Cited by 59History and Developments in AstronomyHistorical Philosophy and ScienceHistorical Astronomy and Related Studies

Copernicus and the Origin of his Heliocentric System

Goldstein, Bernard R.·2002·Journal for the History of Astronomy

Abstract

L'introduction d'un systeme heliocentrique par Copernic etait a l'epoque consideree comme revolutionnaire pour la cosmologie traditionnelle et apparait comme etant un evenement globalement marquant de l'histoire des sciences. Mais quelle etait la base de la recherche qui a abouti a l'heliocentrisme ? L'auteur explore les raisons qui ont pousse Copernic a rejeter les principes relatifs aux distances cosmiques et au systeme geocentrique dans lequel ils etaient ancres.

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Crossref · 10.1177/002182860203300301

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  • Recent trends in historiography of science have critiqued the notion of a scientific revolution and downplayed the Copernicus-Galileo-Newton narrative.

    “recent trends in the historiography of science have resulted in critiques of the very notion of a”

Cited by

Authors
Goldstein, B. R.
Affiliations
University of Pittsburgh (US)
Corresponding author
Goldstein, Bernard R.
Venue
Journal for the History of Astronomy
Published
2002-08
Volume
33
Issue
3
Pages
219-235
ISSN
  • 0021-8286 (ISSN-L)
  • 1753-8556
OpenAlex
W1631164747
Cited by
59
References
0
Citations by year
2026: 2 · 2025: 1 · 2024: 3 · 2022: 15 · 2021: 1 · 2020: 5 · 2019: 2 · 2018: 1 · 2016: 2 · 2015: 4 · 2014: 4 · 2013: 5
FWCI
1.06
Type
journal article
Language
en
Open access
closed
Locations
Journal for the History of Astronomy (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
  • Social Sciences › Arts and Humanities › History and Philosophy of Science › Historical Philosophy and Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Historical Astronomy and Related Studies
Keywords
Copernicus, heliocentrism, cosmological distances, Copernican revolution, history of astronomy

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