Electronic Telegram No. 4382 Central Bureau for Astronomical Telegrams Mailing address: Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network COMET P/2017 G1 (PANSTARRS) R. Weryk and E. Lilly, Institute for Astronomy, University of Hawaii, report the discovery of a diffuse comet on images obtained on Apr. 1.5 UT with the 1.8-m Pan-STARRS1 telescope at Haleakala (discovery observations tabulated below, together with prediscovery Pan-STARRS1 images from Mar. 25). There is a possible tail extending about 5" towards the northeast. 2017 UT R.A. (2000) Decl. Mag. Mar. 25.42796 12 46 15.60 - 9 48 50.2 21.4 25.44006 12 46 15.14 - 9 48 47.5 22.0 25.45218 12 46 14.68 - 9 48 44.6 22.7 25.46431 12 46 14.27 - 9 48 41.3 21.5 Apr. 1.45654 12 42 06.85 - 9 20 44.2 22.0 1.46683 12 42 06.52 - 9 20 41.6 21.8 1.47712 12 42 06.13 - 9 20 39.1 21.8 M. Micheli and R. J. Wainscoat report that three 60-s gri-filtered confirming exposures of the comet were obtained by Wainscoat and D. Woodworth on Apr. 2.3 UT with the 3.6-m Canada-France-Hawaii Telescope at Mauna Kea, which show a diffuse appearance and a tail-like extension to the east. The available astrometry, the following preliminary elliptical orbital elements by G. V. Williams (from 22 observations spanning Mar. 25-Apr. 5), and an ephemeris appear on MPEC 2017-G56. Epoch = 2016 May 12.0 TT T = 2016 May 11.9592 TT Peri. = 218.1586 e = 0.659817 Node = 259.3968 2000.0 q = 2.619693 AU Incl. = 3.5387 a = 7.700839 AU n = 0.0461208 P = 21.37 years NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2017 CBAT 2017 April 6 (CBET 4382) Daniel W. E. Green