Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 9157: P/2010 N1; C/2010 E6; P/2010 J5

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 9156  SEARCH Read IAUC 9158

View IAUC 9157 in .dvi, .ps or .PDF format.
IAUC number


                                                  Circular No. 9157
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
CBAT Director:  D. W. E. Green, Room 209; Department of
 Earth and Planetary Sciences; Harvard University;
 20 Oxford St.; Cambridge, MA  02138; U.S.A.
CBAT@IAU.ORG; CBATIAU@EPS.HARVARD.EDU
URL http://www.cfa.harvard.edu/iau/cbat.html  ISSN 0081-0304


COMET P/2010 N1 (WISE)
     Amy Mainzer, Jet Propulsion Laboratory, reports the discovery
of a comet (discovery observation tabulated below) with a bright
nuclear condensation of diameter about 30" and a tail about 60"
long toward the southeast in WISE spacecraft images; at 12 microns,
the nuclear condensation appears to be about twice as bright as
P/2009 WJ_50 (cf. IAUC 9117) was on Feb. 6 (which was presumably
around mag 20-22 from ground-based CCD imaging in Feb.).  After
posting on the Minor Planet Center's 'NEOCP' webpage, D. Tholen
(University of Hawaii) reports that a stack of six 20-s exposures
made by queue observer J. Luthe with the 3.6-m Canada-France-Hawaii
Telescope on July 10.3 UT shows a tail extending at least 10"
(maybe as much as 15") from an asymmetric head (mag 19.4-19.7) in
p.a. 110-115 deg.

     2010 UT             R.A. (2000) Decl.       Observer
     July  5.47876   13 32 07.62   + 6 26 19.2   WISE

The available astrometry (including pre-discovery observations at
Catalina back to Apr. 13), the following preliminary elliptical
orbital elements, and an ephemeris appear on MPEC 2010-N48.

                    Epoch = 2010 Sept. 1.0 TT
     T = 2010 Aug. 16.1532 TT         Peri. = 153.4966
     e = 0.533831                     Node  = 113.2100  2000.0
     q = 1.494519 AU                  Incl. =  12.8765
       a =  3.205958 AU    n = 0.1716988    P =   5.740 years


COMET C/2010 E6 (STEREO)
     Further to IAUC 9151, K. Battams (Naval Research Laboratory)
adds that this was one of the brightest comets seen in coronagraph
spacecraft data, peaking around magnitude 1 near Mar. 12.625 UT.


COMET P/2010 J5 (McNAUGHT)
     This comet (cf. IAUC 9148) has been shown to be of short
period; below are orbital elements from MPEC 2010-N30:

                    Epoch = 2009 Nov. 25.0 TT
     T = 2009 Nov.  6.4523 TT         Peri. = 150.3572
     e = 0.087808                     Node  =  65.6664  2000.0
     q = 3.748744 AU                  Incl. =   7.3540
       a =  4.109601 AU    n = 0.1183054    P =   8.33 years

                      (C) Copyright 2010 CBAT
2010 July 10                   (9157)            Daniel W. E. Green

Read IAUC 9156  SEARCH Read IAUC 9158

View IAUC 9157 in .dvi, .ps or .PDF format.


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


Valid HTML 4.01!