Experimental determination of the sun's oblateness

Details Experimental determination of the sun's oblateness Experimental determination of the sun's oblateness

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1326a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Nov.-Dec. 1990, p. 1326-1328. In Russian.

Statistics

Computation

6

Computational Astrophysics, Radar Astronomy, Solar Oblateness, Mars (Planet), Mercury (Planet), Planetary Orbits, Venus (Planet)

Scientific paper

The solar dynamic oblateness coefficient J2 was determined on the basis
of radar observations of the near-solar planets during 1964-1986. The
value of J2 was found to be (0.66 + or -0.9) x 10 to the -6th.

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