Trigonometric functions
Trigonometry 


Reference 
Laws and theorems 
Calculus 
In mathematics, the trigonometric functions (also called the circular functions) are functions of an angle. They relate the angles of a triangle to the lengths of its sides. Trigonometric functions are important in the study of triangles and modeling periodic phenomena, among many other applications.
The most familiar trigonometric functions are the sine, cosine, and tangent. In the context of the standard unit circle (a circle with radius 1 unit), where a triangle is formed by a ray originating at the origin and making some angle with the xaxis, the sine of the angle gives the length of the ycomponent (the opposite to the angle or the rise) of the triangle, the cosine gives the length of the xcomponent (the adjacent of the angle or the run), and the tangent function gives the slope (ycomponent divided by the xcomponent). More precise definitions are detailed below. Trigonometric functions are commonly defined as ratios of two sides of a right triangle containing the angle, and can equivalently be defined as the lengths of various line segments from a unit circle. More modern definitions express them as infinite series or as solutions of certain differential equations, allowing their extension to arbitrary positive and negative values and even to complex numbers.
Trigonometric functions have a wide range of uses including computing unknown lengths and angles in triangles (often right triangles). In this use, trigonometric functions are used, for instance, in navigation, engineering, and physics. A common use in elementary physics is resolving a vector into Cartesian coordinates. The sine and cosine functions are also commonly used to model periodic function phenomena such as sound and light waves, the position and velocity of harmonic oscillators, sunlight intensity and day length, and average temperature variations through the year.
In modern usage, there are six basic trigonometric functions, tabulated here with equations that relate them to one another. Especially with the last four, these relations are often taken as the definitions of those functions, but one can define them equally well geometrically, or by other means, and then derive these relations.
Contents
Rightangled triangle definitions
The notion that there should be some standard correspondence between the lengths of the sides of a triangle and the angles of the triangle comes as soon as one recognizes that similar triangles maintain the same ratios between their sides. That is, for any similar triangle the ratio of the hypotenuse (for example) and another of the sides remains the same. If the hypotenuse is twice as long, so are the sides. It is these ratios that the trigonometric functions express.
To define the trigonometric functions for the angle A, start with any right triangle that contains the angle A. The three sides of the triangle are named as follows:
 The hypotenuse is the side opposite the right angle, in this case side h. The hypotenuse is always the longest side of a rightangled triangle.
 The opposite side is the side opposite to the angle we are interested in (angle A), in this case side a.
 The adjacent side is the side having both the angles of interest (angle A and rightangle C), in this case side b.
In ordinary Euclidean geometry, according to the triangle postulate, the inside angles of every triangle total 180° (π radians). Therefore, in a rightangled triangle, the two nonright angles total 90° (π/2 radians), so each of these angles must be in the range of (0°,90°) as expressed in interval notation. The following definitions apply to angles in this 0° – 90° range. They can be extended to the full set of real arguments by using the unit circle, or by requiring certain symmetries and that they be periodic functions. For example, the figure shows sin(θ) for angles θ, π − θ, π + θ, and 2π − θ depicted on the unit circle (top) and as a graph (bottom). The value of the sine repeats itself apart from sign in all four quadrants, and if the range of θ is extended to additional rotations, this behavior repeats periodically with a period 2π.
The trigonometric functions are summarized in the following table and described in more detail below. The angle θ is the angle between the hypotenuse and the adjacent line – the angle at A in the accompanying diagram.
Function  Abbreviation  Description  Identities (using radians) 

sine  sin  opposite / hypotenuse  
cosine  cos  adjacent / hypotenuse  
tangent  tan (or tg)  opposite / adjacent  
cotangent  cot (or cotan or cotg or ctg or ctn)  adjacent / opposite  
secant  sec  hypotenuse / adjacent  
cosecant  csc (or cosec)  hypotenuse / opposite 
Sine, cosine and tangent
The sine of an angle is the ratio of the length of the opposite side to the length of the hypotenuse. (The word comes from the Latin sinus for gulf or bay,^{[1]} since, given a unit circle, it is the side of the triangle on which the angle opens.) In our case
This ratio does not depend on the size of the particular right triangle chosen, as long as it contains the angle A, since all such triangles are similar.
