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Reports from Geisei Observatory <September 20, 2001>


• Observation data: C/2000 WM1(LINEAR), C/2001 Q4(NEAT),
P/2001 R1(LONEOS)

In summer time any objects fainter than the 18th magnitude is difficult due to film fogging. C/2001 Q4, which is predicted to be a great comet in four years, is still a microscopic existence on film. The coma is only 5" in diameter without any tail. P/2001 Q2 has become fainter by nearly a whole magnitude since its discovery, but I will continue to observe it by the 20cm refractor. C/2000 WM1, presented here today, is expected to brighten in January.

CK00W01M   2001 08 23.69167 04 25 07.60 +49 42 55.9  14.4 T  372
CK00W01M   2001 08 27.76215 04 29 48.02 +49 54 22.5  14.6 T  372
CK00W01M   2001 09 16.63333 04 49 10.92 +50 44 27.6  13.4 T  372
CK00W01M   2001 09 17.76337 04 50 02.75 +50 46 55.6          372
CK01Q040   2001 09 16.75799 02 40 12.74 -26 58 14.7  18.5 T  372
PK01R010   2001 09 16.53629 21 30 39.02 -26 01 31.1  18.0 T  372

T.Seki



Copyright (C) 2001 Tsutomu Seki.