A Measurement of the Shape of the Solar Disk: The Solar Quadrupole Moment, the Solar Octopole Moment, and the Advance of Perihelion of the Planet Mercury

T. J. Lydon and S. Sofia
Phys. Rev. Lett. 76, 177 – Published 8 January 1996
PDFExport Citation

Abstract

The Solar Disk Sextant experiment has measured the solar angular diameter for a variety of solar latitudes. Combined with solar surface angular rotation data, the solar quadrupole moment J2 and the solar octopole moment J4 have been derived first by assuming constant internal angular rotation on cylinders and then by assuming constant internal angular rotation on cones. We have derived values of 1.8×107 for J2 and 9.8×107 for J4. We conclude with a discussion of errors and address the prediction of general relativity for the rate of advance of perihelion of the planet Mercury.

  • Received 18 April 1995

DOI:https://doi.org/10.1103/PhysRevLett.76.177

©1996 American Physical Society

Authors & Affiliations

T. J. Lydon and S. Sofia

  • Center for Solar and Space Research, P.O. Box 208101, New Haven, Connecticut 06520-8101

References (Subscription Required)

Click to Expand
Issue

Vol. 76, Iss. 2 — 8 January 1996

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×