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1 The Birth of Science - MSRI

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10.10 Ptolemy and <strong>The</strong>on <strong>of</strong> Smyrna<br />

10.10 Ptolemy and <strong>The</strong>on <strong>of</strong> Smyrna 273<br />

<strong>The</strong> preceding sections have argued that Hipparchus, and perhaps other<br />

astronomers in the second century B.C., reached a sort <strong>of</strong> “dynamical heliocentrism”<br />

based on the principle <strong>of</strong> inertia and the equilibrium between<br />

centrifugal force and the gravitational pull <strong>of</strong> the sun.<br />

<strong>The</strong> greatest obstacle to accepting this picture is that these ideas are<br />

nowhere to be found in the Almagest. But the Almagest itself <strong>of</strong>fers indirect<br />

evidence for the proposed reconstruction, in the form <strong>of</strong> remnants<br />

<strong>of</strong> scientific ideas not understood by Ptolemy and the absence <strong>of</strong> other<br />

ideas whose existence in Hellenistic science is well documented. Dennis page 340<br />

Rawlins makes a strong case that several technical elements <strong>of</strong> Ptolemaic<br />

astronomy can only be explained as derivatives <strong>of</strong> an earlier heliocentric<br />

model. 152<br />

Among the consequences <strong>of</strong> the cultural gap separating Ptolemy from<br />

Hellenistic astronomy was the loss <strong>of</strong> the idea <strong>of</strong> relative motion. Indeed,<br />

the idea that one can choose the reference system, present for example in<br />

Euclid, Herophilus and one <strong>of</strong> Seneca’s sources, 153 was completely foreign<br />

to Ptolemy. Nevertheless he reported recognizably relativistic opinions, 154<br />

which he himself understood simply as a convenience for describing observed<br />

motions, with no consequences to his concept <strong>of</strong> space and motion,<br />

which is squarely Aristotelian. In just the same way physicians like Rufus<br />

Ephesius, though diligently transmitting Herophilus’ neologisms, could<br />

no longer grasp their nature.<br />

Ptolemy not only did not use gravity (or any other dynamical idea) in<br />

astronomy; he also approached the earth’s sphericity in a purely geometric<br />

and descriptive way, seemingly unaware <strong>of</strong> the explanation for it that was<br />

well known in Hellenistic times. 155<br />

<strong>The</strong> Almagest mentions (and contests, <strong>of</strong> course) the opinion that the<br />

“fixed” stars have a uniform linear motion. 157 To Ptolemy the motion in page 341<br />

question was the apparent movement in the sky, but we may conjecture<br />

that his source was not making such a bizarre claim; it was instead referring<br />

to the “real” motion whose existence Hipparchus suspected on the<br />

basis <strong>of</strong> general principles and for whose detection he sought to enlist the<br />

help <strong>of</strong> posterity.<br />

152<br />

[Rawlins: AHPE].<br />

153<br />

See pages 153, 163 and 256.<br />

154<br />

See page 75.<br />

155<br />

Ptolemy, Syntaxis mathematica, I, iv, 14–16 (ed. Heiberg); for the explanation <strong>of</strong> sphericity see<br />

Section 10.8.<br />

157<br />

Ptolemy, Syntaxis mathematica, I, iii, 11 (ed. Heiberg).<br />

Revision: 1.11 Date: 2003/01/06 02:20:46

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