| Analysis index | History Topics Index |
The use of trigonometric functions arises from the early connection
between mathematics and astronomy. Early work with spherical triangles
was as important as plane triangles.
The first work on trigonometric functions related to
chords of a circle. Given a circle of fixed radius, 60 units were often
used in early calculations, then the problem was to find the length of
the chord subtended by a given angle. For a circle of unit radius the
length of the chord subtended by the angle x was 2sin (x/2). The first known table of chords was produced by the Greek mathematician Hipparchus in about 140 BC. Although these tables have not survived, it is claimed that twelve books of tables of chords were written by Hipparchus. This makes Hipparchus the founder of trigonometry.
The next Greek mathematician to produce a table of chords was Menelaus in about 100 AD. Menelaus
worked in Rome producing six books of tables of chords which have been
lost but his work on spherics has survived and is the earliest known
work on spherical trigonometry. Menelaus proved a property of plane
triangles and the corresponding spherical triangle property known the regula sex quantitatum.
Ptolemy was the next author of a book of chords, showing the same Babylonian influence as Hipparchus,
dividing the circle into 360° and the diameter into 120 parts. The
suggestion here is that he was following earlier practice when the
approximation 3 for π was used. Ptolemy, together with the earlier writers, used a form of the relation sin2 x + cos2 x = 1, although of course they did not actually use sines and cosines but chords.
Similarly, in terms of chords rather than sin and cos, Ptolemy knew the formulas
sin(x + y) = sinx cos y + cosx sin ya/sin A = b/sin B = c/sin C.
Ptolemy
calculated chords by first inscribing regular polygons of 3, 4, 5, 6
and 10 sides in a circle. This allowed him to calculate the chord
subtended by angles of 36°, 72°, 60°, 90° and 120°. He then found a
method of finding the cord subtended by half the arc of a known chord
and this, together with interpolation allowed him to calculate chords
with a good degree of accuracy. Using these methods Ptolemy
found that sin 30' (30' = half of 1°) which is the chord of 1° was, as a
number to base 60, 0 31' 25". Converted to decimals this is 0.0087268
which is correct to 6 decimal places, the answer to 7 decimal places
being 0.0087265.
The first actual appearance of the sine of an angle appears in the work of the Hindus. Aryabhata,
in about 500, gave tables of half chords which now really are sine
tables and used jya for our sin. This same table was reproduced in the
work of Brahmagupta (in 628) and detailed method for constructing a table of sines for any angle were give by Bhaskara in 1150.
The Arabs worked with sines and cosines and by 980 Abu'l-Wafa knew that
sin 2x = 2 sin x cos x
although it could have easily have been deduced from Ptolemy's formula sin(x + y) = sin x cos y + cos x sin y with x = y.
The Hindu word jya for the sine was adopted by the Arabs who called the sine jiba, a meaningless word with the same sound as jya. Now jiba became jaib
in later Arab writings and this word does have a meaning, namely a
'fold'. When European authors translated the Arabic mathematical works
into Latin they translated jaib into the word sinus meaning fold in
Latin. In particular Fibonacci's use of the term sinus rectus arcus soon encouraged the universal use of sine.
Chapters of Copernicus's book giving all the trigonometry relevant to astronomy was published in 1542 by Rheticus. Rheticus also produced substantial tables of sines and cosines which were published after his death. In 1533 Regiomontanus's work De triangulis omnimodis
was published. This contained work on planar and spherical trigonometry
originally done much earlier in about 1464. The book is particularly
strong on the sine and its inverse.
The term sine certainly was not accepted straight away
as the standard notation by all authors. In times when mathematical
notation was in itself a new idea many used their own notation. Edmund Gunter
was the first to use the abbreviation sin in 1624 in a drawing. The
first use of sin in a book was in 1634 by the French mathematician Hérigone while Cavalieri used Si and Oughtred S.
It is perhaps surprising that the second most important trigonometrical
function during the period we have discussed was the versed sine, a
function now hardly used at all. The versine is related to the sine by
the formula
versin x = 1 - cos x.
It is just the sine turned (versed) through 90°.
The cosine follows a similar course of development in notation as the sine. Viète used the term sinus residuae for the cosine, Gunter (1620) suggested co-sinus. The notation Si.2 was used by Cavalieri, s co arc by Oughtred and S by Wallis.
Viète knew formulas for sin nx in terms of sin x and cos x. He gave explicitly the formulas (due to Pitiscus)
sin 3x = 3 cos 2x sin x - sin 3 xcos 3x = cos 3x - 3 sin 2x cos x.
The tangent and cotangent came via a different route
from the chord approach of the sine. These developed together and were
not at first associated with angles. They became important for
calculating heights from the length of the shadow that the object cast.
The length of shadows was also of importance in the sundial. Thales used the lengths of shadows to calculate the heights of pyramids.
The first known tables of shadows were produced by the Arabs around 860 and used two measures translated into Latin as umbra recta and umbra versa. Viète used the terms amsinus and prosinus. The name tangent was first used by Thomas Fincke in 1583. The term cotangens was first used by Edmund Gunter in 1620.
Abbreviations for the tan and cot followed a similar development to those of the sin and cos. Cavalieri used Ta and Ta.2, Oughtred used t arc and t co arc while Wallis used T and t. The common abbreviation used today is tan by we write tan whereas the first occurrence of this abbreviation was used by Albert Girard in 1626, but tan was written over the angle
tan
A
cot was first used by Jonas Moore in 1674.
The secant and cosecant were not used by the early astronomers or
surveyors. These came into their own when navigators around the 15th Century started to prepare tables. Copernicus knew of the secant which he called the hypotenusa. Viète knew the results
cosec x/sec x = cot x = 1/tan x1/cosec x = cos x/cot x = sin x.
The abbreviations used by various authors were similar to the trigonometric functions already discussed. Cavalieri used Se and Se.2, Oughtred used se arc and sec co arc while Wallis used s and σ. Albert Girard used sec, written above the angle as he did for the tan.
The term 'trigonometry' first appears as the title of a book Trigonometria by B Pitiscus, published in 1595. Pitiscus also discovered the formulas for sin 2x, sin 3x, cos 2x, cos 3x.
The 18th Century saw trigonometric functions of a complex variable being studied. Johann Bernoulli found the relation between sin-1z and log z in 1702 while Cotes, in a work published in 1722 after his death, showed that
ix = log(cos x + i sin x ).
De Moivre published his famous theorem
(cos x + i sin x )n = cos nx + i sin nx
exp(ix) = cos x + i sin x .
The hyperbolic trigonometric functions were introduced by Lambert.
No comments:
Post a Comment