Electronic Telegram No. 4225 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/2015 X8 (NEOWISE) [Editor's note: This text replaces that on CBET 4224 (discovery details).] On Dec. 18, J. Bauer reported to the Minor Planet Center astrometry measured from images of an unknown extended object that was found on infrared images taken with the Near-Earth Object Wide-field Infrared Survey Explorer (or NEOWISE; formerly the WISE earth-orbiting satellite; cf. IAUC 9118). The truncated satellite-centered discovery astrometry is tabulated below, with the listed optical-wavelength magnitude having been roughly estimated based on past NEOWISE cometary observations. 2015 UT R.A. (2000) Decl. Mag. Dec. 14.63534 12 29 57 +32 42.8 16 14.76637 12 29 45 +32 53.7 14.83195 12 29 39 +32 59.2 14.96311 12 29 27 +33 10.2 15.09427 12 29 15 +33 21.3 After the object was posted on the Minor Planet Center's PCCP webpage, ground-based CCD astrometrists have confirmed the cometary appearance. H. Sato, Tokyo, Japan, writes that eleven stacked 20-s exposures taken with an iTelescope 0.43-m f/6.8 astrograph (+ luminance filter) at Nerpio, Spain, on Dec. 18.2 UT show the object to be strongly consensed with a round outer coma 25" in diameter and no tail; the w-band magnitude was 15.9 as measured within a circular aperture of radius 12".6. Ten stacked 60-s CCD images taken by C. Jacques, E. Pimentel, and J. Barros with an iTelescope 0.61-m f/6.5 reflector at the Sierra Remote Observatory near Auberry, CA, USA, on Dec. 18.5 show a strong central condensation 51" in diameter surrounded by a diffuse coma that was measured to be 2'11" in diameter, with red magnitude 17.2-17.4. A. Hale, Cloudcroft, NM, USA, reports that he followed the comet visually for about an hour with a 0.41-m reflector; he notes that the comet was very vague and diffuse with just the very slightest central brightening and without condensation, and he measured total visual magnitude 12.8 with coma diameter 2'.4 on Dec. 18.49. The available astrometry (spanning Dec. 14-18), the following preliminary parabolic orbital elements by G. V. Williams, and an ephemeris appear on MPEC 2015-Y20. T = 2015 Oct. 25.5236 TT Peri. = 22.2043 Node = 190.7933 2000.0 q = 1.211900 AU Incl. = 155.0360 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 December 19 (CBET 4225) Daniel W. E. Green