Trigonometry (from Greek trigōnon "triangle" + metron "measure")^{[1]} is a branch of mathematics that studies triangles, particularly right triangles. Trigonometry deals with relationships between the sides and the angles of triangles and with the trigonometric functions, which describe those relationships, as well as describing angles in general and the motion of waves such as sound and light waves.
Trigonometry is usually taught in secondary schools either as a separate course or as part of a precalculus course. It has applications in both pure mathematics and in applied mathematics, where it is essential in many branches of science and technology. A branch of trigonometry, called spherical trigonometry, studies triangles on spheres, and is important in astronomy and navigation.
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Ancient Egyptian and Babylonian mathematicians lacked the concept of an angle measure, but they studied the ratios of the sides of similar triangles and discovered some properties of these ratios. Ancient Greek mathematicians such as Euclid and Archimedes studied the properties of the chord of an angle and proved theorems that are equivalent to modern trigonometric formulae, although they presented them geometrically rather than algebraically. The modern sine function was first defined in the Surya Siddhanta and its properties were further documented by the 5th century Indian mathematician and astronomer Aryabhata.^{[2]} These Indian works were translated and expanded by medieval Islamic mathematicians. By the 10th century, Islamic mathematicians were using all six trigonometric functions, had tabulated their values, and were applying them to problems in spherical geometry. At about the same time, Chinese mathematicians developed trigonometry independently, although it was not a major field of study for them. Knowledge of trigonometric functions and methods reached Europe via Latin translations of the works of Persian and Arabic astronomers such as Al Battani and Nasir alDin alTusi.^{[3]} One of the earliest works on trigonometry by a European mathematician is De Triangulis by the 15th century German mathematician Regiomontanus. Trigonometry was still so little known in 16th century Europe that Nicolaus Copernicus devoted two chapters of De revolutionibus orbium coelestium to explaining its basic concepts.
If one angle of a triangle is 90 degrees and one of the other angles is known, the third is thereby fixed, because the three angles of any triangle add up to 180 degrees. The two acute angles therefore add up to 90 degrees: they are complementary angles. The shape of a right triangle is completely determined, up to similarity, by the angles. This means that once one of the other angles is known, the ratios of the various sides are always the same regardless of the overall size of the triangle. These ratios are given by the following trigonometric functions of the known angle A, where a, b and c refer to the lengths of the sides in the accompanying figure:
The hypotenuse is the side opposite to the 90 degree angle in a right triangle; it is the longest side of the triangle, and one of the two sides adjacent to angle A. The adjacent leg is the other side that is adjacent to angle A. The opposite side is the side that is opposite to angle A. The terms perpendicular and base are sometimes used for the opposite and adjacent sides respectively. Many people find it easy to remember what sides of the right triangle are equal to sine, cosine, or tangent, by memorizing the word SOHCAHTOA (see below under Mnemonics).
The reciprocals of these functions are named the cosecant (csc or cosec), secant (sec) and cotangent (cot), respectively. The inverse functions are called the arcsine, arccosine, and arctangent, respectively. There are arithmetic relations between these functions, which are known as trigonometric identities.
With these functions one can answer virtually all questions about arbitrary triangles by using the law of sines and the law of cosines. These laws can be used to compute the remaining angles and sides of any triangle as soon as two sides and an angle or two angles and a side or three sides are known. These laws are useful in all branches of geometry, since every polygon may be described as a finite combination of triangles.
Graphing process of y = sin(x) using a unit circle. 
Graphing process of y = tan(x) using a unit circle. 
Graphing process of y = csc(x) using a unit circle. 
The above definitions apply to angles between 0 and 90 degrees (0 and π/2 radians) only. Using the unit circle, one can extend them to all positive and negative arguments (see trigonometric function). The trigonometric functions are periodic, with a period of 360 degrees or 2π radians. That means their values repeat at those intervals.
The trigonometric functions can be defined in other ways besides the geometrical definitions above, using tools from calculus and infinite series. With these definitions the trigonometric functions can be defined for complex numbers. The complex function cis is particularly useful
See Euler's and De Moivre's formulas.
A common use of mnemonics is to remember facts and relationships in trigonometry. For example, the sine, cosine, and tangent ratios in a right triangle can be remembered by representing them as strings of letters, as in SOHCAHTOA.
The memorization of this mnemonic can be aided by expanding it into a phrase, such as "Some Officers Have Curly Auburn Hair Till Old Age".^{[4]} Any memorable phrase constructed of words beginning with the letters SOHCAHTOA will serve.
Trigonometric functions were among the earliest uses for mathematical tables. Such tables were incorporated into mathematics textbooks and students were taught to look up values and how to interpolate between the values listed to get higher accuracy. Slide rules had special scales for trigonometric functions.
Today scientific calculators have buttons for calculating the main trigonometric functions (sin, cos, tan and sometimes cis) and their inverses. Most allow a choice of angle measurement methods: degrees, radians and, sometimes, grad. Most computer programming languages provide function libraries that include the trigonometric functions. The floating point unit hardware incorporated into the microprocessor chips used in most personal computers have builtin instructions for calculating trigonometric functions.
There are an enormous number of uses of trigonometry and trigonometric functions. For instance, the technique of triangulation is used in astronomy to measure the distance to nearby stars, in geography to measure distances between landmarks, and in satellite navigation systems. The sine and cosine functions are fundamental to the theory of periodic functions such as those that describe sound and light waves.
Fields which make use of trigonometry or trigonometric functions include astronomy (especially, for locating the apparent positions of celestial objects, in which spherical trigonometry is essential) and hence navigation (on the oceans, in aircraft, and in space), music theory, acoustics, optics, analysis of financial markets, electronics, probability theory, statistics, biology, medical imaging (CAT scans and ultrasound), pharmacy, chemistry, number theory (and hence cryptology), seismology, meteorology, oceanography, many physical sciences, land surveying and geodesy, architecture, phonetics, economics, electrical engineering, mechanical engineering, civil engineering, computer graphics, cartography, crystallography and game development.
Certain equations involving trigonometric functions are true for all angles and are known as trigonometric identities. There are some identities which equate an expression to a different expression involving the same angles and these are listed in List of trigonometric identities, and then there are the triangle identities which relate the sides and angles of a given triangle and these are listed below.
In the following identities, A, B and C are the angles of a triangle and a, b and c are the lengths of sides of the triangle opposite the respective angles.
The law of sines (also known as the "sine rule") for an arbitrary triangle states:
where R is the radius of the circumcircle of the triangle:
Another law involving sines can be used to calculate the area of a triangle. If you know two sides and the angle between the sides, the area of the triangle becomes:
The law of cosines (known as the cosine formula, or the "cos rule") is an extension of the Pythagorean theorem to arbitrary triangles:
or equivalently:
The law of tangents:


Wikibooks has a book on the topic of Trigonometry. 
Trigonometry (from Greek trigōnon "triangle" + metron "measure"^{[1]}) is a branch of mathematics that deals with triangles, particularly triangles in a plane where one angle of the triangle is 90 degrees (right angled triangles). It specifically deals with the relationships between the sides and the angles of triangles; the trigonometric functions, and calculations based upon them. The insights of trigonometry permeate other branches of geometry, such as the study of spheres using spherical trigonometry.
Trigonometry has important applications in many branches of pure mathematics as well as of applied mathematics and, consequently remains applicable in natural sciences. Trigonometry is usually taught in secondary schools, often in a precalculus course.
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Trigonometry was probably invented for the purposes of astronomy.^{[2]} The origins of trigonometry can be traced to the civilizations of ancient Egypt, Mesopotamia and the Indus Valley, more than 4000 years ago. The common practice of measuring angles in degrees, minutes and seconds comes from the Babylonian's base sixty system of numeration. The Sulba Sutras written in India, between 800 BC and 500 BC, correctly compute the sine of π/4 (45°) as 1/√2 in a procedure for circling the square (the opposite of squaring the circle).
The first recorded use of trigonometry came from the Hellenistic mathematician Hipparchus[1] circa 150 BC, who compiled a trigonometric table using the sine for solving triangles. Ptolemy further developed trigonometric calculations circa 100 AD.
The ancient Sinhalese in Sri Lanka, when constructing reservoirs in the Anuradhapura kingdom, used trigonometry to calculate the gradient of the water flow. Archeological research also provides evidence of trigonometry used in other unique hydrological structures dating back to 4 BC.^{[3]}
The Indian mathematician Aryabhata in 499, gave tables of half chords which are now known as sine tables, along with cosine tables. He used zya for sine, kotizya for cosine, and otkram zya for inverse sine, and also introduced the versine. Another Indian mathematician, Brahmagupta in 628, used an interpolation formula to compute values of sines, up to the second order of the NewtonStirling interpolation formula.
In the 10th century, the Persian mathematician and astronomer Abul Wáfa introduced the tangent function and improved methods of calculating trigonometry tables. He established the angle addition identities, e.g. sin (a + b), and discovered the sine formula for spherical geometry:
Also in the late 10th and early 11th centuries, the Egyptian astronomer Ibn Yunus performed many careful trigonometric calculations and demonstrated the formula cos(a)cos(b) = (1 / 2)[cos(a + b) + cos(a − b)].
[Indian mathematicians]] were the pioneers of variable computations algebra for use in astronomical calculations along with trigonometry. Lagadha (circa 13501200 BC) is the first person thought to have used geometry and trigonometry for astronomy, in his Vedanga Jyotisha.
[[Persian people] Islamic mathematician Omar Khayyám (10481131) combined trigonometry and approximation theory to provide methods of solving algebraic equations by geometrical means. Khayyam solved the cubic equation x^{3} + 200x = 20x^{2} + 2000 and found a positive root of this cubic by considering the intersection of a rectangular hyperbola and a circle. An approximate numerical solution was then found by interpolation in trigonometric tables.
Detailed methods for constructing a table of sines for any angle were given by the Indian mathematician Bhaskara in 1150, along with some sine and cosine formulae. Bhaskara also developed spherical trigonometry.
The 13th century Persian mathematician Nasir alDin Tusi, along with Bhaskara, was probably the first to treat trigonometry as a distinct mathematical discipline. Nasir alDin Tusi in his Treatise on the Quadrilateral was the first to list the six distinct cases of a right angled triangle in spherical trigonometry.
In the 14th century, Persian mathematician alKashi and Timurid mathematician Ulugh Beg (grandson of Timur) produced tables of trigonometric functions as part of their studies of astronomy.
The mathematician Bartholemaeus Pitiscus published an influential work on trigonometry in 1595 which may have coined the word "trigonometry".
By definition, one angle of a right triangle is 90 degrees. If one of the other angles is known, the third can be calculated since all three angles of any triangle must add up to 180 degrees. The shape of a right triangle is completely determined, up to similarity, by the angles. This means that once one of the other angles is known, the ratios of the various sides are always the same regardless of the overall size of the triangle. These ratios are given by the following trigonometric functions of the known angle:
The adjacent leg is the side of the angle that is not the hypotenuse. The hypotenuse is the side opposite to the 90 degree angle in a right triangle; it is the longest side of the triangle. The terms perpendicular and base are sometimes used for the opposite and adjacent sides respectively.
The reciprocals of these functions are named the cosecant (csc or cosec), secant (sec) and cotangent (cot), respectively. The inverse functions are called the arcsine, arccosine, and arctangent, respectively. There are arithmetic relations between these functions, which are known as trigonometric identities.
With these functions one can answer virtually all questions about arbitrary triangles by using the law of sines and the law of cosines. These laws can be used to compute the remaining angles and sides of any triangle as soon as two sides and an angle or two angles and a side or three sides are known. These laws are useful in all branches of geometry, since every polygon may be described as a finite combination of triangles.
The above definitions apply to angles between 0 and 90 degrees (0 and π/2 radians) only. Using the unit circle, one may extend them to all positive and negative arguments (see trigonometric function). The trigonometric functions are periodic, with a period of 360 degrees or 2π radians. That means their values repeat at those intervals.
The trigonometric functions can be defined in other ways besides the geometrical definitions above, using tools from calculus and infinite series. With these definitions the trigonometric functions can be defined for complex numbers. The complex function cis is particularly useful
See Euler's formula.
Students often make use of mnemonics to remember the relationships and facts in trigonometry. For example, the sine, cosine and tangent ratios in right triangles can be remembered by representing all three rations at once as a string of letters; SOH CAH TOA (sineoppositehypotenuse cosineadjacenthypotenuse tangentoppositeadjacent), which can be pronounced as a single word. In addition, many remember similar letter sequences by creating sentences that consist of words that begin with the letters to be remembered, so that they are remembered in the correct order. For example, to remember Tan = Opposite/Adjacent, the letters TOA must be remembered in order. Any memorable phrase constructed of words beginning with the letters 'T, O, A' will serve, and often sentences are constructed to remember all three ratios at once. Other types of mnemonic simply describe facts in a simple, memorable way, such as "Plus to the right, minus to the left, positive height, negative depth" when referring to the trigonometric functions of a revolving line.
Trigonometric functions were among the earliest uses for mathematical tables. Such tables were incorporated into mathematics textbooks and students were taught to look up values and how to interpolate between the values listed to get higher accuracy. Slide rules had special scales for trigonometric functions.
Today scientific calculators have buttons for calculating the main trigonometric functions (sin, cos, tan and sometimes cis) and their inverses. Most allow a choice of angle measurement methods, degrees, radians and, sometimes, Grad. Most computer programming languages provide function libraries that include the trigonometric functions. The floating point unit hardware incorporated into the microprocessor chips used in most personal computers have built in instructions for calculating trigonometric functions.
