Trigonometric functions: Difference between revisions

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{{Trigonometry}}
{{Trigonometry}}


The trigonometric functions most widely used in modern mathematics are the [[sine]], the [[cosine]], and the '''tangent''' functions. Their [[multiplicative inverse|reciprocal]]s are respectively the '''cosecant''', the '''secant''', and the '''cotangent''' functions, which are less used. Each of these six trigonometric functions has a corresponding [[Inverse trigonometric functions|inverse function]], and an analog among the [[hyperbolic functions]].
The trigonometric functions most widely used in modern mathematics are the [[sine]], the [[cosine]], and the '''tangent''' functions. {{anchor|Reciprocal_functions}}Their [[multiplicative inverse|reciprocal]]s are respectively the '''cosecant''', the '''secant''', and the '''cotangent''' functions, which are less used. Each of these six trigonometric functions has a corresponding [[Inverse trigonometric functions|inverse function]] and has an analog among the [[hyperbolic functions]].


The oldest definitions of trigonometric functions, related to right-angle triangles, define them only for [[acute angle]]s. To extend the sine and cosine functions to functions whose [[domain of a function|domain]] is the whole [[real line]], geometrical definitions using the standard [[unit circle]] (i.e., a circle with [[radius]] 1 unit) are often used; then the domain of the other functions is the real line with some isolated points removed. Modern definitions express trigonometric functions as [[Series (mathematics)|infinite series]] or as solutions of [[differential equation]]s. This allows extending the domain of sine and cosine functions to the whole [[complex plane]], and the domain of the other trigonometric functions to the complex plane with some isolated points removed.
The oldest definitions of trigonometric functions, related to right-angle triangles, define them only for [[acute angle]]s. To extend the sine and cosine functions to functions whose [[domain of a function|domain]] is the whole [[real line]], geometrical definitions using the standard [[unit circle]] (i.e., a circle with [[radius]] 1 unit) are often used; then the domain of the other functions is the real line with some isolated points removed. Modern definitions express trigonometric functions as [[Series (mathematics)|infinite series]] or as solutions of [[differential equation]]s. This allows extending the domain of sine and cosine functions to the whole [[complex plane]], and the domain of the other trigonometric functions to the complex plane with some isolated points removed.
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In a right-angled triangle, the sum of the two acute angles is a right angle, that is, {{math|90°}} or {{math|{{sfrac|π|2}} [[radian]]s}}. Therefore <math>\sin(\theta)</math> and <math>\cos(90^\circ - \theta)</math> represent the same ratio, and thus are equal. This identity and analogous relationships between the other trigonometric functions are summarized in the following table.
In a right-angled triangle, the sum of the two acute angles is a right angle, that is, {{math|90°}} or {{math|{{sfrac|π|2}} [[radian]]s}}. Therefore <math>\sin(\theta)</math> and <math>\cos(90^\circ - \theta)</math> represent the same ratio, and thus are equal. This identity and analogous relationships between the other trigonometric functions are summarized in the following table.


[[File:Periodic sine.svg|thumb|'''Top:''' Trigonometric function {{math|sin ''θ''}} for selected angles {{math|''θ''}}, {{math|{{pi}} − ''θ''}}, {{math|{{pi}} + ''θ''}}, and {{math|2{{pi}} − ''θ''}} in the four quadrants.<br>'''Bottom:''' Graph of sine versus angle. Angles from the top panel are identified.]]
[[File:Periodic sine.svg|thumb|'''Top:''' Trigonometric function {{math|sin ''θ''}} for selected angles {{mvar|θ}}, {{math|{{pi}} − ''θ''}}, {{math|{{pi}} + ''θ''}}, and {{math|2{{pi}} − ''θ''}} in the four quadrants.<br>'''Bottom:''' Graph of sine versus angle. Angles from the top panel are identified.]]


{| class="wikitable sortable"
{| class="wikitable sortable"
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! tangent
! tangent
|align=center|{{math|{{sfrac|opposite|adjacent}}}}
|align=center|{{math|{{sfrac|opposite|adjacent}}}}
| <math>\tan \theta = \frac{\sin \theta}{\cos \theta} = \cot\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\cot \theta} </math>
| <math>\tan \theta = \frac{\sin \theta}{\cos \theta} = \cot\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\cot \theta}</math>
| <math>\tan x = \frac{\sin x}{\cos x} = \cot\left(90^\circ - x \right) = \frac{1}{\cot x} </math>
| <math>\tan x = \frac{\sin x}{\cos x} = \cot\left(90^\circ - x \right) = \frac{1}{\cot x}</math>
|-
|-
! cotangent
! cotangent
|align=center|{{math|{{sfrac|adjacent|opposite}}}}
|align=center|{{math|{{sfrac|adjacent|opposite}}}}
| <math>\cot \theta = \frac{\cos \theta}{\sin \theta} = \tan\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\tan \theta} </math>
| <math>\cot \theta = \frac{\cos \theta}{\sin \theta} = \tan\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\tan \theta}</math>
| <math>\cot x = \frac{\cos x}{\sin x} = \tan\left(90^\circ - x \right) = \frac{1}{\tan x} </math>
| <math>\cot x = \frac{\cos x}{\sin x} = \tan\left(90^\circ - x \right) = \frac{1}{\tan x}</math>
|-
|-
! secant
! secant
|align=center|{{math|{{sfrac|hypotenuse|adjacent}}}}
|align=center|{{math|{{sfrac|hypotenuse|adjacent}}}}
| <math>\sec \theta = \csc\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\cos \theta} </math>
| <math>\sec \theta = \csc\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\cos \theta}</math>
| <math>\sec x = \csc\left(90^\circ - x \right) = \frac{1}{\cos x} </math>
| <math>\sec x = \csc\left(90^\circ - x \right) = \frac{1}{\cos x}</math>
|-
|-
! cosecant
! cosecant
|align=center|{{math|{{sfrac|hypotenuse|opposite}}}}
|align=center|{{math|{{sfrac|hypotenuse|opposite}}}}
| <math>\csc \theta = \sec\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\sin \theta} </math>
| <math>\csc \theta = \sec\left(\frac{\pi}{2} - \theta \right) = \frac{1}{\sin \theta}</math>
| <math>\csc x = \sec\left(90^\circ - x \right) = \frac{1}{\sin x} </math>
| <math>\csc x = \sec\left(90^\circ - x \right) = \frac{1}{\sin x}</math>
|}
|}


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In geometric applications, the argument of a trigonometric function is generally the measure of an [[angle]]. For this purpose, any [[angular unit]] is convenient. One common unit is [[degree (angle)|degrees]], in which a right angle is 90° and a complete turn is 360° (particularly in [[elementary mathematics]]).
In geometric applications, the argument of a trigonometric function is generally the measure of an [[angle]]. For this purpose, any [[angular unit]] is convenient. One common unit is [[degree (angle)|degrees]], in which a right angle is 90° and a complete turn is 360° (particularly in [[elementary mathematics]]).


However, in [[calculus]] and [[mathematical analysis]], the trigonometric functions are generally regarded more abstractly as functions of [[real number|real]] or [[complex number]]s, rather than angles. In fact, the functions {{math|sin}} and {{math|cos}} can be defined for all complex numbers in terms of the [[exponential function]], via power series,<ref name=":0">{{Cite book|last=Rudin, Walter, 1921–2010|url=https://www.worldcat.org/oclc/1502474|title=Principles of mathematical analysis|isbn=0-07-054235-X|edition=Third |location=New York|oclc=1502474}}</ref> or as solutions to [[differential equation]]s given particular initial values<ref>{{Cite journal|last=Diamond|first=Harvey|date=2014|title=Defining Exponential and Trigonometric Functions Using Differential Equations|url=https://www.tandfonline.com/doi/full/10.4169/math.mag.87.1.37|journal=Mathematics Magazine|language=en|volume=87|issue=1|pages=37–42|doi=10.4169/math.mag.87.1.37|s2cid=126217060|issn=0025-570X|url-access=subscription}}</ref> (''see below''), without reference to any geometric notions. The other four trigonometric functions ({{math|tan}}, {{math|cot}}, {{math|sec}}, {{math|csc}}) can be defined as quotients and reciprocals of {{math|sin}} and {{math|cos}}, except where zero occurs in the denominator. It can be proved, for real arguments, that these definitions coincide with elementary geometric definitions if the argument is regarded as an angle in radians.<ref name=":0" /> Moreover, these definitions result in simple expressions for the [[derivative]]s and [[Antiderivative|indefinite integrals]] for the trigonometric functions.<ref name=":1">{{Cite book|last=Spivak|first=Michael|title=Calculus|publisher=Addison-Wesley|year=1967|chapter=15|pages=256–257|lccn=67-20770}}</ref> Thus, in settings beyond elementary geometry, radians are regarded as the mathematically natural unit for describing angle measures.
However, in [[calculus]] and [[mathematical analysis]], the trigonometric functions are generally regarded more abstractly as functions of [[real number|real]] or [[complex number]]s, rather than angles. In fact, the functions {{math|sin}} and {{math|cos}} can be defined for all complex numbers in terms of the [[exponential function]], via power series,<ref name=":0">{{Cite book|last=Rudin, Walter, 1921–2010|title=Principles of mathematical analysis|isbn=0-07-054235-X|edition=Third |location=New York|oclc=1502474}}</ref> or as solutions to [[differential equation]]s given particular initial values<ref>{{Cite journal|last=Diamond|first=Harvey|date=2014|title=Defining Exponential and Trigonometric Functions Using Differential Equations|url=https://www.tandfonline.com/doi/full/10.4169/math.mag.87.1.37|journal=Mathematics Magazine|language=en|volume=87|issue=1|pages=37–42|doi=10.4169/math.mag.87.1.37|s2cid=126217060|issn=0025-570X|url-access=subscription}}</ref> (''see below''), without reference to any geometric notions. The other four trigonometric functions ({{math|tan}}, {{math|cot}}, {{math|sec}}, {{math|csc}}) can be defined as quotients and reciprocals of {{math|sin}} and {{math|cos}}, except where zero occurs in the denominator. It can be proved, for real arguments, that these definitions coincide with elementary geometric definitions if the argument is regarded as an angle in radians.<ref name=":0" /> Moreover, these definitions result in simple expressions for the [[derivative]]s and [[Antiderivative|indefinite integrals]] for the trigonometric functions.<ref name=":1">{{Cite book|last=Spivak|first=Michael|title=Calculus|publisher=Addison-Wesley|year=1967|chapter=15|pages=256–257|lccn=67-20770}}</ref> Thus, in settings beyond elementary geometry, radians are regarded as the mathematically natural unit for describing angle measures.


When [[radian]]s (rad) are employed, the angle is given as the length of the [[arc (geometry)|arc]] of the [[unit circle]] subtended by it: the angle that subtends an arc of length 1 on the unit circle is 1 rad (≈ 57.3°),<ref>{{cite oeis|A072097|Decimal expansion of 180/Pi}}</ref> and a complete [[turn (angle)|turn]] (360°) is an angle of 2{{pi}} (≈ 6.28) rad.<ref>{{cite oeis|A019692|Decimal expansion of 2*Pi}}</ref> For real number ''x'', the notation {{math|sin ''x''}}, {{math|cos ''x''}}, etc. refers to the value of the trigonometric functions evaluated at an angle of ''x'' rad. If units of degrees are intended, the degree sign must be explicitly shown ({{math|sin ''x°''}}, {{math|cos ''x°''}}, etc.). Using this standard notation, the argument ''x'' for the trigonometric functions satisfies the relationship ''x'' = (180''x''/{{pi}})°, so that, for example, {{math|1=sin {{pi}} = sin 180°}} when we take ''x'' = {{pi}}. In this way, the degree symbol can be regarded as a mathematical constant such that 1° = {{pi}}/180 ≈ 0.0175.<ref>{{cite oeis|A019685|Decimal expansion of Pi/180}}</ref>
When [[radian]]s (rad) are employed, the angle is given as the length of the [[arc (geometry)|arc]] of the [[unit circle]] subtended by it: the angle that subtends an arc of length 1 on the unit circle is 1 rad (≈ 57.3°),<ref>{{cite oeis|A072097|Decimal expansion of 180/Pi}}</ref> and a complete [[turn (angle)|turn]] (360°) is an angle of 2{{pi}} (≈ 6.28) rad.<ref>{{cite oeis|A019692|Decimal expansion of 2*Pi}}</ref> Since radian is dimensionless, i.e. 1 rad = 1, the degree symbol can also be regarded as a [[mathematical constant]] [[Factor (arithmetic)|factor]] such that 1° = {{pi}}/180 ≈ 0.0175.{{citation needed |date=July 2025}}


==Unit-circle definitions==
==Unit-circle definitions==
[[Image:Circle-trig6.svg|right|thumb|upright=1.35|All of the trigonometric functions of the angle {{math|''θ''}} (theta) can be constructed geometrically in terms of a unit circle centered at ''O''.]]
[[Image:Circle-trig6.svg|right|thumb|upright=1.35|All of the trigonometric functions of the angle {{mvar|θ}} (theta) can be constructed geometrically in terms of a unit circle centered at {{mvar|O}}.]]
[[File:Periodic sine.svg|thumb|Sine function on unit circle (top) and its graph (bottom)]]
[[File:Periodic sine.svg|thumb|Sine function on unit circle (top) and its graph (bottom)]]
[[File:Unit Circle Definitions of Six Trigonometric Functions.svg|thumb|upright=1.2|In this illustration, the six trigonometric functions of an arbitrary angle {{math|''θ''}} are represented as [[Cartesian coordinates]] of points related to the [[unit circle]]. The {{mvar|y}}-axis ordinates of {{math|A}}, {{math|B}} and {{math|D}} are {{math|sin ''θ''}}, {{math|tan ''θ''}} and {{math|csc ''θ''}}, respectively, while the {{mvar|x}}-axis abscissas of {{math|A}}, {{math|C}} and {{math|E}} are {{math|cos ''θ''}}, {{math|cot ''θ''}} and {{math|sec ''θ''}}, respectively.]]
[[File:Unit Circle Definitions of Six Trigonometric Functions.svg|thumb|upright=1.2|In this illustration, the six trigonometric functions of an arbitrary angle {{mvar|θ}} are represented as [[Cartesian coordinates]] of points related to the [[unit circle]]. The {{mvar|y}}-axis ordinates of {{math|A}}, {{math|B}} and {{math|D}} are {{math|sin ''θ''}}, {{math|tan ''θ''}} and {{math|csc ''θ''}}, respectively, while the {{mvar|x}}-axis abscissas of {{math|A}}, {{math|C}} and {{math|E}} are {{math|cos ''θ''}}, {{math|cot ''θ''}} and {{math|sec ''θ''}}, respectively.]]
[[File:trigonometric function quadrant sign.svg|thumb|Signs of trigonometric functions in each quadrant. [[mnemonics in trigonometry|Mnemonics]] like "'''all''' '''s'''tudents '''t'''ake '''c'''alculus" indicates when '''s'''ine, '''c'''osine, and '''t'''angent are positive from quadrants I to IV.<ref name=steuben>{{Cite book |last1=Stueben |first1=Michael |title=Twenty years before the blackboard: the lessons and humor of a mathematics teacher |last2=Sandford |first2=Diane |date=1998 |publisher=Mathematical Association of America |isbn=978-0-88385-525-6 |series=Spectrum series |location=Washington, DC|page=119|url=https://books.google.com/books?id=qnd0P-Ja-O8C&dq=%22All+Students+Take+Calculus%22&pg=PA119}}</ref>]]
[[File:trigonometric function quadrant sign.svg|thumb|Signs of trigonometric functions in each quadrant. [[mnemonics in trigonometry|Mnemonics]] like "'''all''' '''s'''tudents '''t'''ake '''c'''alculus" indicates when '''s'''ine, '''c'''osine, and '''t'''angent are positive from quadrants I to IV.<ref name=steuben>{{Cite book |last1=Stueben |first1=Michael |title=Twenty years before the blackboard: the lessons and humor of a mathematics teacher |last2=Sandford |first2=Diane |date=1998 |publisher=Mathematical Association of America |isbn=978-0-88385-525-6 |series=Spectrum series |location=Washington, DC|page=119|url=https://books.google.com/books?id=qnd0P-Ja-O8C&dq=%22All+Students+Take+Calculus%22&pg=PA119}}</ref>]]


The six trigonometric functions can be defined as [[Cartesian coordinate system|coordinate values]] of points on the [[Euclidean plane]] that are related to the [[unit circle]], which is the [[circle]] of radius one centered at the origin {{math|O}} of this coordinate system. While [[#Right-angled triangle definitions|right-angled triangle definitions]] allow for the definition of the trigonometric functions for angles between {{math|0}} and <math display="inline">\frac{\pi}{2}</math> [[radian]]s {{math|(90°),}} the unit circle definitions allow the domain of trigonometric functions to be extended to all positive and negative real numbers.
The six trigonometric functions can be defined as [[Cartesian coordinate system|coordinate values]] of points on the [[Euclidean plane]] that are related to the [[unit circle]], which is the [[circle]] of radius one centered at the origin {{math|O}} of this coordinate system. While [[#Right-angled triangle definitions|right-angled triangle definitions]] allow for the definition of the trigonometric functions for angles between {{math|0}} and <math display="inline">\frac{\pi}{2}</math> [[radian]]s {{math|(90°),}} the unit circle definitions allow the domain of trigonometric functions to be extended to all positive and negative real numbers.


