Central Bureau for Astronomical Telegrams

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IAUC 8672: C/2005 W16, W17, X2-X9, Y3-Y6

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IAUC number


                                                  Circular No. 8672
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/2005 W16, W17, X2-X9, Y3-Y6 (SOHO)
     Additional Kreutz sungrazing comets have been found on SOHO
website images (cf. IAUC 8657).  According to K. Battams, C/2005
W16 and C/2005 X5 were small and stellar in appearance in C3 images,
the former reaching mag 7.3 at 10.1 solar radii on Nov. 28.471 UT,
and the latter reaching mag 6.4 at 9.3 solar radii on Dec. 8.846;
in C2 images, C/2005 W16 showed a faint, thin tail that reached a
length of about 9' on Nov. 28.854 at 5.7 solar radii, while C/2005
X5 was fairly diffuse with a very faint tail that reached a length
of about 6' on Dec. 9.083 at 6.7 solar radii.  C/2005 W17, C/2005
X2, and C/2005 X6 were tiny and too faint for photometry; C/2005
W17 was diffuse and the latter two were stellar in appearance.
C/2005 X3 was small and diffuse, reaching mag 7.7 at 6.5 solar
radii on Dec. 4.600.  C/2005 X4 was small, faint, and diffuse,
reaching mag about 8.  C/2005 X7 was tiny and stellar in appearance,
yet persistent (despite reaching mag about 8), curiously surviving
as long as did C/2005 X5.  C/2005 X8 and C/2005 Y5 were extremely
faint -- the former described as tiny, and the latter as small and
diffuse; C/2005 Y6 was a near-identical twin to C/2005 Y5, but
marginally brighter.  C/2005 X9 was small and diffuse, reaching mag
7.7 at 7.3 solar radii on Dec. 12.917.  C/2005 Y3 was small and a
little too diffuse for good photometry in C3 images; in C2 images,
it was also diffuse, reaching mag 6.6 at 7.4 solar radii on Dec.
20.379.  C/2005 Y4 was very faint and diffuse.

 Comet        2005 UT       R.A.(2000)Decl.   Inst.  F    MPEC
 C/2005 W16   Nov. 28.113  16 09.4   -25 06   C3/2   RM   2006-C59
 C/2005 W17        29.704  16 23.1   -23 19   C2     HS   2006-C59
 C/2005 X2    Dec.  3.442  16 40.5   -23 55   C2     HS   2006-C59
 C/2005 X3          4.583  16 45.6   -24 09   C2     HS   2006-C59
 C/2005 X4          6.567  16 54.5   -24 21   C2     KC   2006-C60
 C/2005 X5          8.321  16 59.0   -26 59   C3/2   JR   2006-C60
 C/2005 X6          8.392  17 03.0   -24 37   C2     JR   2006-C60
 C/2005 X7          9.075  17 07.9   -24 46   C2     HS   2006-C60
 C/2005 X8         11.908  17 19.5   -24 58   C2     QY   2006-C61
 C/2005 X9         12.908  17 23.9   -25 03   C2     RM   2006-C61
 C/2005 Y3         19.988  17 57.4   -26 25   C3/2   QY   2006-C61
 C/2005 Y4         20.938  18 01.5   -25 11   C2     SH   2006-C61
 C/2005 Y5         22.354  18 07.5   -25 13   C2     KB   2006-C61
 C/2005 Y6         22.454  18 07.9   -25 10   C2     KB   2006-C61

                      (C) Copyright 2006 CBAT
2006 February 13               (8672)            Daniel W. E. Green

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