There are an enormous number of applications of trigonometry and trigonometric functions. For instance, the technique of triangulation is used in astronomy to measure the distance to nearby stars, in geography to measure distances between landmarks, and in satellite navigation systems. The sine and cosine functions are fundamental to the theory of periodic functions such as those that describe sound and light waves.
Fields which make use of trigonometry or trigonometric functions include astronomy (especially, for locating the apparent positions of celestial objects, in which spherical trigonometry is essential) and hence navigation (on the oceans, in aircraft, and in space), music theory, acoustics, optics, analysis of financial markets, electronics, probability theory, statistics, biology, medical imaging (CAT scans and ultrasound), pharmacy, chemistry, number theory (and hence cryptology), seismology, meteorology, oceanography, many physical sciences, land surveying and geodesy, architecture, phonetics, economics, electrical engineering, mechanical engineering, civil engineering, computer graphics, cartography, crystallography and game development.
Certain equations involving trigonometric functions are true for all angles and are known as trigonometric identities. Many express important geometric relationships. For example, the Pythagorean identities are an expression of the Pythagorean Theorem. Here are some of the more commonly used identities, as well as the most important formulae connecting angles and sides of an arbitrary triangle. For more identities see trigonometric identity.
Note that are correct, it means it may be either one, depending on the value of A/2.
The law of sines for an arbitrary triangle states:
or equivalently:
The law of cosines (also known as the cosine formula) is an extension of the Pythagorean theorem to arbitrary triangles:
or equivalently:
The law of tangents:
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TRIGONOMETRY (from Gr. rpiywvov, a triangle, /2/2 Tpov, measure), the branch of mathematics which is concerned with the measurement of plane and spherical triangles, that is, with the determination of three of the parts of such triangles when the numerical values of the other three parts are given. Since any plane triangle can be divided into rightangled triangles, the solution of all plane triangles can be reduced to that of rightangled triangles; moreover, according to the theory of similar triangles, the ratios between pairs of sides of a rightangled triangle depend only upon the magnitude of the acute angles of the triangle, and may therefore be regarded as functions of either of these angles. The primary object of trigonometry, therefore, requires a classification and numerical tabulation of these functions of an angular magnitude; the science is, however, now understood to include the complete investigation not only of such of the properties of these functions as are necessary for the theoretical and practical solution of triangles but also of all their analytical properties. It appears that the solution of spherical triangles is effected by means of the same functions as are required in the case of plane triangles. The trigonometrical functions are employed in many branches of mathematical and physical science not directly concerned with the measurement of angles, and hence arises the importance of analytical trigonometry. The solution of triangles of which the sides are geodesic lines on a spheroidal surface requires the introduction of other functions than those required for the solution of triangles on a plane or spherical surface, and therefore gives rise to a new branch of science,which is from analogy frequently called spheroidal trigonometry. Every new class of surfaces which may be considered would have in this extended sense a trigonometry of its own, which would consist in an investigation of the nature and properties of the functions necessary for the measurement of the sides and angles of triangles bounded by geodesics drawn on such surfaces.
History Trigonometry, in its essential form of showing how to deduce the values of the angles and sides of a triangle when other angles and sides are given, is an invention of the Greeks. It found its origin in the computations demanded for the reduction of astronomical observations and in other problems connected with astronomical science; and since spherical triangles specially occur, it happened that spherical trigonometry was developed before the simpler plane trigonometry. Certain theorems were invented and utilized by Hipparchus, but material progress was not recorded until Ptolemy collated, amended and developed the work of his predecessors. In book xi. of the Almagest the principles of spherical trigonometry are stated in the form of a few simple and useful lemmas; plane trigonometry does not receive systematic treatment although several theorems and problems are stated incidentally. The solution of triangles necessitated the construction of tables of chords  the equivalent of our modern tables of sines; Ptolemy treats this subject in book i., stating several theorems relating to multiple angles, and by ingenious methods successfully deducing approximate results. He did not invent the idea of tables of chords, for, on the authority of Theon, the principle had been stated by Hipparchus (see Ptolemy).
The Indians, who were much more apt calculators than the Greeks, availed themselves of the Greek geometry which came from Alexandria, and made it the basis of trigonometrical calculations. The principal improvement which they introduced consists in the formation of tables of halfchords or sines instead of chords. Like the Greeks, they divided the circumference of the circle into 360 degrees or 21,600 minutes, and they found the length in minutes of the arc which can be straightened out into the radius to be 3438. The value of the ratio of the circumference of the circle to the diameter used to make this determination is 62832: 20000, or = 3.1416, which value was given by the astronomer Aryabhata (476550) in a work called Aryabhaiya, written in verse, which was republished i in Sanskrit by Dr Kern at Leiden in 1874. The relations between the sines and cosines of the same and of complementary arcs were known, and the formula sin la = iI { 1719 (343 8  c o sa) } was applied to the determination of the sine of a half angle when the sine and cosine of the whole angle were known. In the SuryaSiddhanta, an astronomical treatise which has been translated by Ebenezer Bourgess in vol. vi. of the Journal of the American Oriental Society (New Haven, 1860), the sines of angles at an interval of 3° 45' up to 90° are given; these were probably obtained from the sines of 60° and 45° by continual application of the dimidiary formula given above and by the use of the complementary angle. The values sin 15° = 890', sin 7° 3 0 ' = 449', sin 3° 45' =225' were thus obtained. Now the angle 3° 45' is itself 225'; thus the arc and the sine of of the circumference were found to be the same, and consequently special importance was attached to this arc, which was called the right sine. From the tables of sines of angles at intervals of 3° 45' the law expressed by the equation sin (n I.225')  sin (n.225') = sin (n.225') (n. 225')  sin (n  I . 225')  sin 225 was discovered empirically, and used for the purpose of recalculation. Bhaskara (fl. 1150) used the method, to which we have now returned, of expressing sines and cosines as fractions of the radius; he obtained the more correct values sin 3° 45' = 100/1529, cos 3° 45' =466/467, and showed how to form a table, according to degrees, from the values sin 1 ° = 10/573, cos 1 0 =6568/6569, which are much more accurate than Ptolemy's values. The Indians did not apply their trigonometrical knowledge to the solution of triangles; for astronomical purposes they solved rightangled plane and spherical triangles by geometry.
The Arabs were acquainted with Ptolemy's Almagest, and they probably learned from the Indians the use of the sine. The celebrated astronomer of Batnae, Albategnius, who died in A.D. 929930, and whose Tables were translated in the 12th century by Plato of Tivoli into Latin, under the title De scientia stellarum, employed the sine regularly, and was fully conscious of the advantage of the sine over the chord; indeed, he remarks that the continual doubling is saved by the use of the former. He was the first to calculate sin ¢ from the equation sin 4)/cos =k, and he also made a table of the length of shadows of a vertical object of height 12 for altitudes 1°, 2°, ... of the sun; this is a sort of cotangent table. He was acquainted not only with the triangle formulae in the Almagest, but also with the formula cos a=cos b cos c + sin b sin c cos A for a spherical triangle ABC. Abu'lWard of Bagdad (b. 940) was the first to introduce the tangent as an independent function: his " umbra " is the half of the tangent of the double arc, and the secant he defines as the " diameter umbrae." He employed the umbra to find the angle from a table and not merely as an abbreviation for sin/cos; this improvement was, however, afterwards forgotten, and the tangent was reinvented in the 15th century. Ibn Yunos of Cairo, who died in 1008, showed even more skill than Albategnius in the solution of problems in spherical trigonometry and gave improved approximate formulae for the calculation of sines. Among the West Arabs, Geber, who lived ' See also vol. ii. of the Asiatic Researches (Calcutta).
at Seville in the iith century, wrote an astronomy in nine books, which was translated into Latin in the 12th century by Gerard of Cremona and was published in 1534. The first book contains a trigonometry which is a considerable improvement on that in the Almagest. He gave proofs of the formulae for rightangled spherical triangles, depending on a rule of four quantities, instead of Ptolemy's rule of six quantities. The formulae cos B =cos b sin A, cos c= cot A cot B, in a triangle of which C is a right angle had escaped the notice of Ptolemy and were given for the first time by Geber. Strangely enough, he made no progress in plane trigonometry. Arrachel, a Spanish Arab who lived in the 12th century, wrote a work of which we have an analysis by Purbach, in which, like the Indians, he made the sine and the arc for the value 3° 45' coincide.
Georg Purbach (14231461), professor of mathematics at Vienna, wrote a work entitled Tractatus super propositiones Ptolemaei de sinubus et chordis (Nuremberg, 1541). This treatise consists of a development of Arrachel's method of interpolation for the calculation of tables of sines, and was published by Regiomontanus at the end of one of his works. Johannes Muller (14361476), known as Regiomontanus, was a pupil of Purbach and taught astronomy at Padua; he wrote an exposition of the Almagest, and a more important work, De triangulis planis et sphericis cum tabulis sinuum, which was published in 1533, a later edition appearing in 1561. He reinvented the tangent and calculated a table of tangents for each degree, but did not make any practical applications of this table, and did not use formulae involving the tangent. His work was the first complete European treatise on trigonometry, and contains a number of interesting problems; but his methods were in some respects behind those of the Arabs. Copernicus (14731543) gave the first simple demonstration of the fundamental formula of spherical trigonometry; the Trigonometria Copernici was published by Rheticus in 1542. George Joachim (15141576), known as Rheticus, wrote Opus palatinum de triangulis (see Tables, Mathematical), which contains tables of sines, tangents and secants of arcs at intervals of 10" from 0° to 90°. His method of calculation depends upon the formulae which give sin na and cos na in terms of the sines and cosines of (n  I) a and (n  2) a; thus these formulae may be regarded as due to him. Rheticus found the formulae for the sines of the half and third of an angle in terms of the sine of the whole angle. In 1599 there appeared an important work by Bartholomew Pitiscus (15611613), entitled Trigonometriae seu De dimensione triangulorum; this contained several important theorems on the trigonometrical functions of two angles, some of which had been given before by Finck, Landsberg (or Lansberghe de Meuleblecke) and Adriaan van Roomen. Francois Viete or Vieta (15401603) employed the equation (2 cos 40) 3  3 (2 cos 20) =2 cos 0 to solve the cubic x 3 3a 2 x = a 2 b(a> lb); he obtained, however, only one root of the cubic. In 1593 Van Roomen proposed, as a problem for all mathematicians, to solve the equation 453'37953' 3 +95 6 343' 5 
+945y41453'43+35=C.
Vieta gave y =2 sin 4,0, where C = 2 sin 0, as a solution, and also twentytwo of the other solutions, but he failed to obtain the negative roots. In his work Ad angulares sectiones Vieta gave formulae for the chords of multiples of a given arc in terms of the chord of the simple arc.
A new stage in the development of the science was commenced after John Napier's invention of logarithms in 1614. Napier also simplified the solution of spherical triangles by his wellknown analogies and by his rules for the solution of rightangled triangles. The first tables of logarithmic sines and tangents were constructed by Edmund Gunter (15811626), professor of astronomy at Gresham College, London; he was also the first to employ the expressions cosine, cotangent and cosecant for the sine, tangent and secant of the complement of an arc. A treatise by Albert Girard (15901634), published at the Hague in 1626, contains the theorems which give areas of spherical triangles and polygons, and applications of the properties of the supplementary triangles to the reduction of the number of different cases in the solution of spherical triangles. He used the notation sin, tin, sec for the sine, tangent and secant of an arc. In the second half of the 17th century the theory of infinite series was developed by John Wallis, Gregory, Mercator, and afterwards by Newton and Leibnitz. In the Analysis per aequationes numero terminorum infinitas, which was written before 1669, Newton gave the series for the arc in powers of its sine; from this he obtained the series for the sine and cosine in powers of the arc; but these series were given in such a form that the law of the formation of the coefficients was hidden. James Gregory discovered in 1670 the series for the arc in powers of the tangent and for the tangent and secant in powers of the arc. The first of these series was also discovered independently by Leibnitz in 1673, and published without proof in the Acta eruditorum for 1682. The series for the sine in powers of the arc he published in 1693; this he obtained by differentiation of a series with undetermined coefficients.
In the 18th century the science began to take a more analytical form; evidence of this is given in the works of Kresa in 1720 and Mayer in 1727. Friedrich Wilhelm v. Oppel's Analysis triangulorum (5746) was the first complete work on analytical trigonometry. None of these mathematicians used the notation sin, cos, tan, which is the more surprising in the case of Oppel, since Leonhard Euler had in 1744 employed it in a memoir in the Acta eruditorum. Jean Bernoulli was the first to obtain real results by the use of the symbol  I; he published in 1712 the general formula for tan i u in terms of tan 4), which he obtained by means of transformation of the arc into imaginary logarithms. The greatest advance was, however, made by Euler, who brought the science in all essential respects into the state in which it is at present. He introduced the present notation into general use, whereas until his time the trigonometrical functions had been, except by Girard, indicated by special letters, and had been regarded as certain straight lines the absolute lengths of which depended on the radius of the circle in which they were drawn. Euler's great improvement consisted in his regarding the sine, cosine, &c., as functions of the angle only, thereby giving to equations connecting these functions a purely analytical interpretation, instead of a geometrical one as heretofore. The exponential values of the sine and cosine, De Moivre's theorem, and a great number of other analytical properties of the trigonometrical functions, are due to Euler, most of whose writings are to be found in the Memoirs of the St Petersburg Academy.
