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A history of Greek mathematics - Wilbourhall.org

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106 ERATOSTHENES<br />

geometric mean between CP, CP' ', the loci <strong>of</strong> A, G respectively<br />

are conies. Zeuthen therefore suggests that these loci and<br />

the corresponding loci <strong>of</strong> the points on CPP' at a distance<br />

from C equal to the subcontraries <strong>of</strong> the geometric and<br />

harmonic means between CP and CP' are the 'loci with<br />

reference to means ' <strong>of</strong> Eratosthenes ; the latter two loci are<br />

'linear', i.e. higher curves than conies. Needless to say, we<br />

have no confirmation <strong>of</strong> this conjecture.<br />

Eratosthenes s measurement <strong>of</strong> the Earth.<br />

But the most famous scientific achievement <strong>of</strong> Eratosthenes<br />

was his measurement <strong>of</strong> the earth. Archimedes mentions, as<br />

we have seen, that some had tried to prove that the circumference<br />

<strong>of</strong> the earth is about 300,000 stades. This was<br />

evidently the measurement based on observations made at<br />

Lysimachia (on the Hellespont) and Syene. It was observed<br />

that, while both these places were on one meridian, the head<br />

<strong>of</strong> Draco was in the zenith at Lysimachia, and Cancer in the<br />

zenith at Syene ; the arc <strong>of</strong> the meridian separating the two<br />

in the heavens was taken to be 1/I5th <strong>of</strong> the complete circle.<br />

.<br />

^ The distance between the two towns<br />

was estimated at 20,000 stades, and<br />

accordingly the whole circumference <strong>of</strong><br />

the earth was reckoned at 300,000<br />

Eratosthenes improved on this.<br />

stades.<br />

He observed (1) that at Syene, at<br />

noon, at the summer solstice, the<br />

sun cast no shadow from an upright<br />

gnomon (this was confirmed by the<br />

observation that a well dug at the<br />

same place was entirely lighted up at<br />

the same time), while (2) at the same moment the gnomon fixed<br />

upright at Alexandria (taken to be on the same meridian with<br />

Syene) cast a shadow corresponding to an angle between the<br />

gnomon and the sun's rays <strong>of</strong> l/50th <strong>of</strong> a complete circle or<br />

four right angles. The sun's rays are <strong>of</strong> course assumed to be<br />

parallel at the two places represented by S and A in the<br />

annexed figure.<br />

If oc be the angle made at A by the sun's rays<br />

with the gnomon (DA produced), the angle SOA is also equal to

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