News - March 2002
03/29/2002
03/28/2002
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The 415th SOHO comet is a member of the Kreutz group. C/2002 F3 (SOHO)
was detected by M. Meyer.
(MPEC 2002-F61)
03/22/2002
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New Discovery!:
An asteroidal object, discovered by LINEAR
already on Feb. 07, 2002, which received the designation 2002 CW134 has
shown cometary activity as reported by M. Tichy and M. Kocer (Klet) and G. Masi and
F. Mallia (Campo Catino) after placement on the NEO Confirmation Page. The comet
P/2002 CW134 (LINEAR) passed perihelion already on Feb. 28, 2002,
at about 1.8 AU. The period is about 6.8 years. The comet is currently at maximum
brightness with about 15m. This is LINEARs 78th new comet
discovery. (IAUC 7858, MPEC 2002-F49)
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An impressive animation of comet C/2002 C1 (Ikeya-Zhang) has been produced
by M. Karrer. The
650kB animation
shows very fine details and the dynamic behaviour of the tail and is worth the download.
(Comets Mailing List)
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Five additional SOHO comets received orbits and designations. C/1999 P6 (SOHO),
C/1999 P8 (SOHO) and C/1999 P9 (SOHO) are members of the
Marsden group.
C/1999 P7 (SOHO) is a member of the Meyer group.
All four comets were detected by R. Kracht. The Meyer and Marsden groups now consist
of 13 and 10 members, respectively. R. Kracht also suggested that his find of last year,
C/2001 Q7 (SOHO) may be a member of the extended Marsden group. This was
finally confirmed and this group is now called the
Kracht group.
C/2002 F2 (SOHO) was detected by S. Hönig and is a member of the
Kreutz group. SOHO has now
found 414 comets. (MPEC 2002-F43)
03/21/2002
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A first and still preliminary orbit for comet C/2002 F1 (Utsunomiya) shows
a perihelion on Apr. 23, 2002, at about 0.46 AU. The comet might then reach 5m
but it will be close to the sun. In the coming weeks the comet decreases its
elongation and will stay within 35° until June when its brightness will be
fainter than 10m. (IAUC 7855,
MPEC 2002-F39)
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C/2002 E3 (SOHO) is a Kreutz comet detected by X. Leprette. This is SOHOs
409th comet.
(MPEC 2002-F35)
03/20/2002
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New Discovery!:
A new comet has been discovered visually on Mar. 18, 2002, by
Syogo Utsunomiya (Minami Oguni-machi, Aso-gun, Kumamoto-ken, Japan).
Comet 2002 F1 is about 10m. This is Utsunomiyas third comet
discovery. The comet is located in the
morning twilight. Astrometric followup is urgently required. A search ephemeris
can be generated on the
NEO Confirmation Page.
03/18/2002
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There are hints that comet C/2002 C1 (Ikeya-Zhang) may exhibit a so-called
perihelion asymmetry - a phenomenon which is characterised by an unusual lightcurve
with reaching the maximum brightness after the perihelion and not following the
standard model of cometary brightness evolution. This can be caused by active
regions on the surface of the comet which become more and more exposed to direct
sunlight after perihelion leading to an increased activity. J. Bortle has
analysed the presumed 1661 apparition of this comet which was the reason for him
to assume a likely perihelion asymmetry. He estimates that if an asymmetry
occurs then the maximum brightness may be reached at T+10 days (with T =
perihelion) with about 2.0m to T+15 days with about 1.4m.
His analysis of the 1661 apparition will appear in the March issue of
The Astronomer.
(Comets Mailing List)
03/17/2002
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Two further archival SOHO comets, both found by R. Kracht, received orbits and
designations. C/1999 N6 (SOHO) is the seventh clear member of the
Marsden group.
C/1999 N6 (SOHO) is a likely member of the
extended population with almost
the same orbital elements as C/1999 M3, but B. G. Marsden notes that the orbit solution
is not unique. SOHO has now found 408 comets offcially.
