------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1374 1999 Jan 09 19.30UT 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 TYC 2904 0849 BY 385 ILMATAR Richard Miles reports: There is a good chance that the following event will be visible from the U.K., Ireland and the Canary Islands: 385 ILMATAR early on Sunday evening, January 10/11 This medium-sized asteroid, some 94 km across, is predicted to occult the star, TYC 2904 0849 (V=9.64) soon after dusk on Sunday evening. Details are as follows: Location of star: RA(2000): 05h 18m 52s Dec(2000) +42deg 24'04" Observational coverage should span 18:17-18:29 UT, with the expected mid-time (from the UK) = 18:22:42 UT Event Rating: Favourable The maximum duration of the event is expected to be about nine seconds. The star may dip in brightness by about 2.2 magnitudes (i.e. by a factor of about 7). Note that seen from the UK, the event takes place at a high altitude above the horizon in the range, 48-54 deg, and an azimuth of about 84 deg. The Moon will not have risen and so will not interfere with observation. Observers equipped with a telescope of at least 0.15-m aperture are encouraged to visually monitor this very close appulse / occultation, using a suitable watch/stopwatch to time a possible occultation (start and finish). The star will not disappear entirely in larger apertures since it will dip in brightness only seven-fold. NOTE that the event is predicted for a convenient time and so observers are encouraged to go out and participate in coverage of this event. Indeed, it would be good if a number of people succeeded in timing an occultation so soon after Hazel McGee's success on January 06. I have observed this asteroid photometrically in the past and found a lightcurve having a large amplitude (about 0.7 mag) indicative of an object having a rather unusual shape. Richard Miles A finder chart is available at: http://www.ast.cam.ac.uk/~baa/385.gif Watch out for any updates in your e-mail shortly before the predicted event. Last-minute astrometry may show that the shadow path has shifted. My current information indicates that the track will nominally pass just west of the UK and Ireland. However, uncertainties in the asteroid position and star position may shift the shadow track so as to cross populated areas. Guy M Hurst