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Circular No. 9070
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Mailstop 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 ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)
COMET C/2009 Q5 (McNAUGHT)
R. H. McNaught reports his discovery of a comet with a
circular 18" coma on CCD images obtained with the 0.5-m Uppsala
Schmidt telescope (discovery tabulated below); five stacked 30-s
images obtained after moonset on Aug. 31.7-31.8 UT show a 0'.4 coma
and a 50" tail in p.a. 285 deg. After posting on the Minor Planet
Center's 'NEOCP' webpage, other CCD astrometrists have noted the
object's cometary appearance. S. Foglia reports that fifteen
stacked 60-s CCD images taken by R. Holmes (Charleston, IL, U.S.A.,
0.61-m telescope) reveal a round coma of diameter 10" with a 30"
tail in p.a. 260 deg. Fifteen stacked 120-s unfiltered exposures
taken remotely on Sept. 1.3 by E. Guido and G. Sostero with a
0.25-m reflector near Mayhill, NM, U.S.A., show a compact coma of
diameter about 12" and a broad tail nearly 20" long in p.a. 255
deg. H. Sato (Tokyo, Japan, remotely using a Rent-A-Scope 0.25-m
reflector near Mayhill on Sept. 1.35) finds a diffuse coma of
diameter 8"-20" and no tail. Frames taken by R. Miles with the
Haleakala 2.0-m 'Faulkes Telescope North' on Sept. 1.6 show a
diffuse 15" coma elongated toward p.a. 285 deg.
2009 UT R.A. (2000) Decl. Mag. Observer
Aug. 31.63470 1 29 04.36 -17 26 52.9 17.0 McNaught
The available astrometry, the following preliminary parabolic
orbital elements, and an ephemeris appear on MPEC 2009-R02.
T = 2010 Mar. 11.218 TT Peri. = 293.151
Node = 160.070 2000.0
q = 1.55732 AU Incl. = 40.823
COMETS C/2009 D7 AND C/2009 D8 (SOHO)
Further to IAUC 9059, additional presumed comets have been
found on SOHO website images. C/2009 D7 was bright (mag about 4)
with a short tail in LASCO C3 images, while it showed a short tail
and faded quickly in C2 images; this comet was also detected in
STEREO COR2-A and COR2-B images with a tail about 0.3 deg long.
C/2009 D8 was slightly elongated, small, and stellar in apperance
(mag about 7, but it faded rapidly).
Comet 2009 UT R.A.(2000)Decl. Inst. F MPEC
C/2009 D7 Feb. 26.029 23 09.7 -10 31 C3/2* MU 2009-N01
C/2009 D8 26.129 22 42.2 - 7 03 C2 BZ 2009-N01
(C) Copyright 2009 CBAT
2009 September 1 (9070) Daniel W. E. Green
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