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1 The Birth of Science - MSRI

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326 11. <strong>The</strong> Age-Long Recovery<br />

“toys” in reconstructing Alexandrian technology). But when the source<br />

is a nontechnical writer <strong>of</strong> the imperial age, rather than Euclid or Archimedes,<br />

the effect is unmistakable. <strong>The</strong> metaphysical ingredient, largely<br />

absent from Galileo, looms large. For already the ancient writer, unable to<br />

make clear demarcations between scientific theory and the reality it models,<br />

tends to frame the discussion in pre-Hellenistic, usually Aristotelian,<br />

concepts: a mix that early modern scientists are wont to contaminate further<br />

with biblical influences (Newton was a passionate commentator <strong>of</strong><br />

the Bible).<br />

Plutarch is not the only literary classical source used by Newton. In the<br />

following passage we clearly recognize Seneca as the source, through it is<br />

not explicitly stated:<br />

<strong>The</strong> Chaldeans, the most learned astronomers <strong>of</strong> their time, looked<br />

upon the comets (which <strong>of</strong> ancient times before had been numbered<br />

among the celestial bodies) as a particular sort <strong>of</strong> planets, which, describing<br />

eccentric orbits, presented themselves to view only by turns,<br />

once in a revolution, when they descended into the lower parts <strong>of</strong><br />

their orbits. 127<br />

<strong>The</strong> same applies to this very significant passage:<br />

<strong>The</strong>refore the earth, the sun and all the planets which [are] in our<br />

system, according to the ancients have weight with respect to one<br />

another, and would fall toward each other because <strong>of</strong> mutual gravity<br />

and coalesce into one mass, if their fall were not prevented by their<br />

circular motions. 128<br />

Where does this lead us?<br />

As we learned in school, the conceptual leap from a purely descriptive<br />

astronomy to a gravitation-based theory lay in taking the sun, the moon page 401<br />

and the planets and realizing — though these bodies are only a handful<br />

and there was no hope <strong>of</strong> observing others — that their regular motions<br />

did not depend on their “heavenly nature”, but on their having “weight”,<br />

and that these motions could be generalized through a theory that renders<br />

just as regular the motion <strong>of</strong> anything whatsoever: a stone, an apple<br />

127 Newton, De mundi systemate liber, 1, anonymous translation <strong>of</strong> 1728 (probably by Motte), as<br />

revised by Cajori. Compare the passages <strong>of</strong> Seneca quoted on page 271.<br />

128 “Igitur Terra Sol et Planetae omnes qui in nostro systemate ex mente veterum graves sunt in<br />

se mutuo et vi gravitatis mutuae caderent in se invicem & in unam massam coirent nisi descensus<br />

ille a motibus circularibus impediretur” (Classical scholia, folio 271r = [Casini], p. 46 or p. 37). Thus<br />

Newton, who <strong>of</strong> course was immune to the modern scholarly fear <strong>of</strong> committing anachronisms by<br />

attributing “Newtonian” notions to ancient authors, provides authoritative corroboration for the<br />

interpretations <strong>of</strong> Seneca’s passages proposed in Sections 10.5 and 10.9.<br />

Revision: 1.11 Date: 2003/01/06 07:48:20

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