------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1748 2002 Feb 26 17.27UT Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074 INTERNET: GUY@TAHQ.DEMON.CO.UK GMH at AST.STAR.RL.AC.UK WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- SUPERNOVA 2002aw IN ANONYMOUS GALAXY Tim Puckett and M.Peoples, USA report in IAU Circular 7831, that they have discovered a mag 16.6 supernova with the 0.60-m automated supernova patrol telescope on images of Feb 15 and 16. The location is: RA 16h 37m 29.06s DEC +40 52' 50.3" (2000), placing it 1.6"W and 1.5"N of the centre of an anonymous galaxy. R. Kushida in Japan confirmed the object on an image of Feb 16. SUPERNOVAE 2002ax-2002be The Deep Lens Survey Team have reported on IAU Circular 7833 details of their discovery of eight supernova on Feb 14-16 with the Cerro Tololo 4-m telescope. All objects are fainter than magnitude 21. COMET C/2002 C1 (IKEYA-ZHANG) The following updated orbital elements have appeared on MPEC 2002-D36: T 2002 Mar. 18.9784 TT MPC q 0.507061 (2000.0) P Q z +0.019502 Peri. 34.6666 -0.5491635 -0.6906790 Node 93.3718 +0.6195893 -0.7143048 e 0.990111 Incl. 28.1206 +0.5608284 +0.1128330 >From 309 observations 2002 Feb. 1-24. Brian Marsden comments that numerical integration backward of the perturbed equivalent of the above unperturbed solution yields a previous perihelion date in March 1659. He adds that identity with C/1661 C1 now looks more likely than with C/1532 R1. Graeme Waddington, Oxford, has e-mailed the editor to comment on the above findings by Brian. Graeme reports that integrating the given unperturbed orbit yields, using DE405 planetary masses, a previous perihelion of 1659 May 13.3 (Gregorian). Guy M Hurst