IAU Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 7899: C/2000 H6, H7, J8, N4; C/2002 J3 (SOHO); C/2002 J4

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 7898  SEARCH Read IAUC 7900

View IAUC 7899 in .dvi or .ps format.
IAUC number


                                                  Circular No. 7899
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://cfa-www.harvard.edu/iau/cbat.html  ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)


COMETS C/2000 H6, H7, J8, N4; C/2002 J3 (SOHO)
     Further to IAUC 7898, D. Hammer reports his measurements for
additional comets found by R. Kracht (2000 comets; C2 coronagraph)
and by K. Cernis (C/2002 J3; C3) in the SOHO archive.  The reduced
astrometry and orbital elements by B. G. Marsden appear on the
MPECs cited below.  Comets C/2000 H6, C/2000 H7, and C/2002 J3 are
members of the Kreutz group; the other two belong to the Meyer
group (cf. IAUC 7832).

  Comet         2000 UT          R.A. (2000) Decl.       MPEC
  C/2000 H6     Apr. 26.063       2 18.6   +12 14       2002-H49
  C/2000 H7          28.663       2 30.2   +13 11       2002-H49
  C/2000 J8     May   6.226       2 58.0   +17 46       2002-H49
  C/2000 N4     July  4.660       6 55.0   +23 50       2002-J09

  Comet         2002 UT          R.A. (2000) Decl.       MPEC
  C/2002 J3     May  13.446       3 32.7   +14 14       2002-J46


COMET C/2002 J4 (NEAT)
     S. Pravdo, E. Helin, and K. Lawrence, Jet Propulsion
Laboratory, report the discovery by NEAT, on CCD images taken on
May 13.5 UT with the Palomar 1.2-m Schmidt telescope, of a comet
with nebulosity extending about 5" toward the southwest.  Following
posting on the NEO Confirmation Page, additional observations
obtained elsewhere on May 13.9 confirm the cometary nature:  P.
Kusnirak at Ondrejov (0.65-m reflector; m_1 = 18.3, faint 7" coma
slightly elongated to the southwest); M. Tichy and M. Kocer at Klet
(1.06-m KLENOT telescope; compact coma of diameter 16"); and L.
Kornos at Modra (0.6-m reflector; m_1 = 16.6, coma diameter about
15").  Additional observations made by LONEOS and LINEAR on May 4,
7, and 8 were then identified by the Minor Planet Center staff.

     2002 UT             R.A. (2000) Decl.        m1
     May  13.45406   15 49 37.19   + 0 26 39.8   18.0

Astrometry and the following preliminary parabolic orbital elements
appear on MPEC 2002-J47:

                      (C) Copyright 2002 CBAT
2002 May 13                    (7899)            Daniel W. E. Green

Read IAUC 7898  SEARCH Read IAUC 7900

View IAUC 7899 in .dvi or .ps format.


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


Valid HTML 4.01!