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A history of Greek mathematics - Wilbourhall.org

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:<br />

:<br />

276 TRIGONOMETRY<br />

bo given here. Book I : Indispensable preliminaries to the<br />

study <strong>of</strong> the Ptolemaic system, general explanations <strong>of</strong><br />

the different motions <strong>of</strong> the heavenly bodies in relation to<br />

the earth as centre, propositions required for<br />

the preparation<br />

<strong>of</strong> Tables <strong>of</strong> Chords, the Table itself, some propositions in<br />

spherical geometry leading to trigonometrical calculations <strong>of</strong><br />

the relations <strong>of</strong> arcs <strong>of</strong> the equator, ecliptic, horizon and<br />

meridian, a ' Table <strong>of</strong> Obliquity ', for calculating declinations<br />

for each degree-point on the ecliptic, and finally a method <strong>of</strong><br />

finding the right ascensions for arcs <strong>of</strong> the ecliptic equal to<br />

one-third <strong>of</strong> a sign or 10°. Book II: The same subject continued,<br />

i.e. problems on the sphere, with special reference to<br />

the differences between various latitudes, the length <strong>of</strong> the<br />

longest day at any degree <strong>of</strong> latitude, and the like. Book III<br />

On the length <strong>of</strong> the year and the motion <strong>of</strong> the sun on the<br />

eccentric and epicycle hypotheses. Book IV : The length <strong>of</strong> the<br />

months and the theory <strong>of</strong> the moon. Book V : The construction<br />

<strong>of</strong> the<br />

astrolabe, and the theory <strong>of</strong> the moon continued,<br />

the diameters <strong>of</strong> the sun, the moon and the earth's shadow,<br />

the distance <strong>of</strong> the sun and the dimensions <strong>of</strong> the sun, moon<br />

and earth. Book VI : Conjunctions and oppositions <strong>of</strong> sun<br />

and moon, solar and lunar eclipses and their periods. Books<br />

VII and VIII are about the fixed stars and the precession <strong>of</strong><br />

the equinoxes, and Books IX-XIII are devoted to the movements<br />

<strong>of</strong> the planets.<br />

Trigonometry in<br />

Ptolemy.<br />

What interests the historian <strong>of</strong> <strong>mathematics</strong> is the trigonometry<br />

in Ptolemy. It is evident that no part <strong>of</strong> the trigonometry,<br />

or <strong>of</strong> the matter preliminary to it, in Ptolemy was new.<br />

What he did was to abstract from earlier treatises, and to<br />

condense into the smallest possible space, the minimum <strong>of</strong><br />

propositions necessary to establish the methods and formulae<br />

used. Thus at the beginning <strong>of</strong> the preliminaries to the<br />

Table <strong>of</strong> Chords in Book I he says<br />

1<br />

We will first show how we can establish a systematic and<br />

speedy method <strong>of</strong> obtaining the lengths <strong>of</strong> the chords based on<br />

the uniform use <strong>of</strong> the smallest possible number <strong>of</strong> propositions,<br />

so that we may not only have the lengths <strong>of</strong> the chords

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