Plane Trigonometry. 1. Imagine a straight line terminated at a fixed point 0, and initially coincident with a fixed straight line OA, to revolve round 0, and finally to take up any position OB. We shall suppose that, when this revolv of Angles ing straight line is turning of any in one direction, say that opposite to that in which the hands of a clock turn, it is describing a positive angle, and when it is turning in the other direction it is describing a negative angle. Before finally taking up the position OB the straight line may have passed any number of times through the position OB, making any number of complete revolutions round 0 in either FIG. I. direction. Each time that the straight line makes a complete revolution round 0 we consider it to have described four right angles, taken with the positive or negative sign, according to the direction in which it has revolved; thus, when it stops in the position OB, it may have revolved through any one of an infinite number of positive or negative angles any two of which differ from one another by a positive or negative multiple of four right angles, and all of which have the same bounding lines OA and OB. If OB' is the final position of the revolving line, the smallest positive angle which can have been described is that described by the revolving line making more than onehalf and less than the whole of a complete revolution, so that in this case we have a positive angle greater than two and less than four right angles. We have thus shown how we may conceive an angle not restricted to be less than two right angles, but of any positive or negative magnitude, to be generated.
2. Two systems of numerical measurement of angular magnitudes are in ordinary use. For practical measurements the sexagesimal system is the one employed: the ninetieth part of a right angle is taken as the unit and is called a degree; the degree is divided into sixty equal parts called minutes; of and the minute into sixty equal parts called seconds; A n tar angles smaller than a second are usually measured as M decimals of a second, the thirds, fourths, &c., not being in ordinary use. In the common notation an angle, for example, of 120 degrees, 17 minutes and 14.36 seconds is written 120° 17' 14.36". The decimal system measurement of angles has never come into ordinary use. In analytical trigonometry the circular measure of an angle is employed. In this system the unit angle or radian is the angle subtended at the centre of a circle by an arc equal in length to the radius. The constancy of this angle follows from the geometrical propositions  (I) the circumferences of different circles vary as their radii; (2) in the same circle angles at the centre are proportional to the arcs which subtend them. It thus follows that the radian is an angle independent of the particular circle used in defining it. The constant ratio of the circumference of a circle to its diameter is a number incommensurable with unity, usually denoted by 7r. We shall indicate later on some of the methods which have been employed to approximate to the value of this number. Its value to 20 places is 3.14159265358979323846 its reciprocal to the same number of places is 0 31830988618379067153. In circular measure every angle is measured by the ratio which it bears to the unit angle. Two right angles are measured by the number 7, and, since. the same angle is 180°, we see that the number of degrees in an angle of circular measure e is obtained from the formula 180 Xehr. The value of the radian has been found to 41 places of decimals by Glaisher (Proc. London Math. Soc. vol. iv.); the value of 1/7r, from which the unit can easily be calculated, is given to 140 places of decimals in Grunerts Archiv (1841), vol. i. To 10 decimal places the value of the unit angle is 57° 1 7' 44.8062470964". The unit of circular measure is too large to be convenient for practical purposes, but its use introduces a simplification into the series in analytical trigonometry, owing to the fact that the size of B' ' B' to B for BOB'. Suppose OP of fixed length, equal to OA, and let PM, PN be drawn perpendicular to A'A, respectively; then OM and ON, taken with their proper signs, are the projections of OP on A'A and B'B. The ratio of the projection of OP on B'B to the absolute length of OP is dependent only on the magnitude of the angle POA, and is called the sine of that angle; the ratio of the projection of OP on A'A to the length OP is called the  cosine of the angle POA. The ratio of the sine of an angle to its cosine is called the tangent of the angle, and that of the cosine to the sine the cotangent of the angle; the reciprocal of the cosine is called the secant, and that of sine the cosecant of the angle. These functions of an angle of magnitude a are denoted by sin a, cos a, tan a, cot a, sec a, cosec a respectively. If any straight line RS be drawn parallel to OP, the projection of RS on either of the straight lines A'A, can be easily seen to bear to RS the same ratios which the corresponding projections of OP bear to OP; thus, if a be the angle which RS makes with A'A, the projections of RS on A'A, B'B are RS cos a and RS sin a respectively, where RS denotes the absolute length RS. It must be observed that the line SR is to be considered as parallel not to OP but to OP", and therefore makes an angle 7r+a with A'A; this is consistent with the fact that the projections of SR are of opposite sign to those of RS. By observing the signs of the projections of OP for the positions P, P', P", P" of P we see that the sine and cosine of the angle POA are both positive; the sine of the angle P'OA is positive and its cosine is negative; both the sine and the cosine of the angle P"OA are negative; and the sine of the angle P"'OA is negative and its cosine positive. If a be the numerical value of the smallest angle of which OP and OA are boundaries, we see that, since these straight lines also bound all the angles 2n7r+a, where n is any positive or negative integer, the sines and cosines of all these angles are the same as the sine and cosine of a. Hence the sine of any angle 211lr+a is positive if a is between o and 7r and negative if a is between 7r and 27r, and the cosine of the same angle is positive if a is between o and 27r or and 27r and negative if a is between 27r and  7r.
In fig. 2 the angle POA is a, the angle P"'OA is a, P'OA is 7r  a, P"OA is 7r+a, POB is 27ra. By observing the signs of the projections we see that sin( a) = sin a, sin(7ra) =sin a, sin (7r+a) = sin a, COs( a) = cos a, cos(7ra) = cos a, cos(7r+a) = cos a, sin(27ra) = COs a, cos(21ra) =sin a.
Also sin(21r+ a) =sin(7r  27r  a) = sin (27r a) = cos a, cos(27r+a) = cos(7r27ra) = cos(27ra) = sin a.
From these equations we have tan(a) _ tan a, t j an(7ra) = tan a, tan(+a) = tan a, tan(27ra) =cot a, tan (17r+a) = cot a, with corresponding equations for the cotangent.
The only angles for which the projection of OP on B'B is the same as for the given angle POA (= a) are the two sets of angles bounded by OP, OA and OP', OA; these angles are 2n7r+a and 2n7r+(7ra), and are all included in the formula rlr+(Ora, where r is any integer; this therefore is the formula for all angles having the same sine as a. The only angles which have the same cosine as a are those bounded by OA, OP and OA, OP", and these are all included in the formula 2n1r =a. Similarly it can be shown that nlr+a includes all the angles which have the same tangent as a.
Angle . 
o 
0...27r 
27r 
17r...7r 
7r 
7r...27r 
zir 
2 r...27r 
27r 
Sine. . 
o 
I 
+D 
o 
I 
I 
D 
o 

Cosine . 
I 
+D 
o 
I 
1 
D 
0 
+I 
I 
Tangent . 
o 
+I 
too 
D 
o 
+I 
=oo 
D 
o 
Cotangent 
t oo 
D 
o 
 I 
t 
D 
o 
8 

Secant . 
I 
+I 
t o o 
D 
I 
I 
t oo 
+D 
I 
Cosecant . 
=00 
+D 
I 
+1 
 D 
I 
 I 
=8 
From the Pythagorean theorem, the sum of the squares of the projections of any straight line upon two straight lines at right angles to one another is equal to the square on the projected line, we get sin 2 a+cos 2 a=1, and from this by the help of the definitions of the other functions we we deduce the relations I + tan 2 a = sec 2 a, I + cot t a = cosec 2 a. We have now six relations between the six functions; !these enable us to express any five of these functions in terms of the sixth. The following table shows the values of the trigonometrical functions of the angles o, 27r, 7r, 7r, 27r, and the signs of the functions of angles between these values; I denotes numerical increase and D numerical decrease:  The correctness of the table may be verified from the figure by considering the magnitudes of the projections of OP for different positions.
7r 12 
?5° 
sine_ ?6?2 
cosine ,?6?,?2 
?5° 
5 ? 12 

4 
4 

7r 
18° 
A/ 5 I 
00+2A75 
7 2 ° 
2 
Io 
4 
4 
5' 

T. 
30 ° 
2 
23 
60 ° 
I 3 'r 
36 ° 
?IIO2?5 
1,/541 
54 ° 
Io'r 

4 

I 
I 
. 

4 
45 ° 
2 cosine 
2 sine 
45 ° 
7r 4 
The following table shows the sine and cosine of some angles for which the values of the functions may be obtained geometrically:  These are obtained as follows. (I) fir. The sine and cosine of this angle are equal to one another, since sin 47r =cos (7r17r); and since the sum of the squares of the sine and cosine is unity each is I/ i / 2. (2) 47r and 37r. Consider an equilateral triangle; the projection of one side on another is obviously half a side; hence the cosine of an angle of the triangle is z or cos 37r = 2, and from this the sine is found. (3) 7r/IO, 7r/5, 21r/5, 37r/10. In the triangle constructed in Euc. iv. 10 each angle at the base is 27r, and the vertical angle is Air. If a be a side and b the base, we have by the construction a(ab)= b 2 ; hence 2b.a 6/51); the sine of 7r/to is b/2a or 1(1/5i), and cos 57r is a/2b=4 (A/5+I), (4) 1127, Consider a rightangled triangle, having an angle 67r. Bisect this angle, then the opposite side is cut by the bisector in the ratio of 3 /3 to 2; hence the length of the smaller segment is to that of the whole in the ratio of 3 13 to 1,13+2, therefore tan 1 27r= { 3 13/(3 13+2) l tan 67r or tan A7r=23 (3, and from this we can obtain sin 17r and cos 117r.
5. Draw a straight line OD making any angle A with a fixed straight line OA, and draw OF making b an angle B with OD, this angle being measured po i tively in the same direction of as A; draw FE a perpen S dicular on DO (produced if necessary). The projection Di f f erence of of OF on OA is the sum of Two Angles. the projections of OE and EF on OA. FIG. 3 Now OE is the projection of OF on DO, and is therefore equal to OF cos B, and EF is the projection of OF an angle and the angle itself in this measure, when the magnitude of the angle is indefinitely diminished, are ultimately in a ratio of equality.
3. if a point moves from a position A to another position B on a straight line, it has described a length AB of the straight line. It Sign of is convenient to have a simple mode of indicating in S which direction on the straight line the length AB has been described; this may be done by supposing that a point moving in one specified direction is describing a positive length, and when moving in the opposite direction a negative length. Thus, if a point moving from A to B is moving in the positive direction, we consider the length AB as positive; and, since a point moving from B to A is moving in the negative direction, we consider the length BA as negative. Hence any portion of an infinite straight line is considered to be positive or negative according to the direction in which we suppose this portion to be described by a moving point; which direction is the positive one is, of course, a matter of convention.
If perpendiculars AL, BM be drawn from two points, A, B on any straight line, not necessarily in the same plane with AB, the length LM, taken with the positive or negative sign according to the convention as stated above, is called the projection of AB on the given straight line; the p rojection of BA being ML has the opposite sign to the projection of AB. If two points A, B be joined by a number of lines in any manner, the algebraical sum of the projections of all these lines is LM  that is, the same as the projection of AB. Hence the sum of the projections of all the sides, taken in order, of any closed polygon, not necessarily plane, on any straight line, is zero. This principle of projections we shall apply below to obtain some of the most important propositions in trigonometry.
4. Let us now return to the conception of the generation of an angle as in fig. I. Draw BOB at right angles to and equal to AA'. We shall suppose that the direction from A to A is the of Trigono positive one for the straight line AOA', and that from FIG. 2.
F on a straight line making an angle +17r with OD, and is therefore equal to OF sin B; hence OF cos (A+B) =OE cos A+EF cos (7r+A) =OF (cos A cos B  sin A sin B), or cos (A+B) =cos A cos B  sin A sin B. The angles A, B are absolutely unrestricted in magnitude, and thus this formula is perfectly general. We may change the sign of B, thus cos (A  B) =cos A cos ( B)  sin A sin ( B), or cos (A  B) =cos A cos B+sin A sin B. If we projected the sides of the triangle OEF on a straight line making an angle +i r with OA we should obtain the formulae sin (A B) = sin A cos B cos A sin B, which are really contained in the cosine formula, since we may put fir  B for B. The formulae tan A= tan B cot A cot B tan (A t B) = I tan A tan B' cot (A t B) = cot B t cot A are immediately deducible from the above formulae. The equations sin C+sin D=2 sin 2 (C+D) cos 1(C  D), sin C  sin D =2 sin 2 (C  D) cos z (C+D), cos D+cos C=2 cos 2 (C+D) cos 1(C  D), cos D  cos C=2 sin a (C+D) sin 2 (C  D), may be obtained directly by the method of projections. Take two equal straight lines OC, OD, making angles C, D, with OA, and draw OE perpendicular to CD. The angle which OE makes with OA is a (C+D) and that which DC makes is z (ir+C+D); the angle COE is 1(C  D). The sum of the projections of OD and DE on OA is equal to that of GE, and the sum of the projections of OC and CE is equal to that of OE; hence the sum of the projections of OC and OD is twice that of OE, or cos C+cos D=2 cos 2 (C+D) cos 1(C  D). The difference of the A projections of OD and OC an OA is equal to twice that of ED, hence we have the formula cos D  cos C =2 sin z (C+D) sin 1(C  D). The other two formulae will b? obtained by projecting on a straight line inclined at an angle +27r to OA. As another example of the use of projections, we will find the sum of the series cos a+cos (a+$) +cos (a +20) +. .. +cos (a+n  13).
