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M.P.E.C. 2011-Y23 Issued 2011 Dec. 25, 15:35 UT
The Minor Planet Electronic Circulars contain information on unusual
minor planets and routine data on comets. They are published
on behalf of Commission 20 of the International Astronomical Union by the
Minor Planet Center, Smithsonian Astrophysical Observatory,
Cambridge, MA 02138, U.S.A.
Prepared using the Tamkin Foundation Computer Network
MPC@CFA.HARVARD.EDU
URL http://www.minorplanetcenter.net/ ISSN 1523-6714
COMET C/2011 W3 (LOVEJOY)
Observations:
CK11W030 QC2011 12 23.75224 16 59 17.43 -39 26 10.3 rEY023E12
CK11W030 QC2011 12 24.74267 16 58 13.06 -41 45 07.0 rEY023E12
CK11W030 QC2011 12 24.74785 16 58 14.07 -41 45 36.8 rEY023E12
Observer details:
E12 Siding Spring Survey. Observer R. H. McNaught. 0.5-m Uppsala Schmidt
+ CCD.
Orbital elements:
C/2011 W3 (Lovejoy)
Epoch 2011 Dec. 25.0 TT = JDT 2455920.5
T 2011 Dec. 16.01211 TT MPC
q 0.0055561 (2000.0) P Q
z +0.0129748 Peri. 53.62275 +0.18408854 -0.90052085
+/-0.0000477 Node 326.53456 -0.96007510 -0.07885569
e 0.9999279 Incl. 134.40945 +0.21063526 +0.42760259
From 96 observations 2011 Nov. 27-Dec. 24, mean residual 0".9.
Ephemeris:
C/2011 W3 (Lovejoy)
Date TT R. A. (2000) Decl. Delta r Elong. Phase m1 m2
2011 11 25 12 01 21.7 -49 42 24 0.7577 0.8314 55.0 76.7 13.1 16.7
...
2011 12 10 16 39 12.4 -40 31 32 0.7591 0.3583 18.5 119.2 9.4 17.0
...
2011 12 18 17 12 08.3 -27 17 20 0.8673 0.1682 7.5 130.1 6.4 16.5
...
2011 12 24 16 58 59.6 -40 00 23 0.6820 0.4337 21.9 122.1 10.0 17.4
2011 12 25 16 57 58.9 -42 21 48 0.6590 0.4697 24.3 120.3 10.3 17.3
2011 12 26 16 57 11.0 -44 49 07 0.6375 0.5043 26.8 118.5 10.5 17.3
...
2012 01 01 16 57 00.2 -61 51 55 0.5399 0.6920 42.8 105.3 11.6 16.8
...
2012 01 09 21 32 04.6 -88 29 18 0.5009 0.9084 66.5 83.1 12.6 16.2
...
2012 01 24 04 37 52.5 -48 38 38 0.6914 1.2573 95.6 51.2 14.7 16.6
C/2011 W3 remains a difficult target for astrometry, as evidenced by
the poor consistency of the latest observations. McNaught writes: "Star fit
RMS 0.3", but measures are much less reliable than that. The positions are of
the tip of the "spine" which lies pretty much on the front edge of the parabolic
hood. It is rather less well defined than on Dec 23. For this reason I cannot
be sure just how closely I am measuring the same point as on Dec 23."
Gareth V. Williams (C) Copyright 2011 MPC M.P.E.C. 2011-Y23
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