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Status of the Copernican theory before Kepler, Galileo, and Newton

 

作者: Douglas R. Martin,  

 

期刊: American Journal of Physics  (AIP Available online 1984)
卷期: Volume 52, issue 11  

页码: 982-986

 

ISSN:0002-9505

 

年代: 1984

 

DOI:10.1119/1.13911

 

出版商: American Association of Physics Teachers

 

关键词: ASTRONOMY;HISTORY;SOLAR SYSTEM

 

数据来源: AIP

 

摘要:

The most obvious evidence supporting the Copernican theory emerged during a period of 300 years following the publication ofDeRevolutionibusby Copernicus in 1543. In this paper a comparison is made between the geo‐centric and helio‐centric theories on the basis of astronomical merit and observational evidence available in 1543. The Copernican theory is not superior on the basis of calculational accuracy, but does possess greater unity and is simpler in the sense thatad‐hocassumptions required by the geo‐centric theory are not required by the Copernican theory. The Copernican theory, however, requires anad‐hocassertion about the size of the universe in order to explain the absence of observed stellar parallax.

 

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