Suppose an unclosed polygon each angle of which Sum of is 7r  i 3 to be inscribed in a circle, and let A, A , A2, Ser i es ofi A 3 . A n be n + I consecutive angular points; Cosines in let D be the diameter of the circle; and suppose a Arithmetical straight line drawn making an angle a with AA 1 , then Progression. a+,, a+2/3,. are the angles it makes with A1 A2, A2, A3, ...; we have by projections AA n cos (a+2n  I(3) =AA 1 {cos a+ cos a+(3+...+cosa+(n  I)0}, also AA1=D sin 1/3, AA n = D sin n(; hence the sum of the series of cosines is cos (a+zn  I g) sin 2n(3 cosec By a double application of the addition formulae we may obtain the formulae Formulae for sin (A i +A 2 +A 3)=sin A 1 cos A2 cos A3 Sine and +cos A 1 sin A2 cos A 3+cos A 1 cos A2 sin A3 of  sin A 1 sin A2 sin A3 i Cosine of cos (A 1 +A 2 +A 3 '') =cos A 1 cos A2 cos A3 Sum .  cos A 1 sin A2 sin A 3  sin A 1 cos A2 sin A3 Angles.  sin A 1 sin A2 cos A3. We can by induction extend these formulae to the case of n angles. Assume sin (A 1 +A 2 + ... +An) =S1  S3+S5  ... cos (A 1 + A 2 + ... +A n) =So  S 2 +S 4  .. where S r denotes the sum of the products of the sines of r of the angles and the cosines of the remaining n  r angles; then we have sin (A 1 +A 2 + ... +A n +A n+1 ) =cos A n+i (S i  S 3 +S 5  ...) +sin A n+1 (So  S 2 +S 4 
.). The righthand side of this equation may be written (S i cos An +1 +So sin A n+1)  (S 3 cos An+1+S2 sin An+1) + ..., or S'1  S'3+ .. where SC denotes the q uantity which corresponds for n+I angles to Sr for n angles; similarly we may proceed with the cosine formula. The theorem ' are true for n=2 and n =3; thus they are true generally. The formulae Formulae cos 2A =cos t A  sin 2 A =2 cos 2 A  1 = I2 sin e A, for Multiple 2 tan A and Sub sin 2A =2 sin A cos A, tan 2A = 2 A' Multiple I  tan A Angles. sin 3A =3 sin A  4 sin 3 A, cos 3A =4 cos 3 A  3 cos A, 'sin' cos n  1 A sin A 71(n I)(n 2) cos" 3 A sin 3 A+ .. 31 (n2r) cos h er 1 A sin2r +1 A, (2r n(r2, tan2A+...+( 1)rn(n1)..(n2T+r)tan2rA In the particular case of n=3 we have tan 3 A = 3 tan A  tan3 A. I  3 ta n A The values of sin 2A, cos 2A, tan 2A are given in terms of cos A by the formulae sin 2 A = ( I)P ( 2 I  cos A) 3, cos z A = ( i)4 (I+cos A 21  co s A l tan 2 A = ( I) T (I +cos A ' where p is the integral part of A/23r, q the integral part of A/27r+2, and r the integral part of A /7r.
Sin 2A, cos zA are givenin terms of sin A by the formulae 2 sin 2A = ( I)P'(I+sin A)+( I)4'(I  sin A), 2 cos 2A = ( +sin A)i  ( I)4'(I  sin A)+, where p' is the integral part of A/27r+4 and q' the integral part of A/21r4.
6. In any plane triangle ABC we will denote the lengths of the sides BC, CA, AB by a, b, c respectively, and the angles BAC, ABC, ACB by A, B, C respectively. The fact that the projec tions of b and c on a straight line perpendicular to the Properties side a are equal to one another is expressed by the equa of Triangles. tion b sin C=c sin B; this equation and the one obtained by projecting c and a on a straight line perpendicular to a may be written a/sin A = b/sin B =c/sin C. The equation a = b cos C+c cos B expresses the fact that the side a is equal to the sum of the projections of the sides b and c on itself; thus we obtain the equations a =b cos C+c cos B b = c cos A +a cos C c= a cos B+b cos A If we multiply the first of these equations by  a, the second by b, and the third by c, and add the resulting equations, we obtain the formula b e dc 2  a 2 = 2bc cos A or cos A = (b 2 +c 2  a 2) /2bc, which gives the cosine of an angle in terms of the sides,. From this expression for cos A the formulae sin 2A = (s  b) (s  c) z ? cos 2A = s(s bc a) 2' tan IA = (s (s)(a) c)? s i n A = b s e{s(s  a)(s  b)(s  c)}2, where s denotes z (a+b+c), can be deduced by means of the dimidiary formula.
From any general relation between the sides and angles of a triangle other relations may be deduced by various methods of transformation, of which we give two examples.
a. In any general relation between the sines and cosines of the angles A, B, C of a triangle we may substitute pA+gB+rC, rAfpB+qC, qA+rB +pC for A, B, C respectively, where p, q, r are any quantities such that p+q+r+I is a positive or negative multiple of 6, provided that we change the signs of all the sines. Suppose p+q+r+I =6n, then the sum of the three angles 2n7r  (pA +qB +rC), 2n7r  (rA +pB +qC), 2nir  (qA +rB+PC) is,r; and, since the given relation follows from the condition A+B+C =r, we may substitute for A, B, C respectively any angles of which the sum is 7r; thus the transformation is admissible.
/3. It may easily be shown that the sides and angles of the triangle formed by joining the feet of the perpendiculars from the angular points A, B, C on the opposite sides of the triangle ABC are respectively a cos A, b cos B, c cos C, 7r2A, 7r2B, 7r2C; we may therefore substitute these expressions for a, b, c, A, B, C respectively in any general formula. By drawing the perpendiculars of this second triangle and joining their feet as before, we obtain a triangle of which the sides are  a cos A cos 2A,  b cos B cos 2B,  c cos C cos 2C and the angles are 4A7r, 4B7r, 4C7r; we may therefore substitute these expressions for the sides and angles of the original triangle; for example, we obtain thus the formula 4A  a 2 cos 2 A cos t 2A  b 2 cos 2 B cos 2 2B  c 2 cos t C cos 2 2C COS 2bc cos B cos C cos 2B cos 2C This transformation obviously admits of further exten sion. Solution of (I) The three sides of a triangle ABC being given, Triangles. the angles can be determined by the formula L tan IA = lo+z log (s  b)+2 log (s  c)  2 log s2 log (s  a) and two corresponding formulae for the other angles.
cos nA =cos"A 11(111) I cos n  2 A sin e A+ ... + ()T n (n  I) ... (n  2 r ? I) cosh  2T A sin e ' A + ... 2Y may all be deduced from the addition formulae by making the angles all equal. From the last two formulae we obtain by division 7)(n2) n(na)...(n 20 n tan A  3 i tan3A+...+( i)r a).. (1 tanzr+1 A+._. tan nA  FIG. 4.
Spherical Trigonometry. 7. We shall throughout assume such elementary propositions in spherical geometry as are required for the purpose of the investigation of formulae given below.
A spherical triangle is the portion of the surface of a sphere bounded by three arcs of great circles of the sphere. If BC, CA, AB denote these arcs, the circular measure of the ofS nition angles subtended by these arcs respectively at the centre of the sphere are the sides a, b, c of the spherical T triangle ABC; and, if the portions of planes passing through these arcs and the centre of the sphere be drawn, the angles between the portions of planes intersecting at A, B, C respectively are the angles A, B, C of the spherical triangle. It is not necessary to consider triangles in which a side is greater than 7r, since we may replace such a side by the remaining arc of the great circle to which it belongs. Since two great circles intersect each other in two points, there are eight triangles of which the sides are arcs of the same three great circles. If we consider one of these triangles ABC as the fundamental one, then one of the others is equal in all respects to ABC, and the remaining six have each one side equal to, or common with, a side of the triangle ABC, the opposite angle equal to the corresponding angle of ABC, and the other sides and angles supplementary to the corresponding sides and angles of ABC. These triangles may be called the associated triangles of the fundamental one ABC. It follows that from any general formula containing the sides and angles of a spherical triangle we may obtain other formulae by replacing two sides and the two angles opposite to them by their supplements, the remaining side and the remaining angle being unaltered, for such formulae are obtained by applying the given formulae to the associated triangles.
If A', B', C are those poles of the arcs BC, CA, AB respectively which lie upon the same sides of them as the opposite angles A, B, C, A then the triangle A'B'C is called the polar triangle of the triangle ABC. The sides of the polar triangle are 7r  A  B, 7  C, and the angles 'r  a, it  b, 7  c. Hence from any general formula connecting the sides and angles of a spherical triangle we may obtain another formula by changing each side into the supplement of the opposite B angle and each angle into the supplement of the opposite side.
8. Let 0 be the centre of the sphere on which is the spherical triangle ABC. Draw AL perpendicular to OC and AM perpendicular to the plane OBC. Then the projection of OA on OB is the sum of the projections of OL, LM, MA on the same straight line. Since AM has no projection on any straight line in the plane OBC, this gives angles.
OA cos c = 0L cos a+LM sin a. Now OL =OA cos b, LM = AL cos C =OA sin b cos C; therefore cos c =cos a cos b+sin a sin b cos C. We may obtain similar formulae by interchanging the Angles. letters a, b, c, thus cos a =cos b cos c+sin b sin c cos A cos b =cos c cos a+sin c sin a cos B (i) cos c =cos a cos b+sin a sin b cos C These formulae (I) may be regarded as the fundamental equations connecting the sides and angles of a spherical triangle; all the other relations which we shall give below may be deduced analytically from them; we shall, however, in most cases give independent proofs. By using the polar triangle transformation we have the formulae cos A=  cos B cos C+sin B sin C cos a cos B=  cos C cos A +sin C sin A cos b (2) cos C=  cos A cos B+sin A sin B cos c In the figures we have AM=AL sin C=r sin b sin C, where r denotes the radius of the sphere. By drawing a perpendicular from A on OB, we may in a similar manner show that AM= r sin c sin B, therefore sin B sin c =sin C sin b. By interchanging the sides we have the equation sin A. sin B sin C  k (3) sin a sin b sin c we shall find below a symmetrical form for k. If we eliminate cos b between the first two formulae of (i) we have cos a sin 2 c = sin b sin c cos A +sin c cos c sin a cos B; therefore cot a sin c= (sin b/sin a) cos A +cos c cos B =sin B cot A +cos c cos B. We thus have the six equations cot a sin b= cot A sin C+cos b cos C cot b sin a= cot B sin C+cos a cos C cot b sin c =cot B sin A +cos c cos A cot c sin b =cot C sin A +cos b cos A cot c sin a =cot C sin B +cos a cos B cot a sin c =cot A sin B +cos c cos B When C= air formula (I) gives cos c =cos a cos b and (3) gives sin b =sin B sin c sin a =sin A sin c from (4) we get tan a= tan A sin b =tan c cos B( tan b = tan B sin a= tan c cos A The formulae cos c= cot A cot B and follow at once from (a), (13), (y). These are the formulae which are used for the solution of right  angled triangles. Napier gave mnemonical rules for remembering them.
The following proposition follows easily from the theorem in equation (3): If AD, BE, CF are three arcs drawn through A, B, C to meet the opposite sides in D, E, F respectively, and if these arcs pass through a point, the segments of the sides satisfy the relation sin BD sin CE sin AF=sin CD sin AE sin BF; and conversely if this relation is satisfied the arcs pass through a point.)~ rom this theorem it follows that the three perpendiculars from the angles on the opposite sides, the three bisectors of the angles, and the three arcs from the angles to the middle points of the through a point.
9. If D be the point of intersection of the three bisectors of the angles A, B, C, and if DE be drawn for Sine perpendicular to BC, it may be shown that BE = 2 (a + c  b) and CE = 1(a + b  c), and that of Half the angles BDE, ADC are supplementary. We have also sin c sin ADB sin b sin ADC , therefore sin e 2A sin BD sin 2 A ' sin CD sin zA in b sin c But sin BD sin BDE = sin BE s =sin 1(a +c  b), and sin CD sin CDE= sin CE= sin (a+b  c); A Csin 2(a+c  b) sin z(a+b  c) z therefore sin 2 = sin b sin c (5) Apply this formula to the associated triangle of which 7  A, 7  B, C are the angles and 7  a, nb, c are the sides; we obtain the formula cos sin 2 (b+c  a) sin z (a+b+c) (6) 2  sin b sin c (2; The two sides a, b and the included angle C being given, the angles A, B can be determined from the formulae A+B=ir  C, L tan 2(A  B) = log (a  b)  log (a+b) + L cot 2C, and the side c is then obtained from the formula log c= log a+L sin C  L sin A. (3) The two sides a, b and the angle A being given, the value of sin B may be found by means of the formula L sin B=L sin A+log b  log a; this gives two supplementary values of the angle B, if b sin A< a. If b sin a there is no solution, and if b sin A= a there is one solution. In the case b sin A< a, both values of B give solutions provided b > a, but the acute value only of B is admissible if b < a. The other side c can be then determined as in case (2).
(4) If two angles A, B and a side a are given, the angle C is determined from the formula C='rr  A  B and the side b from the formula log b= log aFL sin B  L sin A. Areas of The area of a triangle is half the product of a side into the perpendicular from the opposite Quadri an g le on that side; thus we obtain the expressions lbc s i n A, {s(s  a) (s  b)(s  c)}I for the area of a triangle. A large collection of formulae for the area of a triangle are given in the Annals of Mathematics for 1885 by M. Baker.
Let a, b, c, d denote the lengths of the sides AB, BC, CD, DA respectively of any plane quadrilateral and A +C=2a; we may obtain an expression for the area S of the quadrilateral in terms of the sides and the angle a.
We have 2S=ad sin A+bc sin(2a  A) and (a2 ±d 2 1 ,2  c 2) =ad cos A  be cos (Oa  A); hence 45 2 + 4 (a 2 +d 2  b 2  c 2) 2= a 2 d 2 +b 2 c 2  2abcd cos If 2S = a + b+ c + d, the value of S may be written in the form S= {s(s  a)(s  b)(s  c)(s  d)  abed cos2a12.
