The problem of the earth's shape from Newton to Clairaut : the rise of mathematical science in eighteenth-century Paris and the fall of "normal" science
Author(s)
Bibliographic Information
The problem of the earth's shape from Newton to Clairaut : the rise of mathematical science in eighteenth-century Paris and the fall of "normal" science
Cambridge University Press, 1995
Available at 17 libraries
  Aomori
  Iwate
  Miyagi
  Akita
  Yamagata
  Fukushima
  Ibaraki
  Tochigi
  Gunma
  Saitama
  Chiba
  Tokyo
  Kanagawa
  Niigata
  Toyama
  Ishikawa
  Fukui
  Yamanashi
  Nagano
  Gifu
  Shizuoka
  Aichi
  Mie
  Shiga
  Kyoto
  Osaka
  Hyogo
  Nara
  Wakayama
  Tottori
  Shimane
  Okayama
  Hiroshima
  Yamaguchi
  Tokushima
  Kagawa
  Ehime
  Kochi
  Fukuoka
  Saga
  Nagasaki
  Kumamoto
  Oita
  Miyazaki
  Kagoshima
  Okinawa
  Korea
  China
  Thailand
  United Kingdom
  Germany
  Switzerland
  France
  Belgium
  Netherlands
  Sweden
  Norway
  United States of America
Note
Bibliography: p. 755-777
Includes index
Description and Table of Contents
Description
This book investigates, through the problem of the Earth's shape, part of the development of post-Newtonian mechanics by the Parisian scientific community during the first half of the eighteenth century. In the Principia, Newton first raised the question of the Earth's shape. John Greenberg shows how continental scholars outside France influenced efforts in Paris to solve the problem, and he also demonstrates that Parisian scholars, including Bouguer and Fontaine, did work that Alexis-Claude Clairaut used in developing his mature theory of the Earth's shape. The evolution of Parisian mechanics proved not to be the replacement of a Cartesian paradigm by a Newtonian one, a replacement that might be expected from Thomas Kuhn's formulations about scientific revolutions, but a complex process instead involving many areas of research and contributions of different kinds from the entire scientific world. Greenberg both explores the myriad of technical problems that underlie the historical development of part of post-Newtonian mechanics and embeds his technical discussion in a framework that involves social and institutional history, politics, and biography.
Table of Contents
- Preface
- 1. Isaac Newton's theory of a flattened Earth
- 2. The state of the problem of the Earth's shape in the 1720s: stalemate
- 3. The revival of geodesy in Paris (1733-1735)
- 4. Pierre Bouguer and the theory of homogeneous figures of equilibrium (1734)
- 5. Maupertuis: on the theory of the Earth's shape (1734)
- 6. Alexis-Claude Clairaut's first theories of the Earth's shape
- 7. Interlude I: integral calculus (1690-1741)
- 8. Interlude II: the Paris academy contest on the tides (1740)
- 9. Clairaut's mature theory of the Earth's shape (1741-1743): first substantial connections between the revival of mathematics in Paris and progress in mechanics there
- 10. Epilogue: Fontaine's and Clairaut's advances in the partial differential calculus revisited, or the virtues of interrelated developments in mathematics and science, and the fall of 'normal' science
- Notes to chapters
- Biography.
by "Nielsen BookData"