Observations of the mutual phenomena of Saturnian satellites in 1980

Details Observations of the mutual phenomena of Saturnian satellites in 1980 Observations of the mutual phenomena of Saturnian satellites in 1980

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982tokab.267.3039s&link_type=abstract

Tokyo Astronomical Observatory, Tokyo Astronomical Bulletin, Second Series (ISSN 0082-4690), no. 267, June 18, 1982, p. 3039-305

Astronomy and Astrophysics

Astronomy

2

Orbital Mechanics, Saturn Satellites, Computer Programs, Light Curve, Orbital Elements, Tables (Data), Ubv Spectra

Scientific paper

Sinclair's (1977) theory is used in a preliminary orbital analysis of five mutual phenomena of the Saturnian satellites in 1980. Midtimes and light losses (normalized to unity) of the events determined from the observed light curves are given, together with calculations made with the orbital elements obtained. In order to check the present computer calculations, results have been compared with the predictions of Aksnes and Franklin (1978), in which substantially the same orbital elements are used.

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