De Copernic à Descartes
The Copernician revolution has comological consequences upon which Copernic has expressed little, and the scale of which will be measured only by Giordano Bruno or Descartes. The most spectacular aspect of this post-Copernician revolution is of course the suppression of the sphere of fixed stars. Th...
| Main Author: | |
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| Format: | Electronic Article |
| Language: | French |
| Check availability: | HBZ Gateway |
| Journals Online & Print: | Drawer...
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| Fernleihe: | Fernleihe für die Fachinformationsdienste |
| Published: |
Librairie Philosophique J. Vrin
2015
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| In: |
Revue des sciences philosophiques et théologiques
Year: 2015, Volume: 99, Issue: 2, Pages: 239-265 |
| Further subjects: | B
Nicolas Copernic
B Johannes Kepler B Tourbillons B Parallaxe stellaire B Mouvement de la Terre B Ciel empyrée B Agostino Steuco B Réfractions B Galileo Galilei B Tycho Brahe B René Descartes |
| Online Access: |
Volltext (JSTOR) Volltext (kostenfrei) Volltext (kostenfrei) |
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| 520 | |a The Copernician revolution has comological consequences upon which Copernic has expressed little, and the scale of which will be measured only by Giordano Bruno or Descartes. The most spectacular aspect of this post-Copernician revolution is of course the suppression of the sphere of fixed stars. The present article examines this question through two perspectives : (i) that of an empyrean sky and (ii) the (vain) quest for a stellar parallax that for Kepler, Galileo and Descartes supposedly proved a posteriori Copernic’s theory. We underscore finally the great subtlety of the argument layed out in Descartes’ Principia Philosophiae (1644) that uses the « arbitrary » supposition of the empyrea to set the strictly geomobilistic copernicans against their tychonian adversaries who hoped via this supposition to maintain the Earth’s immobility at the center of the World. | ||
| 520 | |a La révolution copernicienne a des conséquences cosmologiques sur lesquelles Copernic a été peu disert, et dont il faut attendre Giordano Bruno ou Descartes pour mesurer l’exacte portée. L’aspect le plus spectaculaire de cette révolution post-copernicienne est bien sûr la suppression de la sphère des étoiles fixes. L’article examine cette question sous deux aspects : (i) les conséquences problématiques de l’immobilisation copernicienne de la sphère des fixes par rapport à la fiction théologique d’un ciel empyrée, et (ii) la (vaine) recherche d’une parallaxe stellaire, supposée, chez Kepler, Galilée et Descartes, constituer une preuve a posteriori de la théorie copernicienne. On souligne enfin la grande subtilité de l’argumentation déployée dans les Principia Philosophiae de Descartes (1644) qui utilisent la supposition « arbitraire » de l’empyrée pour renvoyer dos-à-dos les coperniciens strictement géomobilistes, et leurs adversaires tychoniens, qui espéraient, moyennant cette supposition, pouvoir laisser la Terre immobile au centre du monde. | ||
| 650 | 4 | |a Tycho Brahe | |
| 650 | 4 | |a Tourbillons | |
| 650 | 4 | |a René Descartes | |
| 650 | 4 | |a Réfractions | |
| 650 | 4 | |a Parallaxe stellaire | |
| 650 | 4 | |a Nicolas Copernic | |
| 650 | 4 | |a Mouvement de la Terre | |
| 650 | 4 | |a Johannes Kepler | |
| 650 | 4 | |a Galileo Galilei | |
| 650 | 4 | |a Ciel empyrée | |
| 650 | 4 | |a Agostino Steuco | |
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