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1 The Birth of Science - MSRI

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11.7 Newton’s Natural Philosophy 327<br />

or a mass <strong>of</strong> liquid swinging about the center <strong>of</strong> the earth. <strong>The</strong> ancient<br />

testimonia discussed in Chapter 10 and the use made <strong>of</strong> them by Kepler,<br />

Newton and others show that this leap was achieved only once in history:<br />

in Hellenistic science.<br />

Two sets <strong>of</strong> factors were essential in creating the conditions for a modern<br />

gravitation-based dynamics to take shape as a scientific theory and evolve<br />

into modern physics.<br />

<strong>The</strong> first set consisted <strong>of</strong> certain Hellenistic technical and methodological<br />

tools, found above all in the works <strong>of</strong> Euclid and Archimedes. Some <strong>of</strong><br />

these tools were:<br />

– the hypothetico-deductive method created in the Elements, providing<br />

the general conceptual framework to which there must conform any<br />

scientific theory wishing to use the results <strong>of</strong> classical mathematics — a<br />

use that is <strong>of</strong> course inescapable;<br />

– the so-called “method <strong>of</strong> exhaustion”, whose relation to the seed <strong>of</strong> infinitesimal<br />

analysis developed by Newton will be discussed in the next<br />

section;<br />

– Archimedean mechanics, as laid out specifically in the treatise On the<br />

equilibrium <strong>of</strong> plane figures, which showed how to use the preceding<br />

methods to found a scientific theory <strong>of</strong> mechanics.<br />

<strong>The</strong> second set <strong>of</strong> prerequisites were certain pieces <strong>of</strong> information on<br />

dynamics and gravitation which, with the loss <strong>of</strong> the original treatises,<br />

were found scattered throughout works generally written by scientifically<br />

incompetent authors and representing traditions that were far from scientific.<br />

<strong>The</strong> fragmentary and heterogeneous nature <strong>of</strong> these testimonia<br />

makes their complete identification difficult. Based on an examination <strong>of</strong> page 402<br />

a small part <strong>of</strong> the still extant literature, one can list at least the following<br />

examples.<br />

– <strong>The</strong> hints about inertia, centrifugal force and gravity (toward the earth)<br />

transmitted by Plutarch in the De facie. <strong>The</strong>se hints included a few “exercises<br />

in dynamics” together with their qualitative answers. 129<br />

– Other hints complementary to the first, including those found in the<br />

commentaries to Aristotle by Simplicius and Philoponus and in the<br />

Heronian and pseudo-Aristotelian Mechanics.<br />

– Mentions <strong>of</strong> an attraction between planets and sun, and <strong>of</strong> the use <strong>of</strong><br />

this idea in a heliocentric framework to create a “celestial mechanics”<br />

129 Sambursky (who was first and foremost an experimental physicist) revealingly wrote that<br />

“some <strong>of</strong> [the conclusions in the De facie] call to mind classic exercises from Newton’s <strong>The</strong>ory<br />

<strong>of</strong> Gravitation”: see [Sambursky: PWG], p. 209. Yet he did not consider the question <strong>of</strong> the dialog’s<br />

sources, taking it to be “perhaps the first work in astrophysics ever written” (p. 205) — which<br />

would make Plutarch the founder <strong>of</strong> that science!<br />

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

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