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1 The Birth of Science - MSRI

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

had <strong>of</strong> course triumphed irreversibly after Kepler’s work), so that it no<br />

longer corresponds to any empirical datum. It follows that the motions<br />

that are the object <strong>of</strong> Newton’s axioms or laws <strong>of</strong> motion are beyond our<br />

perception. <strong>The</strong> Nature that concerns his natural philosophy transcends<br />

experience, unlike Aristotle’s, and the first step toward it is to “abstract<br />

from our senses”. This is not, mind you, an abstraction arising from the<br />

substitution <strong>of</strong> a theoretical model for real objects, but one imposed by<br />

the need to completely give up “sensible measures”. In this scheme there<br />

can be no correspondence rule between relative movements and absolute<br />

ones, because the latter refer to a fixed space beyond perception, and bear<br />

no relation to phenomena. Thus Newton is forced, as he himself admits,<br />

not to deal with “common affairs”. If this is the “experimental method”<br />

characteristic <strong>of</strong> modern science, it is likely that it was indeed unknown to<br />

scientists like Archimedes, Ctesibius and Herophilus.<br />

(It is true that the Principia later does characterize absolute space, in the<br />

following way. Newton establishes that the barycenter <strong>of</strong> the solar system<br />

is at rest or in uniform motion, using an implicit, and arguably reasonable,<br />

assumption <strong>of</strong> isolation. At the same time — and here is the crux — he opts<br />

for rest over uniform motion, a gratuitous choice for which there is no<br />

logical justification in his scientific mechanics, but which is very important<br />

from the viewpoint <strong>of</strong> his metaphysical notion <strong>of</strong> space. 117 )<br />

Building, with full methodological coherence, on his notion <strong>of</strong> space,<br />

Newton next talks <strong>of</strong> motion and force:<br />

[E]ntire and absolute motions can be no otherwise determined than<br />

by immovable places. . . . Now no other places are immovable but<br />

those that, from infinity to infinity, do all retain the same given position<br />

one to another; and upon this account must ever remain unmoved;<br />

and do thereby constitute immovable space.<br />

<strong>The</strong> causes by which true and relative motions are distinguished, one<br />

from the other, are the forces impressed upon bodies to generate motion.<br />

True motion is neither generated nor altered, but by some force<br />

impressed upon the body moved; but relative motion may be generated<br />

or altered without any force impressed upon the body. 118<br />

117 See Principia, Book III, proposition XI / theorem XI and its pro<strong>of</strong>. <strong>The</strong> selection is effected<br />

through the immediately preceding hypothesis, “That the centre <strong>of</strong> the system <strong>of</strong> the world is immovable”,<br />

which is justified by a single argument: “This is acknowledged by all.” In this metaphysical<br />

statement, based on an appeal to common sense, Newton prefers to talk <strong>of</strong> “the system <strong>of</strong> the<br />

world” and abandons previously defined terms. <strong>The</strong> pro<strong>of</strong> <strong>of</strong> proposition XI / theorem XI shows<br />

that he conceives “the centre <strong>of</strong> the the system <strong>of</strong> the world” as coinciding with the barycenter <strong>of</strong><br />

the solar system.<br />

118 Newton, Principia mathematica, Definitions, scholium, at 55%, Motte/Cajori translation.<br />

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