Occultations by Uranus and Neptune: 1991-1999

Arnold R. Klemola
UCO/Lick Observatory, Board of Studies in Astronomy and Astrophysics
University of California, Santa Cruz, California 95064
Douglas J. Mink
Harvard-Smithsonian Center for Astrophysics
Cambridge, Massachusetts 02138

Abstract

The results of a photographic plate search for stars as faint as V=14 which may be occulted by Uranus or Neptune or their rings between 1 January 1991 and 31 December 1999 are presented. Circumstances for the closest approach of Uranus to 76 stars and Neptune to 18 stars are presented. Occultations by Neptune's ring "arcs" are predicted in 1992, 1997, and 1999.

Published in 1991 in The Astronomical Journal, Volume 102, pages 389-394.