Let <math>\mathcal L</math> be the [[Ray (geometry)|ray]] obtained by rotating by an angle {{mvar|θ}} the positive half of the {{math|''x''}}-axis ([[counterclockwise]] rotation for <math>\theta > 0,</math> and clockwise rotation for <math>\theta < 0</math>). This ray intersects the unit circle at the point <math>\mathrm{A} = (x_\mathrm{A},y_\mathrm{A}).</math> The ray <math>\mathcal L,</math> extended to a [[line (geometry)|line]] if necessary, intersects the line of equation <math>x=1</math> at point <math>\mathrm{B} = (1,y_\mathrm{B}),</math> and the line of equation <math>y=1</math> at point <math>\mathrm{C} = (x_\mathrm{C},1).</math> The [[tangent line]] to the unit circle at the point {{math|A}}, is [[perpendicular]] to <math>\mathcal L,</math> and intersects the {{math|''y''}}- and {{math|''x''}}-axes at points <math>\mathrm{D} = (0,y_\mathrm{D})</math> and <math>\mathrm{E} = (x_\mathrm{E},0).</math> The [[Cartesian coordinates|coordinates]] of these points give the values of all trigonometric functions for any arbitrary real value of {{mvar|θ}} in the following manner.
Let <math>\mathcal L</math> be the [[Ray (geometry)|ray]] obtained by rotating by an angle {{mvar|θ}} the positive half of the {{mvar|x}}-axis ([[counterclockwise]] rotation for <math>\theta > 0,</math> and clockwise rotation for <math>\theta < 0</math>). This ray intersects the unit circle at the point <math>\mathrm{A} = (x_\mathrm{A},y_\mathrm{A}).</math> The ray <math>\mathcal L,</math> extended to a [[line (geometry)|line]] if necessary, intersects the line of equation <math>x=1</math> at point <math>\mathrm{B} = (1,y_\mathrm{B}),</math> and the line of equation <math>y=1</math> at point <math>\mathrm{C} = (x_\mathrm{C},1).</math> The [[tangent line]] to the unit circle at the point {{math|A}}, is [[perpendicular]] to <math>\mathcal L,</math> and intersects the {{mvar|y}}- and {{mvar|x}}-axes at points <math>\mathrm{D} = (0,y_\mathrm{D})</math> and <math>\mathrm{E} = (x_\mathrm{E},0).</math> The [[Cartesian coordinates|coordinates]] of these points give the values of all trigonometric functions for any arbitrary real value of {{mvar|θ}} in the following manner.


The trigonometric functions {{math|cos}} and {{math|sin}} are defined, respectively, as the ''x''- and ''y''-coordinate values of point {{math|A}}. That is,
The trigonometric functions {{math|cos}} and {{math|sin}} are defined, respectively, as the {{mvar|x}}- and {{mvar|y}}-coordinate values of point {{math|A}}. That is,
:<math>\cos \theta = x_\mathrm{A} \quad</math> and <math>\quad \sin \theta = y_\mathrm{A}.</math><ref>{{Cite web|url=https://www.encyclopediaofmath.org/index.php/Trigonometric_functions|title=Trigonometric Functions|last=Bityutskov|first=V.I.|date=7 February 2011|website=Encyclopedia of Mathematics|language=en|archive-url=https://web.archive.org/web/20171229231821/https://www.encyclopediaofmath.org/index.php/Trigonometric_functions|archive-date=29 December 2017|url-status=live|access-date=29 December 2017}}</ref>
<math display="block">\cos \theta = x_\mathrm{A} \quad</math> and <math>\quad \sin \theta = y_\mathrm{A}.</math><ref>{{Cite web|url=https://www.encyclopediaofmath.org/index.php/Trigonometric_functions|title=Trigonometric Functions|last=Bityutskov|first=V.I.|date=7 February 2011|website=Encyclopedia of Mathematics|language=en|archive-url=https://web.archive.org/web/20171229231821/https://www.encyclopediaofmath.org/index.php/Trigonometric_functions|archive-date=29 December 2017|url-status=live|access-date=29 December 2017}}</ref>


In the range <math>0 \le \theta \le \pi/2</math>, this definition coincides with the right-angled triangle definition, by taking the right-angled triangle to have the unit radius {{math|OA}} as [[hypotenuse]]. And since the equation <math>x^2+y^2=1</math> holds for all points <math>\mathrm{P} = (x,y)</math> on the unit circle, this definition of cosine and sine also satisfies the [[Pythagorean identity]].
In the range <math>0 \le \theta \le \pi/2</math>, this definition coincides with the right-angled triangle definition, by taking the right-angled triangle to have the unit radius {{math|OA}} as [[hypotenuse]]. And since the equation <math>x^2+y^2=1</math> holds for all points <math>\mathrm{P} = (x,y)</math> on the unit circle, this definition of cosine and sine also satisfies the [[Pythagorean identity]].
:<math>\cos^2\theta+\sin^2\theta=1.</math>
<math display="block">\cos^2\theta+\sin^2\theta=1.</math>


The other trigonometric functions can be found along the unit circle as  
The other trigonometric functions can be found along the unit circle as  
:<math>\tan \theta = y_\mathrm{B} \quad</math> and <math> \quad\cot \theta = x_\mathrm{C},</math>
<math display="block">\tan \theta = y_\mathrm{B} \quad</math> and <math> \quad\cot \theta = x_\mathrm{C},</math>
:<math>\csc \theta\ = y_\mathrm{D} \quad</math> and <math> \quad\sec \theta = x_\mathrm{E}.</math>
<math display="block">\csc \theta\ = y_\mathrm{D} \quad</math> and <math> \quad\sec \theta = x_\mathrm{E}.</math>


By applying the Pythagorean identity and geometric proof methods, these definitions can readily be shown to coincide with the definitions of tangent, cotangent, secant and cosecant in terms of sine and cosine, that is
By applying the Pythagorean identity and geometric proof methods, these definitions can readily be shown to coincide with the definitions of tangent, cotangent, secant and cosecant in terms of sine and cosine, that is
: <math>\tan \theta =\frac{\sin \theta}{\cos\theta},\quad \cot\theta=\frac{\cos\theta}{\sin\theta},\quad \sec\theta=\frac{1}{\cos\theta},\quad \csc\theta=\frac{1}{\sin\theta}.</math>
<math display="block">\tan \theta =\frac{\sin \theta}{\cos\theta},\quad \cot\theta=\frac{\cos\theta}{\sin\theta},\quad \sec\theta=\frac{1}{\cos\theta},\quad \csc\theta=\frac{1}{\sin\theta}.</math>


[[File:Trigonometric functions.svg|right|thumb|upright=1.35|link={{filepath:trigonometric_functions_derivation_animation.svg}}|Trigonometric functions:
[[File:Trigonometric functions.svg|right|thumb|upright=1.35|link={{filepath:trigonometric_functions_derivation_animation.svg}}|Trigonometric functions:
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Since a rotation of an angle of <math>\pm2\pi</math> does not change the position or size of a shape, the points {{math|A}}, {{math|B}}, {{math|C}}, {{math|D}}, and {{math|E}} are the same for two angles whose difference is an integer multiple of <math>2\pi</math>. Thus trigonometric functions are [[periodic function]]s with period <math>2\pi</math>. That is, the equalities
Since a rotation of an angle of <math>\pm2\pi</math> does not change the position or size of a shape, the points {{math|A}}, {{math|B}}, {{math|C}}, {{math|D}}, and {{math|E}} are the same for two angles whose difference is an integer multiple of <math>2\pi</math>. Thus trigonometric functions are [[periodic function]]s with period <math>2\pi</math>. That is, the equalities
: <math> \sin\theta = \sin\left(\theta + 2 k \pi \right)\quad</math> and <math>\quad \cos\theta = \cos\left(\theta + 2 k \pi \right)</math>
<math display="block">\sin\theta = \sin\left(\theta + 2 k \pi \right)\quad</math> and <math>\quad \cos\theta = \cos\left(\theta + 2 k \pi \right)</math>
hold for any angle {{mvar|θ}} and any [[integer]] {{mvar|k}}. The same is true for the four other trigonometric functions. By observing the sign and the monotonicity of the functions sine, cosine, cosecant, and secant in the four quadrants, one can show that <math>2\pi</math> is the smallest value for which they are periodic (i.e., <math>2\pi</math> is the [[periodic function|fundamental period]] of these functions). However, after a rotation by an angle <math>\pi</math>, the points {{mvar|B}} and {{mvar|C}} already return to their original position, so that the tangent function and the cotangent function have a fundamental period of <math>\pi</math>. That is, the equalities
hold for any angle {{mvar|θ}} and any [[integer]] {{mvar|k}}. The same is true for the four other trigonometric functions. By observing the sign and the monotonicity of the functions sine, cosine, cosecant, and secant in the four quadrants, one can show that <math>2\pi</math> is the smallest value for which they are periodic (i.e., <math>2\pi</math> is the [[periodic function|fundamental period]] of these functions). However, after a rotation by an angle <math>\pi</math>, the points {{mvar|B}} and {{mvar|C}} already return to their original position, so that the tangent function and the cotangent function have a fundamental period of <math>\pi</math>. That is, the equalities
: <math> \tan\theta = \tan(\theta + k\pi) \quad</math> and <math>\quad \cot\theta = \cot(\theta + k\pi)</math>
<math display="block">\tan\theta = \tan(\theta + k\pi) \quad</math> and <math>\quad \cot\theta = \cot(\theta + k\pi)</math>
hold for any angle {{mvar|θ}} and any integer {{mvar|k}}.
hold for any angle {{mvar|θ}} and any integer {{mvar|k}}.


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The [[algebraic expression]]s for the most important angles are as follows:
The [[algebraic expression]]s for the most important angles are as follows:


:<math>\sin 0 = \sin 0^\circ \quad= \frac{\sqrt0}2 = 0</math> ([[Angle#Types of angles|zero angle]])
<math display="block">\sin 0 = \sin 0^\circ \quad= \frac{\sqrt0}2 = 0</math> ([[Angle#Types of angles|zero angle]])
:<math>\sin \frac\pi6 = \sin 30^\circ = \frac{\sqrt1}2 = \frac{1}{2}</math>
<math display="block">\sin \frac\pi6 = \sin 30^\circ = \frac{\sqrt1}2 = \frac{1}{2}</math>
:<math>\sin \frac\pi4 = \sin 45^\circ = \frac{\sqrt{2}}{2} = \frac{1}{\sqrt{2}}</math>
<math display="block">\sin \frac\pi4 = \sin 45^\circ = \frac{\sqrt{2}}{2} = \frac{1}{\sqrt{2}}</math>
:<math>\sin \frac\pi3 = \sin 60^\circ = \frac{\sqrt{3}}{2}</math>
<math display="block">\sin \frac\pi3 = \sin 60^\circ = \frac{\sqrt{3}}{2}</math>
:<math>\sin \frac\pi2 = \sin 90^\circ = \frac{\sqrt4}2 = 1</math> ([[right angle]])
<math display="block">\sin \frac\pi2 = \sin 90^\circ = \frac{\sqrt4}2 = 1</math> ([[right angle]])


Writing the numerators as [[square roots]] of consecutive non-negative integers, with a denominator of 2, provides an easy way to remember the values.<ref name="Larson_2013"/>
Writing the numerators as [[square roots]] of consecutive non-negative integers, with a denominator of 2, provides an easy way to remember the values.<ref name="Larson_2013"/>
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*For an angle which, measured in degrees, is a multiple of three, the [[exact trigonometric values]] of the sine and the cosine may be expressed in terms of square roots. These values of the sine and the cosine may thus be constructed by [[Compass-and-straightedge construction|ruler and compass]].
*For an angle which, measured in degrees, is a multiple of three, the [[exact trigonometric values]] of the sine and the cosine may be expressed in terms of square roots. These values of the sine and the cosine may thus be constructed by [[Compass-and-straightedge construction|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 non-real [[complex number]]. [[Galois theory]] allows a proof that, if the angle is not a multiple of 3°, non-real cube roots are unavoidable.
*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 non-real [[complex number]]. [[Galois theory]] allows a proof that, if the angle is not a multiple of 3°, non-real cube roots are unavoidable.
*For an angle which, expressed in degrees, is a [[rational number]], the sine and the cosine are [[algebraic number]]s, which may be expressed in terms of [[nth root|{{mvar|n}}th roots]]. This results from the fact that the [[Galois group]]s of the [[cyclotomic polynomial]]s are [[cyclic group|cyclic]].
*For an angle which, expressed in degrees, is a [[rational number]], the sine and the cosine are [[algebraic number]]s, which may be expressed in terms of [[nth root|{{mvar|n}}-th roots]]. This results from the fact that the [[Galois group]]s of the [[cyclotomic polynomial]]s are [[cyclic group|cyclic]].
*For an angle which, expressed in degrees, is not a rational number, then either the angle or both the sine and the cosine are [[transcendental number]]s. This is a corollary of [[Baker's theorem]], proved in 1966.
*For an angle which, expressed in degrees, is not a rational number, then either the angle or both the sine and the cosine are [[transcendental number]]s. This is a corollary of [[Baker's theorem]], proved in 1966.
*If the sine of an angle is a rational number then the cosine is not necessarily a rational number, and vice-versa. However if the tangent of an angle is rational then both the sine and cosine of the double angle will be rational.
*If the sine of an angle is a rational number then the cosine is not necessarily a rational number, and vice-versa. However, if the tangent of an angle is rational then both the sine and cosine of the double angle will be rational.


