• Observation data: C/2001 A2-b(LINEAR), P/2001 Q6(NEAT), C/2000 WM1(LINEAR), P/2001 Q2(Petriew), P/2001 T3(NEAT) P/2001 Q2(Petriew)has become too faint for the 20cm refractor. C/2000 WM1 (LINEAR) now took over and is increasing its brightness and size day by day. It is predicted to become bright enough for binoculars late in November. Photographs of this comet will be presented in the next Comet Bulletin and on my web site. C/2001 A2-b(Linear) R.A (2000) decl. m1 Aug. 23.59358 20 07 53.77 +19 50 31.2 13.0 372 26.64236 20 05 39.77 +19 26 09.2 13.7 372 26.67378 20 05 38.57 +19 25 51.0 372 P/2001 Q6(NEAT) R.A (2000) decl. m1 Oct. 12.67118 3 17 53.16 +62 29 16.2 14.4 372 13.75347 3 13 12.07 +64 11 23.2 14.9 372 24.68899 1 14 06.49 +78 31 16.4 14.3 372 29.76337 22 54 09.6 +80 59 35.9 372 C/2000 WM1(Linear) R.A (2000) decl. m1 Oct. 18.71111 4 53 37.24 +50 59 33.0 13.5 372 29.77118 4 36 56.74 +49 45 07.7 11.4 372 P/2001 Q2(Petriew) R.A (2000) decl. m1 Oct. 18.84132 9 26 28.98 + 2 57 26.2 13.5 372 29.79098 9 49 39.30 - 0 43 36.1 15.0 372 P/2001 T3(NEAT) R.A (2000) decl. m1 Oct. 23.64375 1 38 05.45 - 7 58 09.4 16.7 372 24.63299 1 37 18.70 - 7 53 59.1 16.5 372 T.Seki |
Copyright (C) 2001 Tsutomu Seki.