 2025-11-23. Retrieved 2026-01-08. 58. ^ [***a***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-r_59-0) [***b***](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-r_59-1) ["Trig function - RDocumentation"](https://www.rdocumentation.org/packages/base/versions/3.5.3/topics/Trig). *www.rdocumentation.org*. Retrieved 2026-02-17. 59. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-60)** ["sin, sincos, sinh, sinpi"](https://registry.khronos.org/OpenCL/sdk/1.0/docs/man/xhtml/sin.html). *registry.khronos.org*. Retrieved 2026-02-17. 60. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-61)** ["sinpi » Julia Functions"](http://www.jlhub.com/julia/manual/en/function/sinpi). *www.jlhub.com*. Retrieved 2026-02-17. 61. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-62)** ["Double Precision Mathematical Functions"](http://web.archive.org/web/20240723062728/https://docs.nvidia.com/cuda/cuda-math-api/group__CUDA__MATH__DOUBLE.html). *docs.nvidia.com*. Archived from [the original](https://docs.nvidia.com/cuda/cuda-math-api/group__CUDA__MATH__DOUBLE.html) on 2024-07-23. Retrieved 2026-01-08. 62. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-63)** ["Documentation – Arm Developer"](https://developer.arm.com/documentation/100614/latest/b-opencl-built-in-functions/b2-math-functions). *developer.arm.com*. Retrieved 2026-02-17. 63. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-64)** ["Special functions (scipy.special) — SciPy v1.17.0 Manual"](https://docs.scipy.org/doc/scipy/reference/special.html#convenience-functions). *docs.scipy.org*. Retrieved 25 February 2026. 64. **[^](https://en.wikipedia.org/wiki/Sine_and_cosine#cite_ref-65)** ["AAS33051: Precision Angle Sensor IC with Incremental and Motor Commutation Outputs and On-Chip Linearization"](http://web.archive.org/web/20190417143715/https://www.allegromicro.com/en/Products/Magnetic-Linear-And-Angular-Position-Sensor-ICs/Angular-Position-Sensor-ICs/AAS33051.aspx). *www.allegromicro.com*. Archived from [the original](https://www.allegromicro.com/en/Products/Magnetic-Linear-And-Angular-Position-Sensor-ICs/Angular-Position-Sensor-ICs/AAS33051.aspx) on 2019-04-17. Retrieved 2026-02-17. - [Abramowitz, Milton](https://en.wikipedia.org/wiki/Milton_Abramowitz "Milton Abramowitz"); [Stegun, Irene A.](https://en.wikipedia.org/wiki/Irene_Stegun "Irene Stegun") (1970), *[Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables](https://en.wikipedia.org/wiki/Abramowitz_and_Stegun "Abramowitz and Stegun")*, New York: [Dover Publications](https://en.wikipedia.org/wiki/Dover_Publications "Dover Publications"), Ninth printing - Adlaj, Semjon (2012), ["An Eloquent Formula for the Perimeter of an Ellipse"](https://www.ams.org/notices/201208/rtx120801094p.pdf) (PDF), *American Mathematical Society*, **59** (8): 1097 - Axler, Sheldon (2012), *Algebra and Trigonometry*, [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0470-58579-5](https://en.wikipedia.org/wiki/Special:BookSources/978-0470-58579-5 "Special:BookSources/978-0470-58579-5") - [Bourchtein, Ludmila](https://en.wikipedia.org/wiki/Ludmila_Bourchtein "Ludmila Bourchtein"); Bourchtein, Andrei (2022), *Theory of Infinite Sequences and Series*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-3-030-79431-6](https://doi.org/10.1007%2F978-3-030-79431-6), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-3-030-79431-6](https://en.wikipedia.org/wiki/Special:BookSources/978-3-030-79431-6 "Special:BookSources/978-3-030-79431-6") - [Gunter, Edmund](https://en.wikipedia.org/wiki/Edmund_Gunter "Edmund Gunter") (1620), *Canon triangulorum* - Howie, John M. (2003), *Complex Analysis*, Springer Undergraduate