===Simple algebraic values===
===Simple algebraic values===
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{| class="wikitable" style="text-align:center;"
{| class="wikitable" style="text-align:center;"
|-
|-
! colspan=2 | Angle, ''θ'', in
! colspan=2 | Angle, {{mvar|θ}}, in
! rowspan=2 | <math>\sin(\theta)</math>
! rowspan=2 | <math>\sin(\theta)</math>
! rowspan=2 | <math>\cos(\theta)</math>
! rowspan=2 | <math>\cos(\theta)</math>
Line 213: Line 213:
[[File:Taylorreihenentwicklung des Kosinus.svg|thumb|<math>\cos(x)</math> together with the first Taylor polynomials <math>p_n(x)=\sum_{k=0}^n (-1)^k \frac{x^{2k}}{(2k)!}</math>]]
[[File:Taylorreihenentwicklung des Kosinus.svg|thumb|<math>\cos(x)</math> together with the first Taylor polynomials <math>p_n(x)=\sum_{k=0}^n (-1)^k \frac{x^{2k}}{(2k)!}</math>]]


[[G. H. Hardy]] noted in his 1908 work ''[[A Course of Pure Mathematics]]'' that the definition of the trigonometric functions in terms of the unit circle is not satisfactory, because it depends implicitly on a notion of angle that can be measured by a real number.<ref name="Hardy">{{citation|first=G.H.|last=Hardy|title=A course of pure mathematics|year=1950|edition=8th|pages=432–438}}</ref> Thus in modern analysis, trigonometric functions are usually constructed without reference to geometry.
[[G. H. Hardy]] noted in his 1908 work ''[[A Course of Pure Mathematics]]'' that the definition of the trigonometric functions in terms of the unit circle is not satisfactory, because it depends implicitly on a notion of angle that can be measured by a real number.{{clarify|date=September 2025}}<ref name="Hardy">{{citation|first=G.H.|last=Hardy|title=A course of pure mathematics|year=1950|edition=8th|pages=432–438}}</ref> Thus in modern analysis, trigonometric functions are usually constructed without reference to geometry.


Various ways exist in the literature for defining the trigonometric functions in a manner suitable for analysis; they include:
Various ways exist in the literature for defining the trigonometric functions in a manner suitable for analysis; they include:
* Using the "geometry" of the unit circle, which requires formulating the arc length of a circle (or area of a sector) analytically.<ref name="Hardy"/>
* Using the "geometry" of the unit circle, which requires formulating the arc length of a circle (or area of a sector) analytically.<ref name="Hardy"/>
* By a power series, which is particularly well-suited to complex variables.<ref name="Hardy"/><ref name="WW">Whittaker, E. T., & Watson, G. N. (1920). A course of modern analysis: an introduction to the general theory of infinite processes and of analytic functions; with an account of the principal transcendental functions. University press.</ref>
* By a [[power series]], which is particularly well-suited to complex variables.<ref name="Hardy"/><ref name="WW">Whittaker, E. T., & Watson, G. N. (1920). A course of modern analysis: an introduction to the general theory of infinite processes and of analytic functions; with an account of the principal transcendental functions. University press.</ref>
* By using an infinite product expansion.<ref name="Hardy"/>
* By using an infinite product expansion.<ref name="Hardy"/>
* By inverting the inverse trigonometric functions, which can be defined as integrals of algebraic or rational functions.<ref name="Hardy"/>
* By inverting the inverse trigonometric functions, which can be defined as integrals of algebraic or rational functions.<ref name="Hardy"/>
Line 225: Line 225:


Sine and cosine can be defined as the unique solution to the [[initial value problem]]:{{sfn|Bartle|Sherbert|1999|p=247}}
Sine and cosine can be defined as the unique solution to the [[initial value problem]]:{{sfn|Bartle|Sherbert|1999|p=247}}
:<math>\frac{d}{dx}\sin x= \cos x,\ \frac{d}{dx}\cos x= -\sin x,\ \sin(0)=0,\ \cos(0)=1. </math>
<math display="block">\frac{d}{dx}\sin x= \cos x,\ \frac{d}{dx}\cos x= -\sin x,\ \sin(0)=0,\ \cos(0)=1.</math>


Differentiating again, <math display="inline">\frac{d^2}{dx^2}\sin x = \frac{d}{dx}\cos x = -\sin x</math> and <math display="inline">\frac{d^2}{dx^2}\cos x = -\frac{d}{dx}\sin x = -\cos x</math>, so both sine and cosine are solutions of the same [[ordinary differential equation]]
Differentiating again, <math display="inline">\frac{d^2}{dx^2}\sin x = \frac{d}{dx}\cos x = -\sin x</math> and <math display="inline">\frac{d^2}{dx^2}\cos x = -\frac{d}{dx}\sin x = -\cos x</math>, so both sine and cosine are solutions of the same [[ordinary differential equation]]
:<math>y''+y=0\,.</math>
<math display="block">y''+y=0\,.</math>
Sine is the unique solution with {{math|''y''(0) {{=}} 0}} and {{math|''y''′(0) {{=}} 1}}; cosine is the unique solution with {{math|''y''(0) {{=}} 1}} and {{math|''y''′(0) {{=}} 0}}.
Sine is the unique solution with {{math|''y''(0) {{=}} 0}} and {{math|''y''′(0) {{=}} 1}}; cosine is the unique solution with {{math|''y''(0) {{=}} 1}} and {{math|''y''′(0) {{=}} 0}}.


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Applying the [[quotient rule]] to the tangent <math>\tan x = \sin x / \cos x</math>,  
Applying the [[quotient rule]] to the tangent <math>\tan x = \sin x / \cos x</math>,  
:<math>\frac{d}{dx}\tan x = \frac{\cos^2 x + \sin^2 x}{\cos^2 x} = 1+\tan^2 x\,,</math>
<math display="block">\frac{d}{dx}\tan x = \frac{\cos^2 x + \sin^2 x}{\cos^2 x} = 1+\tan^2 x\,,</math>
so the tangent function satisfies the ordinary differential equation
so the tangent function satisfies the ordinary differential equation
:<math>y' = 1 + y^2\,.</math>
<math display="block">y' = 1 + y^2\,.</math>
It is the unique solution with {{math|''y''(0) {{=}} 0}}.
It is the unique solution with {{math|''y''(0) {{=}} 0}}.


===Power series expansion===
===Power series expansion===
The basic trigonometric functions can be defined by the following power series expansions.<ref>Whitaker and Watson, p 584</ref> These series are also known as the [[Taylor series]] or [[Maclaurin series]] of these trigonometric functions:
The basic trigonometric functions can be defined by the following [[power series]] expansions.<ref>Whitaker and Watson, p 584</ref> These series are also known as the [[Taylor series]] or [[Maclaurin series]] of these trigonometric functions:
:<math>
<math display="block">
\begin{align}
\begin{align}
\sin x & = x - \frac{x^3}{3!} + \frac{x^5}{5!} - \frac{x^7}{7!} + \cdots \\[6mu]
\sin x &= x - \frac{x^3}{3!} + \frac{x^5}{5!} - \frac{x^7}{7!} + \cdots &&= \sum_{n=0}^\infty (-1)^n \frac{x^{2n+1}}{(2n+1)!} \\
& = \sum_{n=0}^\infty \frac{(-1)^n}{(2n+1)!}x^{2n+1} \\[8pt]
\cos x & = 1 - \frac{x^2}{2!} + \frac{x^4}{4!} - \frac{x^6}{6!} + \cdots &&= \sum_{n=0}^\infty (-1)^n \frac{x^{2n}}{(2n)!}
\cos x & = 1 - \frac{x^2}{2!} + \frac{x^4}{4!} - \frac{x^6}{6!} + \cdots \\[6mu]
& = \sum_{n=0}^\infty \frac{(-1)^n}{(2n)!}x^{2n}.
\end{align}
\end{align}
</math>
</math>
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More precisely, defining
More precisely, defining
: {{mvar|U<sub>n</sub>}}, the {{mvar|n}}th [[up/down number]],
: {{mvar|U<sub>n</sub>}}, the {{mvar|n}}-th [[up/down number]],
: {{mvar|B<sub>n</sub>}}, the {{mvar|n}}th [[Bernoulli number]], and
: {{mvar|B<sub>n</sub>}}, the {{mvar|n}}-th [[Bernoulli number]], and
: {{mvar|E<sub>n</sub>}}, is the {{mvar|n}}th [[Euler number]],
: {{mvar|E<sub>n</sub>}}, is the {{mvar|n}}-th [[Euler number]],
one has the following series expansions:<ref>Abramowitz; Weisstein.</ref>  
one has the following series expansions:<ref>Abramowitz; Weisstein.</ref>  
: <math>
<math display="block">
\begin{align}
\begin{align}
\tan x & {} = \sum_{n=0}^\infty \frac{U_{2n+1}}{(2n+1)!}x^{2n+1} \\[8mu]
\tan x & {} = \sum_{n=0}^\infty \frac{U_{2n+1}}{(2n+1)!}x^{2n+1} \\[8mu]
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</math>
</math>


: <math>
<math display="block">
\begin{align}
\begin{align}
\csc x &= \sum_{n=0}^\infty \frac{(-1)^{n+1} 2 \left(2^{2n-1}-1\right) B_{2n}}{(2n)!}x^{2n-1} \\[5mu]
\csc x &= \sum_{n=0}^\infty \frac{(-1)^{n+1} 2 \left(2^{2n-1}-1\right) B_{2n}}{(2n)!}x^{2n-1} \\[5mu]
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</math>
</math>


: <math>
<math display="block">
\begin{align}
\begin{align}
\sec x &= \sum_{n=0}^\infty \frac{U_{2n}}{(2n)!}x^{2n}
\sec x &= \sum_{n=0}^\infty \frac{U_{2n}}{(2n)!}x^{2n}
Line 285: Line 283:
</math>
</math>


: <math>
<math display="block">
\begin{align}
\begin{align}
\cot x &= \sum_{n=0}^\infty \frac{(-1)^n 2^{2n} B_{2n}}{(2n)!}x^{2n-1} \\[5mu]
\cot x &= \sum_{n=0}^\infty \frac{(-1)^n 2^{2n} B_{2n}}{(2n)!}x^{2n-1} \\[5mu]
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The following [[continued fraction]]s are valid in the whole complex plane:
The following [[continued fraction]]s are valid in the whole complex plane:


:<math> \sin x =
<ref>C. D. Olds, Continued fractions, 1963, Random House, Inc., p. 138, pp 11, (without authorship)</ref>
<math display="block">\sin x =
\cfrac{x}{1 + \cfrac{x^2}{2\cdot3-x^2 +
\cfrac{x}{1 + \cfrac{x^2}{2\cdot3-x^2 +
\cfrac{2\cdot3 x^2}{4\cdot5-x^2 +
\cfrac{2\cdot3 x^2}{4\cdot5-x^2 +
\cfrac{4\cdot5 x^2}{6\cdot7-x^2 + \ddots}}}}</math>
\cfrac{4\cdot5 x^2}{6\cdot7-x^2 + \ddots}}}}</math>


:<math> \cos x = \cfrac{1}{1 + \cfrac{x^2}{1 \cdot 2 - x^2 + \cfrac{1 \cdot 2x^2}{3 \cdot 4 - x^2 + \cfrac{3 \cdot 4x^2}{5 \cdot 6 - x^2 + \ddots}}}}</math>
<math display="block">\cos x = \cfrac{1}{1 + \cfrac{x^2}{1 \cdot 2 - x^2 + \cfrac{1 \cdot 2x^2}{3 \cdot 4 - x^2 + \cfrac{3 \cdot 4x^2}{5 \cdot 6 - x^2 + \ddots}}}}</math>


:<math>\tan x = \cfrac{x}{1 - \cfrac{x^2}{3 - \cfrac{x^2}{5 - \cfrac{x^2}{7 - \ddots}}}}=\cfrac{1}{\cfrac{1}{x} - \cfrac{1}{\cfrac{3}{x} - \cfrac{1}{\cfrac{5}{x} - \cfrac{1}{\cfrac{7}{x} - \ddots}}}}</math>
{{citation needed|date=October 2025|reason=In MATHEMATICAL ANALYSIS Functions, Limits, Series,Continued Fractions. E d i t e d b y L. A. LYUSTERNIK and A. R. YANPOL’SKII
T r a n s l a t e d b y D. E. BROWN T r a n s l a t i o n e d i t e d b y E. SPENCE,1965, PERGAMON PRESS, OXFORD • LONDON • EDINBURGH • NEW YORK
p.279 "The general form of the expansion as a continued fraction of sin x
is not known."
p.280 "The general form of the expansion as a continued fraction of cos x
is unknown."
 
Question: Where do these continued fractions for sin(x) and cos(x) come from?}}
 
 
<math display="block">\tan x = \cfrac{x}{1 - \cfrac{x^2}{3 - \cfrac{x^2}{5 - \cfrac{x^2}{7 - \ddots}}}}=\cfrac{1}{\cfrac{1}{x} - \cfrac{1}{\cfrac{3}{x} - \cfrac{1}{\cfrac{5}{x} - \cfrac{1}{\cfrac{7}{x} - \ddots}}}}</math>


The last one was used in the historically first [[proof that π is irrational]].<ref>{{citation|editor1-last = Berggren|editor1-first = Lennart|editor2-last = Borwein|editor2-first = Jonathan M.|editor2-link = Jonathan M. Borwein| editor3-last = Borwein|editor3-first = Peter B.|editor3-link = Peter B. Borwein|last = Lambert|first = Johann Heinrich|orig-year = 1768|chapter = Mémoire sur quelques propriétés remarquables des quantités transcendantes circulaires et logarithmiques|title = Pi, a source book|place = New York|publisher = [[Springer Science+Business Media|Springer-Verlag]] |year = 2004|edition = 3rd|pages = 129&ndash;140|isbn = 0-387-20571-3}}</ref>
The last one was used in the historically first [[proof that π is irrational]].<ref>{{citation|editor1-last = Berggren|editor1-first = Lennart|editor2-last = Borwein|editor2-first = Jonathan M.|editor2-link = Jonathan M. Borwein| editor3-last = Borwein|editor3-first = Peter B.|editor3-link = Peter B. Borwein|last = Lambert|first = Johann Heinrich|orig-year = 1768|chapter = Mémoire sur quelques propriétés remarquables des quantités transcendantes circulaires et logarithmiques|title = Pi, a source book|place = New York|publisher = [[Springer Science+Business Media|Springer-Verlag]] |year = 2004|edition = 3rd|pages = 129&ndash;140|isbn = 0-387-20571-3}}</ref>
There is a rapidly convergent continued fraction for <math >\tan(x)</math>:
<ref>{{cite book |last1=Khovanski |first1=A. N. |title=The Applications Of Continued Fractions And Their Generalizations To Problems In Approximation Theory |publisher=Noordhoff |year=1963 |location=Groningen, The Netherlands}}</ref>
<math display="block">\tan x=1+\cfrac{5x^2}{T_{0}+5x^2}, T_{k}= (4k+1)(4k+3)(4k+5)-4x^2(4k+3)+ \cfrac{x^2(4k+1)}{1+ \cfrac{x^2(4k+9)}{T_{k+1}}}</math>
Let <math>x=1</math> then the following continued fraction representation gives (asymptotically) 12.68 new correct decimal places per cycle:
<math display="block">\tan 1=1+\cfrac{5}{T_{0}+5}, T_{k}= (4k+1)(4k+3)(4k+5)-4(4k+3)+ \cfrac{4k+1}{1+ \cfrac{4k+9}{T_{k+1}}}</math>


