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A history of Greek mathematics - Wilbourhall.org

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;<br />

236 SOME HANDBOOKS<br />

the first century B. 0. As he seems to know nothing <strong>of</strong> the<br />

works <strong>of</strong> Ptolemy, he can hardly, in any case, have lived<br />

later than the beginning <strong>of</strong> the second century A. D.<br />

Book I begins with a chapter the object <strong>of</strong> which is to<br />

prove that the universe, which has the shape <strong>of</strong> a sphere,<br />

is limited and surrounded by void extending without limit in<br />

all directions, and to refute objections to this view. Then<br />

follow chapters on the five parallel circles in the heaven and<br />

the zones, habitable and uninhabitable (chap. 2)<br />

; on the<br />

motion <strong>of</strong> the fixed stars and the independent (irpoaiptTLKai)<br />

movements <strong>of</strong> the planets including the sun and moon<br />

(chap. 3); on the zodiac and the effect <strong>of</strong> the sun's motion in<br />

it (chap. 4)<br />

; on the inclination <strong>of</strong> the axis <strong>of</strong> the universe and<br />

its effects on the lengths <strong>of</strong> days and nights at different places<br />

(chap. 5); on the inequality in the rate <strong>of</strong> increase in the<br />

lengths <strong>of</strong> the days and nights according to the time <strong>of</strong> year,<br />

the different lengths <strong>of</strong> the seasons due to the motion <strong>of</strong> the<br />

sun in an eccentric circle, the difference between a day-andnight<br />

and an exact revolution <strong>of</strong> the universe owing to the<br />

separate motion <strong>of</strong> the sun (chap. 6)<br />

; on the habitable regions<br />

<strong>of</strong> the globe including Britain and the island <strong>of</strong> Thule ' ', said<br />

to have been visited by Pytheas, where, when the sun is in<br />

Cancer and visible, the day is a month long ; and so on (chap. 7).<br />

Chap. 8 purports to prove that the universe is a sphere by<br />

proving first that the earth is a sphere, and then that the air<br />

about it, and the ether about that, must necessarily make up<br />

larger spheres. The earth is proved to be a sphere by the<br />

method <strong>of</strong> exclusion ; it is assumed that the only possibilities<br />

are that it is (a) flat and plane, or (b) hollow and deep, or<br />

(c) square, or (d) pyramidal, or (e) spherical, and, the first four<br />

hypotheses being successively disposed <strong>of</strong>, only the fifth<br />

remains. Chap. 9 maintains that the earth is in the centre <strong>of</strong><br />

the universe ;<br />

chap. 10, on the size <strong>of</strong> the earth, contains the<br />

interesting reproduction <strong>of</strong> the details <strong>of</strong> the measurements <strong>of</strong><br />

the earth by Posidonius and Eratosthenes respectively which<br />

have been given above in their proper places (p. 220, pp. 1 06-7)<br />

chap. 1 1<br />

argues that the earth is in the relation <strong>of</strong> a point to,<br />

i. e. is negligible in size in comparison with, the universe or<br />

even the sun's circle, but not the moon's circle (cf. p. 3 above).<br />

Book II, chap. 1, is evidently the 'piece de resistance, con-

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