The cosine of an angle is the ratio of the length of the adjacent side to the length of the hypotenuse: so called because it is the sine of the complementary or coangle.^{[2]} In our case
The tangent of an angle is the ratio of the length of the opposite side to the length of the adjacent side: so called because it can be represented as a line segment tangent to the circle, that is the line that touches the circle, from Latin linea tangens or touching line (cf. tangere, to touch).^{[3]} In our case
The acronyms "SOHCAHTOA" ("Soakatoe", "Sockatoa", "Sokahtoa") and "OHSAHCOAT" are commonly used mnemonics for these ratios.
Reciprocal functions
The remaining three functions are best defined using the above three functions.
The cosecant csc(A), or cosec(A), is the reciprocal of sin(A); i.e. the ratio of the length of the hypotenuse to the length of the opposite side; so called because it is the secant of the complementary or coangle:
The secant sec(A) is the reciprocal of cos(A); i.e. the ratio of the length of the hypotenuse to the length of the adjacent side:
It is so called because it represents the line that cuts the circle (from Latin: secare, to cut).^{[4]}
The cotangent cot(A) is the reciprocal of tan(A); i.e. the ratio of the length of the adjacent side to the length of the opposite side; so called because it is the tangent of the complementary or coangle:
Slope definitions
Equivalent to the righttriangle definitions, the trigonometric functions can also be defined in terms of the rise, run, and slope of a line segment relative to horizontal. The slope is commonly taught as "rise over run" or ^{rise}⁄_{run}. The three main trigonometric functions are commonly taught in the order sine, cosine, tangent. With a line segment length of 1 (as in a unit circle), the following mnemonic devices show the correspondence of definitions:
 "Sine is first, rise is first" meaning that Sine takes the angle of the line segment and tells its vertical rise when the length of the line is 1.
 "Cosine is second, run is second" meaning that Cosine takes the angle of the line segment and tells its horizontal run when the length of the line is 1.
 "Tangent combines the rise and run" meaning that Tangent takes the angle of the line segment and tells its slope; or alternatively, tells the vertical rise when the line segment's horizontal run is 1.
This shows the main use of tangent and arctangent: converting between the two ways of telling the slant of a line, i.e., angles and slopes. (The arctangent or "inverse tangent" is not to be confused with the cotangent, which is cosine divided by sine.)
While the length of the line segment makes no difference for the slope (the slope does not depend on the length of the slanted line), it does affect rise and run. To adjust and find the actual rise and run when the line does not have a length of 1, just multiply the sine and cosine by the line length. For instance, if the line segment has length 5, the run at an angle of 7° is 5 cos(7°)
Unitcircle definitions
The six trigonometric functions can also be defined in terms of the unit circle, the circle of radius one centered at the origin. The unit circle relies on right triangles for most angles.
The unit circle definition does, however, permit the definition of the trigonometric functions for all positive and negative arguments, not just for angles between 0 and π/2 radians.
From the Pythagorean theorem the equation for the unit circle is
Let a line through the origin, making an angle of θ with the positive half of the xaxis. The line intersects the unit circle at a point P whose x and ycoordinates are cos(θ) and sin(θ)
Let us consider the right triangle whose vertexes are the point P, the center of the circle O, and the point H of the xaxis, that has the same xcoordinate as P. The radius of the circle is equal to the hypotenuse OP, and has length 1, so we have sin(θ) = y/1 and cos(θ) = x/1. The unit circle can be thought of as a way of looking at an infinite number of triangles by varying the lengths of their legs but keeping the lengths of their hypotenuses equal to 1.
For angles greater than 2π or less than −2π, one simply continues to rotate around the circle; sine and cosine are periodic functions with period 2π:
for any angle θ and any integer k.
The smallest positive period of a periodic function is called the primitive period of the function.
The primitive period of the sine or cosine is a full circle, i.e. 2π radians or 360° degrees.
