Electronic Telegram No. 4381 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 C/2017 F2 (PANSTARRS) E. Lilly and R. Weryk, Institute for Astronomy, University of Hawaii, report the discovery of another comet on images obtained with the 1.8-m Pan-STARRS1 telescope at Haleakala (discovery observations tabulated below). The object has a soft appearance, with full-width-at-half-maximum of approximately 1".7, compared to adjacent stars that had FWHM = 1".4; there is some evidence for a very faint tail extending for a few arcseconds to the southwest. 2017 UT R.A. (2000) Decl. Mag. Mar. 31.40889 12 01 22.22 +46 20 42.9 21.2 31.42334 12 01 21.75 +46 20 40.9 21.6 31.43782 12 01 21.32 +46 20 38.9 21.0 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. 1.26 UT with the 3.6-m Canada-France-Hawaii Telescope at Mauna Kea, which show clear cometary activity with a broad tail to the west. After the comet was posted on the Minor Planet Center's PCCP webpage, R. S. McMillan found the comet to be more diffuse than surrounding stars with a coma extending westward on CCD images obtained in 1".8 seeing at Kitt Peak on Apr. 6.45 and 6.46 with the Spacewatch 1.8-m f/2.7 reflector (+ Schott OG-515 filter; bandpass 515-950 nm); the red magnitude was measured to be 19.9-20.0. The available astrometry, the following preliminary elliptical orbital elements by G. V. Williams (from 24 observations spanning Mar. 31-Apr. 6), and an ephemeris appear on MPEC 2017-G56. Epoch = 2017 Oct. 14.0 TT T = 2017 Oct. 6.5682 TT Peri. = 130.9563 e = 0.970816 Node = 38.3701 2000.0 q = 7.029649 AU Incl. = 42.6234 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars.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 4381) Daniel W. E. Green