Electronic Telegram No. 1882 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) CBAT@CFA.HARVARD.EDU (science) URL http://www.cfa.harvard.edu/iau/cbat.html TRANSIENT FEATURES ON JUPITER J. H. Rogers, Jupiter Section Director, British Astronomical Association, reports on BAA Electronic Bulletin No. 00429 word of the discovery by Anthony Wesley (Murrumbateman, NSW, Australia) of a "virtually black" spot in Jupiter's South Polar Region, very similar in appearance to the impact spots of comet D/1993 F2 in July 1994. Information at the web site http://www.acquerra.com.au/astro/ notes that the discovery was made by Wesley (0.37-m f/5 reflector) on July 19.56 UT and shows an image he obtained (Point Grey Research Dragonfly2 mono camera, 60-s exposure) on July 19.66. Rogers adds that the spot is at longitude 216 deg (System II) and that T. Mishina (Japan) also reported the same spot in an image taken at about the same time. F. Marchis, University of California, Berkeley (UCB), and SETI Institute; and M. H. Wong, Space Telescope Science Institute, report that analysis of observations of Jupiter's atmosphere collected by P. Kalas, M. Fitzgerald and J. Graham (UCB) using the NIRC2 near-infrared camera at the W. M. Keck II telescope during July 20.468-20.474 UT (central meridian longitudes 283-288 deg, System III) revealed the presence of an anomalous bright feature centered at planetographic coordinates 305 +/- 1.5 deg west, 57 +/- 1.5 deg south. This feature is most likely linked to Wesley's dark spot, interpreted to be an impact in the atmosphere of Jupiter. The scar, having an area of about 200 million square km and well seen in the Kp filter centered at 2.124 microns, has a complex shape, composed of an impact site with two prominent features separated by about 2 degrees and an ejecta field that extends some 10 deg toward the west. The scar is marginally detected in observations recorded in H band (centered at 1.633 microns) and in CH4 (centered at 1.681 microns) filters. Further observations during July 20.619-20.627 (central meridian longitudes 54-62 deg) do not show evidence for additional impacts. See also http://cilaos.berkeley.edu/~fmarchis2/Jupiter2009/OurImages/Image_Keck.jpg and http://astro.berkeley.edu/~mikewong/G510/ircolor_annotation.pdf . NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2009 CBAT 2009 July 21 (CBET 1882) Brian G. Marsden