Above, only sine and cosine were defined directly by the unit circle, but other trigonometric functions can be defined by:
So :
 The primitive period of the secant, or cosecant is also a full circle, i.e. 2π radians or 360° degrees.
 The primitive period of the tangent or cotangent is only a halfcircle, i.e. π radians or 180° degrees.
The image at right includes a graph of the tangent function.
 Its θintercepts correspond to those of sin(θ) while its undefined values correspond to the θintercepts of cos(θ).
 The function changes slowly around angles of kπ, but changes rapidly at angles close to (k + 1/2)π.
 The graph of the tangent function also has a vertical asymptote at θ = (k + 1/2)π, the θintercepts of the cosine function, because the function approaches infinity as θ approaches (k + 1/2)π from the left and minus infinity as it approaches (k + 1/2)π from the right.
Alternatively, all of the basic trigonometric functions can be defined in terms of a unit circle centered at O (as shown in the picture to the right), and similar such geometric definitions were used historically.
 In particular, for a chord AB of the circle, where θ is half of the subtended angle, sin(θ) is AC (half of the chord), a definition introduced in India^{[6]} (see history).
 cos(θ) is the horizontal distance OC, and versin(θ) = 1 − cos(θ) is CD.
 tan(θ) is the length of the segment AE of the tangent line through A, hence the word tangent for this function. cot(θ) is another tangent segment, AF.
 sec(θ) = OE and csc(θ) = OF are segments of secant lines (intersecting the circle at two points), and can also be viewed as projections of OA along the tangent at A to the horizontal and vertical axes, respectively.
 DE is exsec(θ) = sec(θ) − 1 (the portion of the secant outside, or ex, the circle).
 From these constructions, it is easy to see that the secant and tangent functions diverge as θ approaches π/2 (90° degrees) and that the cosecant and cotangent diverge as θ approaches zero. (Many similar constructions are possible, and the basic trigonometric identities can also be proven graphically.^{[7]})
Algebraic values
The algebraic expressions for sin(0°), sin(30°), sin(45°), sin(60°) and sin(90°) are
respectively. Such simple expressions generally do not exist for other angles.
For an angle, which, measured in degrees, is a multiple of three, the sine and the cosine may be expressed in terms of square roots, as shown below. These values of the sine and the cosine may thus be constructed by ruler and compass.
For an angle of an integer number of degrees, the sine and the cosine may be expressed in terms of square roots and the cube root of a nonreal complex number. Galois theory allows to prove that, if the angle is not a multiple of 3°, nonreal cube roots are unavoidable.
For an angle, which, measured in degrees, is a rational number, the sine and the cosine are algebraic numbers, which may be expressed in terms of nth roots. This results from the fact that the Galois groups of the cyclotomic polynomials are cyclic.
For an angle, which, measured in degrees, is not a rational number, then either the angle or both the sine and the cosine are transcendental numbers. This is a corollary of Baker's theorem, proved in 1966.
Explicit values
Algebraic expressions for 15°, 18°, 36°, 54°, 72° and 75° are as follows:^{[citation needed]}
From these, the algebraic expressions for all multiples of 3° can be computed. For example:^{[citation needed]}
Algebraic expressions can be deduced for other angles of an integer number of degrees, for example,
where z = a + ib, and a and b are the above algebraic expressions for, respectively, cos 3° and sin 3°, and the principal cube root (that is the cube root with the largest real part) is to be taken.
Series definitions
Trigonometric functions are analytic functions. Using only geometry and properties of limits, it can be shown that the derivative of sine is cosine and the derivative of cosine is the negative of sine. (Here, and generally in calculus, all angles are measured in radians; see also the significance of radians below.) One can then use the theory of Taylor series to show that the following identities hold for all real numbers x:^{[8]}
The infinite series appearing in these identities are convergent in the whole complex plane and are often taken as the definitions of the sine and cosine functions of a complex variable. Another standard (and equivalent) definition of the sine and the cosine as functions of a complex variable is through their differential equation, below.
Other series can be found.^{[9]} For the following trigonometric functions:
 U_{n} is the nth up/down number,
 B_{n} is the nth Bernoulli number, and
 E_{n} (below) is the nth Euler number.
