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Inertia

from ENTRIES

Published online by Cambridge University Press:  05 January 2016

Hylarie Kochiras
Affiliation:
École Normale Supérieure de Paris (ENS)
Lawrence Nolan
Affiliation:
California State University, Long Beach
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Summary

The term “inertia” was first introduced by Kepler (Epitome of Copernican Astronomy, IV.3, 59; IV.2, 54, 55) to designate the opposition to motion that he considered natural to matter. One component of this opposition was a variant of Aristotelian doctrine about “violent motion” that Galileo, Gassendi, Beeckman, and Descartes would reject: persistence of motion requires some external agent, because bodies in motion tend toward rest. Although the Keplerian concept of inertia is sometimes erroneously identified with this first component alone, Kepler's view included a second component claim, a variant of which future physics would retain: bodies resist being put into motion, and their resistance varies with density (Kepler 1858 and 1896, 1:161; 6:174–75, 342; Jammer 1961, 57, 56, 55).

Descartes uses the term “inertia” much as Kepler did. In response to Debeaune's claim that resistance is due to a tardiveté naturelle, Descartes denies that bodies possess any such natural inertia or sluggishness. His own view emerging, he too acknowledges resistance, though correlating it with size rather than density, as his definition of matter in terms of extension alone demands. Diverging from Kepler, he pairs his recognition of resistance with the anti-Aristotelian claim that bodies in motion tend to stay in motion (AT II 466–67).

The term “inertia” eventually labeled a principle based upon Newton's first law of motion, which states, “Every body perseveres in its state of being at rest or of moving uniformly straight forward, except insofar as it is compelled to change its state by forces impressed” (Principia, 417). The concept of an inertial state is inseparable from such concepts as space and motion, and whereas Newton saw rest and uniform motion as distinct if humanly indistinguishable states, they were eventually classified as distinct only in connection with a chosen reference frame.

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Publisher: Cambridge University Press
Print publication year: 2015

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References

Kepler, Johannes. 1618–21 (1995). Epitome of Copernican Astronomy, trans. Wallis, C. G.. Amherst: Prometheus Books.Google Scholar
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  • Inertia
  • Edited by Lawrence Nolan, California State University, Long Beach
  • Book: The Cambridge Descartes Lexicon
  • Online publication: 05 January 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9780511894695.142
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  • Inertia
  • Edited by Lawrence Nolan, California State University, Long Beach
  • Book: The Cambridge Descartes Lexicon
  • Online publication: 05 January 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9780511894695.142
Available formats
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To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Inertia
  • Edited by Lawrence Nolan, California State University, Long Beach
  • Book: The Cambridge Descartes Lexicon
  • Online publication: 05 January 2016
  • Chapter DOI: https://doi.org/10.1017/CBO9780511894695.142
Available formats
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