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Faculae and the solar oblateness - A summaryDicke and Goldenberg (1967) inferred a value of the solar oblateness by projecting an image of the sun on a circular occulting disk and measuring the light flux from the portion of the sun exposed beyond the disk. These measurements have the implication that if the optical oblateness measured is mirrored in a true gravitational oblateness, then the non-Newtonian part of Mercury's perihelion advance cannot agree with Einstein's prediction based on general relativity. The present analysis shows that faculae may have contributed all of Dicke and Goldenberg's excess signal. There is overwhelming evidence that this signal is contaminated by faculae at some level, and very little evidence to exclude faculae as a cause of the signal.
Document ID
19740040546
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Chapman, G. A.
(San Fernando Observatory Los Angeles, Calif., United States)
Ingersoll, A. P.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
December 14, 1973
Subject Category
Space Sciences
Accession Number
74A23296
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-003
Distribution Limits
Public
Copyright
Other

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