Tangent
When this series for the tangent function is expressed in a form in which the denominators are the corresponding factorials, the numerators, called the "tangent numbers", have a combinatorial interpretation: they enumerate alternating permutations of finite sets of odd cardinality.^{[10]} The series itself can be found by a power series solution of the aforementioned differential equation.
Cosecant
Secant
When this series for the secant function is expressed in a form in which the denominators are the corresponding factorials, the numerators, called the "secant numbers", have a combinatorial interpretation: they enumerate alternating permutations of finite sets of even cardinality.^{[11]}
Cotangent
From a theorem in complex analysis, there is a unique analytic continuation of this real function to the domain of complex numbers. They have the same Taylor series, and so the trigonometric functions are defined on the complex numbers using the Taylor series above.
There is a series representation as partial fraction expansion where just translated reciprocal functions are summed up, such that the poles of the cotangent function and the reciprocal functions match:^{[12]}
This identity can be proven with the Herglotz trick.^{[13]} Combining the (–n)th with the nth term lead to absolutely convergent series:
Relationship to exponential function and complex numbers
It can be shown from the series definitions^{[14]} that the sine and cosine functions are respectively the imaginary and real parts of the exponential function of a purely imaginary argument. That is, if x is real, we have
and
The latter identity remains valid for a nonreal x, and is called Euler's formula.
Euler's formula can be used to derive most trigonometric identities from the properties of the exponential function, by writing sine and cosine as:
It is also sometimes useful to express the complex sine and cosine functions in terms of the real and imaginary parts of their arguments.
This exhibits a deep relationship between the complex sine and cosine functions and their real (sin, cos) and hyperbolic real (sinh, cosh) counterparts.
Complex graphs
In the following graphs, the domain is the complex plane pictured, and the range values are indicated at each point by color. Brightness indicates the size (absolute value) of the range value, with black being zero. Hue varies with argument, or angle, measured from the positive real axis. (more)
Definitions via differential equations
Both the sine and cosine functions satisfy the differential equation:
That is to say, each is the additive inverse of its own second derivative. Within the 2dimensional function space V consisting of all solutions of this equation,
 the sine function is the unique solution satisfying the initial condition and
 the cosine function is the unique solution satisfying the initial condition .
Since the sine and cosine functions are linearly independent, together they form a basis of V. This method of defining the sine and cosine functions is essentially equivalent to using Euler's formula. (See linear differential equation.) It turns out that this differential equation can be used not only to define the sine and cosine functions but also to prove the trigonometric identities for the sine and cosine functions.
Further, the observation that sine and cosine satisfies y′′ = −y means that they are eigenfunctions of the secondderivative operator.
The tangent function is the unique solution of the nonlinear differential equation
satisfying the initial condition y(0) = 0. There is a very interesting visual proof that the tangent function satisfies this differential equation.^{[15]}
The significance of radians
Radians specify an angle by measuring the length around the path of the unit circle and constitute a special argument to the sine and cosine functions. In particular, only sines and cosines that map radians to ratios satisfy the differential equations that classically describe them. If an argument to sine or cosine in radians is scaled by frequency,
then the derivatives will scale by amplitude.
Here, k is a constant that represents a mapping between units. If x is in degrees, then
This means that the second derivative of a sine in degrees does not satisfy the differential equation
but rather
The cosine's second derivative behaves similarly.
This means that these sines and cosines are different functions, and that the fourth derivative of sine will be sine again only if the argument is in radians.
Identities
Many identities interrelate the trigonometric functions. Among the most frequently used is the Pythagorean identity, which states that for any angle, the square of the sine plus the square of the cosine is 1. This is easy to see by studying a right triangle of hypotenuse 1 and applying the Pythagorean theorem. In symbolic form, the Pythagorean identity is written
where is standard notation for
Other key relationships are the sum and difference formulas, which give the sine and cosine of the sum and difference of two angles in terms of sines and cosines of the angles themselves. These can be derived geometrically, using arguments that date to Ptolemy. One can also produce them algebraically using Euler's formula.