Let R denote the radius of the circumscribed circle, r of the in scribed, and rl, r2, r 3 of the escribed circles of a triangle ABC; the values of these radii are given by the following formulae: R = abc/4S = a/2 sin A, and Escribed r=S/s= (s  a)tan ZA=4R sin IA sin ZB sin IC, Circles of a r i =S/(s  a) =s tan ZA =4R sin 2A cos 2B cos C. Triangle. sin BD sin CD sin CDE sin BDE FIG.
cos A =cos A sin B cos B =cos b sin A r (4) (a) (a) ('Y) (E) (i") A E FIG. 6.
opposite sides, each pass By division we have A sin 2(a+c  b) sin 2(a+b  c) I tan 2 = sin 2(b+c  a) sin 2(a+b+c) 5 (7) and by multiplication sinA =2{sin (a+b+c) sin 2(b+c  a) sin 2(c+a  b) sin 2(a+b  c)}2 sin b sin c = { I  cos t a  cos' b  cos t c +2 cos a cos b cos c} i sin b sin c. Hence the quantity k in (3) is {1  cos t a  cos t b  cos t c+2 cos a cos b cos c}i/sin a sin b sin c. (8) Of Half Apply the polar triangle transformation to the formulae (7) (8) and we obtain a cos 1(A +C  B) cos 2(A}B  C1 1 cos t  sin B sin C (9) a 1  cos 2(B+C  A) cos 2(A+B+C I sin g = sin B sin C (t o)  cos 2(B+C  A) cos 2(A+B+C 4 cos 1(A B) cos 1(A+B  C (I I) If k' = { I  cos 2 A  cos 2 B  cos t C  2 cos A cos Bcos C} 2/sin A sin B sin C, we have. kk' =I (12) Io. Let E be the middle point of AB; draw ED at right angles to D AB to meet AC in D; then DE bisects the angle ADB. Let CF bisect the angle For DCB and draw FG per pendicular to BC, then CG=2(a  b,L FBE =2(A+B), L FCG =90°  ZC. From the triangle CFG we have cos CFG = cos CG sin FCG, and B from the triangle FEB cos EFB = cos EB sin FBE. Now the angles CFG, EFB are each supplementary to the angle DFB, therefore cos 2(a  b)cosl C=sin2(A +B)cos2c. (13) Also sin CG = sin CF sin CFG and sin EB = sin BF sin EFB; therefore sin2(a  b)cos2C= sin 2 (A  B)sin2c. (14) Apply the formulae (13), (14) to the associated triangle of which a, 7r  b, 7r  c, A, 7r  B, 7r  C are the sides and angles, we then have sin2(a+b)sin2C=cos2(A  B)sin2c (15) cos2(a+b)sin2 C=cost (A +B)cos2c. (16) The four formulae (13), (14), (15) (16) were first given by Delambre in the Connaissance des Temps for 1808. Formulae equivalent to these were given by Mollweide in Zach's Monatliche Correspondenz for November 1808. They were also given by Gauss (Theoria motus, 1809), and are usually called after him.
II. From the same figure we have
tan FG = tan FCG sin CG = tan FBG sin BG; therefore cot ICsin2(a  b)tan2(A  B)sin2 (a+ b), or tan2 (A  B) =i n 2(a+b)cotIC. (17) s Apply this formulae to the associated triangle (Or  a, b, it  c, it  A, B, zr  C), and we have cot (A +B)  co cos 2(a  b)tan 2C, or tan 1(A 1B)  cos 2(a+b)cot ZC. (18) If we apply these formulae (17), (18) to the polar triangle, we have tan 2(a  b)  sin 2 (A +B)tan 2c (19) tan 2(A IB) = cos +B)tan Zc. (20) The formulae (17), (18), (19), (20) are called Napier's " Analogies "; they were given in the Mirif. logar. canonis descriptio. 12. If we use the values of sin la, sin lb, sin lc, cos la, cos lb, cos 4c, given by (9), (Jo) and the analogous formulae obtained by interchanging the letters we obtain by multiplication 1 1 1 i z z z z sin la lb C =s i n l 13. The formulae we have given are sufficient to determine three parts of a triangle when the other three parts are given; moreover such formulae may always be chosen as are adapted to logarithmic calculation. The solutions will be unique T i except in the two cases (I) where two sides and the angle opposite one of them are the given parts, and (2) where two angles and the side opposite one of them are given.
Suppose a, b, A are the given parts. We determine B from the formula sin B =sin b sin A/sin a; this gives two supplementary values of B, one acute and the other Ambiguous obtuse. Then C and c are determined from the C equations sin 1(A tan 2C= sin z(a+b) cot 1 (A B), tan Zc= sin (A  B) tan 2(a  b).
Now tan 2 C, tan lc, must both be positive; hence A  B and a  must have the same sign. We shall distinguish three cases. First, suppose sin b< sin a; then we have sin B< sin A. Hence A lies between the two values of B, and therefore only one of these values is admissible, the acute or the obtuse value according as a is greater or less than b; there is therefore in this case always one solution. Secondly, if sin b> sin a, there is no solution when sin b sin A> sin a; but if sin b sin A< sin a there are two values of B, both greater or both less than A. If a is acute, a  b, and therefore A  B, is negative; hence there are two solutions if A is acute and none if A is obtuse. These two solutions fall together if sin b sin A =sin a. If a is obtuse there is no solution unless A is obtuse, and in that case there are two, which coincide as before if sin b sin A =sin a. Hence in this case there are two solutions if sin b sin A< sin a and the two parts A, a are both acute or both obtuse, these being coincident in case sin b sin A =sin a; and there is no solution if one of the two A, a, is acute and the other obtuse, or if sin b sin A >sin a. Thirdly, if sin b =sin a then B=A or 7 =A. If a is acute, a  b is zero or negative, hence A  B is zero or negative; thus there is no solution unless A is acute, and then there is one. Similarly, if a is obtuse, A must be so too in order that there may be a solution. If a = b = 27r, there is no solution unless A = Z7r, and then there are an infinite number of solutions, since the values of C and c become indeterminate.
The other case of ambiguity may be discussed in a similar manner, or the different cases may be deduced from the above by the use of the polar triangle transformation. The method of classification according to the three cases sin b,sin a was given by Professor Lloyd Tanner (Messenger of Math., vol. xiv.)..
14. If r is the angular radius of the small circle inscribed in the triangle ABC, we have at once tan r=tan ZA sin (s  a), where 2s=a+b+c; from this we can derive the formulae for Spherical Excess. tan r =n cosec s =1N sec ZA sec ZB sec IC= sin a sin ZB sin ZC sec ZA (21) where n, N denote the expressions {sin ssin (s  a) 'sin (s  b) sin (s  c)}2, {  cos S cos (S  A) cos (S  B) cos (S  C)}2.
The escribed circles are the small circles inscribed in three of the associated triangles; thus, applying the above formulae to the triangle (a, it  b, 7r  c, A, 7r  B, zr  C), we have for r 1, the radius of the escribed circle opposite to the angle A, the following formulae tan 1' 1 =tan ZA sin s = n cosec (s  a) = IN sec 2A cosec 2B cosec 2 C =sin a cos ZB cos LC sec A. (22) The pole of the circle circumscribing a triangle is that of the circle inscribed in the polar triangle, and the radii of the two circles are complementary; hence, if R be the radius of the circumscribed circle of the triangle, and R i, R2, R the radii of the circles circumscribing the associated triangles, we have by writing 2,r  R for r, 17r  R 1 for r l, 7r  a for A, &c., in the above formulae cot R= cot la cos (S  A) = I n cosec la cosec 2b cosec lc =  N sec S =sin A cos lb cos lc cosec la (23) cot R 1 =  cot la cos S= in cosec la sec lb sec lc = N sec (S  A) =sin A sin lb sin lc cosec 4a. (24) The following relations follow from the formulae just given: 2tanR =cot r 1 +cot r 2 +cot r 3  cot r, 2tanR i =cot r +cot r 2 +cot ra  cot r1, tan r tan r 1 tan r 2 tan r 3 = n 2, sin 2 s = cot r tan r 1 tan r 2 tan r3, sin 2 (s  a) =tan r cot r 1 tan r 2 tan r3.
15. If E=A+B+C7r, it may be shown that E multiplied by the square of the radius is the area of the triangle. We give some of the more important expressions for the quantity E, which is called the spherical excess.
We have cos 2(A + B) cos 2(a + b) sin 2(A + B) cos 2(a  b) sin ZC  d lc and cos ZC  cos lc ' sin (C  E) cos 2(a + b) cos (C  E) cos 2(a  b), or sin ZC  cos lc and cos ZC  cos lc ' sin 2 C  sin 2(C  E) cos lc  cos 2(a+ b) hence sin ZC + sin 2(C  E)  cos lc + cos 2(a + b)' tan g 'a = ' (B+C  A) cos la cos lb sin C= cos lc cos 2 (A +B  C). sin la sin sin C= cos lc cos 2 (A +B + C) These formulae were given by Schmiesser in Crelle's Journ., vol. x. The relation sin b sin c+cos b cos c cos A =sin B sin C  cos B cos C cos a was given by Cagnoli in his Trigonometry (1786), s and was rediscovered by Cayley (Phil. Mag., 1859). It follows from (I), (2) and (3) thus: the righthand s i de of the equation equals sin B sin C+cos a (cos A  sin B sin C cos a) =sin B sin C sin 2 a+cos a cos A, and this is equal to sin b sin c + cos A (cos a  sin b sin c cos A) or sin b sin c + cos b cos c cos A. tang±(CE) =tan 2 s tan (sc).
Similarly tan 4E tan' ±(CE) =tan 1(s a) tan 2(sb); therefore tan 4E={tan zs tan 2(s a) tan 1(s b) tan 2(sc)}1 (25) This formula was given by J. Lhuilier.
1 1 1 cos 2(a {b) 1 2 Also sin z C cos 1Ecos 2 C sin 2 E = sin C; COS 2G cos 1C cos 1E+sin 1C sin ZE = cos Ra i b) cos 1C; COS 2G 0 2 +cos a+cos b +cos c (26) cos E = 4 cos la cos 2b cos 1c 26 This formula was given by Euler (Nova acra, vol. x.). If we find sin 2E from this formula, we obtain after reduction sin lE  2 1 1 ' 2 cos 2 a cos 2 b cos 2c a formula given by Lexell (Acta Petrop., 1782).
From the equations (21), (22), (23), (24) we obtain formulae for the spherical excess: sin 2 2E = tan R cot R1 cot R2 cot R3 4(COt r 1 +cot r 2 +cot r3)  (cot rcot r l +cot r 2 +cot r 8) (cot r+cot r1 cot (cot r+cot r i +cot r 2 +cot r3).
The formula (26) may be expressed geometrically. the middle points of the sides AB, AC. Then we _ 1 +cos a+cos b +cos c hence cos l E i = cos MN sec a.
4 COS 2b COS IC 2 A geometrical construction has been given for E by Gudermann (in Crelle's Journ., vi. and viii.). It has been shown by Cornelius Keogh that the volume of the parallelepiped of which the radii of the sphere passing through the middle points of the sides of the triangle are edges is sin 2 E.
16. Let ABCD be a spherical quadrilateral inscribed i n a small circle; let a, b, c, d denote the sides AB, BC, of Spherical CD, DA respectively, and x, y the diagonals AC, BD. It can easily be shown by joining the angular points of the quadrilateral to the pole of the circle that inscribed A +C = B +D. If we use the last expression in 2) in Small p (3 Circle, for the radii of the circles circumscribing the triangles BAD, BCD, we have sin A cos 2a cos 2d cosec 2y= sin C cos lb cos ZC cosec 2y; whence sin A sin C w cos 2b cos lc  cos la cos 2d This is the proposition corresponding to the relation A +C= 7r for a plane quadrilateral. Also we obtain in a similar manner the theorem sin lx sin 2y sin B cos lb  sin A cos id' analogous to the theorem for a plane quadrilateral, that the diagonals are proportional to the sines of the angles opposite to them. Also the chords AB, BC, CD, DA are equal to 2 sin la, 2 sin lb, 2 sin lc, 2 sin Zd respectively, and the plane quadrilateral formed by these chords is inscribed in the same circle as the spherical quadrilateral; hence by Ptolemy's theorem for a plane quadrilateral we obtain the analogous theorem for a spherical one sin lx sin 2y = sin la sin Zc+sin lb sin 2d.
It has been shown by Remy (in Crelle's Journ., vol. iii.) that for any quadrilateral, if z be the spherical distance between the middle points of the diagonals, cos a+cos b+cos c+cos d = 4 cos lx cos 2y cos Zz.
This theorem is analogous to the theorem for any plane quadrilateral, that the sum of the squares of the sides is equal to the sum of the squares of the diagonals, together with twice the square on the straight line joining the middle points of the diagonals.
A theorem for a rightangled spherical triangle, analogous to the Pythagorean theorem, has been given by Gudermann (in Crelle's Journ., vol. xlii.).
