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From the reviews:
"...I find Meanest Foundations and Nobler Superstructures to be an excellent resource in the history of science and particularly valuable for its recognition of Hooke's scientific style."
(Physics Today, September 2003)
"This book is very densely packed with theses, issues, new ideas, and historical and philosophical comparisons – all very well researched and thoroughly documented. ... a well-written and in particular very well researched study in the history and philosophy of science of one of the most important and interesting periods in the history of Western science and in intellectual history as a whole. Students of the period and of history and philosophy of science in general will find it an important addition to the discipline’s literature." (Zvi Solow, The Jerusalem Philosophical Quarterly, Vol. 54, July, 2005)
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Book Description Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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). 268 pp. Englisch. Seller Inventory # 9781402007323
Book Description Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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 &. Seller Inventory # 4092065
Book Description Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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). Seller Inventory # 9781402007323
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Book Description Condition: New. New. In shrink wrap. Looks like an interesting title! 1.41. Seller Inventory # Q-1402007329