 Sum
 Difference
These in turn lead to the following threeangle formulae:
When the two angles are equal, the sum formulas reduce to simpler equations known as the doubleangle formulae.
When three angles are equal, the threeangle formulae simplify to
These identities can also be used to derive the producttosum identities that were used in antiquity to transform the product of two numbers into a sum of numbers and greatly speed operations, much like the logarithm function.
Calculus
For integrals and derivatives of trigonometric functions, see the relevant sections of Differentiation of trigonometric functions, Lists of integrals and List of integrals of trigonometric functions. Below is the list of the derivatives and integrals of the six basic trigonometric functions. The number C is a constant of integration.
Definitions using functional equations
In mathematical analysis, one can define the trigonometric functions using functional equations based on properties like the difference formula. Taking as given these formulas, one can prove that only two real functions satisfy those conditions. Symbolically, we say that there exists exactly one pair of real functions — and — such that for all real numbers and , the following equation hold:^{[16]}
with the added condition that
Other derivations, starting from other functional equations, are also possible, and such derivations can be extended to the complex numbers. As an example, this derivation can be used to define trigonometry in Galois fields.
Computation
The computation of trigonometric functions is a complicated subject, which can today be avoided by most people because of the widespread availability of computers and scientific calculators that provide builtin trigonometric functions for any angle. This section, however, describes details of their computation in three important contexts: the historical use of trigonometric tables, the modern techniques used by computers, and a few "important" angles where simple exact values are easily found.
The first step in computing any trigonometric function is range reduction—reducing the given angle to a "reduced angle" inside a small range of angles, say 0 to π/2, using the periodicity and symmetries of the trigonometric functions.
Prior to computers, people typically evaluated trigonometric functions by interpolating from a detailed table of their values, calculated to many significant figures. Such tables have been available for as long as trigonometric functions have been described (see History below), and were typically generated by repeated application of the halfangle and angleaddition identities starting from a known value (such as sin(π/2) = 1).
Modern computers use a variety of techniques.^{[17]} One common method, especially on higherend processors with floating point units, is to combine a polynomial or rational approximation (such as Chebyshev approximation, best uniform approximation, and Padé approximation, and typically for higher or variable precisions, Taylor and Laurent series) with range reduction and a table lookup—they first look up the closest angle in a small table, and then use the polynomial to compute the correction.^{[18]} Devices that lack hardware multipliers often use an algorithm called CORDIC (as well as related techniques), which uses only addition, subtraction, bitshift, and table lookup. These methods are commonly implemented in hardware floatingpoint units for performance reasons.
For very high precision calculations, when series expansion convergence becomes too slow, trigonometric functions can be approximated by the arithmeticgeometric mean, which itself approximates the trigonometric function by the (complex) elliptic integral.^{[19]}
Finally, for some simple angles, the values can be easily computed by hand using the Pythagorean theorem, as in the following examples. For example, the sine, cosine and tangent of any integer multiple of radians (3°) can be found exactly by hand.
Consider a right triangle where the two other angles are equal, and therefore are both radians (45°). Then the length of side b and the length of side a are equal; we can choose . The values of sine, cosine and tangent of an angle of radians (45°) can then be found using the Pythagorean theorem:
Therefore:
To determine the trigonometric functions for angles of π/3 radians (60 degrees) and π/6 radians (30 degrees), we start with an equilateral triangle of side length 1. All its angles are π/3 radians (60 degrees). By dividing it into two, we obtain a right triangle with π/6 radians (30 degrees) and π/3 radians (60 degrees) angles. For this triangle, the shortest side = 1/2, the next largest side =(√3)/2 and the hypotenuse = 1. This yields:
Special values in trigonometric functions
There are some commonly used special values in trigonometric functions, as shown in the following table.
Function  

sin  
cos  
tan  ^{[20]}  
cot  ^{[20]}  
sec  ^{[20]}  
csc  ^{[20]} 
The symbol here represents the point at infinity on the real projective line, the limit on the extended real line is on one side and on the other.