(MPEC 2002-F03)
03/13/2002
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A first and preliminary orbit for comet C/2002 E2 (Snyder-Murakami) shows
a perihelion on Feb. 22, 2002, at about 1.5 AU. The comet will remain at 10m
in March moving northward in the morning sky. (IAUC 7852,
MPEC 2002-E43)
03/12/2002
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New Discovery!:
A new comet has been discovered visually by amateurs D. Snyder (Palominas, AZ, USA)
and independently by S. Murakami (Matsunoyama, Niigata, Japan) on Mar 11, 2002. The
comet was estimated at 10.5m visually. The comet 2002 E2 moves
northward. A search ephemeris can be found on the
NEO Confirmation Page.
(IAUC 7850)
03/09/2002
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Another three archival SOHO comets received orbits and designations.
C/1998 A2 (SOHO) and C/1998 A3 (SOHO) are members of the
Marsden group and were found
by R. Kracht. B. Marsden again noted the possibility that these comets could have
orbits which differ from parabolas, making a connection with the daytime Arietid
meteor stream possible, as proposed originally by D. A. J. Seargent. Marsden also
noted the similarity of the longitude and latitude of the direction of the
perihelion with that of comet 96P/Machholz and the Quadrantid meteor stream. The
Marsden group has now six firmly established members.
C/2000 B8 (SOHO) is a member of the Meyer group
and was found by M. Meyer. This group has now 12 established members. SOHO has now
discovered 406 comets officially.
(MPEC 2002-E25)
03/08/2002
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Two SOHO comets received orbits and designations. C/1999 M3 (SOHO) is an archival
non-Kreutz comet found by R. Kracht. Although the comet seems unrelated to others
when looking at the orbital elements alone, it might nevertheless be loosely
connected with the Marsden group.
R. Kracht noted the similarity of the longitude and latitude of the direction of
the perihelion with that of the Marsden group and comet C/2000 O3 (SOHO). There may
exist an extended relationship between the four firm members of the Marsden group and
C/2000 O3 and C/1999 M3.
C/2002 E1 (SOHO) is a member of the
Kreutz group and was found by
S. Hönig. SOHO has now officially discovered 403 comets.
(MPEC 2002-E18)
03/02/2002
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Three archival SOHO comets, all found by R. Kracht, received orbits and designations.
C/1999 K16 (SOHO) and C/1999 L9 (SOHO) are members of the
Meyer group which has now 11
members. C/1999 K17 (SOHO) is a member of the Kreutz group.
SOHO has now officially discovered 401 comets.
(MPEC 2002-E05)
03/01/2002
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Seven archival and one real time SOHO comet received orbits and designations. Comets
C/1997 H4 (SOHO) and C/1997 H5 (SOHO) are members of the
Meyer group and were found by
R. Kracht. Comets C/1998 H5 (SOHO), C/1998 H6 (SOHO) (found by S.
Hönig), C/1999 H8 (SOHO), C/1999 H9 (SOHO), C/1999 J13 (SOHO)
(found by R. Kracht) and C/2002 D1 (SOHO) (found by X. Leprette) are members
of the Kreutz group. SOHO
has now officially discovered 398 comets.
(MPEC 2002-D41,
MPEC 2002-D42),
MPEC 2002-D45)
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J. Shanklin proposed the possible identity of comet C/2002 C1 (Ikeya-Zhang)
with the comet of 877 for which no orbit has been determined. C/2002 C1, which is
very likely the same comet as C/1661 C1 was already observed with the naked eye.
(BAA Comet Section Homepage,
Comets Mailing List)
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Comet 46P/Wirtanen was observed with ESO's VLT at Paranal (Chile). The comet
was almost as far from the sun like it will be in 2011, when the Rosetta spacecraft
will have an encounter with this comet. There is an
ESO Press Release
with more information about the observations and Rosetta.