===Partial fraction expansion===
===Partial fraction expansion===


There is a series representation as [[partial fraction expansion]] where just translated [[Multiplicative inverse|reciprocal function]]s are summed up, such that the [[Pole (complex analysis)|pole]]s of the cotangent function and the reciprocal functions match:<ref name="Aigner_2000"/>
There is a series representation as [[partial fraction expansion]] where just translated [[Multiplicative inverse|reciprocal function]]s are summed up, such that the [[Pole (complex analysis)|pole]]s of the cotangent function and the reciprocal functions match:<ref name="Aigner_2000"/>
: <math>
<math display="block">
\pi \cot \pi x = \lim_{N\to\infty}\sum_{n=-N}^N \frac{1}{x+n}.
\pi \cot \pi x = \lim_{N\to\infty}\sum_{n=-N}^N \frac{1}{x+n}.
</math>
</math>
This identity can be proved with the [[Gustav Herglotz|Herglotz]] trick.<ref name="Remmert_1991"/>
This identity can be proved with the [[Gustav Herglotz|Herglotz]] trick.<ref name="Remmert_1991"/>
Combining the {{math|(–''n'')}}th with the {{math|''n''}}th term lead to [[absolute convergence|absolutely convergent]] series:
Combining the {{math|(–''n'')}}-th with the {{mvar|n}}-th term lead to [[absolute convergence|absolutely convergent]] series:
:<math>
<math display="block">
\pi \cot \pi x = \frac{1}{x} + 2x\sum_{n=1}^\infty \frac{1}{x^2-n^2}.
\pi \cot \pi x = \frac{1}{x} + 2x\sum_{n=1}^\infty \frac{1}{x^2-n^2}.
</math>
</math>
Similarly, one can find a partial fraction expansion for the secant, cosecant and tangent functions:
Similarly, one can find a partial fraction expansion for the secant, cosecant and tangent functions:
:<math>
<math display="block">
\pi\csc\pi x = \sum_{n=-\infty}^\infty \frac{(-1)^n}{x+n}=\frac{1}{x} + 2x\sum_{n=1}^\infty \frac{(-1)^n}{x^2-n^2},
\pi\csc\pi x = \sum_{n=-\infty}^\infty \frac{(-1)^n}{x+n}=\frac{1}{x} + 2x\sum_{n=1}^\infty \frac{(-1)^n}{x^2-n^2},
</math>
</math>
:<math>\pi^2\csc^2\pi x=\sum_{n=-\infty}^\infty \frac{1}{(x+n)^2},</math>
<math display="block">\pi^2\csc^2\pi x=\sum_{n=-\infty}^\infty \frac{1}{(x+n)^2},</math>
:<math>
<math display="block">
\pi\sec\pi x = \sum_{n=0}^\infty (-1)^n \frac{(2n+1)}{(n+\tfrac12)^2 - x^2},
\pi\sec\pi x = \sum_{n=0}^\infty (-1)^n \frac{(2n+1)}{(n+\tfrac12)^2 - x^2},
</math>
</math>
:<math>
<math display="block">
\pi \tan \pi x = 2x\sum_{n=0}^\infty \frac{1}{(n+\tfrac12)^2 - x^2}.
\pi \tan \pi x = 2x\sum_{n=0}^\infty \frac{1}{(n+\tfrac12)^2 - x^2}.
</math>
</math>
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===Infinite product expansion===
===Infinite product expansion===
The following infinite product for the sine is due to [[Leonhard Euler]], and is of great importance in complex analysis:<ref>Whittaker and Watson, p 137</ref>
The following infinite product for the sine is due to [[Leonhard Euler]], and is of great importance in complex analysis:<ref>Whittaker and Watson, p 137</ref>
:<math>\sin z = z \prod_{n=1}^\infty \left(1-\frac{z^2}{n^2 \pi^2}\right), \quad z\in\mathbb C.</math>
<math display="block">\sin z = z \prod_{n=1}^\infty \left(1-\frac{z^2}{n^2 \pi^2}\right), \quad z\in\mathbb C.</math>
This may be obtained from the partial fraction decomposition of <math>\cot z</math> given above, which is the logarithmic derivative of <math>\sin z</math>.<ref>Ahlfors, p 197</ref> From this, it can be deduced also that
This may be obtained from the partial fraction decomposition of <math>\cot z</math> given above, which is the logarithmic derivative of <math>\sin z</math>.<ref>Ahlfors, p 197</ref> From this, it can be deduced also that
:<math>\cos z = \prod_{n=1}^\infty \left(1-\frac{z^2}{(n-1/2)^2 \pi^2}\right), \quad z\in\mathbb C.</math>
<math display="block">\cos z = \prod_{n=1}^\infty \left(1-\frac{z^2}{(n-1/2)^2 \pi^2}\right), \quad z\in\mathbb C.</math>


=== Euler's formula and the exponential function ===
=== Euler's formula and the exponential function ===
Line 340: Line 362:


[[Euler's formula]] relates sine and cosine to the [[exponential function]]:
[[Euler's formula]] relates sine and cosine to the [[exponential function]]:
:<math> e^{ix}  = \cos x + i\sin x.</math>  
<math display="block">e^{ix}  = \cos x + i\sin x.</math>  
This formula is commonly considered for real values of {{mvar|x}}, but it remains true for all complex values.
This formula is commonly considered for real values of {{mvar|x}}, but it remains true for all complex values.


Line 346: Line 368:


One has
One has
:<math>\begin{align}
<math display="block">\begin{align}
e^{ix}  &= \cos x + i\sin x\\[5pt]
e^{ix}  &= \cos x + i\sin x\\[5pt]
e^{-ix}  &= \cos x - i\sin x.
e^{-ix}  &= \cos x - i\sin x.
Line 352: Line 374:


Solving this [[linear system]] in sine and cosine, one can express them in terms of the exponential function:
Solving this [[linear system]] in sine and cosine, one can express them in terms of the exponential function:
: <math>\begin{align}\sin x &= \frac{e^{i x} - e^{-i x}}{2i}\\[5pt]
<math display="block">\begin{align}\sin x &= \frac{e^{i x} - e^{-i x}}{2i}\\[5pt]
\cos x &= \frac{e^{i x} + e^{-i x}}{2}.
\cos x &= \frac{e^{i x} + e^{-i x}}{2}.
\end{align}</math>
\end{align}</math>


When {{mvar|x}} is real, this may be rewritten as  
When {{mvar|x}} is real, this may be rewritten as  
: <math>\cos x = \operatorname{Re}\left(e^{i x}\right), \qquad \sin x = \operatorname{Im}\left(e^{i x}\right).</math>
<math display="block">\cos x = \operatorname{Re}\left(e^{i x}\right), \qquad \sin x = \operatorname{Im}\left(e^{i x}\right).</math>


Most [[List of trigonometric identities|trigonometric identities]] can be proved by expressing trigonometric functions in terms of the complex exponential function by using above formulas, and then using the identity <math>e^{a+b}=e^ae^b</math> for simplifying the result.
Most [[List of trigonometric identities|trigonometric identities]] can be proved by expressing trigonometric functions in terms of the complex exponential function by using above formulas, and then using the identity <math>e^{a+b}=e^ae^b</math> for simplifying the result.
Line 363: Line 385:
Euler's formula can also be used to define the basic trigonometric function directly, as follows, using the language of [[topological group]]s.<ref>{{cite book |last=Bourbaki |first=Nicolas |author-link=Nicolas Bourbaki |title=Topologie generale |publisher=Springer |year=1981|at=§VIII.2}}</ref> The set <math>U</math> of complex numbers of unit modulus is a compact and connected topological group, which has a neighborhood of the identity that is homeomorphic to the real line. Therefore, it is isomorphic as a topological group to the one-dimensional torus group <math>\mathbb R/\mathbb Z</math>, via an isomorphism
Euler's formula can also be used to define the basic trigonometric function directly, as follows, using the language of [[topological group]]s.<ref>{{cite book |last=Bourbaki |first=Nicolas |author-link=Nicolas Bourbaki |title=Topologie generale |publisher=Springer |year=1981|at=§VIII.2}}</ref> The set <math>U</math> of complex numbers of unit modulus is a compact and connected topological group, which has a neighborhood of the identity that is homeomorphic to the real line. Therefore, it is isomorphic as a topological group to the one-dimensional torus group <math>\mathbb R/\mathbb Z</math>, via an isomorphism
<math display="block">e:\mathbb R/\mathbb Z\to U.</math>
<math display="block">e:\mathbb R/\mathbb Z\to U.</math>
In pedestrian terms <math>e(t) = \exp(2\pi i t)</math>, and this isomorphism is unique up to taking complex conjugates.
In simple terms, <math>e(t) = \exp(2\pi i t)</math>, and this isomorphism is unique up to taking complex conjugates.


For a nonzero real number <math>a</math> (the ''base''), the function <math>t\mapsto e(t/a)</math> defines an isomorphism of the group <math>\mathbb R/a\mathbb Z\to U</math>. The real and imaginary parts of <math>e(t/a)</math> are the cosine and sine, where <math>a</math> is used as the base for measuring angles. For example, when <math>a=2\pi</math>, we get the measure in radians, and the usual trigonometric functions. When <math>a=360</math>, we get the sine and cosine of angles measured in degrees.
For a nonzero real number <math>a</math> (the ''base''), the function <math>t\mapsto e(t/a)</math> defines an isomorphism of the group <math>\mathbb R/a\mathbb Z\to U</math>. The real and imaginary parts of <math>e(t/a)</math> are the cosine and sine, where <math>a</math> is used as the base for measuring angles. For example, when <math>a=2\pi</math>, we get the measure in radians, and the usual trigonometric functions. When <math>a=360</math>, we get the sine and cosine of angles measured in degrees.
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For example,<ref name="Kannappan_2009"/> the sine and the cosine form the unique pair of [[continuous function]]s that satisfy the difference formula
For example,<ref name="Kannappan_2009"/> the sine and the cosine form the unique pair of [[continuous function]]s that satisfy the difference formula
: <math>\cos(x- y) = \cos x\cos y + \sin x\sin y\,</math>
<math display="block">\cos(x- y) = \cos x\cos y + \sin x\sin y\,</math>
and the added condition
and the added condition
: <math>0 < x\cos x < \sin x < x\quad\text{ for }\quad 0 < x < 1.</math>
<math display="block">0 < x\cos x < \sin x < x\quad\text{ for }\quad 0 < x < 1.</math>


===In the complex plane===
===In the complex plane===
The sine and cosine of a [[complex number]] <math>z=x+iy</math> can be expressed in terms of real sines, cosines, and [[hyperbolic function]]s as follows:
The sine and cosine of a [[complex number]] <math>z=x+iy</math> can be expressed in terms of real sines, cosines, and [[hyperbolic function]]s as follows:
: <math>\begin{align}\sin z &= \sin x \cosh y + i \cos x \sinh y\\[5pt]
<math display="block">\begin{align}\sin z &= \sin x \cosh y + i \cos x \sinh y\\[5pt]
\cos z &= \cos x \cosh y - i \sin x \sinh y\end{align}</math>
\cos z &= \cos x \cosh y - i \sin x \sinh y\end{align}</math>


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===Parity===
===Parity===
The cosine and the secant are [[even function]]s; the other trigonometric functions are [[odd function]]s. That is:
The cosine and the secant are [[even function]]s; the other trigonometric functions are [[odd function]]s. That is:
:<math>\begin{align}
<math display="block">\begin{align}
\sin(-x) &=-\sin x\\
\sin(-x) &=-\sin x\\
\cos(-x) &=\cos x\\
\cos(-x) &=\cos x\\
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===Periods===
===Periods===
All trigonometric functions are [[periodic function]]s of period {{math|2{{pi}}}}. This is the smallest period, except for the tangent and the cotangent, which have {{pi}} as smallest period. This means that, for every integer {{mvar|k}}, one has
All trigonometric functions are [[periodic function]]s of period {{math|2{{pi}}}}. This is the smallest period, except for the tangent and the cotangent, which have {{pi}} as smallest period. This means that, for every integer {{mvar|k}}, one has
:<math>\begin{array}{lrl}
<math display="block">\begin{array}{lrl}
\sin(x+&2k\pi) &=\sin x \\
\sin(x+&2k\pi) &=\sin x \\
\cos(x+&2k\pi) &=\cos x \\
\cos(x+&2k\pi) &=\cos x \\
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The Pythagorean identity, is the expression of the [[Pythagorean theorem]] in terms of trigonometric functions. It is  
The Pythagorean identity, is the expression of the [[Pythagorean theorem]] in terms of trigonometric functions. It is  
:<math>\sin^2 x  + \cos^2 x  = 1</math>.
<math display="block">\sin^2 x  + \cos^2 x  = 1</math>.
Dividing through by either <math>\cos^2 x</math> or <math>\sin^2 x</math> gives
Dividing through by either <math>\cos^2 x</math> or <math>\sin^2 x</math> gives
:<math>\tan^2 x  + 1  = \sec^2 x</math>
<math display="block">\tan^2 x  + 1  = \sec^2 x</math>
:<math>1  + \cot^2 x  = \csc^2 x</math>
<math display="block">1  + \cot^2 x  = \csc^2 x</math>
and
and
:<math>\sec^2 x  + \csc^2 x  = \sec^2 x \csc^2 x</math>.
<math display="block">\sec^2 x  + \csc^2 x  = \sec^2 x \csc^2 x</math>.


===Sum and difference formulas===
===Sum and difference formulas===
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The sum and difference formulas allow expanding the sine, the cosine, and the tangent of a sum or a difference of two angles in terms of sines and cosines and tangents of the angles themselves. These can be derived geometrically, using arguments that date to [[Ptolemy]] (see [[List_of_trigonometric_identities#Angle_sum_and_difference_identities|Angle sum and difference identities]]). One can also produce them algebraically using [[Euler's formula]].
The sum and difference formulas allow expanding the sine, the cosine, and the tangent of a sum or a difference of two angles in terms of sines and cosines and tangents of the angles themselves. These can be derived geometrically, using arguments that date to [[Ptolemy]] (see [[List_of_trigonometric_identities#Angle_sum_and_difference_identities|Angle sum and difference identities]]). One can also produce them algebraically using [[Euler's formula]].
; Sum
; Sum
:<math>\begin{align}
<math display="block">\begin{align}
\sin\left(x+y\right)&=\sin x \cos y + \cos x \sin y,\\[5mu]
\sin\left(x+y\right)&=\sin x \cos y + \cos x \sin y,\\[5mu]
\cos\left(x+y\right)&=\cos x \cos y - \sin x \sin y,\\[5mu]
\cos\left(x+y\right)&=\cos x \cos y - \sin x \sin y,\\[5mu]
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\end{align}</math>
\end{align}</math>
; Difference
; Difference
:<math>\begin{align}
<math display="block">\begin{align}
\sin\left(x-y\right)&=\sin x \cos y - \cos x \sin y,\\[5mu]
\sin\left(x-y\right)&=\sin x \cos y - \cos x \sin y,\\[5mu]
\cos\left(x-y\right)&=\cos x \cos y + \sin x \sin y,\\[5mu]
\cos\left(x-y\right)&=\cos x \cos y + \sin x \sin y,\\[5mu]
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When the two angles are equal, the sum formulas reduce to simpler equations known as the [[double-angle formulae]].
When the two angles are equal, the sum formulas reduce to simpler equations known as the [[double-angle formulae]].


