MPEC 2010-M42 : COMET C/2010 G3 (WISE)
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M.P.E.C. 2010-M42 Issued 2010 June 22, 15:07 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 https://www.minorplanetcenter.org/iau/mpc.html ISSN 1523-6714
COMET C/2010 G3 (WISE)
Observations:
CK10G030 C2010 05 22.97847 17 54 30.87 +57 23 07.1 18.5 N EM042473
CK10G030 C2010 05 22.97986 17 54 30.65 +57 23 08.1 18.5 N EM042473
CK10G030 C2010 06 06.00932 17 22 12.23 +59 26 01.9 EM042204
CK10G030 C2010 06 06.01995 17 22 10.63 +59 26 05.7 18.7 N EM042204
CK10G030 C2010 06 15.21633 16 59 08.92 +60 06 21.1 18.9 N EM042705
CK10G030 C2010 06 15.36926 16 58 45.54 +60 06 44.2 18.8 N EM042H10
CK10G030 C2010 06 15.37583 16 58 44.61 +60 06 45.8 19.2 N EM042H10
CK10G030 C2010 06 15.38242 16 58 43.47 +60 06 46.2 18.9 N EM042H10
CK10G030 C2010 06 15.38899 16 58 42.57 +60 06 47.4 18.7 N EM042H10
CK10G030 C2010 06 15.39558 16 58 41.72 +60 06 47.8 18.6 N EM042H10
CK10G030 C2010 06 15.39997 16 58 40.91 +60 06 48.7 18.7 N EM042H10
CK10G030 C2010 06 16.95775 16 54 45.64 +60 10 14.2 18.4 N EM042J01
CK10G030 C2010 06 16.96350 16 54 44.75 +60 10 15.5 18.5 N EM042J01
CK10G030 C2010 06 16.96924 16 54 43.75 +60 10 16.2 18.9 N EM042J01
CK10G030 C2010 06 18.30998 16 51 21.71 +60 12 28.4 18.6 N EM042H10
CK10G030 C2010 06 18.31596 16 51 20.66 +60 12 29.0 18.6 N EM042H10
CK10G030 C2010 06 18.32200 16 51 19.68 +60 12 29.2 18.4 N EM042H10
CK10G030 C2010 06 18.32792 16 51 18.83 +60 12 28.8 18.6 N EM042H10
CK10G030 C2010 06 18.33432 16 51 17.88 +60 12 30.3 18.1 N EM042H10
Observer details:
204 Schiaparelli Observatory. Observer L. Buzzi. 0.38-m f/6.8 reflector
+ CCD.
473 Remanzacco. Observers L. Donato, V. Gonano, E. Guido, G. Sostero. 0.45-m
f/4.4 Newtonian reflector + CCD.
705 Apache Point. Observer M. Huber. Measurer T. Grav. 0.5-m f/8.5
reflector + CCD.
H10 Tzec Maun Observatory, Mayhill. Observer E. Bryssinck. 0.36-m f/3.8
Maksutov-Newtonian + CCD, 0.41-m f/9 Ritchey-Chretien + CCD.
J01 Observatorio Cielo Profundo, Oviedo. Observer J. Gonzalez. 0.23-m f/10
Schmidt-Cassegrain + CCD.
Orbital elements:
C/2010 G3 (WISE)
Epoch 2010 Mar. 25.0 TT = JDT 2455280.5
T 2010 Apr. 10.86152 TT MPC
q 4.9075889 (2000.0) P Q
z +0.0003878 Peri. 75.16999 -0.04213018 -0.72602749
+/-0.0000577 Node 313.71406 -0.72699851 +0.49351630
e 0.9980969 Incl. 108.26678 +0.68534532 +0.47887967
Residuals in seconds of arc
100414 C51 1.0+ 0.4- 100425 A77 0.0 0.3+ 100604 J01 0.1+ 0.2+
100414 C51 (0.3+ 3.9-) 100425 A77 0.0 0.1+ 100604 J01 0.1+ 0.1+
100414 C51 (1.1+ 5.1-) 100426 118 0.5- 0.9+ 100604 213 0.5+ 0.5+
100414 C51 (1.0+ 3.5-) 100426 118 0.7- 0.5+ 100604 213 0.6+ 0.2+
100414 C51 1.1+ 0.9+ 100426 118 0.4- 0.8+ 100604 213 0.6+ 0.1+
100414 C51 (0.6+ 4.5-) 100426 G96 0.5+ 0.4- 100604 367 0.0 0.2+
100414 C51 1.4- 1.6- 100426 G96 0.0 0.1+ 100604 367 0.0 0.6-
100414 C51 1.9+ 1.0- 100426 G96 0.2- 0.3+ 100604 367 0.5+ 0.2-
100414 C51 0.6+ 1.8- 100426 G96 0.1+ 0.4- 100605 235 0.1+ 0.3-
100414 C51 (1.3+ 4.0-) 100501 349 0.2- 0.6- 100605 235 0.1- 0.4-