Inverse functions
The trigonometric functions are periodic, and hence not injective, so strictly they do not have an inverse function. Therefore, to define an inverse function we must restrict their domains so that the trigonometric function is bijective. In the following, the functions on the left are defined by the equation on the right; these are not proved identities. The principal inverses are usually defined as:
Function  Definition  Value Field 

The notations sin^{−1} and cos^{−1} are often used for arcsin and arccos, etc. When this notation is used, the inverse functions could be confused with the multiplicative inverses of the functions. The notation using the "arc" prefix avoids such confusion, though "arcsec" can be confused with "arcsecond".
Just like the sine and cosine, the inverse trigonometric functions can also be defined in terms of infinite series. For example,
These functions may also be defined by proving that they are antiderivatives of other functions. The arcsine, for example, can be written as the following integral:
Analogous formulas for the other functions can be found at Inverse trigonometric functions. Using the complex logarithm, one can generalize all these functions to complex arguments:
Connection to the inner product
In an inner product space, the angle between two nonzero vectors is defined to be
Properties and applications
The trigonometric functions, as the name suggests, are of crucial importance in trigonometry, mainly because of the following two results.
Law of sines
The law of sines states that for an arbitrary triangle with sides a, b, and c and angles opposite those sides A, B and C:
where is the area of the triangle, or, equivalently,
where R is the triangle's circumradius.
It can be proven by dividing the triangle into two right ones and using the above definition of sine. 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. This is a common situation occurring in triangulation, a technique to determine unknown distances by measuring two angles and an accessible enclosed distance.
Law of cosines
The law of cosines (also known as the cosine formula or cosine rule) is an extension of the Pythagorean theorem:
or equivalently,
In this formula the angle at C is opposite to the side c. This theorem can be proven by dividing the triangle into two right ones and using the Pythagorean theorem.
The law of cosines can be used to determine a side of a triangle if two sides and the angle between them are known. It can also be used to find the cosines of an angle (and consequently the angles themselves) if the lengths of all the sides are known.
Law of tangents
The following all form the law of tangents^{[21]}
The explanation of the formulae in words would be cumbersome, but the patterns of sums and differences; for the lengths and corresponding opposite angles, are apparent in the theorem.
Law of cotangents
If
(the radius of the inscribed circle for the triangle) and
(the semiperimeter for the triangle), then the following all form the law of cotangents^{[22]}
It follows that
In words the theorem is: the cotangent of a halfangle equals the ratio of the semiperimeter minus the opposite side to the said angle, to the inradius for the triangle.
Periodic functions
The trigonometric functions are also important in physics. The sine and the cosine functions, for example, are used to describe simple harmonic motion, which models many natural phenomena, such as the movement of a mass attached to a spring and, for small angles, the pendular motion of a mass hanging by a string. The sine and cosine functions are onedimensional projections of uniform circular motion.
Trigonometric functions also prove to be useful in the study of general periodic functions. The characteristic wave patterns of periodic functions are useful for modeling recurring phenomena such as sound or light waves.^{[23]}
Under rather general conditions, a periodic function ƒ(x) can be expressed as a sum of sine waves or cosine waves in a Fourier series.^{[24]} Denoting the sine or cosine basis functions by φ_{k}, the expansion of the periodic function ƒ(t) takes the form:
For example, the square wave can be written as the Fourier series
In the animation of a square wave at top right it can be seen that just a few terms already produce a fairly good approximation. The superposition of several terms in the expansion of a sawtooth wave are shown underneath.
History
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 BC) and Ptolemy of Roman Egypt (90–165 AD).
The functions sine and cosine can be traced to the jyā and kotijyā functions used in Gupta period Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.^{[25]}
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.^{[26]} alKhwārizmī produced tables of sines, cosines and tangents. They were studied by authors including Omar Khayyám, Bhāskara II, Nasir alDin alTusi, Jamshīd alKāshī (14th century), Ulugh Beg (14th century), Regiomontanus (1464), Rheticus, and Rheticus' student Valentinus Otho.^{[citation needed]}
Madhava of Sangamagrama (c. 1400) made early strides in the analysis of trigonometric functions in terms of infinite series.^{[27]}
The first published use of the abbreviations 'sin', 'cos', and 'tan' is by the 16th century French mathematician Albert Girard.
