Circular No. 3608 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 1981 N 1 H. J. Reitsema, Lunar and Planetary Laboratory, reports that observations of the May 24 Neptune appulse (Mink et al. 1981, A.J. 86, 135) suggest that Neptune may possess a previously unsuspected satellite at least 180 km in diameter and situated some 3 Neptune radii from the center of mass of the system (if the object is in Neptune's equatorial plane). Observations with two University of Arizona telescopes, situated ~ 5 km apart, each showed an abrupt occultation event, ~ 8 seconds in duration and corresponding to full stellar intensity, beginning at 8h36m40s UT. The observations were made by Reitsema and W. B. Hubbard with the 1.5-m reflector at the Catalina station and by L. A. Lebofsky and D. Tholen with the 1.0-m reflector on Mt. Lemmon. SATELLITES OF SATURN C. Veillet, CERGA, observing with the 1.5-m Danish telescope at the European Southern Observatory, has refined the longitude difference of 1981 S 2 from Saturn III (from 29 observations during Apr. 10-14) to 55o.1 +/- 0o.6 (p.e.). Another satellite, presumably 1981 S 1, of comparable brightness, was noted (from 12 observations on Apr. 12 and 14) at a longitude difference of +58o.79 +/- 0o.24 (p.e.). COMET RUSSELL (1980l) The following ephemeris continuation, from the elements on MPC 5837, replaces that given on MPC 5652: 1981 ET R. A. (1950) Decl. Delta r m1 May 26 16 33.48 -59 06.5 June 5 15 27.11 -51 54.6 1.449 2.363 15.0 15 14 45.81 -43 21.5 25 14 21.97 -35 25.0 1.705 2.474 15.6 July 5 14 08.82 -28 53.3 15 14 02.28 -23 49.4 2.152 2.599 16.3 25 13 59.94 -19 58.8 Aug. 4 14 00.41 -17 04.7 2.669 2.735 17.0 14 14 02.84 -14 52.8 24 14 06.65 -13 12.1 3.181 2.880 17.6 Sept. 3 14 11.47 -11 54.0 13 14 17.03 -10 52.3 3.642 3.031 18.1 1981 May 29 (3608) Brian G. Marsden
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