Results from the 10 March 1977 occultation by the Uranus system

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Astrometry, Astronomical Photometry, Stellar Occultation, Uranus (Planet), Uranus Rings, Data Reduction, Light Curve, Miranda, Orbital Resonances (Celestial Mechanics), Radii, Uranus Atmosphere

Scientific paper

Timings of occultation events observed at Perth, Australia during the appulse of Uranus to SAO 158687 are presented. In addition to pre- and post-appulse observations of the alpha ring, a search of the data confirms events by the '4', '5', and '6' rings on the pre-appulse side of Venus, and the '5' and beta rings on the post-appulse side. A table of other suspected events obtained from a statistical search of the data down to the same level of significance as the '4', '5', and '6' events is presented. A fairly strong 'event', so far unconfirmed, is noted near the 5:1 Miranda resonance orbit. Examination of the light curves at high time resolution indicates that the alpha ring was, during this aspect, about 10 km in radial extent and about 50% transparent.

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