Electronic Telegram No. 4392 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 K1 (PANSTARRS) R. J. Wainscoat reports the discovery of an apparent comet on four 45-s w-band exposures taken with the 1.8-m Pan-STARRS1 telescope at Haleakala (discovery images tabulated below), the object appearing clearly soft compared to nearby stars (FWHM 2".0, vs. 1".0 for the stars) with no evidence of a tail. 2017 UT R.A. (2000) Decl. Mag. May 21.40011 15 45 41.77 -28 17 47.7 20.3 21.41065 15 45 41.17 -28 17 44.8 20.4 21.42120 15 45 40.58 -28 17 41.6 20.4 21.43174 15 45 39.97 -28 17 38.6 20.3 A series of nine 60-s w-band follow-up exposures taken by Wainscoat and D. Woodworth with the 3.6-m Canada-France-Hawaii Telescope at Mauna Kea on May 23.47 UT show that the comet appears to be extended in each image (FWHM approximately 1".7, compared approximately 0".9 for nearby stars; measured by M. Micheli and Wainscoat), the G-band magnitude given as 19.8. After posting on the Minor Planet Center's PCCP webpage, H. Sato (Tokyo, Japan) stacked ten 60-s exposures taken on May 22.6 with an iTelescope 0.51-m f/6.8 astrograph at Siding Spring to find a strongly condensed coma of size 6" x 8" but no tail; the w-band magnitude was 19.2 as measured within a circular aperture of radius 4".9. The available astrometry, the following very preliminary parabolic orbital elements by G. V. Williams (from 17 observations spanning May 21-23), and an ephemeris appear on MPEC 2017-K34. T = 2018 Oct. 25.7764 TT Peri. = 23.8005 Node = 226.2144 2000.0 q = 6.574998 AU Incl. = 153.1715 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2017 CBAT 2017 May 24 (CBET 4392) Daniel W. E. Green