Analytical Trigonometry. 17. Analytical trigonometry is that branch of mathematical analysis in which the analytical properties of the trigonometrical functions are investigated. These functions derive their city importance in analysis from the fact that they are the sim. Plest singly periodic functions, and are therefore adapted to the representation of undulating magnitude. The sine, cosine, secant and cosecant have the single real period 27r; i.e. each is unaltered in value by the addition of 27r to the variable. The tangent and cotangent have the period 7r. The sine, tangent, cosecant and cotangent belong to the class of odd functions; that is, they change sign when the sign of the variable is changed. The cosine and secant are even functions, since they remain unaltered when the sign of the variab12. is reversed., The theory of the trigonometrical functions is intimately connected with that of complex numbers  that is, of numbers of the form x+cy(c = 1). Suppose we multiply together, by the rules of ordinary algebra, two such numbers we have with Theory (x 1 Lyl) (x2 } 0/2)_ (xlx2yly2) + 6(x 1 y 2 + x2y1) We observe that the real part and the real factor of the Quantities. imaginary part of the expression on the righthand side of this equation are similar in form to the expressions which occur in the addition formulae for the cosine and sine of the sum of two angles; in fact, if we put x 1 = r i cos 0 1, y 1 = r i sin 01, x 2 = r 2 cos 02, y 2 = r 2 sin 0 2, the above equations becomes r i (cos 01+c sin 0 1) X r 2 (cos 02+ c sin 0 2) = r 1 r 2 cos 01+02 +I sin 01+02). We may now, in accordance with the usual mode of representing complex numbers, give a geometrical interpretation of the meaning of this equation. Let P 2 be the point whose coordinates referred to rectangular axes Ox, Oy are xi, y 1; then the point P 2 is employed to represent the number xl +cyl. In this mode or representation real numbers are measured along the axis of x and imaginary ones along the axis of y, additions being performed according to the parallelogram law. The points A, A l represent the numbers =1, the points a, a l the numbers c. Let P2 represent the expression x 2 +cy 2 and P the expression (x1+ oil) (x2 + (.3/ 2). The quantities rl, 0 1, r2, 0 2 are the polar coordinates of P i and P2 respectively, referred to 0 as origin and Ox as initial line; the above equation shows that r 1 r 2 and 0 1 +0 2 are the polar coordinates of P; hence OA: OP 1 :: OP2' OP FIG, 8.
and the angle POP 2 is equal to the angle P 1 0A. Thus we have the following geometrical construction for the determination of the point P. On OP 2 draw a triangle similar to the triangle OAP 1 so that the sides OP2, OP are homologous to the sides OA, OP 1 , and so that the angle POP 2 is positive; then the vertex P represents the product of the numbers represented by P1, P2. If x 2 +cy 2 were to be divided by xi+cyl the triangle OP'P 2 would be drawn on the negative side of P2, similar to the triangle OAP 1 and having the sides OP', OP 2 homologous to OA, OP1, and P' would represent the quotient.
18. If we extend the above to n complex numbers by continual repetition of a similar operation, we have  = Cos (0 1 = 0 2 +
+ 072) + c sin (o 1 + 0 2 +. .. + on).
P 
If 0 1 =0 2 = ... =0,2=01, this equation becomes (cos 0+c sin 0)n =cos n0+c sin n0; this shows that cos o +c sin 0 is a value of (cos n0+c sin n0)9. If now we change 0 into 0/n, we see that cos 0/n+c sin 0/n is a value of (cos 0+ c sin 0)n; raising each of these quantities to any positive integral power m, cos mo/n+c sin mein is one value of (cos 0+L sin 0; 11,, i. Also cos ( m0/n)+ c sin (m0/n) = cos mo/n + c sin m0/n' hence the expression of the lefthand side is one value of (cos 0+ e sin 0)' n / n . We have thus De Moivre's theorem that cos k0+c sin k0 is always one value of (cos 0+c sin 0) k , where k is any rational number. This theorem can be extended to the case in which k is irrational, if we postulate that a value of (cos 0+c sin 0) k denotes the limit of a sequence of corresponding values of (cos 0+c sin 0)ks, where k1, k2... ks... is a sequence of rational numbers of which k is the limit, and further observe that as cos k0+c sin ko is the limit of cos k s 0+c sin ks0. The principal object of De Moivre's theorem is to enable us to find all the values of an expression of the form (a+cb)'n 1n, where m and n are positive integers prime to each other. n If a = r cos 0, r sin 0, we require the values of I' m in (cos 0+c sin o)" n / n . One value is immediately fur of aComplex nished by the theorem; but we observe that since the expression cos o+c sin 0 is unaltered by adding any multiple of 27r to 0, the n/mth power of I' m '. (cos m.0+2s7r/n+c sin m.0+2s7rIn) is a+cb, if s is any integer; hence this expression is one of the values required. Suppose that for two values s 1 and s 2 of s the values of this expression are the same; then we must have m.0 +2s 1 7r /nm.0+2s 2 7r/n; a multiple of 2r, or si 52 must be a multiple of n. Therefore, if we give s the values o, 1, 2,, ..n  1 successively, we shall get n different values of (a+cb)' n1n , and these will be repeated if we give s other values; hence all the values of whence, solving for cos 2E, we get the following r 2 +cot r 3) X Let M, N be find cos MN (cos 0 1 + c sin 0 1) (cos 0 2 + c sin 02). .. (cos 0n + e sin 0n) m i n are obtained by giving s the values o, 1, 2, ... n  I in the expression rm!n (cos m. ° + 2s7r/n + c sin m .0 + 2s7r/n), where r = (a 2 +1, 2)1 and ° =arc tan b/a. We now return to the geometrical representation of the complex numbers. If the points B 1 , B2, B3.... B. represent the expres sion + cy, (x + cy) 2, (x+cy)3, B 4 (x+cy)n respectively, the triangles OAB i, OB 1 B 2,
OB,,, 1 B n are all similar. Let (x+cy) n =a+cb, then the converse problem of finding the nth root of a+cb is equivalent to the geometrical problem of describing such a series of triangles that OA is the first side of the first triangle and OB„., the second side of the nth. Now it is obvious that this geometrical problem has more solutions than one, since any number of complete revolutions round 0 may be made in travelling from B 1 to B. The first solution is that in which the vertical angle of each triangle is 13 7 ,0A /n; the second is that in which each is (B n OA +27r) In, in this case one complete revolution being made round 0; the third has (B n OA +47r)ln for the vertical angle of each triangle; and so on. There are n sets of triangles which satisfy the required conditions. For simplicity we will take the case of the determina B tion of the values of (cos ° + c sin 0)A.
Suppose B to represent the expression ' cos 0+ c
sin 0. If the angle AOP 1 is 30, P i
represent the root cos c sin 30; the angle AOB is
m filled up by the angles O of the three siilar triangles
A0131, P10p1, p10B. Also, if P2 i P3 be such that the
angles P 1 0P 2 P 1 0P 3 are 37r, s ir respectively, the
two sets of triangles AOP 2, P 2 0p 3, p 3 OB and AOP
31 P30p2, p 2 OB satisfy the conditions of similarity
and of having OA, OB for the bounding sides; thus P 2,
P 3 represent the roots cos 1(0127r) +/.. sin 3(0+27r),
COS 3 0+47r)+1. sin 3(0+47r) respectively. If B coincides
with A, the problem is reduced to that of finding the
three cube roots of unity. One
will be represented by A and the others by the two angular
points of an equilateral triangle, with A as one angular
point, inscribed in the circle.
The problem of determining the values of the nth roots of unity is equivalent to the geometrical problem of inscribing a regular polygon of n sides in a circle. Gauss has shown in his Disquisitiones arithmeticae that this can always be done by the compass and ruler only when n is a prime of the form 2 p +I. The determination of the nth root of any complex number requires in addition, for its geometrical solution, the division of an angle into n equal parts.
19. We are now in a position to factorize an expression of the form n (a+cb). Using the values which we have obtained above for (a +0)1 n , we have I xn(a+ cb)=P =n1 s [ xrn(cos °+ns7r +c sin B+ s7rl? (1) s= 0 ) If b =o, a =I, this becomes s=n1 C 2.512S7r1 x n  I=P xco s sin n J s=0 s =1(n  1) (x n  I = ( I)P x2 2x COS  h s=1 x22xy cos °+ 2 n? +y 2 ]. (6) Airy and Adams have given proofs of this theorem which do not invol v e the use of the symbol c (see Camb. Phil. Trans., vol. xi).
A large number of interesting theorems may be derived from De Moivre's theorem and the factorizations which we have deduced from it; we shall notice one of them.
In equation (6) put y = i/x, take logarithms, and then differentiate each side with respect to x, and we get 2n(x2n1 x 2n1) s=n1 2(xx 3)
x 24 2 cos n0+x2n 0 x 2 2 COS ° 2 n +x2 Put x 2 = a/b, then we have the expression n (a2n  b2n) (a2  b2) (a2n2a n b n cos n°+b2n) for the sum of the series s=n1
s= o a 2 2ab cos °+ 2s7r+b 2 n 20. Denoting the complex number x+iy by z, let us consEx ider the series I +z+z 2 /2 ! + ... +z n /n ! + ... This series converges uniformly and absolutely for all values of z whose The moduli do not exceed an arbitrarily chosen positive The x number R. Consequently the function E(z), defined as the limiting sum of the above series, is continuous Series. in every finite domain. The two series representing E(z 1) and E(z2),. when multiplied together give the series represented by E(z1+z2) In accordance with a known theorem, since the series for E(z i) E(z2) are absolutely convergent, we have E (z 1) XE(z 2) =E(zi+z2) From this fundamental relation, we deduce at once that {E(z) }n =E(nz), where n is any positive integer. The number E(I), the sum of the convergent series I+I+1/2!+1/3!.. ., is usually denoted by e; its value can be shown to be 2.5 18281828459
. It is known to be a transcendental number, i.e. it
cannot be the root of any algebraical equation with rational
coefficients; this was first established by Hermite. Writing z=1,
we have E(n)=e n , where n is a positive integer.
If z has as a value a positive fraction p/q, we find that
{E(p/q) }qE(p) =e 5; hence E(p/q) is the real positive
value of P%q . Again E(plq) XE(plq) = E(o) =I,
hence E(plq) is the real positive value of e P / q
. It has been thus shown that for any real and rational number
x, the value of E(x) is the principal value of
e 1 . This result can be extended to irrational values of
x, if we assume that e x is for such a value of x
defined as the limit of the sequence e xl, e x2,. , where
x 1, x 2 ,.. is a sequence of rational numbers of which x
is the limit, since E(x 1), E(x 2) ..., then converges to E(x).
Next consider (1 +z/m) m, where m is a positive integer. We have by the binomial theorem, (j zs I m S! +...+(1) m m) (Im) ...
(TIT + +... +s m l ); equals I 0 s s . s 1 /2m where O s is such that (i+)m=i++ (I?) z2 ?.. .+ L I9 s s. si I 2m + I  °m 2 m!
+©5(s2)!+...+°m(m 2)! )) Since the series for E(z) converges, s can be fixed so that for all values of m > s the modulus of z s+1 /(s+ I) ! +  +z m /m! is less than an arbitrarily chosen number 3E. Also the modulus of 1+0 3 z/1+ ... +°m zm2 l(m 2) ! is less than that of I + I III /I ! + I z I 2 /2! +..., or of e mod z, hence mod Rs<3s+(1/2m). mod (z 2 e z ) <E, if m be chosen sufficiently great. It follows that lim m. (I +z/m) m =E(z), where z is any complex number. To evaluate E(z), write I +x/m =p cos cp, y/m = p sin 4, then s =in1 (xI)(x+I)P (x_cossis2 2 = (x I)(x+ I)P 'x' x22x cos 2 n 7r +I) (n even). (2) s= I Also x 2n 200y n cos n0 +y2' = (x n  y n cos n°+ c sin n°)(x n y n cos n° c sin n°) s=n1 =P ( xy cos ° 57 sin ©+ s7r) s= 0 J s=n1[ P o L Also lies between I and hence the product O<6s< I.
We have now If in (I) we put a = 1, b =o, and therefore ° = 7r, we have c n s= 0 n [ s=n1 2"+171i x n +I= P x cos n JI 2S +17rl s= 1(n2) r = rx2 2x cos 2S n 17r +I ] s=0 (n even). (4) (n odd). (5) xn +I=(x+I)P Ex12x cos n 17r +1 ] s=0 FIG. 9.
P P3 f 3 FIG. 10.
E(z) = lim m. {p m (cos m¢ +i sin mcp)}, by De Moivre's theorem. m Since p = (i +) m y we have limm pm =e. lim m ) I +m (.I m 1x /0m) 2 1m Let r be a fixed number less than ,l m+x/ J / m, then lim m  o, I+ between i and lim m = o, I F;; 5 gym, or between i and e v2 /2r2; hence since r can be taken arbitrarily large, the limit is I. The limit of mo or m tan 1 {y/(x+m)} is the same as that of my/(x+rn) which is y. Hence we have shown that E(z) =e x (cos y+i sin y). 21. Since E(x+iy) =i (cos y+sin y, we have cos y+i sin y =E(iy), and cos y  i sin y=E( iy). Therefore cos y= 4{E (iy) +E( FE( sin y=Zi{E(iy)  E( iy)}; and using f the series defined by E(iy) and E( iy), we find that Cos 5 y = I  y2 / 2 ! + y 4 /4!  ..., sin y = y  y 3 /3 !
metrical + y /5 ..., where y is any real number. These m . are the wellknown expansions of cos y, sin y in powers of the circular measure y. Where z is a complex number, the symbol e may be defined to be such that its principal value is E(z); thus the principal values of e 5 are E(iy), E( iy). The above expressions for cos y, sin y may then be written cos y = a (e , sin y = Zi(e v  e These are known as the exponential values of the cosine and sine. It can be shown that the symbol as defined here satisfies the usual laws of combination for exponents.