:<math>\begin{align}
<math display="block">\begin{align}
\sin 2x &= 2 \sin x \cos x = \frac{2\tan x}{1+\tan^2 x}, \\[5mu]
\sin 2x &= 2 \sin x \cos x = \frac{2\tan x}{1+\tan^2 x}, \\[5mu]
\cos 2x &= \cos^2 x - \sin^2 x = 2 \cos^2 x - 1 = 1 - 2 \sin^2 x = \frac{1-\tan^2 x}{1+\tan^2 x},\\[5mu]
\cos 2x &= \cos^2 x - \sin^2 x = 2 \cos^2 x - 1 = 1 - 2 \sin^2 x = \frac{1-\tan^2 x}{1+\tan^2 x},\\[5mu]
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These identities can be used to derive the [[product-to-sum identities]].
These identities can be used to derive the [[product-to-sum identities]].


By setting <math>t=\tan \tfrac12 \theta,</math> all trigonometric functions of <math>\theta</math> can be expressed as [[rational fraction]]s of <math>t</math>:
By setting <math>t=\tan \tfrac12 \theta</math> (see [[List_of_trigonometric_identities#Half-angle_formulae|half-angle formulae]]), all trigonometric functions of <math>\theta</math> can be expressed as [[rational fraction]]s of <math>t</math>:
:<math>\begin{align}
<math display="block">\begin{align}
\sin \theta &= \frac{2t}{1+t^2}, \\[5mu]
\sin \theta &= \frac{2t}{1+t^2}, \\[5mu]
\cos \theta &= \frac{1-t^2}{1+t^2},\\[5mu]
\cos \theta &= \frac{1-t^2}{1+t^2},\\[5mu]
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\end{align}</math>
\end{align}</math>
Together with  
Together with  
:<math>d\theta = \frac{2}{1+t^2} \, dt,</math>
<math display="block">d\theta = \frac{2}{1+t^2} \, dt,</math>
this is the [[tangent half-angle substitution]], which reduces the computation of [[integral]]s and [[antiderivative]]s of trigonometric functions to that of rational fractions.
this is the [[tangent half-angle substitution]], which reduces the computation of [[integral]]s and [[antiderivative]]s of trigonometric functions to that of rational fractions.


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|<math>\cot x</math>||<math>-\csc^2 x</math>||<math>-\ln \left| \csc x \right| + C</math>
|<math>\cot x</math>||<math>-\csc^2 x</math>||<math>-\ln \left| \csc x \right| + C</math>
|}
|}
Note: For <math>0<x<\pi</math> the integral of <math>\csc x</math> can also be written as <math>-\operatorname{arsinh}(\cot x),</math> and for the integral of <math>\sec x</math> for <math>-\pi/2<x<\pi/2</math> as <math>\operatorname{arsinh}(\tan x),</math> where <math>\operatorname{arsinh}</math> is the [[inverse hyperbolic sine]].
Note: For <math>0<x<\pi</math> the integral of <math>\csc x</math> can also be written as <math>-\operatorname{arsinh}(\cot x),</math> and the integral of <math>\sec x</math> for <math>-\pi/2<x<\pi/2</math> as <math>\operatorname{arsinh}(\tan x),</math> where <math>\operatorname{arsinh}</math> is the [[inverse hyperbolic sine]].


Alternatively, the derivatives of the 'co-functions' can be obtained using trigonometric identities and the chain rule:
Alternatively, the derivatives of the 'co-functions' can be obtained using trigonometric identities and the chain rule:


:<math>
<math display="block">
\begin{align}
\begin{align}
\frac{d\cos x}{dx} &= \frac{d}{dx}\sin(\pi/2-x)=-\cos(\pi/2-x)=-\sin x \, , \\
\frac{d\cos x}{dx} &= \frac{d}{dx}\sin(\pi/2-x)=-\cos(\pi/2-x)=-\sin x \, , \\
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{{main|Law of tangents}}
{{main|Law of tangents}}
The law of tangents says that:
The law of tangents says that:
:<math>\frac{\tan \frac{A-B}{2 }}{\tan \frac{A+B}{2 } } = \frac{a-b}{a+b}</math>.
<math display="block">\frac{\tan \frac{A-B}{2 }}{\tan \frac{A+B}{2 } } = \frac{a-b}{a+b}</math>.


====Law of cotangents====
====Law of cotangents====
{{main|Law of cotangents}}
{{main|Law of cotangents}}
If ''s'' is the triangle's semiperimeter, (''a'' + ''b'' + ''c'')/2, and ''r'' is the radius of the triangle's [[incircle]], then ''rs'' is the triangle's area. Therefore [[Heron's formula]] implies that:
If {{mvar|s}} is the triangle's semiperimeter, {{math|(''a'' + ''b'' + ''c'')/2}}, and {{mvar|r}} is the radius of the triangle's [[incircle]], then {{math|''rs''}} is the triangle's area. Therefore [[Heron's formula]] implies that:


:<math> r = \sqrt{\frac{1}{s} (s-a)(s-b)(s-c)}</math>.
<math display="block">r = \sqrt{\frac{1}{s} (s-a)(s-b)(s-c)}</math>.


The law of cotangents says that:<ref name="Allen_1976"/>
The law of cotangents says that:<ref name="Allen_1976"/>
:<math>\cot{ \frac{A}{2}} = \frac{s-a}{r}</math>
<math display="block">\cot{ \frac{A}{2}} = \frac{s-a}{r}</math>
It follows that
It follows that
:<math>\frac{\cot \dfrac{A}{2}}{s-a}=\frac{\cot \dfrac{B}{2}}{s-b}=\frac{\cot \dfrac{C}{2}}{s-c}=\frac{1}{r}.</math>
<math display="block">\frac{\cot \dfrac{A}{2}}{s-a}=\frac{\cot \dfrac{B}{2}}{s-b}=\frac{\cot \dfrac{C}{2}}{s-c}=\frac{1}{r}.</math>


===Periodic functions===
===Periodic functions===
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Under rather general conditions, a periodic function {{math|1=''f''&hairsp;(''x'')}} can be expressed as a sum of sine waves or cosine waves in a [[Fourier series]].<ref name="Folland_1992"/> Denoting the sine or cosine [[basis functions]] by {{mvar|φ<sub>k</sub>}}, the expansion of the periodic function {{math|1=''f''&hairsp;(''t'')}} takes the form:
Under rather general conditions, a periodic function {{math|1=''f''&hairsp;(''x'')}} can be expressed as a sum of sine waves or cosine waves in a [[Fourier series]].<ref name="Folland_1992"/> Denoting the sine or cosine [[basis functions]] by {{mvar|φ<sub>k</sub>}}, the expansion of the periodic function {{math|1=''f''&hairsp;(''t'')}} takes the form:
<math display="block">f(t) = \sum _{k=1}^\infty c_k \varphi_k(t). </math>
<math display="block">f(t) = \sum _{k=1}^\infty c_k \varphi_k(t).</math>


For example, the [[Square wave (waveform)|square wave]] can be written as the [[Fourier series]]
For example, the [[Square wave (waveform)|square wave]] can be written as the [[Fourier series]]
<math display="block"> f_\text{square}(t) = \frac{4}{\pi} \sum_{k=1}^\infty {\sin \big( (2k-1)t \big) \over 2k-1}.</math>
<math display="block">f_\text{square}(t) = \frac{4}{\pi} \sum_{k=1}^\infty {\sin \big( (2k-1)t \big) \over 2k-1}.</math>


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.
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.
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==History==
==History==
{{Main|History of trigonometry}}
{{Main|History of trigonometry}}
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 (geometry)|chord]] function was defined by [[Hipparchus]] of [[İznik|Nicaea]] (180–125&nbsp;BCE) and [[Ptolemy]] of [[Egypt (Roman province)|Roman Egypt]] (90–165&nbsp;CE). The functions of sine and [[versine]] (1 cosine) are closely related to the [[Jyā, koti-jyā and utkrama-jyā|''jyā'' and ''koti-jyā'']] functions used in [[Gupta period]] [[Indian astronomy]] (''[[Aryabhatiya]]'', ''[[Surya Siddhanta]]''), via translation from Sanskrit to Arabic and then from Arabic to Latin.<ref name="Boyer_1991"/> (See [[Aryabhata's sine table]].)
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 (geometry)|chord]] function was defined by [[Hipparchus]] of [[İznik|Nicaea]] (180–125&nbsp;BCE) and [[Ptolemy]] of [[Egypt (Roman province)|Roman Egypt]] (90–165&nbsp;CE). The functions of sine and [[versine]] (1 cosine) are closely related to the [[Jyā, koti-jyā and utkrama-jyā|''jyā'' and ''koti-jyā'']] functions used in [[Gupta period]] [[Indian astronomy]] (''[[Aryabhatiya]]'', ''[[Surya Siddhanta]]''), via translation from Sanskrit to Arabic and then from Arabic to Latin.<ref name="Boyer_1991"/> (See [[Aryabhata's sine table]].)


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]].<ref name="Gingerich_1986"/> [[Al-Khwārizmī]] (c. 780–850) produced tables of sines and cosines. Circa 860, [[Habash al-Hasib al-Marwazi]] defined the tangent and the cotangent, and produced their tables.<ref name="Sesiano">Jacques Sesiano, "Islamic mathematics", p. 157, in {{Cite book |title=Mathematics Across Cultures: The History of Non-western Mathematics |editor1-first=Helaine |editor1-last=Selin |editor1-link=Helaine Selin |editor2-first=Ubiratan |editor2-last=D'Ambrosio |editor2-link=Ubiratan D'Ambrosio |year=2000 |publisher=[[Springer Science+Business Media]] |isbn=978-1-4020-0260-1}}</ref><ref name="Britannica">{{cite web |title=trigonometry |date=17 November 2023 |url=http://www.britannica.com/EBchecked/topic/605281/trigonometry |publisher=Encyclopedia Britannica}}</ref> [[Muhammad ibn Jābir al-Harrānī al-Battānī]] (853–929) defined the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.<ref name="Britannica"/> The trigonometric functions were later studied by mathematicians including [[Omar Khayyám]], [[Bhāskara II]], [[Nasir al-Din al-Tusi]], [[Jamshīd al-Kāshī]] (14th century), [[Ulugh Beg]] (14th century), [[Regiomontanus]] (1464), [[Georg Joachim Rheticus|Rheticus]], and Rheticus' student [[Valentinus Otho]].
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]].<ref name="Gingerich_1986"/> [[Al-Khwārizmī]] (c. 780–850) produced tables of sines and cosines. Circa 860, [[Habash al-Hasib al-Marwazi]] defined the tangent and the cotangent, and produced their tables.<ref name="Sesiano">Jacques Sesiano, "Islamic mathematics", p. 157, in {{Cite book |title=Mathematics Across Cultures: The History of Non-western Mathematics |editor1-first=Helaine |editor1-last=Selin |editor1-link=Helaine Selin |editor2-first=Ubiratan |editor2-last=D'Ambrosio |editor2-link=Ubiratan D'Ambrosio |year=2000 |publisher=[[Springer Science+Business Media]] |isbn=978-1-4020-0260-1}}</ref><ref name="Britannica">{{cite web |title=trigonometry |date=17 November 2023 |url=http://www.britannica.com/EBchecked/topic/605281/trigonometry |publisher=Encyclopedia Britannica}}</ref> [[Muhammad ibn Jābir al-Harrānī al-Battānī]] (853–929) defined the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.<ref name="Britannica"/> The trigonometric functions were later studied by mathematicians including [[Omar Khayyám]], [[Bhāskara II]], [[Nasir al-Din al-Tusi]], [[Jamshīd al-Kāshī]] (14th century), [[Ulugh Beg]] (14th century), [[Regiomontanus]] (1464), [[Georg Joachim Rheticus|Rheticus]], and Rheticus' student [[Valentinus Otho]].
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The terms ''tangent'' and ''secant'' were first introduced by the Danish mathematician [[Thomas Fincke]] in his book ''Geometria rotundi'' (1583).<ref name="Fincke"/>
The terms ''tangent'' and ''secant'' were first introduced by the Danish mathematician [[Thomas Fincke]] in his book ''Geometria rotundi'' (1583).<ref name="Fincke"/>


The 17th century French mathematician [[Albert Girard]] made the first published use of the abbreviations ''sin'', ''cos'', and ''tan'' in his book ''Trigonométrie''.<ref name=MacTutor>{{MacTutor|id=Girard_Albert}}</ref>
The 17th century French mathematician [[Albert Girard]] made the first published use of the abbreviations {{math|sin}}, {{math|cos}}, and {{math|tan}} in his book ''Trigonométrie''.<ref name=MacTutor>{{MacTutor|id=Girard_Albert}}</ref>


In a paper published in 1682, [[Gottfried Leibniz]] proved that {{math|sin ''x''}} is not an [[algebraic function]] of {{mvar|x}}.<ref name="Bourbaki_1994"/> Though defined as ratios of sides of a [[right triangle]], and thus appearing to be [[rational function]]s, Leibnitz result established that they are actually [[transcendental function]]s of their argument. The task of assimilating circular functions into algebraic expressions was accomplished by Euler in his ''[[Introduction to the Analysis of the Infinite]]'' (1748). His method was to show that the sine and cosine functions are [[alternating series]] formed from the even and odd terms respectively of the [[exponential function|exponential series]]. He presented "[[Euler's formula]]", as well as near-modern abbreviations (''sin.'', ''cos.'', ''tang.'', ''cot.'', ''sec.'', and ''cosec.'').<ref name="Boyer_1991"/>
In a paper published in 1682, [[Gottfried Leibniz]] proved that {{math|sin ''x''}} is not an [[algebraic function]] of {{mvar|x}}.<ref name="Bourbaki_1994"/> Though defined as ratios of sides of a [[right triangle]], and thus appearing to be [[rational function]]s, Leibnitz result established that they are actually [[transcendental function]]s of their argument. The task of assimilating circular functions into algebraic expressions was accomplished by Euler in his ''[[Introduction to the Analysis of the Infinite]]'' (1748). His method was to show that the sine and cosine functions are [[alternating series]] formed from the even and odd terms respectively of the [[exponential function|exponential series]]. He presented "[[Euler's formula]]", as well as near-modern abbreviations ({{math|sin.}}, {{math|cos.}}, {{math|tang.}}, {{math|cot.}}, {{math|sec.}}, and {{math|cosec.}}).<ref name="Boyer_1991"/>


A few functions were common historically, but are now seldom used, such as the [[chord (geometry)|chord]], [[versine]] (which appeared in the earliest tables<ref name="Boyer_1991"/>), [[haversine]], [[coversine]],<ref>{{harvtxt|Nielsen|1966|pp=xxiii–xxiv}}</ref> half-tangent (tangent of half an angle), and [[exsecant]]. [[List of trigonometric identities]] shows more relations between these functions.
A few functions were common historically, but are now seldom used, such as the [[chord (geometry)|chord]], [[versine]] (which appeared in the earliest tables<ref name="Boyer_1991"/>), [[haversine]], [[coversine]],<ref>{{harvtxt|Nielsen|1966|pp=xxiii–xxiv}}</ref> half-tangent (tangent of half an angle), and [[exsecant]]. [[List of trigonometric identities]] shows more relations between these functions.