Mathematics Series, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-1-4471-0027-0](https://doi.org/10.1007%2F978-1-4471-0027-0), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4471-0027-0](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4471-0027-0 "Special:BookSources/978-1-4471-0027-0") - Traupman, Ph.D., John C. (1966), [*The New College Latin & English Dictionary*](https://archive.org/details/boysgirlsbookabo00gard_0), Toronto: Bantam, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [0-553-27619-0](https://en.wikipedia.org/wiki/Special:BookSources/0-553-27619-0 "Special:BookSources/0-553-27619-0") - Katz, Victor J. (2008), [*A History of Mathematics*](http://deti-bilingual.com/wp-content/uploads/2014/06/3rd-Edition-Victor-J.-Katz-A-History-of-Mathematics-Pearson-2008.pdf) (PDF) (3rd ed.), Boston: Addison-Wesley, "The English word "sine" comes from a series of mistranslations of the Sanskrit *jyā-ardha* (chord-half). Āryabhaṭa frequently abbreviated this term to *jyā* or its synonym *jīvá*. When some of the Hindu works were later translated into Arabic, the word was simply transcribed phonetically into an otherwise meaningless Arabic word *jiba*. But since Arabic is written without vowels, later writers interpreted the consonants *jb* as *jaib*, which means bosom or breast. In the twelfth century, when an Arabic trigonometry work was translated into Latin, the translator used the equivalent Latin word *sinus*, which also meant bosom, and by extension, fold (as in a toga over a breast), or a bay or gulf." - Maor, Eli (1998), *Trigonometric Delights*, [Princeton University Press](https://en.wikipedia.org/wiki/Princeton_University_Press "Princeton University Press"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [1-4008-4282-4](https://en.wikipedia.org/wiki/Special:BookSources/1-4008-4282-4 "Special:BookSources/1-4008-4282-4") - Merlet, Jean-Pierre (2004), "A Note on the History of the Trigonometric Functions", in Ceccarelli, Marco (ed.), *International Symposium on History of Machines and Mechanisms*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/1-4020-2204-2](https://doi.org/10.1007%2F1-4020-2204-2), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-4020-2203-6](https://en.wikipedia.org/wiki/Special:BookSources/978-1-4020-2203-6 "Special:BookSources/978-1-4020-2203-6") - [Merzbach, Uta C.](https://en.wikipedia.org/wiki/Uta_Merzbach "Uta Merzbach"); [Boyer, Carl B.](https://en.wikipedia.org/wiki/Carl_B._Boyer "Carl B. Boyer") (2011), *A History of Mathematics* (3rd ed.), [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"), "It was Robert of Chester's translation from Arabic that resulted in our word "sine". The Hindus had given the name jiva to the half-chord in trigonometry, and the Arabs had taken this over as jiba. In the Arabic language, there is also the word jaib meaning "bay" or "inlet". When Robert of Chester came to translate the technical word jiba, he seems to have confused this with the word jaib (perhaps because vowels were omitted); hence, he used the word sinus, the Latin word for "bay" or "inlet"." - Plofker (2009), [*Mathematics in India*](https://en.wikipedia.org/wiki/Mathematics_in_India_\(book\) "Mathematics in India (book)"), [Princeton University Press](https://en.wikipedia.org/wiki/Princeton_University_Press "Princeton University Press") - [Powell, Michael J. D.](https://en.wikipedia.org/wiki/Michael_J._D._Powell "Michael J. D. Powell") (1981), *Approximation Theory and Methods*, [Cambridge University Press](https://en.wikipedia.org/wiki/Cambridge_University_Press "Cambridge University Press"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-521-29514-7](https://en.wikipedia.org/wiki/Special:BookSources/978-0-521-29514-7 "Special:BookSources/978-0-521-29514-7") - [Rudin, Walter](https://en.wikipedia.org/wiki/Walter_Rudin "Walter Rudin") (1987), *Real and complex analysis* (3rd ed.), New York: [McGraw-Hill](https://en.wikipedia.org/wiki/McGraw-Hill "McGraw-Hill"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0-07-054234-1](https://en.wikipedia.org/wiki/Special:BookSources/978-0-07-054234-1 "Special:BookSources/978-0-07-054234-1") , [MR](https://en.wikipedia.org/wiki/MR_\(identifier\) "MR (identifier)") [0924157](https://mathscinet.ams.org/mathscinet-getitem?mr=0924157) - Smith, D. E. (1958) \[1925\], *History of Mathematics*, vol. I, [Dover Publications](https://en.wikipedia.org/wiki/Dover_Publications "Dover Publications"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [0-486-20429-4](https://en.wikipedia.org/wiki/Special:BookSources/0-486-20429-4 "Special:BookSources/0-486-20429-4") - Varberg, Dale E.; Purcell, Edwin J.; Rigdon, Steven E. (2007), [*Calculus*](https://archive.org/details/matematika-a-purcell-calculus-9th-ed/mode/2up) (9th ed.), [Pearson Prentice Hall](https://en.wikipedia.org/wiki/Pearson_Prentice_Hall "Pearson Prentice Hall"), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-0131469686](https://en.wikipedia.org/wiki/Special:BookSources/978-0131469686 "Special:BookSources/978-0131469686") - Vince, John (2023), *Calculus for Computer Graphics*, Springer, [doi](https://en.wikipedia.org/wiki/Doi_\(identifier\) "Doi (identifier)"):[10\.1007/978-3-031-28117-4](https://doi.org/10.1007%2F978-3-031-28117-4), [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-3-031-28117-4](https://en.wikipedia.org/wiki/Special:BookSources/978-3-031-28117-4 "Special:BookSources/978-3-031-28117-4") - [Young, Cynthia](https://en.wikipedia.org/wiki/Cynthia_Y._Young "Cynthia Y. Young") (2012), *Trigonometry* (3rd ed.), John Wiley & Sons, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-119-32113-2](https://en.wikipedia.org/wiki/Special:BookSources/978-1-119-32113-2 "Special:BookSources/978-1-119-32113-2") - ——— (2017), *Trigonometry* (4th ed.), John Wiley & Sons, [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)") [978-1-119-32113-2](https://en.wikipedia.org/wiki/Special:BookSources/978-1-119-32113-2 "Special:BookSources/978-1-119-32113-2") - Zimmermann, Paul (2006), "Can we trust floating-point numbers?", [*Grand Challenges of Informatics*](http://www.jaist.ac.jp/~bjorner/ae-is-budapest/talks/Sept20pm2_Zimmermann.pdf) (PDF), p. 14/31 - [Zygmund, Antoni](https://en.wikipedia.org/wiki/Antoni_Zygmund "Antoni Zygmund") (1968), [*Trigonometric Series*](https://archive.org/details/trigonometricser0012azyg/) (2nd, reprinted ed.), [Cambridge University Press](https://en.wikipedia.org/wiki/Cambridge_University_Press "Cambridge University Press"), [MR](https://en.wikipedia.org/wiki/MR_\(identifier\) "MR (identifier)") [0236587](https://mathscinet.ams.org/mathscinet-getitem?mr=0236587) [![Wiktionary logo](https://upload.wikimedia.org/wikipedia/commons/thumb/9/99/Wiktionary-logo-en-v2.svg/40px-Wiktionary-logo-en-v2.svg.png)](https://en.wikipedia.org/wiki/File:Wiktionary-logo-en-v2.svg) Look up ***[sine](https://en.wiktionary.org/wiki/sine "wiktionary:sine")*** in Wiktionary, the free dictionary. - [![Wikimedia Commons logo](https://upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/20px-Commons-logo.svg.png)](https://en.wikipedia.org/wiki/File:Commons-logo.svg) Media related to [Sine function](https://commons.wikimedia.org/wiki/Category:Sine_function "commons:Category:Sine function") at Wikimedia Commons
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