------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1233 1997 Sep 14 16.05UT 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.demon.co.uk/astronomer ------------------------------------------------------------------- OCCULTATION OF PPM 709119 BY 314 (ROSALIA) Further to the prediction on E1232, Gary Poyner, Birmingham, England e-mails: Negative observation. 52,32,32N 1,52,30W Rosalia's magnitude estimated at 13.7 using GSC values. September 12/13 1997 Start: 23h 50m UT End: 00h 10m UT Telescope Type: Newtonian f5 Aperture: 40cm Mag. x118 Mount: Alt-Az. Motor Drive: No Mode of time recording: Digital watch Atmosphere Transparency: Very transparent Star image stability: 4 (Ant) Wind Speed: Calm Temp: 7oC Richard Miles reports: No positive observation of the September 12/13 event involving 314 Rosalia has been reported to the author. Three negative observations have been reported by: Hazel McGee, Clandon, Surrey, UK (51 16 N, 00 30 W ) Terry Platt, Binfield, Berkshire, UK (51 25.5 N, 00 47.4 W, Height 45 m) Gary Poyner, Birmingham, UK (52 32.53 N, 01 52.5 W ). Several observers (including Alan Bowden, Geoff Kirby, myself and probably many others too) were 'rained off' shortly before the predicted time. Although last-minute astrometry was provided by two sources, Jim Roe in Montana, US, and Angel Lopez in Mallorca, Spain, the reductions were not posted up until an hour or so before the actual event by both Jan Manek and David Dunham. This astrometry indicated that the path had shifted significantly south passing over Sardinia, central Italy near Rome and part of the Ukraine. A plot of the 'last-minute' prediction from Jan Manek is available at http://www.ast.cam.ac.uk/~baa/314a.gif OCCULTATION OF GSC 1228 0174 BY 37 (FIDES) Richard Miles provides predictions for two further events: 37 FIDES on September 16/17 (Observable photoelectrically) This 112 km diameter object is predicted to occult the star, GSC 1228 0174 (V=11.6 approx.) located at: RA(2000): 3h 09m 28s Dec(2000) +19deg 22'43" at 22:27-22:55 UT, mid-time (from the UK) = 22:41 UT The maximum duration of the event: about 30 seconds. The star may dip in brightness by only about 0.4 magnitudes. The asteroid should be readily visible at around V=10.9, diameter 0.100". OCCULTATION OF PPM 94351 BY 27 (EUTERPE) 27 EUTERPE on September 17/18 (Observable visually) This 119 km diameter object is predicted to occult the star, PPM 94351 = GSC 1308 1492 = SAO 77160 (V=9.7 approx.) located at: RA(2000): 5h 25m 31s Dec(2000) +21deg 55'07" at 00:15-00:26 UT, mid-time (from the UK) = 00:21 UT The maximum duration of the event: about 6.5 seconds. The star may dip in brightness by about 1.5 magnitudes. The asteroid should be readily visible at around V=11.0, diameter 0.097". Guy M Hurst