Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 8933: C/2008 B1-B4, C/2008 C3-C5,, C/2008 E4; C/2008 E1

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 8932  SEARCH Read IAUC 8934

View IAUC 8933 in .dvi, .ps or .PDF format.
IAUC number


                                                  Circular No. 8933
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)


COMETS C/2008 B1-B4, C/2008 C3-C5, AND C/2008 E4 (SOHO)
     Further to IAUC 8932, additional apparent comets have been
found on SOHO website images; all are Kreutz sungrazers except for
C/2008 C3 (no known group) and C/2008 E4 (Kracht group).  In the
tabulated column below for instrument, an asterisk (*) indicates
that astrometry was also measured and reduced from HI1 images
aboard the STEREO-A spacecraft.  C/2008 B1 was tiny, stellar, and
faint (mag about 7).  C/2008 B2 reached mag about 6 in H1A and C3
images and was just barely visible with a thin, faint tail in C2
images.  C/2008 B3, C/2008 B4, and C/2008 C4 were very faint (mag
7.5), the first and third being slightly diffuse and the second
being quite diffuse.  C/2008 C3 was stellar in appearance and
brightened slowly and gradually, reaching mag about 7 as it left
the field-of-view.  C/2008 C5 was also stellar in appearance,
reaching mag about 6.5.
     C/2008 E4 is described by K. Battams as "typically [for a
Kracht-group object] small, stellar, and faint (maybe peaking at
mag 7 as it entered the C2 coronagraph), fading fast as it neared
the sun".  R. Kracht suggested the identity of the Kracht group
comets C/2002 Q8 and C/2008 E4 on the basis of the MPEC 2002-Q46
measurements of the former and his own measurements of the latter;
Kracht gave the previous perihelion date T = 1997 Feb. 14.9 but was
unable to locate the comet on C2 images from that time.  Linked
orbital elements (P = 5.52 yr) for 2002 and 2008 by B. G. Marsden
appear on MPEC 2008-F32.

 Comet        2008 UT       R.A.(2000)Decl.   Inst.  F    MPEC
 C/2008 B1    Jan. 26.221   20 46.1  -21 03   C3     HS   2008-G59
 C/2008 B2         27.138   21 00.0  -21 43   C3/2*  AK   2008-G59
 C/2008 B3         28.696   20 57.9  -19 43   C3     HS   2008-G59
 C/2008 B4         29.904   21 03.8  -19 33   C3     BZ   2008-G59
 C/2008 C3    Feb.  3.146   21 02.9  -18 12   C2     RK   2008-G60
 C/2008 C4          3.821   21 22.3  -18 16   C3*    HS   2008-G60
 C/2008 C5          5.738   21 33.9  -17 30   C3*    AK   2008-G60
 C/2008 E4    Mar.  3.254   23 02.6  - 5 18   C2     HS   2008-F32


COMET C/2008 E1 (CATALINA)
     Prediscovery astrometry (MPEC 2008-F36) shows this comet (IAUC
8923) to be of intermediate period; elements from MPEC 2008-G33:
epoch 2008 Aug. 2.0 TT, T = 2008 Aug. 11.284 TT, q = 4.82971 AU, e
= 0.54759, Peri. = 269.910 deg, Node. = 189.035 deg, i = 35.038 deg
(equinox 2000.0), P = 34.9 years.

                      (C) Copyright 2008 CBAT
2008 April 10                  (8933)            Daniel W. E. Green

Read IAUC 8932  SEARCH Read IAUC 8934

View IAUC 8933 in .dvi, .ps or .PDF format.


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


Valid HTML 4.01!