22. The two functions cos z, sin z may be defined for all complex or real values of z by means of the equations cos y=z{E(z) E( z)}, sin z = (2 i) {E(z)  z)}, where E(z) represents Analytical the sumfunction of i+ z+ z 2 /2! + ..: + z n; n! ... For real values of z this is in accordance with the ordinary definitions, as appears from the series obtained metrical above for cos y, sin y. The fundamental properties of cos z, sin z can be deduced from this definition. Thus cos z } i sin z = E(z), cos z  i sin z = E( iz); therefore cos 2 z+sin 2 z = E (iz). E( iz) =I. Again cos (z 1 +z2) is given by { E (iz i + iz 2) E( iz 1  iz 2) } =1 { E (iz 1) E (iz 2') +' E( iz1) E ( iz 2) } or;{E (iz1)} E( iz1)}{E (iz2 ) E(  iz2)}+4{ E (izl)  E(  izi)} { E (iz2)  E ( iz 2) } , whence we have cos (z 1 +z 2) = cos z 1 cos z2  sin z 1 sin z2. Similarly, we find that sin (z 1 +z 2) =sin z 1 cos z2+ cos z 1 sin z2. Again the equation E(z) =I has no real roots except z =o, for e > 1, if z is real and >o. Also E(z) =1 has no complex root a+iO, for a43 would then also be a root, and E(2a) = E(a+10)E(a  10) = 1, which is impossible unless a= o. The roots of E(z) = I are therefore purely imaginary (except z = o); the smallest numerically we denote by 2 iir, so that E(21ir) = i. We have then E(21irr) = { E(21ir) } r = I, if r is any integer; therefore 21jrr is a root. It can be shown that no root lies between 21irr and 2(r+I)ilr; and thus that all the roots are given by z= ?21irr. Since E(y+217r) =E(z)E(2171) =E(z), we see that E(z) is periodic, of period 21rr. It follows that cos z, sin z are periodic, of periods 21r. The number here introduced may be identified with the ratio of the circumference to the diameter of a circle by considering the case of real values of z.
23. Consider the binomial theorem (a +b)n = a n+ na nlb n (2 i I) an?b2+ .. .
Arc. + n(n  i) ... (n  r±I)2 cos(n2r)O+... r! When n is odd the last term is 2 n(n 2 I 12.(n +3) cos 0, and when n is even it is n(n  I) ... (zn}I) 2n ! If we put a =e', b=  e we obtain the formula ( I) i n (2 sin 0) = 2 cos n02n cos (n2)O +n(I 2 I) 2 cos (n4)0  ...
+( i)n7.12(n  I).. y (n  ri) 2 cos(n2r)0.. .
when n is even, and ( I)2(n1)(2 sin 0)" 2sin nOn . 2 sin(n2)8 n(I 2 1) 2 sin(n4)8...
) n I n(n  ? n  I(n+3) sin 0 z when n is odd. These formulae enable us to express any positive integral power of the sine or cosine in terms of sines or cosines of multiples of the argument. There are corresponding formulae when n is not a positive integer.
Consider the identity log(I  +log(I  qx) = log(1  p+gx+pgx 2). Expand both sides of this equation in powers of x, and equate the coefficients of x we then get p + q n = (p+q)n  n(p fq)n2pq + n(21 3) (p +q) n4 p 2 g 2 +
+( I) _ r_ I)(n  r2) ... (n2r+I) r! If we
write this series in the reverse order, we have n n2 n l
pn+qn  I[(pg)  (pg) (P +n2(n 4 22) (pq)2 2
(p+q) 2 n2(n2 22)(n242)(pq)3 (p 2 q) 6 ... ( 02 " a(p
+g)n] when n is even, and I 2  I n21 ( 2 n(3 
(P+) +n(n2  12)(n23 2) (pq) n 2 5 (p 5 ...
I) n21 2 (p+g)n] 5!
when n is odd. If in these three formulae we put p = e'e, q= e' , we obtain the following series for cos nO 2 cos n0= (2 '') n n(2 °)1±(2 cos 0)n4  ... +( I)rn(n  r  I)(n  rl2)...(n2r±i)(2 cos ...(7) when n is any positive integer; n n2 rz2 (n2  22) 4 n2 (n2  22)(n2 4 2) s ( I)2cos uB = I  2 ! cos 2 B  ?, cos 6 i cos 60 4 ... ( I)22 n1 cos "0 (8) when n is an even positive integer; n1 n (n2  12) (1122) (n 2  3 2) 5 ( I) 2 cos nO =n cos nO  3! cos + 5! cos 9  n1 ... I) 2 2 n1 cos no (9) when n is odd. If in the same three formulae we put p = eie, =   we obtain the following four formulae:  ( i)2 cos nO = (2 sin 0)  n(2 sin O)"2 + n (n ! 3) (2 sin 0)n4 . +( 1)r n(n  r  I) y. l. (n2r 1)(2 sin 6) n2r +... (n even); (io) n1 (  0'2 2 sin nO = the same series (n odd) 22222) 2(n2  22)(n2  4 2) cos =  2? s i n B s inB sin8 4 + (n  3)(n4) 2 (p +q) n5 p2g2  ... .  ( I )r (n  r  1)(n  r2) ... (n  21) (+ q)n211 prgr ... If, as before, we write this in the reverse order, we have the series ( I) 2 1 [n 1  n(n 2 i 22) (P±) 3 (pq)23 3. 2 +n(n225)i n242) () 2 5 + ... + ( I) 2 1. (p + q) n1 I)1..(2n?I) 2n! m(1/m+xm)2 1m lies + n (n  i). .. (n  r } 1) a  '1) +. .. +b.. r! Putting a= b= we obtain (2 cos O) = 2 cos nO+n2 cos n  20 + n(n I) 2 cos n40±... 2 !!
Multiple Arcs in Powers of Sines and Cosines of Arc. (II) 6!
±... +2n1 sin (n even); (12)  sin n9 = n sin B n(n2 3 12) sin 3 0 { n(n2  12)(n2  32) s i n 5 0  .
n1 +( I) 2 2 n1 sin n O (n odd). (13) Next consider the identity ?px I q qx = i  (p + q)x + pgx2' Expand both sides of this equation in powers of x, and equate the coefficients of then we obtain the equation An n = (p +g) n1  (n  2) (p+q) pq p  g n1 n1 n3 ( I) 2 Epq)2 n i 12 (P 4) 2 (pq) 2 2 (n' '?In' 3') p l q l 4 (pq) n 2 5 +... +( I) n 2 1 (p+q)n,1l when n is odd. If we put p = e` e, q = e  ` e , we obtain the formulae sin no=sine) (2 cos o)n1(n2)(2 cos 0)n3 +(n32)(x4)(2 cos o)ns  I)r(nrI)(nr2.. . (n2r) +(r. where n is any positive integer; (I) 2' sinno=sino{ncoson(n 3 122)cos30+n(nz2' nz  4))(n 1 +(I) 2 (2 cos o) 7  1 (n even); (I) 2l sin no =sin j n'2112 c os 'B+ (n212 i n232) cos 4 e.. .
+(I) 2 ' (2 cos 0) n  1 (n odd). (16) If we put in the same three formulae p = ce, q= eo , we obtain the series n 2 (  I) 2 sin ne=coso[sinh10 (n2)sinn3e+ (n 3)(n4) sinnso... 2!
+(I)T (nr 1) (n i 2)... (n2r) sin n ' 2T  1 0+...] (n even); (17) r. n 1 ( I) 2 cos no =the same series (n odd); (r8) n(n' 2) 3 n(n'2') (n 2 4 2) 5 sin no=cos o n sin o i 5 Sin B+ ! sin o+ 3 (1) 2 ' (2 sin 0) n  1 (n even); (19) cos no = cos 01 In22112 sin'0 + (n212) (n232) sin 4 o .. .
+ (2 sin 0) n  i. (n odd). (20) We have thus obtained formulae for cos nO and sin nO both in ascending and in descending powers of cos 0 and sin O. Vieta obtained formulae for chords of multiple arcs in powers of chords of the simple or complementary arcs equivalent to the formulae (13) and (19) above. These are contained in his work Theoremata ad angulares sectiones. Jacques Bernoulli found formulae equivalent to (12) and (13) (Mem. de l'Academie des Sciences, 1702), and transformed these series into a form equivalent to (io) and (I I). Jean Bernoulli published in the Acta eruditorum for 1701, among other formulae already found by Vieta, one equivalent to (17). These formulae have been extended to cases in which n is fractional, negative or irrational; see a paper by D. F. Gregory in Camb. Math. Journ. vol. iv., in which the series for cos nO, sin nO in ascending powers of cos 0 and sin 0 are extended to the case of a fractional value of n. These series have been considered by Euler in a memoir in the Nova acta, vol. ix., by Lagrange in his Calcul des fonctions (1806), and by Poinsot in Recherches sur l'analyse des sections angulaires (1825).
24. The general definition of Napierian logarithms is that, if +v = a+ eb, then x+ ty = log (a+tb). Now we know that exE L Y= excos y+eex sin y; hence ex cos y =a, ex sin y Logarithms. is b, or ex= (a'+b 2) a, y = arc tan b/a m7r, where m s an integer. If b =o, then m must be even or odd according as a is positiveor negative; hence log e (a+tb) =loge (a'14')2+ c (arc tan b/a 2n7r) or loge (a+ib) =loge (a2+b2)2+ t (arc tan 2n Fr), according as a is positive or negative. Thus the logarithm of any complex or real quantity is a multiplevalued function, the differ Hyrbolic ence between successive values being 27ri; in particular, pe Hyperbo the most general form of the logarithm of a real positive metry. quantity is obtained by adding positive or nega tive multiples of to the arithmetical logarithm. On this subject, see De Morgan's Trigonometry and Double Algebra, ch. iv., and a paper by Professor Cayley in vol. ii. of Proc. London Math. Soc. 25. We have from the definitions given in § 21, cos cy = 2(0+e and sin zy=21(e y ey). The expressions, 2(eY+eY), 1(0e Y) are said to define the hyperbolic cosine and sine of y and are written cosh y, sinh y; thus cosh y = cos ty, sinh y=  t sin ty. The functions cosh y, sinh y are connected with the rectangular hyperbola in a manner analogous to that in which the cosine and sine are connected with the circle. We may easily show from the definitions that cos 2 (x{cy) Fsin2(x+cy) cosh' y  y cos(x + ay) sin(x{cy) = cosh (a +13) = Expansion 6=sin 0+ 1 sin' 9 + I_3 sins 9 + I.3.5 sin? 9 +; (21) 3 2.4 5 2.4.6 7 0 must lie between the values t z 7r. This equation of may also be written in the form I x 3 1.3 x 5.3.5 57 arc sin x= F  { +... 2 3 2.4 5 2.4. 6 7 when x lies between =1.
By equating the coefficients of n' on both sides of equation (12) we get 0 2 = sin' 0+2 sin' 0 + 2_4 sin s 0 + 2.4.6 sin g o+ 3 2 3.5 3 3.5. 7 4 which may also be written in the form 2_ 2 2x_4 2.4X6+2.4.6 x8 (arc sin x) = x + 3 2 + 3533.5. 7 4 + .
when x is between =i. Differentiating this equation with regard to x, we get arc sin x 2 2.2. 4.6  x2 =x + 3 x 3 } 31 5x 5 + 3 S. 7 x 7
It can be shown that if mod x < 1, then for any such real or complex value of x, a value of loge (1 +x) is given by the sum of the series x' x' /2 +x 3 /3  .. .
We then have 2 log x5 x 7 Gregory's Series. put ty for x, the left side then becomes z f log (I Hy) log (I  cy) } or i arc tan y on7r; Y3 y5 y7 hence arc tan y =y3 +57+...
The series is convergent if y lies between =I; if we suppose arc tan y restricted to values between = 47r, we have arc tan y=y3 + 5  ..., 3 5 (24) which is Gregory's series.
Various series derived from (24) have been employed to calculate the value of 7r. At the end of the 17th century 7r was calculated to 72 places of decimals by Abraham Sharp, by means of the series obtained by putting arc tan y=7r/6, 'Series for ' y=I/sl3 in (24). The calculation is to be found in Calculation Sherwin's Mathematical Tables (1742). About the same of' time J. Machin employed the series obtained from the equation 4 arc tan arc tan 233 =1. . 7r to calculate 7 to 100 decimal places. Long afterwards Euler employed the series obtained from 47r =arc tan 2 + arc tan 1, which, however, gives less rapidly converging series (Introd., Anal. infin. vol. i.). T. F. de Lagny employed the formula arc tan I/ i /3 =7/6 to calculate 7 to 127 places; the result was communicated to the Paris Academy in 1719. G. Vega calculated 7 to 240 decimal places by means of the series obtained from the equation 47r =5 arc tan 4 +2 arc tan i o. The formula 47r =arc tan 11arc tanidarc tan e was used by J. M. Z. Dase to calculate 7r to 200 decimal places. W. Rutherford used the equation 7r =4 arc tan  arc tan ,', + arc tan If in (23) we put y =1 and 4, we have = 8 arc tan s + 4 arc tan =2.4 1E 2
I + 2=4123 Io 3.5 Io + 561+3'IOO?3.51OO)`+..., a rapidly convergent series for 7r which was first given by Hutton in Phil. Trans. for 1776, and afterwards by Euler in Nova acta for 2793. Euler gives an equation deduced in the same manner from the identity 20 arc tan 4+8 arc tan A. The calculation of 7r has been carried out to 707 places of decimals; see Proc. Roy. Soc. vols. xxi. and xxii.; also Circle.
= I, =I; =cos x cosh yi sin x sinh y, sin x cosh y+c cos x sinh y, cosh a cosh, +sinh a sinh 0, sinh(a+a) =sinh a cosh a+cosh a sinh 0.
These formulae are the basis of a complete hyperbolic trigonometry. The connexion of these functions with the hyperbola was first pointed out by Lambert.
26. If we equate the coefficients of n on both sides of equation (13), this process requiring, however, a justification of its validity, we get (2 cos 0)n.2'1 +.. .