: <math>\begin{align}
<math display="block">\begin{align}
\operatorname{crd}\theta &= 2 \sin\tfrac12\theta, \\[5mu]
\operatorname{crd}\theta &= 2 \sin\tfrac12\theta, \\[5mu]
\operatorname{vers}\theta&=1-\cos \theta = 2\sin^2\tfrac12\theta, \\[5mu]
\operatorname{vers}\theta&=1-\cos \theta = 2\sin^2\tfrac12\theta, \\[5mu]
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==Notes==
==Notes==
{{notelist}}
{{notelist}}
{{reflist|refs=
<references>
<ref name=klein>{{cite book |chapter=Die goniometrischen Funktionen |at={{nobr|Ch. 3.2}}, {{pgs|175 ff.}} |title=Elementarmathematik vom höheren Standpunkt aus: Arithmetik, Algebra, Analysis|volume=1|author-first=Felix |author-last=Klein |author-link=Felix Klein |date=1924 |orig-year=1902 |edition=3rd |publisher=J. Springer |location=Berlin |language=de |chapter-url=https://books.google.com/books?id=5t8fAAAAIAAJ&pg=PA175 }} Translated as {{cite book|title=Elementary Mathematics from an Advanced Standpoint: Arithmetic, Algebra, Analysis |author-first=Felix |author-last=Klein |author-link=Felix Klein |display-authors=0 |year=1932 |publisher=Macmillan |translator-first1=E. R. |translator-last1=Hedrick |translator-first2=C. A. |translator-last2=Noble |chapter-url=https://archive.org/details/geometryelementa0000feli/page/162/?q=%22ii.+the+goniometric+functions%22 |chapter=The Goniometric Functions |at=Ch. 3.2, {{pgs|162 ff.}} }}</ref>
<ref name=klein>{{cite book |chapter=Die goniometrischen Funktionen |at={{nobr|Ch. 3.2}}, {{pgs|175 ff.}} |title=Elementarmathematik vom höheren Standpunkt aus: Arithmetik, Algebra, Analysis|volume=1|author-first=Felix |author-last=Klein |author-link=Felix Klein |date=1924 |orig-year=1902 |edition=3rd |publisher=J. Springer |location=Berlin |language=de |chapter-url=https://books.google.com/books?id=5t8fAAAAIAAJ&pg=PA175 }} Translated as {{cite book|title=Elementary Mathematics from an Advanced Standpoint: Arithmetic, Algebra, Analysis |author-first=Felix |author-last=Klein |author-link=Felix Klein |display-authors=0 |year=1932 |publisher=Macmillan |translator-first1=E. R. |translator-last1=Hedrick |translator-first2=C. A. |translator-last2=Noble |chapter-url=https://archive.org/details/geometryelementa0000feli/page/162/?q=%22ii.+the+goniometric+functions%22 |chapter=The Goniometric Functions |at=Ch. 3.2, {{pgs|162 ff.}} }}</ref>
<ref name="Larson_2013">{{cite book |title=Trigonometry |edition=9th |first1=Ron |last1=Larson |publisher=Cengage Learning |date=2013 |isbn=978-1-285-60718-4 |page=153 |url=https://books.google.com/books?id=zbgWAAAAQBAJ |url-status=live |archive-url=https://web.archive.org/web/20180215144848/https://books.google.com/books?id=zbgWAAAAQBAJ |archive-date=15 February 2018 }} [https://books.google.com/books?id=zbgWAAAAQBAJ&pg=PA153 Extract of page 153] {{webarchive|url=https://web.archive.org/web/20180215144848/https://books.google.com/books?id=zbgWAAAAQBAJ&pg=PA153 |date=15 February 2018 }}</ref>
<ref name="Larson_2013">{{cite book |title=Trigonometry |edition=9th |first1=Ron |last1=Larson |publisher=Cengage Learning |date=2013 |isbn=978-1-285-60718-4 |page=153 |url=https://books.google.com/books?id=zbgWAAAAQBAJ |url-status=live |archive-url=https://web.archive.org/web/20180215144848/https://books.google.com/books?id=zbgWAAAAQBAJ |archive-date=15 February 2018 }} [https://books.google.com/books?id=zbgWAAAAQBAJ&pg=PA153 Extract of page 153] {{webarchive|url=https://web.archive.org/web/20180215144848/https://books.google.com/books?id=zbgWAAAAQBAJ&pg=PA153 |date=15 February 2018 }}</ref>
Line 723: Line 745:
<ref name="Roegel_2010">{{cite web |title=A reconstruction of Gunter's Canon triangulorum (1620) |editor-first=Denis |editor-last=Roegel |type=Research report |publisher=HAL |date=6 December 2010 |id=inria-00543938 |url=https://hal.inria.fr/inria-00543938/document |access-date=28 July 2017 |url-status=live |archive-url=https://web.archive.org/web/20170728192238/https://hal.inria.fr/inria-00543938/document |archive-date=28 July 2017}}</ref>
<ref name="Roegel_2010">{{cite web |title=A reconstruction of Gunter's Canon triangulorum (1620) |editor-first=Denis |editor-last=Roegel |type=Research report |publisher=HAL |date=6 December 2010 |id=inria-00543938 |url=https://hal.inria.fr/inria-00543938/document |access-date=28 July 2017 |url-status=live |archive-url=https://web.archive.org/web/20170728192238/https://hal.inria.fr/inria-00543938/document |archive-date=28 July 2017}}</ref>
<ref name="Plofker_2009">See Plofker, ''[[Mathematics in India (book)|Mathematics in India]]'', Princeton University Press, 2009, p. 257<br>See {{cite web |url=http://www.clarku.edu/~djoyce/trig/ |title=Clark University |url-status=live |archive-url=https://web.archive.org/web/20080615133310/http://www.clarku.edu/~djoyce/trig/ |archive-date=15 June 2008 }}<br>See Maor (1998), chapter 3, regarding the etymology.</ref>
<ref name="Plofker_2009">See Plofker, ''[[Mathematics in India (book)|Mathematics in India]]'', Princeton University Press, 2009, p. 257<br>See {{cite web |url=http://www.clarku.edu/~djoyce/trig/ |title=Clark University |url-status=live |archive-url=https://web.archive.org/web/20080615133310/http://www.clarku.edu/~djoyce/trig/ |archive-date=15 June 2008 }}<br>See Maor (1998), chapter 3, regarding the etymology.</ref>
}}
</references>


==References==
==References==

Latest revision as of 13:05, 18 November 2025

Template:Short description Template:Redir-multi Template:Use dmy dates

File:Academ Base of trigonometry.svg
Basis of trigonometry: if two right triangles have equal acute angles, they are similar, so their corresponding side lengths are proportional.

In mathematics, the trigonometric functions (also called circular functions, angle functions or goniometric functions)Template:R are real functions which relate an angle of a right-angled triangle to ratios of two side lengths. They are widely used in all sciences that are related to geometry, such as navigation, solid mechanics, celestial mechanics, geodesy, and many others. They are among the simplest periodic functions, and as such are also widely used for studying periodic phenomena through Fourier analysis. Template:Trigonometry

The trigonometric functions most widely used in modern mathematics are the sine, the cosine, and the tangent functions. Script error: No such module "anchor".Their reciprocals are respectively the cosecant, the secant, and the cotangent functions, which are less used. Each of these six trigonometric functions has a corresponding inverse function and has an analog among the hyperbolic functions.

The oldest definitions of trigonometric functions, related to right-angle triangles, define them only for acute angles. To extend the sine and cosine functions to functions whose domain is the whole real line, geometrical definitions using the standard unit circle (i.e., a circle with radius 1 unit) are often used; then the domain of the other functions is the real line with some isolated points removed. Modern definitions express trigonometric functions as infinite series or as solutions of differential equations. This allows extending the domain of sine and cosine functions to the whole complex plane, and the domain of the other trigonometric functions to the complex plane with some isolated points removed.

Notation

Conventionally, an abbreviation of each trigonometric function's name is used as its symbol in formulas. Today, the most common versions of these abbreviations are "Template:Math" for sine, "Template:Math" for cosine, "Template:Math" or "Template:Math" for tangent, "Template:Math" for secant, "Template:Math" or "Template:Math" for cosecant, and "Template:Math" or "Template:Math" for cotangent. Historically, these abbreviations were first used in prose sentences to indicate particular line segments or their lengths related to an arc of an arbitrary circle, and later to indicate ratios of lengths, but as the function concept developed in the 17th–18th century, they began to be considered as functions of real-number-valued angle measures, and written with functional notation, for example Template:Math. Parentheses are still often omitted to reduce clutter, but are sometimes necessary; for example the expression sinx+y would typically be interpreted to mean (sinx)+y, so parentheses are required to express sin(x+y).

A positive integer appearing as a superscript after the symbol of the function denotes exponentiation, not function composition. For example sin2x and sin2(x) denote (sinx)2, not sin(sinx). This differs from the (historically later) general functional notation in which f2(x)=(ff)(x)=f(f(x)).

In contrast, the superscript 1 is commonly used to denote the inverse function, not the reciprocal. For example sin1x and sin1(x) denote the inverse trigonometric function alternatively written arcsinx. The equation θ=sin1x implies sinθ=x, not θsinx=1. In this case, the superscript could be considered as denoting a composed or iterated function, but negative superscripts other than 1 are not in common use.

Right-angled triangle definitions

File:TrigonometryTriangle.svg
In this right triangle, denoting the measure of angle BAC as A: Template:Math; Template:Math; Template:Math.
File:TrigFunctionDiagram.svg
Plot of the six trigonometric functions, the unit circle, and a line for the angle Template:Math. The points labeled Template:Ifsubst style="color:#D00">1, Template:Ifsubst style="color:#02D">Sec(θ), Template:Ifsubst style="color:#0D1">Csc(θ) represent the length of the line segment from the origin to that point. Template:Ifsubst style="color:#D00">Sin(θ), Template:Ifsubst style="color:#02D">Tan(θ), and Template:Ifsubst style="color:#0D1">1 are the heights to the line starting from the Template:Mvar-axis, while Template:Ifsubst style="color:#D00">Cos(θ), Template:Ifsubst style="color:#02D">1, and Template:Ifsubst style="color:#0D1">Cot(θ) are lengths along the Template:Mvar-axis starting from the origin.

If the acute angle Template:Mvar is given, then any right triangles that have an angle of Template:Mvar are similar to each other. This means that the ratio of any two side lengths depends only on Template:Mvar. Thus these six ratios define six functions of Template:Mvar, which are the trigonometric functions. In the following definitions, the hypotenuse is the length of the side opposite the right angle, opposite represents the side opposite the given angle Template:Mvar, and adjacent represents the side between the angle Template:Mvar and the right angle.[1][2]

sine
sinθ=oppositehypotenuse
cosecant
cscθ=hypotenuseopposite
cosine
cosθ=adjacenthypotenuse
secant
secθ=hypotenuseadjacent
tangent
tanθ=oppositeadjacent
cotangent
cotθ=adjacentopposite

Various mnemonics can be used to remember these definitions.

In a right-angled triangle, the sum of the two acute angles is a right angle, that is, Template:Math or Template:Math. Therefore sin(θ) and cos(90θ) represent the same ratio, and thus are equal. This identity and analogous relationships between the other trigonometric functions are summarized in the following table.

File:Periodic sine.svg
Top: Trigonometric function Template:Math for selected angles Template:Mvar, Template:Math, Template:Math, and Template:Math in the four quadrants.
Bottom: Graph of sine versus angle. Angles from the top panel are identified.
Summary of relationships between trigonometric functions[3]
Function Description Relationship
using radians using degrees
sine Template:Math sinθ=cos(π2θ)=1cscθ sinx=cos(90x)=1cscx
cosine Template:Math cosθ=sin(π2θ)=1secθ cosx=sin(90x)=1secx
tangent Template:Math tanθ=sinθcosθ=cot(π2θ)=1cotθ tanx=sinxcosx=cot(90x)=1cotx
cotangent Template:Math cotθ=cosθsinθ=tan(π2θ)=1tanθ cotx=cosxsinx=tan(90x)=1tanx
secant Template:Math secθ=csc(π2θ)=1cosθ secx=csc(90x)=1cosx
cosecant Template:Math cscθ=sec(π2θ)=1sinθ cscx=sec(90x)=1sinx

Radians versus degrees

In geometric applications, the argument of a trigonometric function is generally the measure of an angle. For this purpose, any angular unit is convenient. One common unit is degrees, in which a right angle is 90° and a complete turn is 360° (particularly in elementary mathematics).

However, in calculus and mathematical analysis, the trigonometric functions are generally regarded more abstractly as functions of real or complex numbers, rather than angles. In fact, the functions Template:Math and Template:Math can be defined for all complex numbers in terms of the exponential function, via power series,[4] or as solutions to differential equations given particular initial values[5] (see below), without reference to any geometric notions. The other four trigonometric functions (Template:Math, Template:Math, Template:Math, Template:Math) can be defined as quotients and reciprocals of Template:Math and Template:Math, except where zero occurs in the denominator. It can be proved, for real arguments, that these definitions coincide with elementary geometric definitions if the argument is regarded as an angle in radians.[4] Moreover, these definitions result in simple expressions for the derivatives and indefinite integrals for the trigonometric functions.[6] Thus, in settings beyond elementary geometry, radians are regarded as the mathematically natural unit for describing angle measures.

When radians (rad) are employed, the angle is given as the length of the arc of the unit circle subtended by it: the angle that subtends an arc of length 1 on the unit circle is 1 rad (≈ 57.3°),[7] and a complete turn (360°) is an angle of 2Template:Pi (≈ 6.28) rad.[8] Since radian is dimensionless, i.e. 1 rad = 1, the degree symbol can also be regarded as a mathematical constant factor such that 1° = Template:Pi/180 ≈ 0.0175.Script error: No such module "Unsubst".

Unit-circle definitions

File:Circle-trig6.svg
All of the trigonometric functions of the angle Template:Mvar (theta) can be constructed geometrically in terms of a unit circle centered at Template:Mvar.
File:Periodic sine.svg
Sine function on unit circle (top) and its graph (bottom)
File:Unit Circle Definitions of Six Trigonometric Functions.svg
In this illustration, the six trigonometric functions of an arbitrary angle Template:Mvar are represented as Cartesian coordinates of points related to the unit circle. The Template:Mvar-axis ordinates of Template:Math, Template:Math and Template:Math are Template:Math, Template:Math and Template:Math, respectively, while the Template:Mvar-axis abscissas of Template:Math, Template:Math and Template:Math are Template:Math, Template:Math and Template:Math, respectively.
File:Trigonometric function quadrant sign.svg
Signs of trigonometric functions in each quadrant. Mnemonics like "all students take calculus" indicates when sine, cosine, and tangent are positive from quadrants I to IV.[9]

The six trigonometric functions can be defined as coordinate values of points on the Euclidean plane that are related to the unit circle, which is the circle of radius one centered at the origin Template:Math of this coordinate system. While right-angled triangle definitions allow for the definition of the trigonometric functions for angles between Template:Math and π2 radians Template:Math the unit circle definitions allow the domain of trigonometric functions to be extended to all positive and negative real numbers.

