Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 9058: C/2009 O3; C/2008 Y18

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 9057  SEARCH Read IAUC 9059

View IAUC 9058 in .dvi, .ps or .PDF format.
IAUC number


                                                  Circular No. 9058
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 O3 (HILL)
     R. E. Hill reports his discovery of a comet with the Catalina
0.68-m Schmidt telescope (discovery observation tabulated below),
noting that co-added 30-s exposures show a nuclear condensation
elongated northeast-southwest and a 6" x 10" coma with a broad,
diffuse tail about 2' long in p.a. 260 deg (though on July 30.4 UT,
the coma < 2").  After posting on the 'NEOCP' webpage, other CCD
astrometrists have noted the cometary appearance.  Below are given
measured coma diameters and tail information from images obtained
July 30.0-30.5:  10" coma (diffuse with central condensation), 30"
tail in p.a. 250 deg (P. Birtwhistle, Great Shefford, Berkshire,
England, 0.40-m reflector); strong central condensation with a tail
at least 40" long in p.a. 255 deg (L. Buzzi, Varese, Italy, 0.60-m
reflector); tail > 1' long toward p.a. 245 deg (E. Prosperi,
Larciano, Italy, 0.35-m reflector; fifty co-added 30-s exposures
taken by P. Camilleri, E. Guido, G. Sostero, and himself); compact
nuclear condensation and a broad, diffuse tail 27".7 long in p.a.
247.5 deg (R. Holmes and H. Devore, Charleston, IL, U.S.A., 0.61-m
astrograph); about 5" compact coma and a 30" tail in p.a. 225 deg
(E. Guido and G. Sostero, remotely using a 0.25-m reflector near
Mayhill, NM, U.S.A.; six co-added unfiltered 120-s exposures);
round 10" coma (J. E. McGaha, Tucson, AZ, U.S.A., 0.36-m reflector;
five stacked 60-s exposures); faint tail in p.a. about 225 deg (W.
H. Ryan, Magdalena Ridge 2.4-m reflector).

     2009 UT             R.A. (2000) Decl.       Mag.   Observer
     July 29.43294    1 31 27.03   +10 16 52.4   17.5   Hill

The available astrometry, the following preliminary parabolic
orbital elements by B. G. Marsden, and an ephemeris appear on MPEC
2009-O54.

     T = 2009 Apr. 21.770 TT          Peri. = 130.389
                                      Node  = 180.985   2000.0
     q = 1.88365 AU                   Incl. =  12.750


COMET C/2008 Y18 (SOHO)
     Further to IAUC 9042, another Kreutz sungrazer has been found
on SOHO website images, being extremely faint (mag about 8.5-9) and
slightly diffuse in C2 images, and diffuse (mag about 11.5) in
STEREO HI1-A images.

 Comet        2008 UT       R.A.(2000)Decl.   Inst.  F    MPEC
 C/2008 Y18   Dec. 25.829   18 24.5  -24 47   C2*    MK   2009-M41

                      (C) Copyright 2009 CBAT
2009 July 30                   (9058)            Daniel W. E. Green

Read IAUC 9057  SEARCH Read IAUC 9059

View IAUC 9058 in .dvi, .ps or .PDF format.


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!