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Zustand: New. Presents a fresh perspective on the scientific revolution of the seventeenth century. Instead of celebrating the triumph of reason and rationality, the authors study the paradoxes and anxieties that stemmed from the New Science and the intellectual compromises that shaped it and enabled its spectacular success. Num Pages: 352 pages, 51 halftones. BIC Classification: 1D; 3JD; HBJD; HBLH; PDX. Category: (G) General (US: Trade). Dimension: 230 x 152 x 20. Weight in Grams: 484. . 2014. Illustrated. Paperback. . . . . Books ship from the US and Ireland.
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Taschenbuch. Zustand: Neu. Neuware - The Origins of Modern Science is the first synthetic account of the history of science from antiquity through the Scientific Revolution in many decades. Providing readers of all backgrounds and students of all disciplines with the tools to study science like a historian, Ofer Gal covers everything from Pythagorean mathematics to Newton's Principia, through Islamic medicine, medieval architecture, global commerce and magic. Richly illustrated throughout, scientific reasoning and practices are introduced in accessible and engaging ways with an emphasis on the complex relationships between institutions, beliefs and political structures and practices. Readers gain valuable new insights into the role that science plays both in history and in the world today, placing the crucial challenges to science and technology of our time within their historical and cultural context.
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Taschenbuch. Zustand: Neu. Neuware - Presents a fresh perspective on the scientific revolution of the seventeenth century. Instead of celebrating the triumph of reason and rationality, the authors study the paradoxes and anxieties that stemmed from the New Science and the intellectual compromises that shaped it and enabled its spectacular success.
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Taschenbuch. Zustand: Neu. Motion and Knowledge in the Changing Early Modern World | Orbits, Routes and Vessels | Ofer Gal (u. a.) | Taschenbuch | Studies in History and Philosophy of Science | viii | Englisch | 2016 | Springer | EAN 9789401779210 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Sprache: Englisch
Verlag: Kluwer Academic Publishers, 2002
ISBN 10: 1402007329 ISBN 13: 9781402007323
Anbieter: Kennys Bookstore, Olney, MD, USA
Zustand: New. A historical-epistemological study of one the most consequential idea of early modern celestial mechanics: Robert Hooke's proposal to 'compoun[d] the celestial motions of the planets of a direct motion by the tangent and an attractive motion towards a central body,' a proposal which Isaac Newton adopted and realized in his "Principia". Series: Boston Studies in the Philosophy and History of Science. Num Pages: 266 pages, biography. BIC Classification: PDX; PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 15. Weight in Grams: 543. . 2002. Hardback. . . . . Books ship from the US and Ireland.
Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume comprises studies of the early modern drama of motion and transformation of knowledge. It is unique in taking its global nature as fundamental and contains studies of the theme of motion and knowledge in China, Europe and the Pacific from the 16th to the 18th century.People living around the turn of the 17th century were experiencing motion in ways beyond the grasp of anyone less than a century earlier. Goods and people were crossing lands and oceans to distances never envisioned and in scales hardly imaginable by their recent predecessors. The earth itself has been set in motion and the heavens were populated by a whole new array of moving objects: comets, moons, sun spots. Even the motion of terrestrial objects-so close at hand and seemingly obvious-was being thoroughly reshaped. In the two centuries to follow, this incessant, world-changing motion would transform the creation, interpretation and dissemination of knowledge and the life and experiences of the people producing it: savants, artisans, pilots, collectors.
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume comprises studies of the early modern drama of motion and transformation of knowledge. It is unique in taking its global nature as fundamental and contains studies of the theme of motion and knowledge in China, Europe and the Pacific from the 16th to the 18th century.People living around the turn of the 17th century were experiencing motion in ways beyond the grasp of anyone less than a century earlier. Goods and people were crossing lands and oceans to distances never envisioned and in scales hardly imaginable by their recent predecessors. The earth itself has been set in motion and the heavens were populated by a whole new array of moving objects: comets, moons, sun spots. Even the motion of terrestrial objects-so close at hand and seemingly obvious-was being thoroughly reshaped. In the two centuries to follow, this incessant, world-changing motion would transform the creation, interpretation and dissemination of knowledge and the life and experiences of the people producing it: savants, artisans, pilots, collectors.
Taschenbuch. Zustand: 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).
Buch. Zustand: 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).
Zustand: Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher | This volume comprises studies of the early modern drama of motion and transformation of knowledge. It is unique in taking its global nature as fundamental and contains studies of the theme of motion and knowledge in China, Europe and the Pacific from the 16th to the 18th century.People living around the turn of the 17th century were experiencing motion in ways beyond the grasp of anyone less than a century earlier. Goods and people were crossing lands and oceans to distances never envisioned and in scales hardly imaginable by their recent predecessors. The earth itself has been set in motion and the heavens were populated by a whole new array of moving objects: comets, moons, sun spots. Even the motion of terrestrial objects¿so close at hand and seemingly obvious¿was being thoroughly reshaped. In the two centuries to follow, this incessant, world-changing motion would transform the creation, interpretation and dissemination of knowledge and the life and experiences of the people producing it: savants, artisans, pilots, collectors. .