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Meanest Foundations and Nobler Superstructures: Hooke, Newton and the Compounding of the Celestiall Motions of the Planetts

Meanest Foundations and Nobler Superstructures

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"Meanest Foundations and Nobler Superstructures" by Ofer Gal is a astronomy book and space science reference focused on Celestial Motion. Best for students, researchers, and serious astronomy enthusiasts.

This book is a historical-epistemological study of one of the most consequential breakthroughs in the history of celestial mechanics: Robert Hooke's (1635-1703) proposal to "compoun[d] the celestial motions of the planets of a direct motion by the tangent & an attractive motion towards a centrat body" (Newton, The Correspondence li, 297. Henceforth: Correspondence). This is the challenge Hooke presented to Isaac Newton (1642-1727) in a short but intense correspondence in the winter of 1679-80, which set Newton on course for his 1687 Principia, transforming the very concept of "the planetary heavens" in the process (Herivel, 301: De Motu, Version III). 1 It is difficult to overstate the novelty of Hooke 's Programme • The celestial motions, it suggested, those proverbial symbols of stability and immutability, werein fact a process of continuous change: a deflection of the planets from original rectilinear paths by "a centraU attractive power" (Correspondence, li, 313). There was nothing necessary or essential in the shape of planetary orbits. Already known to be "not circular nor concentricall" (ibid. ), Hooke claimed that these apparently closed "curve Line[ s ]" should be understood and calculated as mere effects of rectilinear motions and rectilinear attraction. And as Newton was quick to realize, this also implied that "the planets neither move exactly in ellipse nor revolve twice in the same orbit, so that there are as many orbits to a planet as it has revolutions" (Herivel, 301: De Motu, Version III).

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Best For: Readers interested in the history and philosophy of science, particularly in celestial mechanics and the development of orbital theory.
Focus: The historical and epistemological analysis of Robert Hooke's contribution to understanding planetary motion and its influence on Isaac Newton's work.
Covers: The development of celestial motion theories in the 17th century, focusing on Hooke's proposal and its impact on Newton's formulation of planetary motion.
Why It Matters: It sheds light on a key scientific breakthrough that shaped modern astronomy and physics by exploring the interaction between two foundational figures in science.

"Meanest Foundations and Nobler Superstructures" by Ofer Gal is a astronomy book and space science reference focused on Celestial Motion. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Celestial Motion

Author: Ofer Gal

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

This book is a historical-epistemological study of one of the most consequential breakthroughs in the history of celestial mechanics: Robert Hooke's (1635-1703) proposal to "compoun[d] the celestial motions of the planets of a direct motion by the tangent & an attractive motion towards a centrat body" (Newton, The Correspondence li, 297. Henceforth: Correspondence). This is the challenge Hooke presented to Isaac Newton (1642-1727) in a short but intense correspondence in the winter of 1679-80, which set Newton on course for his 1687 Principia, transforming the very concept of "the planetary heavens" in the process (Herivel, 301: De Motu, Version III). 1 It is difficult to overstate the novelty of Hooke 's Programme • The celestial motions, it suggested, those proverbial symbols of stability and immutability, werein fact a process of continuous change: a deflection of the planets from original rectilinear paths by "a centraU attractive power" (Correspondence, li, 313). There was nothing necessary or essential in the shape of planetary orbits. Already known to be "not circular nor concentricall" (ibid. ), Hooke claimed that these apparently closed "curve Line[ s ]" should be understood and calculated as mere effects of rectilinear motions and rectilinear attraction. And as Newton was quick to realize, this also implied that "the planets neither move exactly in ellipse nor revolve twice in the same orbit, so that there are as many orbits to a planet as it has revolutions" (Herivel, 301: De Motu, Version III).

AuthorOfer Gal
PublisherSpringer
Published2010-12-09
ISBN-139789048160679
BindingPaperback
Pages252
LanguageEnglish
SubjectsHistory
TopicCelestial Motion
SeriesBoston Studies in the Philosophy and History of Science

Format: Paperback

Length: 252 pages

Language: English

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