------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 3002 2014 May 17 08.52UT 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 Backup: gmh@wdcc1.bnsc.rl.ac.uk WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- POSSIBLE NEW METEOR SHOWER FROM COMET 209P/LINEAR Editor: For those who attended the recent 50th anniversary meeting of 'The Astronomer' in Basingstoke you will be aware that a presentation of slides by Robert McNaught was kindly given on his behalf by Tony Markham (see TA WWW 'latest news' and link to Powerpoint file). This related to a possibility of a new meteor shower linked to Comet 209/LINEAR which might appear for observers in the USA on May 24. Subsequently the Central Bureau have issued the following notice: P. Jenniskens, SETI Institute et. al. report that a new meteor shower may be visible for observers in the United States and southern parts of Canada between 2014 May 24d 06h03m and 8h09mUT, with peak activity most likely between 6h33m and 7h49m UT. The new shower is anticipated because the orbit of the Jupiter-family comet 209P/LINEAR (period 5.03 years) has gradually moved closer to the earth's orbit, and the earth will have an exceptionally close encounter with the comet itself in late May at a minimum distance of 0.0554AU. Moreover, the earth will pass the comet's orbit near perihelion, where most past dust ejecta are concentrated in a relatively small region of space. Whether or not a meteor shower will be visible depends on the unknown past activity of this now-weakly-active comet, long before it was first detected in 2004. If the shower manifests itself, then meteors will radiate from R.A. = 125 deg, Decl. = +78 deg (equinox 2000.0), in the constellation Camelopardalis and will have a slow apparent entry speed of 19.4 km/s. A summary of more-recent prediction modelling and a tool to calculate the best local times for viewing this event can be seen at URL http://meteor.seti.org. Editor: We would welcome reports from our subscribers in USA and Canada. SUPERNOVA 2014Y (TNTS) 2014Y Mar 2.59 07 23 33.39 +54 26 30.2 18.3 1.7"W 3.2"N J.-J. Zhang: spectrum Mar 7 type-IIn a few weeks after maximum and closely matching SN 1996L at + 58 days. SUPERNOVA 2014Z IN ESO 114-G4 (PARKER) 2014Z Mar 6.39 01 44 07.99 -61 07 07.4 15.2r 6 "E 16 "N An image of the new variable can be viewed via website URL http://tinyurl.com/lrn4773 Y. Cao: near-infrared spectrum Mar 8 type-Ia near maximum. SUPERNOVA 2014ab (CATALINA REAL-TIME SURVEY) 2014ab Mar 9.43 13 48 05.99 + 7 23 16.4 16.4 1.5"N E. Y. Hsiao: near-infrared spectrum Mar 10 type-IIn a month past maximum Guy M Hurst reports V photometry with the Bradford Robotic telescope on 2014 April 4 at magnitude 16.8. SUPERNOVA 2014ac IN NGC 5837 (LEONINI ET. AL.) 2014ac Mar 9.99 15 04 40.09 +12 37 54.0 16.6 8 "W 10 "S L. Tomasella: noisy spectrum Mar 10 type-Ia a few days after maximum Guy M Hurst