Let be the ray obtained by rotating by an angle Template:Mvar the positive half of the Template:Mvar-axis (counterclockwise rotation for θ>0, and clockwise rotation for θ<0). This ray intersects the unit circle at the point A=(xA,yA). The ray , extended to a line if necessary, intersects the line of equation x=1 at point B=(1,yB), and the line of equation y=1 at point C=(xC,1). The tangent line to the unit circle at the point Template:Math, is perpendicular to , and intersects the Template:Mvar- and Template:Mvar-axes at points D=(0,yD) and E=(xE,0). The coordinates of these points give the values of all trigonometric functions for any arbitrary real value of Template:Mvar in the following manner.

The trigonometric functions Template:Math and Template:Math are defined, respectively, as the Template:Mvar- and Template:Mvar-coordinate values of point Template:Math. That is, cosθ=xA and sinθ=yA.[10]

In the range 0θπ/2, this definition coincides with the right-angled triangle definition, by taking the right-angled triangle to have the unit radius Template:Math as hypotenuse. And since the equation x2+y2=1 holds for all points P=(x,y) on the unit circle, this definition of cosine and sine also satisfies the Pythagorean identity. cos2θ+sin2θ=1.

The other trigonometric functions can be found along the unit circle as tanθ=yB and cotθ=xC, cscθ =yD and secθ=xE.

By applying the Pythagorean identity and geometric proof methods, these definitions can readily be shown to coincide with the definitions of tangent, cotangent, secant and cosecant in terms of sine and cosine, that is tanθ=sinθcosθ,cotθ=cosθsinθ,secθ=1cosθ,cscθ=1sinθ.

File:Trigonometric functions.svg
Trigonometric functions: Template:Ifsubst style="color:#00A">Sine, Template:Ifsubst style="color:#0A0">Cosine, Template:Ifsubst style="color:#A00">Tangent, Template:Ifsubst style="color:#00A">Cosecant (dotted), Template:Ifsubst style="color:#0A0">Secant (dotted), Template:Ifsubst style="color:#A00">Cotangent (dotted) – [ animation]

Since a rotation of an angle of ±2π does not change the position or size of a shape, the points Template:Math, Template:Math, Template:Math, Template:Math, and Template:Math are the same for two angles whose difference is an integer multiple of 2π. Thus trigonometric functions are periodic functions with period 2π. That is, the equalities sinθ=sin(θ+2kπ) and cosθ=cos(θ+2kπ) hold for any angle Template:Mvar and any integer Template:Mvar. The same is true for the four other trigonometric functions. By observing the sign and the monotonicity of the functions sine, cosine, cosecant, and secant in the four quadrants, one can show that 2π is the smallest value for which they are periodic (i.e., 2π is the fundamental period of these functions). However, after a rotation by an angle π, the points Template:Mvar and Template:Mvar already return to their original position, so that the tangent function and the cotangent function have a fundamental period of π. That is, the equalities tanθ=tan(θ+kπ) and cotθ=cot(θ+kπ) hold for any angle Template:Mvar and any integer Template:Mvar.

Algebraic values

File:Unit circle angles color.svg
The unit circle, with some points labeled with their cosine and sine (in this order), and the corresponding angles in radians and degrees.

The algebraic expressions for the most important angles are as follows:

sin0=sin0=02=0 (zero angle) sinπ6=sin30=12=12 sinπ4=sin45=22=12 sinπ3=sin60=32 sinπ2=sin90=42=1 (right angle)

Writing the numerators as square roots of consecutive non-negative integers, with a denominator of 2, provides an easy way to remember the values.[11]

Such simple expressions generally do not exist for other angles which are rational multiples of a right angle.

  • For an angle which, measured in degrees, is a multiple of three, the exact trigonometric values of the sine and the cosine may be expressed in terms of square roots. 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 non-real complex number. Galois theory allows a proof that, if the angle is not a multiple of 3°, non-real cube roots are unavoidable.
  • For an angle which, expressed in degrees, is a rational number, the sine and the cosine are algebraic numbers, which may be expressed in terms of [[nth root|Template:Mvar-th roots]]. This results from the fact that the Galois groups of the cyclotomic polynomials are cyclic.
  • For an angle which, expressed 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.
  • If the sine of an angle is a rational number then the cosine is not necessarily a rational number, and vice-versa. However, if the tangent of an angle is rational then both the sine and cosine of the double angle will be rational.

Simple algebraic values

Script error: No such module "Labelled list hatnote".

The following table lists the sines, cosines, and tangents of multiples of 15 degrees from 0 to 90 degrees.

Angle, Template:Mvar, in sin(θ) cos(θ) tan(θ)
radians degrees
0 0 0 1 0
π12 15 624 6+24 23
π6 30 12 32 33
π4 45 22 22 1
π3 60 32 12 3
5π12 75 6+24 624 2+3
π2 90 1 0 Undefined

Definitions in analysis

File:Trigonometrija-graf.svg
Graphs of sine, cosine and tangent
File:Taylorsine.svg
The sine function (blue) is closely approximated by its Taylor polynomial of degree 7 (pink) for a full cycle centered on the origin.
File:Taylor cos.gif
Animation for the approximation of cosine via Taylor polynomials.
File:Taylorreihenentwicklung des Kosinus.svg
cos(x) together with the first Taylor polynomials pn(x)=k=0n(1)kx2k(2k)!

G. H. Hardy noted in his 1908 work A Course of Pure Mathematics that the definition of the trigonometric functions in terms of the unit circle is not satisfactory, because it depends implicitly on a notion of angle that can be measured by a real number.Template:Clarify[12] Thus in modern analysis, trigonometric functions are usually constructed without reference to geometry.

Various ways exist in the literature for defining the trigonometric functions in a manner suitable for analysis; they include:

  • Using the "geometry" of the unit circle, which requires formulating the arc length of a circle (or area of a sector) analytically.[12]
  • By a power series, which is particularly well-suited to complex variables.[12][13]
  • By using an infinite product expansion.[12]
  • By inverting the inverse trigonometric functions, which can be defined as integrals of algebraic or rational functions.[12]
  • As solutions of a differential equation.[14]

Definition by differential equations

Sine and cosine can be defined as the unique solution to the initial value problem:Template:Sfn ddxsinx=cosx, ddxcosx=sinx, sin(0)=0, cos(0)=1.

Differentiating again, d2dx2sinx=ddxcosx=sinx and d2dx2cosx=ddxsinx=cosx, so both sine and cosine are solutions of the same ordinary differential equation y+y=0. Sine is the unique solution with Template:Math and Template:Math; cosine is the unique solution with Template:Math and Template:Math.

One can then prove, as a theorem, that solutions cos,sin are periodic, having the same period. Writing this period as 2π is then a definition of the real number π which is independent of geometry.

Applying the quotient rule to the tangent tanx=sinx/cosx, ddxtanx=cos2x+sin2xcos2x=1+tan2x, so the tangent function satisfies the ordinary differential equation y=1+y2. It is the unique solution with Template:Math.

Power series expansion

The basic trigonometric functions can be defined by the following power series expansions.[15] These series are also known as the Taylor series or Maclaurin series of these trigonometric functions: sinx=xx33!+x55!x77!+=n=0(1)nx2n+1(2n+1)!cosx=1x22!+x44!x66!+=n=0(1)nx2n(2n)! The radius of convergence of these series is infinite. Therefore, the sine and the cosine can be extended to entire functions (also called "sine" and "cosine"), which are (by definition) complex-valued functions that are defined and holomorphic on the whole complex plane.

Term-by-term differentiation shows that the sine and cosine defined by the series obey the differential equation discussed previously, and conversely one can obtain these series from elementary recursion relations derived from the differential equation.

Being defined as fractions of entire functions, the other trigonometric functions may be extended to meromorphic functions, that is functions that are holomorphic in the whole complex plane, except some isolated points called poles. Here, the poles are the numbers of the form (2k+1)π2 for the tangent and the secant, or kπ for the cotangent and the cosecant, where Template:Mvar is an arbitrary integer.

Recurrences relations may also be computed for the coefficients of the Taylor series of the other trigonometric functions. These series have a finite radius of convergence. Their coefficients have a combinatorial interpretation: they enumerate alternating permutations of finite sets.[16]

More precisely, defining

Template:Mvar, the Template:Mvar-th up/down number,
Template:Mvar, the Template:Mvar-th Bernoulli number, and
Template:Mvar, is the Template:Mvar-th Euler number,

one has the following series expansions:[17] tanx=n=0U2n+1(2n+1)!x2n+1=n=1(1)n122n(22n1)B2n(2n)!x2n1=x+13x3+215x5+17315x7+,for |x|<π2.

cscx=n=0(1)n+12(22n11)B2n(2n)!x2n1=x1+16x+7360x3+3115120x5+,for 0<|x|<π.

secx=n=0U2n(2n)!x2n=n=0(1)nE2n(2n)!x2n=1+12x2+524x4+61720x6+,for |x|<π2.

cotx=n=0(1)n22nB2n(2n)!x2n1=x113x145x32945x5,for 0<|x|<π.

Continued fraction expansion

The following continued fractions are valid in the whole complex plane:

[18] sinx=x1+x223x2+23x245x2+45x267x2+

cosx=11+x212x2+12x234x2+34x256x2+

Script error: No such module "Unsubst".


tanx=x1x23x25x27=11x13x15x17x

The last one was used in the historically first proof that π is irrational.[19]

There is a rapidly convergent continued fraction for tan(x): [20]

tanx=1+5x2T0+5x2,Tk=(4k+1)(4k+3)(4k+5)4x2(4k+3)+x2(4k+1)1+x2(4k+9)Tk+1 Let x=1 then the following continued fraction representation gives (asymptotically) 12.68 new correct decimal places per cycle: tan1=1+5T0+5,Tk=(4k+1)(4k+3)(4k+5)4(4k+3)+4k+11+4k+9Tk+1




Partial fraction expansion

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:[21] πcotπx=limNn=NN1x+n. This identity can be proved with the Herglotz trick.[22] Combining the Template:Math-th with the Template:Mvar-th term lead to absolutely convergent series: πcotπx=1x+2xn=11x2n2. Similarly, one can find a partial fraction expansion for the secant, cosecant and tangent functions: πcscπx=n=(1)nx+n=1x+2xn=1(1)nx2n2, π2csc2πx=n=1(x+n)2, πsecπx=n=0(1)n(2n+1)(n+12)2x2, πtanπx=2xn=01(n+12)2x2.

Infinite product expansion

The following infinite product for the sine is due to Leonhard Euler, and is of great importance in complex analysis:[23] sinz=zn=1(1z2n2π2),z. This may be obtained from the partial fraction decomposition of cotz given above, which is the logarithmic derivative of sinz.[24] From this, it can be deduced also that cosz=n=1(1z2(n1/2)2π2),z.

Euler's formula and the exponential function

File:Sinus und Kosinus am Einheitskreis 3.svg
cos(θ) and sin(θ) are the real and imaginary part of eiθ respectively.

Euler's formula relates sine and cosine to the exponential function: eix=cosx+isinx. This formula is commonly considered for real values of Template:Mvar, but it remains true for all complex values.

Proof: Let f1(x)=cosx+isinx, and f2(x)=eix. One has dfj(x)/dx=ifj(x) for Template:Math. The quotient rule implies thus that d/dx(f1(x)/f2(x))=0. Therefore, f1(x)/f2(x) is a constant function, which equals Template:Val, as f1(0)=f2(0)=1. This proves the formula.

One has eix=cosx+isinxeix=cosxisinx.

Solving this linear system in sine and cosine, one can express them in terms of the exponential function: sinx=eixeix2icosx=eix+eix2.

When Template:Mvar is real, this may be rewritten as cosx=Re(eix),sinx=Im(eix).

Most trigonometric identities can be proved by expressing trigonometric functions in terms of the complex exponential function by using above formulas, and then using the identity ea+b=eaeb for simplifying the result.

Euler's formula can also be used to define the basic trigonometric function directly, as follows, using the language of topological groups.[25] The set U of complex numbers of unit modulus is a compact and connected topological group, which has a neighborhood of the identity that is homeomorphic to the real line. Therefore, it is isomorphic as a topological group to the one-dimensional torus group /, via an isomorphism e:/U. In simple terms, e(t)=exp(2πit), and this isomorphism is unique up to taking complex conjugates.

For a nonzero real number a (the base), the function te(t/a) defines an isomorphism of the group /aU. The real and imaginary parts of e(t/a) are the cosine and sine, where a is used as the base for measuring angles. For example, when a=2π, we get the measure in radians, and the usual trigonometric functions. When a=360, we get the sine and cosine of angles measured in degrees.

Note that a=2π is the unique value at which the derivative ddte(t/a) becomes a unit vector with positive imaginary part at t=0. This fact can, in turn, be used to define the constant 2π.

Definition via integration

Another way to define the trigonometric functions in analysis is using integration.[12][26] For a real number t, put θ(t)=0tdτ1+τ2=arctant where this defines this inverse tangent function. Also, π is defined by 12π=0dτ1+τ2 a definition that goes back to Karl Weierstrass.[27]

On the interval π/2<θ<π/2, the trigonometric functions are defined by inverting the relation θ=arctant. Thus we define the trigonometric functions by tanθ=t,cosθ=(1+t2)1/2,sinθ=t(1+t2)1/2 where the point (t,θ) is on the graph of θ=arctant and the positive square root is taken.

This defines the trigonometric functions on (π/2,π/2). The definition can be extended to all real numbers by first observing that, as θπ/2, t, and so cosθ=(1+t2)1/20 and sinθ=t(1+t2)1/21. Thus cosθ and sinθ are extended continuously so that cos(π/2)=0,sin(π/2)=1. Now the conditions cos(θ+π)=cos(θ) and sin(θ+π)=sin(θ) define the sine and cosine as periodic functions with period 2π, for all real numbers.

Proving the basic properties of sine and cosine, including the fact that sine and cosine are analytic, one may first establish the addition formulae. First, arctans+arctant=arctans+t1st holds, provided arctans+arctant(π/2,π/2), since arctans+arctant=stdτ1+τ2=0s+t1stdτ1+τ2 after the substitution τs+τ1sτ. In particular, the limiting case as s gives arctant+π2=arctan(1/t),t(,0). Thus we have sin(θ+π2)=1t1+(1/t)2=11+t2=cos(θ) and cos(θ+π2)=11+(1/t)2=t1+t2=sin(θ). So the sine and cosine functions are related by translation over a quarter period π/2.

Definitions using functional equations

One can also define the trigonometric functions using various functional equations.

For example,[28] the sine and the cosine form the unique pair of continuous functions that satisfy the difference formula cos(xy)=cosxcosy+sinxsiny and the added condition 0<xcosx<sinx<x for 0<x<1.

In the complex plane

The sine and cosine of a complex number z=x+iy can be expressed in terms of real sines, cosines, and hyperbolic functions as follows: sinz=sinxcoshy+icosxsinhycosz=cosxcoshyisinxsinhy

By taking advantage of domain coloring, it is possible to graph the trigonometric functions as complex-valued functions. Various features unique to the complex functions can be seen from the graph; for example, the sine and cosine functions can be seen to be unbounded as the imaginary part of z becomes larger (since the color white represents infinity), and the fact that the functions contain simple zeros or poles is apparent from the fact that the hue cycles around each zero or pole exactly once. Comparing these graphs with those of the corresponding Hyperbolic functions highlights the relationships between the two.

