THE ASTRONOMER Electronic Circular No 394 1990 Mar 18 10.30UT Microlink:MAG60138 JANET:GMH at UK.AC.RO-GREENWICH.STARLINK Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP, England. Telephone: (0256)471074 Int:+44256471074 Telex: 94082518 Answerback: TAGUY ------------------------------------------------------------------ COMET CERNIS-KIUCHI-NAKAMURA (1990b) K. Churyumov, Kiev Observatory, telexes the discovery of a new comet by Kazimieras Cernis. H. Kosai, National Astronomical Observatory of Japan, reports independent discoveries by Tsuruhiko Kiuchi and Yuji Nakamura. The comet generally appears diffuse with some condensation, coma diameter about 2'. The following observations are available: 1990 UT R.A. (1950) Decl. m1 Observer Mar. 14.79 0 54.4 +43 04 9 Cernis 16.441 1 03.0 +44 05 9 Kiuchi 16.441 1 03.2 +44 07 9 Nakamura 17.120 1 06.8 +44 31 8.4 Hale 17.84733 1 11.0 +44 52.5 9 Mobberley K. Cernis (Vilnius). 0.12-m refractor. T. Kiuchi (Usuda-machi, Nagano). 25x150 binoculars. Y. Nakamura (Yokkaichi, Mie). 20x120 binoculars. A. Hale (Las Cruces, NM). 0.41-m reflector. Magnitude estimate with 10x50 binoculars. M.Mobberley (Bury St Edmunds) 0.36-m reflector. 2' diameter, diffuse with central condensation. 1' extension in PA 030. IAUC 4980 and other sources COMET AUSTIN (1989c1) Total visual magnitude estimates: Mar. 5.93 UT, 6.8 (V. F. de Assis Neto, Sao Francisco de Oliveira, Brazil, 10x70 binoculars); 7.50, 6.6 (A. Pearce, Scarborough, W. Australia, 20x80 binoculars); 11.50, 6.5 (Pearce); 13.49, 6.4 (Pearce); 14.49, 6.3 (Pearce). IAUC 4979 Z. Sekanina, Jet Propulsion Laboratory, California Institute of Technology, writes: "The orientation and extent of the dust tail on Feb. 25-26 and Mar. 2, as communicated respectively by West (IAUC 4970) and by Gilmore (IAUC 4975), are diagnostic of submillimeter- size and larger particles released between about 900 and 500 days before perihelion, when the comet was at heliocentric distances between 10 and 7 AU. Early tail formation of this kind is characteristic of new, Oort-cloud comets. Predicted position angles for this tail: Mar. 10, 158 deg; 20, 157 deg; 30, 150 deg; Apr. 9, 124 deg; 19, 85 deg; 29, 60 deg; May 9, 42 deg; 19, 24 deg; 29, 358 deg; June 8, 333 deg; 18, 327 deg." IAUC 4977 Guy M Hurst