[Iaude] CBET 4779: COMET C/2020 K1
quai at eps.harvard.edu
quai at eps.harvard.edu
Thu May 21 21:00:19 EDT 2020
Electronic Telegram No. 4779
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 C/2020 K1 (PANSTARRS)
R. Weryk, Institute for Astronomy, University of Hawaii, reports the
discovery of another comet in CCD images obtained with the Pan-STARRS2 1.8-m
Ritchey-Chretien reflector at Haleakala on May 17, with additional
pre-discovery observations made with the same telescope that werre then
identified during the previous month (all astrometry tabulated below).
>From four 45-s w-band exposures taken on Apr. 17, Weryk noted a condensed
coma of diameter 0".5 (full-width-at-half-maximum of 2".5 in 2".0 seeing)
with no tail. Similar exposurs on Apr. 27 showed a 0".9 condensed coma (FWHM
2".6 in 1".7 seeing) and no tail. Four 45-s i-band exposures taken on May 6
show a condensed 0".6 coma (FWHM 1".9 in 1".3 seeing) with no tail. Four
45-s w-band discovery observations on May 17 show a condensed 0".7 coma
(FWHM 2".1 in 1".5 seeing) with no tail.
2020 UT R.A. (2000) Decl. Mag.
Apr. 17.55119 18 42 42.44 +56 19 12.6 20.4
17.56480 18 42 42.28 +56 19 16.2 20.5
17.57844 18 42 42.09 +56 19 19.7 20.1
17.59207 18 42 41.93 +56 19 23.0 20.2
27.55593 18 40 02.57 +56 59 54.5 20.2
27.56963 18 40 02.28 +56 59 57.7 20.1
27.58329 18 40 02.03 +57 00 01.1 20.1
27.59699 18 40 01.73 +57 00 04.1 20.3
May 6.51833 18 36 32.64 +57 32 32.0 20.0
6.53143 18 36 32.26 +57 32 34.7 21.0
6.54453 18 36 31.87 +57 32 37.4 20.3
6.55761 18 36 31.53 +57 32 39.8 20.3
17.51229 18 30 53.00 +58 05 26.4 20.6
17.52592 18 30 52.52 +58 05 28.5 20.4
17.53956 18 30 52.03 +58 05 30.6 20.1
17.55319 18 30 51.56 +58 05 32.8 20.4
Weryk and R. Wainscoat obtained three 60-s gri-band follow-up observations on
May 19.60 UT with the 3.6-m Canada-France-Hawaii Telescope at Mauna Kea
(observers Wainscoat, C. Crowder, and T. Burdullis) that show the object to
be clearly a comet (size FWHM 1".45 in 0".65 seeing) of mag 20.1-20.2; the
comet appears slightly asymmetric, indicating a short tail with a length of
at most about 2" towards the northeast.
After the comet was posted on the Minor Planet Center's PCCP webpage,
A. Aletti and L. Buzzi report that stacks of 30-s CCD exposures taken on May
19.94-20.06 with a 0.36-m f/6 Schmidt-Cassegrain reflector at Varese, Italy,
show a 5" coma with no elongation or tail visible; they measured the red
magnitude as 19.8.
The available astrometry appear on MPEC 2020-K111. The following
preliminary parabolic orbital elements by S. Nakano, Sumoto, Japan, are from
76 observations spanning Apr. 17-May 21 (mean residual 0".3).
T = 2023 May 8.6839 TT Peri. = 213.8786
Node = 94.4049 2000.0
q = 3.078872 AU Incl. = 89.6421
The following ephemeris by the undersigned, from the above orbital elements,
uses photometric power-law parameters H = 7.0 and 2.5n = 8 for the magnitudes.
Date TT R. A. (2000) Decl. Delta r Elong. Phase Mag.
2020 03 12 18 41.83 +53 42.6 10.010 9.922 82.1 5.7 20.0
2020 03 22 18 43.60 +54 23.9 9.912 9.858 84.0 5.8 19.9
2020 04 01 18 44.27 +55 07.2 9.813 9.794 86.0 5.8 19.9
2020 04 11 18 43.74 +55 51.1 9.713 9.729 88.0 5.9 19.8
2020 04 21 18 41.94 +56 33.6 9.613 9.665 90.0 6.0 19.8
2020 05 01 18 38.82 +57 13.0 9.514 9.600 91.9 6.0 19.8
2020 05 11 18 34.41 +57 47.0 9.418 9.535 93.6 6.1 19.7
2020 05 21 18 28.79 +58 13.8 9.326 9.470 95.1 6.1 19.7
2020 05 31 18 22.13 +58 31.5 9.238 9.405 96.4 6.1 19.6
2020 06 10 18 14.68 +58 38.3 9.156 9.340 97.4 6.2 19.6
2020 06 20 18 06.75 +58 33.2 9.079 9.275 98.0 6.2 19.5
2020 06 30 17 58.71 +58 15.2 9.010 9.210 98.2 6.3 19.5
2020 07 10 17 50.95 +57 44.5 8.947 9.144 98.0 6.3 19.4
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2020 CBAT
2020 May 22 (CBET 4779) Daniel W. E. Green
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