Trigonometric functions in the complex plane
File:Trig-sin.png

sinz

File:Trig-cos.png

cosz

File:Trig-tan.png

tanz

File:Trig-cot.png

cotz

File:Trig-sec.png

secz

File:Trig-csc.png

cscz

Periodicity and asymptotes

The sine and cosine functions are periodic, with period 2π, which is the smallest positive period: sin(z+2π)=sin(z),cos(z+2π)=cos(z). Consequently, the cosecant and secant also have 2π as their period.

The functions sine and cosine also have semiperiods π, and sin(z+π)=sin(z),cos(z+π)=cos(z) and consequently tan(z+π)=tan(z),cot(z+π)=cot(z). Also, sin(x+π/2)=cos(x),cos(x+π/2)=sin(x) (see Complementary angles).

The function sin(z) has a unique zero (at z=0) in the strip π<(z)<π. The function cos(z) has the pair of zeros z=±π/2 in the same strip. Because of the periodicity, the zeros of sine are π={,2π,π,0,π,2π,}. There zeros of cosine are π2+π={,3π2,π2,π2,3π2,}. All of the zeros are simple zeros, and both functions have derivative ±1 at each of the zeros.

The tangent function tan(z)=sin(z)/cos(z) has a simple zero at z=0 and vertical asymptotes at z=±π/2, where it has a simple pole of residue 1. Again, owing to the periodicity, the zeros are all the integer multiples of π and the poles are odd multiples of π/2, all having the same residue. The poles correspond to vertical asymptotes limxπtan(x)=+,limxπ+tan(x)=.

The cotangent function cot(z)=cos(z)/sin(z) has a simple pole of residue 1 at the integer multiples of π and simple zeros at odd multiples of π/2. The poles correspond to vertical asymptotes limx0cot(x)=,limx0+cot(x)=+.

Basic identities

Many identities interrelate the trigonometric functions. This section contains the most basic ones; for more identities, see List of trigonometric identities. These identities may be proved geometrically from the unit-circle definitions or the right-angled-triangle definitions (although, for the latter definitions, care must be taken for angles that are not in the interval Template:Math, see Proofs of trigonometric identities). For non-geometrical proofs using only tools of calculus, one may use directly the differential equations, in a way that is similar to that of the above proof of Euler's identity. One can also use Euler's identity for expressing all trigonometric functions in terms of complex exponentials and using properties of the exponential function.

Parity

The cosine and the secant are even functions; the other trigonometric functions are odd functions. That is: sin(x)=sinxcos(x)=cosxtan(x)=tanxcot(x)=cotxcsc(x)=cscxsec(x)=secx.

Periods

All trigonometric functions are periodic functions of period Template:Math. This is the smallest period, except for the tangent and the cotangent, which have Template:Pi as smallest period. This means that, for every integer Template:Mvar, one has sin(x+2kπ)=sinxcos(x+2kπ)=cosxtan(x+kπ)=tanxcot(x+kπ)=cotxcsc(x+2kπ)=cscxsec(x+2kπ)=secx. See Periodicity and asymptotes.

Pythagorean identity

The Pythagorean identity, is the expression of the Pythagorean theorem in terms of trigonometric functions. It is sin2x+cos2x=1. Dividing through by either cos2x or sin2x gives tan2x+1=sec2x 1+cot2x=csc2x and sec2x+csc2x=sec2xcsc2x.

Sum and difference formulas

The sum and difference formulas allow expanding the sine, the cosine, and the tangent of a sum or a difference of two angles in terms of sines and cosines and tangents of the angles themselves. These can be derived geometrically, using arguments that date to Ptolemy (see Angle sum and difference identities). One can also produce them algebraically using Euler's formula.

Sum

sin(x+y)=sinxcosy+cosxsiny,cos(x+y)=cosxcosysinxsiny,tan(x+y)=tanx+tany1tanxtany.

Difference

sin(xy)=sinxcosycosxsiny,cos(xy)=cosxcosy+sinxsiny,tan(xy)=tanxtany1+tanxtany.

When the two angles are equal, the sum formulas reduce to simpler equations known as the double-angle formulae.

sin2x=2sinxcosx=2tanx1+tan2x,cos2x=cos2xsin2x=2cos2x1=12sin2x=1tan2x1+tan2x,tan2x=2tanx1tan2x.

These identities can be used to derive the product-to-sum identities.

By setting t=tan12θ (see half-angle formulae), all trigonometric functions of θ can be expressed as rational fractions of t: sinθ=2t1+t2,cosθ=1t21+t2,tanθ=2t1t2. Together with dθ=21+t2dt, this is the tangent half-angle substitution, which reduces the computation of integrals and antiderivatives of trigonometric functions to that of rational fractions.

Derivatives and antiderivatives

The derivatives of trigonometric functions result from those of sine and cosine by applying the quotient rule. The values given for the antiderivatives in the following table can be verified by differentiating them. The number Template:Mvar is a constant of integration.

f(x) f(x) f(x)dx
sinx cosx cosx+C
cosx sinx sinx+C
tanx sec2x ln|secx|+C
cscx cscxcotx ln|cscxcotx|+C
secx secxtanx ln|secx+tanx|+C
cotx csc2x ln|cscx|+C

Note: For 0<x<π the integral of cscx can also be written as arsinh(cotx), and the integral of secx for π/2<x<π/2 as arsinh(tanx), where arsinh is the inverse hyperbolic sine.

Alternatively, the derivatives of the 'co-functions' can be obtained using trigonometric identities and the chain rule:

dcosxdx=ddxsin(π/2x)=cos(π/2x)=sinx,dcscxdx=ddxsec(π/2x)=sec(π/2x)tan(π/2x)=cscxcotx,dcotxdx=ddxtan(π/2x)=sec2(π/2x)=csc2x.

Inverse functions

Script error: No such module "Labelled list hatnote". The trigonometric functions are periodic, and hence not injective, so strictly speaking, they do not have an inverse function. However, on each interval on which a trigonometric function is monotonic, one can define an inverse function, and this defines inverse trigonometric functions as multivalued functions. To define a true inverse function, one must restrict the domain to an interval where the function is monotonic, and is thus bijective from this interval to its image by the function. The common choice for this interval, called the set of principal values, is given in the following table. As usual, the inverse trigonometric functions are denoted with the prefix "arc" before the name or its abbreviation of the function.

Function Definition Domain Set of principal values
y=arcsinx siny=x 1x1 π2yπ2
y=arccosx cosy=x 1x1 0yπ
y=arctanx tany=x <x< π2<y<π2
y=arccotx coty=x <x< 0<y<π
y=arcsecx secy=x x<1 or x>1 0yπ,yπ2
y=arccscx cscy=x x<1 or x>1 π2yπ2,y0

The notations Template:Math, Template:Math, etc. are often used for Template:Math and Template:Math, etc. When this notation is used, inverse functions could be confused with multiplicative inverses. The notation with the "arc" prefix avoids such a confusion, though "arcsec" for arcsecant can be confused with "arcsecond".

Just like the sine and cosine, the inverse trigonometric functions can also be expressed in terms of infinite series. They can also be expressed in terms of complex logarithms.

Applications

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Angles and sides of a triangle

In this section Template:Mvar, Template:Mvar, Template:Mvar denote the three (interior) angles of a triangle, and Template:Mvar, Template:Mvar, Template:Mvar denote the lengths of the respective opposite edges. They are related by various formulas, which are named by the trigonometric functions they involve.

Law of sines

Script error: No such module "Labelled list hatnote". The law of sines states that for an arbitrary triangle with sides Template:Mvar, Template:Mvar, and Template:Mvar and angles opposite those sides Template:Mvar, Template:Mvar and Template:Mvar: sinAa=sinBb=sinCc=2Δabc, where Template:Math is the area of the triangle, or, equivalently, asinA=bsinB=csinC=2R, where Template:Mvar is the triangle's circumradius.

It can be proved 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

Script error: No such module "Labelled list hatnote". The law of cosines (also known as the cosine formula or cosine rule) is an extension of the Pythagorean theorem: c2=a2+b22abcosC, or equivalently, cosC=a2+b2c22ab.

In this formula the angle at Template:Mvar is opposite to the side Template:Mvar. This theorem can be proved 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

Script error: No such module "Labelled list hatnote". The law of tangents says that: tanAB2tanA+B2=aba+b.

Law of cotangents

Script error: No such module "Labelled list hatnote". If Template:Mvar is the triangle's semiperimeter, Template:Math, and Template:Mvar is the radius of the triangle's incircle, then Template:Math is the triangle's area. Therefore Heron's formula implies that:

r=1s(sa)(sb)(sc).

The law of cotangents says that:[29] cotA2=sar It follows that cotA2sa=cotB2sb=cotC2sc=1r.

Periodic functions

File:Lissajous curve 5by4.svg
A Lissajous curve, a figure formed with a trigonometry-based function.
File:Synthesis square.gif
An animation of the additive synthesis of a square wave with an increasing number of harmonics
File:Sawtooth Fourier Animation.gif
Sinusoidal basis functions (bottom) can form a sawtooth wave (top) when added. All the basis functions have nodes at the nodes of the sawtooth, and all but the fundamental (Template:Math) have additional nodes. The oscillation seen about the sawtooth when Template:Mvar is large is called the Gibbs phenomenon.

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 one-dimensional 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.[30]

Under rather general conditions, a periodic function Template:Math can be expressed as a sum of sine waves or cosine waves in a Fourier series.[31] Denoting the sine or cosine basis functions by Template:Mvar, the expansion of the periodic function Template:Math takes the form: f(t)=k=1ckφk(t).

For example, the square wave can be written as the Fourier series fsquare(t)=4πk=1sin((2k1)t)2k1.

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

Script error: No such module "Labelled list hatnote". 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 defined by Hipparchus of Nicaea (180–125 BCE) and Ptolemy of Roman Egypt (90–165 CE). The functions of sine and versine (1 − cosine) are closely related to the jyā and koti-jyā functions used in Gupta period Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.[32] (See Aryabhata's sine table.)

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.[33] Al-Khwārizmī (c. 780–850) produced tables of sines and cosines. Circa 860, Habash al-Hasib al-Marwazi defined the tangent and the cotangent, and produced their tables.[34][35] Muhammad ibn Jābir al-Harrānī al-Battānī (853–929) defined the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.[35] The trigonometric functions were later studied by mathematicians including Omar Khayyám, Bhāskara II, Nasir al-Din al-Tusi, Jamshīd al-Kāshī (14th century), Ulugh Beg (14th century), Regiomontanus (1464), Rheticus, and Rheticus' student Valentinus Otho.

Madhava of Sangamagrama (c. 1400) made early strides in the analysis of trigonometric functions in terms of infinite series.[36] (See Madhava series and Madhava's sine table.)

The tangent function was brought to Europe by Giovanni Bianchini in 1467 in trigonometry tables he created to support the calculation of stellar coordinates.[37]

The terms tangent and secant were first introduced by the Danish mathematician Thomas Fincke in his book Geometria rotundi (1583).[38]

The 17th century French mathematician Albert Girard made the first published use of the abbreviations Template:Math, Template:Math, and Template:Math in his book Trigonométrie.[39]

In a paper published in 1682, Gottfried Leibniz proved that Template:Math is not an algebraic function of Template:Mvar.[40] Though defined as ratios of sides of a right triangle, and thus appearing to be rational functions, Leibnitz result established that they are actually transcendental functions of their argument. The task of assimilating circular functions into algebraic expressions was accomplished by Euler in his Introduction to the Analysis of the Infinite (1748). His method was to show that the sine and cosine functions are alternating series formed from the even and odd terms respectively of the exponential series. He presented "Euler's formula", as well as near-modern abbreviations (Template:Math, Template:Math, Template:Math, Template:Math, Template:Math, and Template:Math).[32]

A few functions were common historically, but are now seldom used, such as the chord, versine (which appeared in the earliest tables[32]), haversine, coversine,[41] half-tangent (tangent of half an angle), and exsecant. List of trigonometric identities shows more relations between these functions.

crdθ=2sin12θ,versθ=1cosθ=2sin212θ,havθ=12versθ=sin212θ,coversθ=1sinθ=vers(12πθ),exsecθ=secθ1.

Script error: No such module "anchor".Historically, trigonometric functions were often combined with logarithms in compound functions like the logarithmic sine, logarithmic cosine, logarithmic secant, logarithmic cosecant, logarithmic tangent and logarithmic cotangent.[42][43][44][45]

Etymology

Script error: No such module "Labelled list hatnote". The word Script error: No such module "Lang". derives[46] from Latin sinus, meaning "bend; bay", and more specifically "the hanging fold of the upper part of a toga", "the bosom of a garment", which was chosen as the translation of what was interpreted as the Arabic word jaib, meaning "pocket" or "fold" in the twelfth-century translations of works by Al-Battani and al-Khwārizmī into Medieval Latin.[47] The choice was based on a misreading of the Arabic written form j-y-b (Script error: No such module "Lang".), which itself originated as a transliteration from Sanskrit Template:Transliteration, which along with its synonym Template:Transliteration (the standard Sanskrit term for the sine) translates to "bowstring", being in turn adopted from Ancient Greek Script error: No such module "Lang". "string".[48]

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.[49]

The prefix "co-" (in "cosine", "cotangent", "cosecant") is found in Edmund Gunter's Canon triangulorum (1620), which defines the cosinus as an abbreviation of the sinus complementi (sine of the complementary angle) and proceeds to define the cotangens similarly.[50][51]

See also

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Notes

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  12. a b c d e f Script error: No such module "citation/CS1".
  13. Whittaker, E. T., & Watson, G. N. (1920). A course of modern analysis: an introduction to the general theory of infinite processes and of analytic functions; with an account of the principal transcendental functions. University press.
  14. Bartle, R. G., & Sherbert, D. R. (2000). Introduction to real analysis (3rd ed). Wiley.
  15. Whitaker and Watson, p 584
  16. Stanley, Enumerative Combinatorics, Vol I., p. 149
  17. Abramowitz; Weisstein.
  18. C. D. Olds, Continued fractions, 1963, Random House, Inc., p. 138, pp 11, (without authorship)
  19. Script error: No such module "citation/CS1".
  20. Script error: No such module "citation/CS1".
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  22. Script error: No such module "citation/CS1". Extract of page 327 Template:Webarchive
  23. Whittaker and Watson, p 137
  24. Ahlfors, p 197
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  27. Script error: No such module "citation/CS1".
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  29. The Universal Encyclopaedia of Mathematics, Pan Reference Books, 1976, pp. 529–530. English version George Allen and Unwin, 1964. Translated from the German version Meyers Rechenduden, 1960.
  30. Script error: No such module "citation/CS1".
  31. See for example, Script error: No such module "citation/CS1".
  32. a b c Boyer, Carl B. (1991). A History of Mathematics (Second ed.). John Wiley & Sons, Inc. Template:Isbn, p. 210.
  33. Template:Cite magazine
  34. Jacques Sesiano, "Islamic mathematics", p. 157, in Script error: No such module "citation/CS1".
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  46. The anglicized form is first recorded in 1593 in Thomas Fale's Horologiographia, the Art of Dialling.
  47. Various sources credit the first use of Script error: No such module "Lang". to either See Merlet, A Note on the History of the Trigonometric Functions in Ceccarelli (ed.), International Symposium on History of Machines and Mechanisms, Springer, 2004
    See Maor (1998), chapter 3, for an earlier etymology crediting Gerard.
    See Script error: No such module "citation/CS1".
  48. See Plofker, Mathematics in India, Princeton University Press, 2009, p. 257
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  49. Oxford English Dictionary
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References

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External links

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