In a paper published in 1682, Leibniz proved that sin x is not an algebraic function of x.^{[28]}
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 nearmodern abbreviations sin., cos., tang., cot., sec., and cosec.^{[6]}
A few functions were common historically, but are now seldom used, such as the chord (crd(θ) = 2 sin(θ/2)), the versine (versin(θ) = 1 − cos(θ) = 2 sin^{2}(θ/2)) (which appeared in the earliest tables^{[6]}), the haversine (haversin(θ) = versin(θ) / 2 = sin^{2}(θ/2)), the exsecant (exsec(θ) = sec(θ) − 1) and the excosecant (excsc(θ) = exsec(π/2 − θ) = csc(θ) − 1). Many more relations between these functions are listed in the article about trigonometric identities.
Etymology
The word sine derives from Latin sinus ("bend", "bay", "the hanging fold of the upper part of a toga", "the bosom of a garment"). The use of sinus originates in twelfthcentury European translations of the Arabic word jaib ("pocket" or "fold").^{[29]} This was in turn based on a misreading of the Arabic written form jyb, which itself originated as a transliteration from Sanskrit, of either jyā (the standard Sanskrit term for the sine) or the synonymous jīvā (both literally meaning "bowstring").^{[30]}
The word tangent comes from Latin tangens meaning "touching", since the line touches the circle of unit radius, whereas secant stems from Latin secans — "cutting" — since the line cuts the circle.^{[31]}
The prefix "co" (in "cosine", "cotangent", "cosecant") is found in Edmund Gunter's Canon triangulorum (1620), which defines the cosinus as an abbreviation for the sinus complementi (sine of the complementary angle) and proceeds to define the cotangens similarly.^{[32]}
See also
 All Students Take Calculus — a mnemonic for recalling the signs of trigonometric functions in a particular quadrant of a Cartesian plane
 Aryabhata's sine table
 Bhaskara I's sine approximation formula
 Euler's formula
 Gauss's continued fraction — a continued fraction definition for the tangent function
 Generalized trigonometry
 Generating trigonometric tables
 Hyperbolic function
 List of periodic functions
 List of trigonometric identities
 Madhava series
 Madhava's sine table
 Polar sine — a generalization to vertex angles
 Proofs of trigonometric identities
 Table of Newtonian series
 Unit vector (explains direction cosines)
Notes
 ↑ Oxford English Dictionary, sine, n.^{2}
 ↑ Oxford English Dictionary, cosine, n.
 ↑ Oxford English Dictionary, tangent, adj. and n.
 ↑ Oxford English Dictionary, secant, adj. and n.
 ↑ Heng, Cheng and Talbert, "Additional Mathematics", page 228
 ↑ ^{6.0} ^{6.1} ^{6.2} See Boyer (1991).
 ↑ See Maor (1998)
 ↑ See Ahlfors, pages 43–44.
 ↑ Abramowitz; Weisstein.
 ↑ Stanley, Enumerative Combinatorics, Vol I., page 149
 ↑ Stanley, Enumerative Combinatorics, Vol I
 ↑ Aigner, Martin; Ziegler, Günter M. (2000). Proofs from THE BOOK (Second ed.). SpringerVerlag. p. 149. ISBN 9783642008559.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ Remmert, Reinhold (1991). Theory of complex functions. Springer. p. 327. ISBN 0387971955.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>, Extract of page 327
 ↑ For a demonstration, see Euler's formula#Using power series
 ↑ Needham, Tristan. Visual Complex Analysis. ISBN 0198534469.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ Kannappan, Palaniappan (2009). Functional Equations and Inequalities with Applications. Springer. ISBN 9780387894911.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ Kantabutra.
 ↑ However, doing that while maintaining precision is nontrivial, and methods like Gal's accurate tables, Cody and Waite reduction, and Payne and Hanek reduction algorithms can be used.
