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Saturn satellite observations and orbits from the 1980 ring plane crossing
Authors:PK Seidelmann  RS Harrington  D Pascu  WA Baum  DG Currie  JA Westphal  GE Danielson
Institution:U.S. Naval Observatory, 34th St. and Massachusetts Ave., N.W., Washington, D.C. 20390, USA;Lowell Observatory, P.O. Box 1269, Flagstaff, Arizona 86002, USA;University of Maryland, College Park, Maryland 20742, USA;California Institute of Technology, Pasadena, California 91103, USA
Abstract:The ground-based observations of the recently discovered Saturnian satellites, obtained during the 1980 apparition, have been collected from the IAU Circulars and identified with and fit to four orbital groups: (1) the inner pair of coorbital librating satellites, (2) the satellite known as “Dione B” near the L4 point of Dione-Saturn, (3) the satellites associated with the L4 and L5 points of Tethys-Saturn or, alternatively, one satellite unconfortably near the orbit of Tethys, and (4) the F-ring satellites observed by Voyager I.
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