The 20 March 1980 occultation by the Uranian rings

Details The 20 March 1980 occultation by the Uranian rings The 20 March 1980 occultation by the Uranian rings

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..127e&link_type=abstract

Astronomical Journal, vol. 86, Jan. 1981, p. 127-134.

Astronomy and Astrophysics

Astronomy

23

Astronomical Models, Kinematics, Stellar Occultation, Uranus Rings, Orbital Elements, Statistical Analysis, Time Response, Width, Uranus, Rings, Occultations, Observations, Models, Kinematics, Orbits, Precession, Eccentricities, Mass, Data, Data Reduction, Width, Properties, Characteristics, Dispersion, Parameters

Scientific paper

On March 20, 1980, observations of occultations by rings alpha, beta, gamma, delta, and epsilon were observed from Cerro Tololo and Sutherland. A model ring profile was fit to the data to obtain the midtimes of the occultations and the widths of the profiles. A 14-parameter kinematic model, including J2, J4, and some of the orbital elements for rings 4, alpha, beta, and epsilon as free parameters, was fit to these data and previous ring occultation timings. The results yield J2 = (3.396 + or - 0.020) x 10 to the -3 and a 2 sigma upper limit, absolute value of J4 less than 7 x 10 to the -5th. Uniform precession models for rings alpha, beta are established and the dispersion in the values of semimajor axes and eccentricities for rings alpha, beta, and epsilon have been obtained. If self-gravity is the cause of the uniform precession, the mass of the beta ring is estimated at approximately 4 x 10 to the 16th g; the mass of the alpha ring probably is also near this value.

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