(14) (I 5) (22) 27. We shall now obtain expressions for sin x and cos x as infinite products of rational factors. We have sin x =2 sin  s i n x 2 = 2 3 s i n  s i n x 4 4 sin x +2 sin x+37 4 4 proceeding continually in this way with each factor, we obtain x. x + n . x+27r n17r sin x = 2" i sin s i n sin n ... sin n where n is any positive integral power of 2. Now the formula for sin x as an infinite product put x=27r, we then get i  'rI 3355; if we stop after 2n factors in the 2'2.2.4.4.6...
numerator and denominator, we obtain the approximate equation 7r / .3. (2n i)2 I =2 2 2.4 2.6 2 ... (2n) 2 (2n+I) or i. 3 5 Zn n ?n7r, where n is a large integer. This ex pression was obtained in a quite different manner by Wallis (Arithmetica infinitorum, vol. i. of Opp.). 28. We have n ' and sin (x+y) (x+ y )P (1 +) sin x +nrrr +r7r. r x rs x si n n sin sin s i n =sing s i n2 n, x + Z nir x sin n =cos;.
xP Hence the above may be written sin x=2 4  1 sink (sine n  sin e k) (sine n  s ine k) kir sine n sine n) cosh, where k= 2n =I. Let x be indefinitely small, then we have 2 41 7r 27r kw I =  n sin 2 n sine sine hence sin x = n sinco s  (I 2 ( I  2 n n sin e 7r/n in 2 2 /n ') sin e Sin e ks/n) We may write this sin sin 2 cos n (I sin e 7r/n) '
(I sin e m r/n) R ' where denotes the product (I sin2 r m+I /n) (i I sin2m+27r/n)
(I  sin 22 k /) /n ' and m is any fixed integer
independent of n. It is necessary, when we make n infinite, to
determine the limiting value of the quantity R; then,
since the limit of sin x is sin x, and that of n sin
sin cos x sin msr/n ms sin x (I 7 ,2 
2 2,2) ... lim R.
The modulus of RI is less than (I+ sin e m+17r/n) (I+ sin e m+27r/n)
( where p =mod. sin x/n. Now e Ap2 > I +A p 2 ,
if A is positive; hence mod. (R  i) is less than exp.
{ p 2 (cosec 2 m + 17r/n + ... + cosec 2 ks/n)I, or than exp.
4p2n2{i/(m+I)2+... +I/k 2 }I, or than exp. { p 2 n 2 /4m 2 } 1.
Now p 2 = sin e a/n.cosh 2 (3/n +cos 2 a/n. sinh 2
(3/n, if x = a+a/3; or p 2 =sin 2 a/n+sinh 2
,6/n. Hence limn=? p2n2=a2+0, lim n 00 pn= mod. x. It
follows that mod. n (R  I) is between o and exp. { (mod. 4) 2
2 I, and the latter may be made arbitrarily small
by taking m large enough. It has now been shown that sin =x(i  2
/7r 2)(I  x 2 2 2).. (Ix 2 /m 2 7r 2) (I+E m),
where mod. decreases indefinitely as m is increased indefinitely.
When m is indefinitely increased this becomes sin (I  2)
(I2 7f2) ... =xP I (i n2) (25) This has been shown to hold for
any real or complex value of x. The expression for cos x in factors
may be found in a similar manner by means of the equation cos be
deduced thus cos X2 sin x sin 2X P (_ 2 ') 4x2
4x2 P (I  n2r2) .71 (i_4x22) (i  3 2 2)
(15, x2 =P 0 (I (2n+I)27r2)' n=o. 4x2 (26) If we change x
into ex, we have the formulae for sinh x, cosh x as infinite
products  sinh x = xP (+ 2 2 2), cosh x =P ('+ (2fl)252) =0 n=0 or
cos y+sin y cot x +7,_ (I+ x y s) (I +
) (' '+ X2s). .. Equating
the coefficients of the first power of y on both
sides we obtain the series Cot + x +7r + x
1 7r + x + 27r + x I 27r+... (27) From this we may
deduce a corresponding series for cosec x, for, since cosec x=cot
2xcot x, we obtain cosec  + 7r 
x I lr + x + 27r + x I 27r 
5 4 35 x 137r+ (28) By resolving cos (x +y) into
factors we should obtain in a similar y g cos x manner the series
2222 tan x = ? + 37r+2x + 57r ?
2x 57r+2x +" (?9) and thence sec x= tan (+ 2) tan x= 2x +
7r+ 2x 37r2x 37r+2x + .... (30) These four formulae may
also be derived from the product formulae for sin x and cos x by
taking logarithms and then differentiating. Glaisher has proved
them by resolving the expressions for cos x/sin x and
i/sin x ... as products into partial fractions (see Quart.
Journ. Math., vol. xvii.). The series for cot x may also be
obtained by a continued use of the equation cot x = 2 {cot 2x+ cot
2 (x+7r) } (see a paper by Dr Schroter in Schlomilch's
Zeitschrift, vol. xiii.).
Various series for 7r may be derived from the series (27), (28), (29), (30), and from the series obtained by differentiating them one or more times. For example, in the formulae (27) and (28), by putting x = 7r/n we get 2r= n tan n I n I i + n+i 2n I I + 2n +I ' I I I I [7r =n sin n + I nI  n+I 2ni+2n+I"' 7r If we put n=3, these become I I I I I 7r = 3113 (I2+45+2g+..., 7r = 323 (I+24 ' 7+g...) By differentiating (27) we get J cosec2 x= x 2+ (x+70 2+ (x ir) 2+ (x+27r) 2+ (x 127r)2+
These series, among others, were given by Glaisher (Quart. Journ. Math. vol. xii.).
29. We have sinh 7rx = 7rxP I +n2), cosh 7rx =P (i + (2n xe  1) 2); if we differentiate these formulae after taking loga rithms we obtain the series 7r 2222 2x coth 7rx  2x2=12+x2+22+x2+32+x2+
, 7r I 2x tanh 7rx = 12 +x 2 + 32+x2 + 52 + x2 +
.. .
These series were given by Kummer (in Crelle's Journ. vol. xvii.) I I+ I The sum of the more general series I 2n,..r x 2 " + 2 2n+ x 2n 32n.+x2".
x=2 sin 
7r2x 37r2x 4 cos 4, or may 
+ ..., has been found by Glaisher (Proc. Lond. Math. Soc., vol. vii.) If U m denotes the sum of the series. +2„?+Zm+ ..., V"' that is unity, we have 7, I I I of the series F„{3„LdSm+..., and W m that of the series I,,,  3,„  m+..., we obtain by taking loga T I I rithms in the formulae (25) and (26) log (x cosec x) = U2 (r) 2+2 U4 () 4 +3 6 () 6 + . . , log (sec x) = V 2 (L 7r) 2 +2V4 (2 (31 7„) 4) +3 V 6 (317,) 6 + ...; and differentiating these series we get I U2 U4 Us Cot x =2x  7r 2x  714 x37r6 x5  ..., V6 I tan x= 222x+ 1% 424x3+ I 26x5+.... (32) 2 7r 7r 716 In (31) x must lie between =7r and in (32) between 17r. Write equation (30) in the form sec I)n (2n +I)7r (2n+1 and expand each term of this series in powers of x 2, then we get 2 2 W1 + 24W3x2 + 26 W,x4 +... () sec x=7/ ?a 5 33 where x must lie between =17r. By comparing the series (31), (32), (33) with the expansions of cot x, tan x, sec x obtained otherwise, we can calculate the values of U2, U4... V2, V4... and WI, W3.
When U. has been found, V n may be obtained from the formula 2' T in =(2n  I)Un.
For Lord Brounker's series of 7r, see Circle. It can be got at once by putting a =I, b =3, 5 .... in Euler's 'I I I I' a 2 b2 for 7r. th e orem=a  b+c  ... =a+b  a+c  b+... Sylvester gave (Phil. Mag., 1869) the continued fraction 711 1.2 2.3 3_4 2 = I +I+ I+ I+ 1+...; which is equivalent to Wallis's formula for 7r. This fraction was originally given by Euler (Comm. Acad. Petropol. vol. xi.); it is also given by Stern (in Crelle's Journ. vol. x.).
30. It may be shown by means of a transformation of the series sin x x x 2 .x 2 x.3 for cos and x that tan x 3  5  7  This may be also easily shown as follows. Let Y =cos if x, and let y', y "... denote the differential coefficients of y with regard to x, then by forming these we can show that 4xy"+2y'+y=o, and thence by Leibnitz's theorem we have 4 x y (n+2) +(4nf2)y (n+1) =o.
x n 4 Therefore y, =  2  y, ? y,,, y y n+1) =  2(2n + I)  (n+1)x(n+2) i y /y hence  21co t 4x 2  6   to 4X Replacing x by x we have tan x = x x2 x2 1  3 5 Euler gave the continued fraction n tan x (n 2  I) tan 2 x (n 2  4) tan 2 x (n 2  9) tan2x tan nx = I  3  5  7  ..., this was published in Mem. de l'acad. de St Pe'tersb. vol. vi. Glaisher has remarked (Mess. of Math. vols. iv.) that this may be derived by forming the differential equation (I  2)y (m+2)  (2m + I)xy(m+1) + (n 2  m2) y(m) = o, where y=cos (n arc cos x), then replacing x by cos x, and proceeding as in the former case. If we put n=o, this becomes tan x tan 2 x 4 tan 2 x 9 tan2x 1 + 3.+ 5+ 7+ "' whence we have arc tan x = x x2 4x2 9X I + 3+ 5+ 7+" + 2n+I +'
31. It is possible to make the investigation of the properties of the simple circular functions rest on a purely analytical basis other than y the one indicated in § 22. The sine of x would be defined as a function such that, if x= 1 dy, J 011 (1  y2)9 of Circular then y = sin x; the quantity 7would be defined to ,2 i dy be the complete integral 3 ,2) We should then have Now change the variable in the integral to z, where y 2 +z 2 = I, we then have 2  x =fz (dy 2), and z must be defined as the cosine of x, and is thus equal to, sin (17r  x), satisfying the equation sin 2 x+cos 2 x=I.
Next consider the f di l ferentialequation V (I y y 2) + 1 1 (12 Z2) This is equivalent to d{y,/(I  z2)+zJ(I  y2)} =o; hence the integral is yJ (I  z 2) (I  y 2) = a constant.
The constant will be equal to the value u of y when z=0; whence yll (I  z 2) +z (I  y 2) = u. The integral may also be obtained in the form (I C d _ 1 ( z I r u du (I y y 2)' l3  (I 2 y  1V (I  u2)' we have a+a =y, and sin y=sin a cos 1 13+cos a sin 13, cos y =cos a cos l3  sin a sin 43, the addition theorems. By means of the addition theorems and the values sin 17r=l, cos 17r=o we can prove that sin (17r+x)= cos x, cos (27r+x) =  sin x; and thence, by another use of the addition theorems, that sin (71+x) =  sin x cos (7r+x) =  cos x, from which the periodicity of the functions ons sin x, cos x follows d y  c loge{ Y (1  y2)+cy}; whence log e { ' (I  y 2) + c y} +l og e { (I  z 2) + cz} = a constant. Therefore { A l (I  y 2)} + cy{ 1 (I  z 2)+cz} _ I (I  u 2) + cu, since u =y when z = o; whence we have the equation (cos a + c sin a) (cos (3 + c sin 0) = cos (a + 1 3) + c sin (a +13), from which De Moivre's theorem follows.
Further information will be found in Hobson's Plane Trigonometry, and in Chrystal's Algebra. For further information on the history of the subject, see Braunmühl's Vorlesungen über Geschichte der Trigonometrie (Leipzig, 1900). (E. W. H.)
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These pages were moved here from the Algebra book because of restructuring. It is asked that the authors of the trigonometry book either (a) integrate this material into this book, or (b) delete this material.
Trigonometry (from the Greek trigonon = three angles and metro = measure) is a part of elementary mathematics dealing with angles, triangles and trigonometric functions such as sine (abbreviated sin), cosine (abbreviated cos) and tangent (abbreviated tan). It has some connection to geometry, although there is disagreement on exactly what that connection is; for some, trigonometry is just a section of geometry.
[[File:rightthumbnailA standard right triangle. C is the right angle in this picture.]] Trigonometry uses a large number of specific words to describe parts of a triangle. Some of the definitions in trigonometry are:
There are three main trigonometric ratios for right triangles, and three reciprocals of those ratios. There are 6 total ratios. They are:
Sine (sin)  The sine of an angle is equal to the $\{Opposite\; \backslash over\; Hypotenuse\}$
Cosine (cos)  The cosine of an angle is equal to the $\{Adjacent\; \backslash over\; Hypotenuse\}$
Tangent (tan)  The tangent of an angle is equal to the $\{Opposite\; \backslash over\; Adjacent\}$
The reciprocals of these ratios are:
Cosecant (csc)  The cosecant of an angle is equal to the $\{Hypotenuse\; \backslash over\; Opposite\}$ or $\backslash csc\; \backslash theta\; =\; \{1\; \backslash over\; \backslash sin\; \backslash theta\}$
Secant (sec)  The secant of an angle is equal to the $\{Hypotenuse\; \backslash over\; Adjacent\}$ or $\backslash sec\; \backslash theta\; =\; \{1\; \backslash over\; \backslash cos\; \backslash theta\}$
Cotangent (cot)  The cotangent of an angle is equal to the $\{Adjacent\; \backslash over\; Opposite\}$ or $\backslash cot\; \backslash theta\; =\; \{1\; \backslash over\; \backslash tan\; \backslash theta\}$
Students often use a mnemonic to remember this relationship. The sine, cosine, and tangent ratios in a right triangle can be remembered by representing them as strings of letters, such as SOHCAHTOA:
or:
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or:
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