[Iaude] CBET 4823: COMET P/2020 O3
quai at eps.harvard.edu
quai at eps.harvard.edu
Sun Aug 2 19:24:16 EDT 2020
Electronic Telegram No. 4823
Central Bureau for Astronomical Telegrams
Mailing address: Hoffman Lab 209; Harvard University;
20 Oxford St.; Cambridge, MA 02138; U.S.A.
e-mail: cbatiau at eps.harvard.edu (alternate cbat at iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network
COMET P/2020 F3 (PANSTARRS)
R. Weryk, Institute for Astronomy, University of Hawaii, reports the
discovery of another diffuse comet in three 45-s w-band images obtained with
the Pan-STARRS1 1.8-m Ritchey-Chretien reflector at Haleakala on July 28;
in seeng of 1".4, the comet's head showed a full-width-at-half-maximum (FWHM)
of about 2", but there was an obvious straight tail at least 12" long towards
p.a. 240 degrees. Weryk also identified four 45-s pre-discovery w-band
images taken on July 20 with the Pan-STARRS2 1.8-m Ritchey-Chretien reflector
at Haleakala, when the image quality was poor and the comet appeared quite
diffuse (the head having FWHM size of about 2".5 in 1".7 seeing) with an
obvious straight tail at least 6" long in p.a. 245 degrees. The discovery
and pre-discovery observations are tabulated below.
2020 UT R.A. (2000) Decl. Mag.
July 20.48026 22 05 20.07 - 2 06 32.3 20.8
20.49182 22 05 19.83 - 2 06 32.0 21.0
20.50337 22 05 19.55 - 2 06 32.0 20.8
20.51495 22 05 19.23 - 2 06 32.1 21.1
28.50525 22 01 53.74 - 2 09 13.4 21.0
28.51861 22 01 53.36 - 2 09 13.9 21.5
28.53189 22 01 52.94 - 2 09 14.8 20.7
28.54516 22 01 52.57 - 2 09 15.2 21.2
Y. Ramanjooloo, Institute for Astronomy, reports that four additional 60-s
Pan-STARRS1 w-band images taken on July 29.5 show an obvious tail at least
7".5 long towards p.a. 270 degrees; the comet's very condensed head had FWHM
size of about 2".2 in 1".1 seeing. Weryk adds that four additional 60-s
Pan-STARRS1 w-band images taken on July 30.5 show a straight tail about 16"
long toward p.a. 240 deg; the comet's condensed head had a FWHM size of 1".6
in 1".2 seeing.
The available astrometry appears on MPEC 2020-P11. The following very
preliminary parabolic orbital elements by S. Nakano are from 26 observations
spanning July 20-31 (mean residual 0".3). A search by Nakano in archival
astrometry produced nothing.
T = 2020 Dec. 22.4944 TT Peri. = 76.7217
e = 0.105548 Node = 266.9403 2000.0
q = 4.177170 AU Incl. = 8.4462
a = 4.670091 AU n = 0.0976599 P = 10.09 years
The following ephemeris by the undersigned from the above orbital elements
uses photometry power-law parameters H = 12.0 and 2.5n = 10 for the
magnitudes.
Date TT R. A. (2000) Decl. Delta r Elong. Phase Mag.
2020 07 10 22 08.70 -02 12.1 3.432 4.201 133.9 10.0 20.9
2020 07 20 22 05.52 -02 06.5 3.335 4.199 143.8 8.2 20.8
2020 07 30 22 01.19 -02 10.4 3.261 4.196 153.8 6.1 20.8
2020 08 09 21 56.01 -02 22.8 3.212 4.193 163.3 4.0 20.8
2020 08 19 21 50.38 -02 42.5 3.191 4.191 169.9 2.4 20.7
2020 08 29 21 44.75 -03 07.7 3.199 4.189 167.0 3.1 20.7
2020 09 08 21 39.60 -03 35.6 3.235 4.187 158.2 5.1 20.8
2020 09 18 21 35.32 -04 03.9 3.298 4.185 148.2 7.3 20.8
2020 09 28 21 32.27 -04 30.1 3.385 4.184 138.0 9.2 20.9
2020 10 08 21 30.65 -04 52.0 3.493 4.182 127.9 10.9 20.9
2020 10 18 21 30.56 -05 08.3 3.618 4.181 118.1 12.1 21.0
2020 10 28 21 32.03 -05 17.8 3.755 4.180 108.6 13.0 21.1
2020 11 07 21 34.98 -05 19.9 3.901 4.179 99.4 13.5 21.2
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2020 CBAT
2020 August 2 (CBET 4823) Daniel W. E. Green
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