 ↑ "R. P. Brent, "Fast MultiplePrecision Evaluation of Elementary Functions", J. ACM 23, 242 (1976)".<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ ^{20.0} ^{20.1} ^{20.2} ^{20.3} Abramowitz, Milton and Irene A. Stegun, p.74
 ↑ The Universal Encyclopaedia of Mathematics, Pan Reference Books, 1976, page 529. English version George Allen and Unwin, 1964. Translated from the German version Meyers Rechenduden, 1960.
 ↑ The Universal Encyclopaedia of Mathematics, Pan Reference Books, 1976, page 530. English version George Allen and Unwin, 1964. Translated from the German version Meyers Rechenduden, 1960.
 ↑ Stanley J Farlow (1993). Partial differential equations for scientists and engineers (Reprint of Wiley 1982 ed.). Courier Dover Publications. p. 82. ISBN 048667620X.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ See for example, Gerald B Folland (2009). "Convergence and completeness". Fourier Analysis and its Applications (Reprint of Wadsworth & Brooks/Cole 1992 ed.). American Mathematical Society. pp. 77 ff. ISBN 0821847902.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ Boyer, Carl B. (1991). A History of Mathematics (Second ed.). John Wiley & Sons, Inc.. ISBN 0471543977, p. 210.
 ↑ Owen Gingerich (1986). "Islamic Astronomy". 254. Scientific American: 74. Archived from the original on 20131019. Retrieved 20100713. Cite journal requires
journal=
(help)<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>  ↑ J J O'Connor and E F Robertson. "Madhava of Sangamagrama". School of Mathematics and Statistics University of St Andrews, Scotland. Retrieved 20070908.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ Nicolás Bourbaki (1994). Elements of the History of Mathematics. Springer.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
 ↑ various sources credit the first use of sinus to either
 Plato Tiburtinus's 1116 translation of the Astronomy of AlBattani
 Gerard of Cremona's translation of the Algebra of alKhwārizmī
 Robert of Chester's 1145 translation of the tables of alKhwārizmī
 ↑ See Plofker, Mathematics in India, Princeton University Press, 2009, p. 257, also "Clark University".<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles> and Maor (1998), chapter 3, regarding the etymology.
 ↑ Oxford English Dictionary
 ↑ OED. The text of the Canon triangulorum as reconstructed may be found here
References
 Abramowitz, Milton and Irene A. Stegun, Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables, Dover, New York. (1964). ISBN 0486612724.
 Lars Ahlfors, Complex Analysis: an introduction to the theory of analytic functions of one complex variable, second edition, McGrawHill Book Company, New York, 1966.
 Boyer, Carl B., A History of Mathematics, John Wiley & Sons, Inc., 2nd edition. (1991). ISBN 0471543977.
 Gal, Shmuel and Bachelis, Boris. An accurate elementary mathematical library for the IEEE floating point standard, ACM Transaction on Mathematical Software (1991).
 Joseph, George G., The Crest of the Peacock: NonEuropean Roots of Mathematics, 2nd ed. Penguin Books, London. (2000). ISBN 0691006598.
 Kantabutra, Vitit, "On hardware for computing exponential and trigonometric functions," IEEE Trans. Computers 45 (3), 328–339 (1996).
 Maor, Eli, Trigonometric Delights, Princeton Univ. Press. (1998). Reprint edition (February 25, 2002): ISBN 0691095418.^{[dead link]}
 Needham, Tristan, "Preface"" to Visual Complex Analysis. Oxford University Press, (1999). ISBN 0198534469.
 O'Connor, J.J., and E.F. Robertson, "Trigonometric functions", MacTutor History of Mathematics archive. (1996).
 O'Connor, J.J., and E.F. Robertson, "Madhava of Sangamagramma", MacTutor History of Mathematics archive. (2000).
 Pearce, Ian G., "Madhava of Sangamagramma", MacTutor History of Mathematics archive. (2002).
 Weisstein, Eric W., "Tangent" from MathWorld, accessed 21 January 2006.
External links
Wikibooks has a book on the topic of: Trigonometry 
 Hazewinkel, Michiel, ed. (2001), "Trigonometric functions", Encyclopedia of Mathematics, Springer, ISBN 9781556080104<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
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