100414 C51 0.2+ 0.5- 100501 349 0.7+ 0.3+ 100606 204 0.1- 0.2+
100414 C51 (0.7- 2.9-) 100501 461 0.2- 0.8+ 100606 204 0.3- 0.0
100415 C51 (2.1+ 0.9-) 100501 461 0.1- 0.6+ 100606 A71 0.5- 0.1+
100415 C51 1.3+ 1.4- 100501 461 0.0 0.6+ 100606 A71 0.1- 0.4-
100415 C51 (2.2- 1.8-) 100502 A79 0.3- 0.2+ 100607 118 1.0- 0.6-
100415 C51 1.2+ 0.7- 100502 A79 0.0 0.2- 100607 118 0.5- 0.4-
100415 C51 (1.1+ 2.3-) 100502 A79 0.3+ 0.2- 100607 118 0.5- 0.3+
100415 C51 0.6+ 1.3- 100502 473 0.2+ 0.4- 100609 H15 0.4- 0.1+
100415 C51 (0.4- 2.6-) 100502 A79 0.1- 0.2- 100609 H15 0.3- 0.8-
100415 C51 (0.9- 2.5-) 100502 473 0.2+ 0.1- 100610 703 0.1+ 1.0-
100415 C51 0.1+ 0.4+ 100502 900 0.5+ 0.2+ 100610 703 (2.0+ 2.1-)
100415 C51 0.0 0.1- 100502 900 0.2+ 1.5- 100610 703 0.5+ 1.5-
100415 C51 0.3+ 1.9- 100507 367 0.1+ 0.0 100610 703 0.0 0.1+
100415 C51 0.2- 0.1- 100507 367 1.0+ 0.0 100611 H10 0.3+ 0.8-
100415 C51 (0.1- 2.7-) 100507 367 0.5+ 0.6- 100611 H10 0.4- 0.3+
100415 C51 (1.4+ 2.1-) 100508 691 0.0 0.1- 100611 235 0.6- 0.1+
100416 C51 (0.1+ 2.3-) 100508 691 0.0 0.5+ 100611 160 0.2- 0.8+
100416 C51 0.1- 1.8- 100508 691 0.1+ 0.1+ 100611 160 0.6- 0.4+
100416 H01 0.5- 0.4+ 100514 900 0.1+ 0.6+ 100611 235 0.0 0.5+
100416 H01 0.4- 0.6+ 100514 900 0.1+ 0.7+ 100611 160 0.9- 0.1+
100416 H01 0.1- 0.8+ 100516 J24 (0.9+ 2.5-) 100611 585 0.8+ 0.3-
100416 H01 0.4- 0.8+ 100516 J24 (2.0+ 2.1-) 100611 585 0.1+ 0.2+
100416 H01 0.3- 0.8+ 100516 J24 (1.8+ 2.1-) 100611 585 1.3- 1.3+
100417 372 0.2+ 0.9+ 100518 B90 0.6- 1.1- 100613 703 0.7+ 1.4-
100417 900 1.4- 1.0+ 100518 B90 0.3- 1.6- 100613 703 (2.6+ 2.2-)
100417 372 0.3- 1.0+ 100518 B90 (0.6+ 2.6-) 100613 703 0.2+ 0.4+
100417 372 0.4- 0.9+ 100519 213 0.1- 0.3+ 100613 703 1.3+ 1.0-
100417 900 1.0- 0.3- 100519 213 0.1- 0.2+ 100615 705 0.0 0.0
100418 215 0.2- 0.2+ 100519 213 0.1+ 0.2- 100615 H10 0.3- 0.1-
100418 215 0.3- 0.7+ 100520 703 0.3- 1.1- 100615 H10 0.2+ 0.6+
100418 215 0.4- 0.6+ 100520 703 0.1- 0.3+ 100615 H10 0.8- 0.0
100420 372 0.2- 0.3+ 100520 703 0.8+ 1.3- 100615 H10 0.1- 0.3+
100420 372 0.2+ 0.2+ 100520 703 0.8+ 1.5- 100615 H10 1.1+ 0.3-
100421 204 0.0 1.0+ 100522 473 0.2+ 0.0 100615 H10 0.0 0.0
100421 204 0.3- 0.4+ 100522 473 0.1- 0.1+ 100616 J01 0.6+ 0.3-
100421 H06 0.1+ 0.4- 100522 B33 0.5+ 0.2+ 100616 J01 0.5+ 0.3+
100421 H06 0.2+ 0.6- 100522 B33 0.2+ 0.1- 100616 J01 0.5- 0.4+
100421 H06 0.5+ 0.6- 100522 B33 0.1- 0.2- 100618 H10 0.8+ 0.6+
100423 585 0.5- 0.1- 100524 461 0.3- 0.3+ 100618 H10 0.3- 0.7+
100423 585 0.8- 0.1+ 100524 461 0.1- 0.5+ 100618 H10 0.8- 0.5+
100423 585 1.3- 1.3+ 100525 B49 0.9+ 1.1+ 100618 H10 0.4- 0.4-
100423 372 (0.3- 2.4+) 100525 B49 0.3- 1.2+ 100618 H10 0.3- 0.6+
100423 372 1.4- 0.9+ 100525 B49 0.9+ 0.3-
100425 A77 0.3- 0.1- 100603 J01 0.0 0.0
The "original" and "future" barycentric values of 1/a are +0.000613
and +0.000922 (+/- 0.000058) AU^-1, respectively.
Brian G. Marsden (C) Copyright 2010 MPC M.P.E.C. 2010-M42
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