[Iaude] CBET 5329: COMET P/2023 Y2

quai at eps.harvard.edu quai at eps.harvard.edu
Sat Jan 13 18:09:00 EST 2024


                                                  Electronic Telegram No. 5329
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/2023 Y2 (GIBBS)
     Alexander R. Gibbs reports his discovery of a comet on CCD images
obtained on 2023 Dec. 17 with the Mt. Lemmon Survey's 1.5-m reflector in great
seeing conditions (astrometry tabulated below).  The comet showed a condensed
coma of size 5' with a slightly fanned and curved tail 40" long in p.a. 295
degrees.

     2023 UT             R.A. (2000) Decl.       Mag.   Observer
     Dec. 17.47372   10 59 42.19   +14 17 32.8   19.4   Gibbs
          17.47888   10 59 42.45   +14 17 32.8            "
          17.48404   10 59 42.67   +14 17 32.3            "
          17.48920   10 59 42.86   +14 17 32.5            "

After the comet was posted on the Minor Planet Center's PCCP webpage, other
CCD astrometrists have reported cometary appearance to the Central Bureau.
R. Weryk (Department of Physics and Astronomy, University of Western Ontario)
found pre-discovery observations of the comet in images obtained on 2023 Dec.
13.6 UT in very poor conditions with the Pan-STARRS1 1.8-m Ritchey-Chretien
reflector at Haleakala; four 45-s w-band survey images taken in 1".9 seeing
show a diffuse coma of size about 2".5 (full-width-at-half-maximum) with a
broad tail > 10" long in p.a. 275-305 degrees.  Four additional 45-s w-band
survey images taken with the Pan-STARRS2 1.8-m Ritchey-Chretien reflector at
Haleakala on Dec. 17.6 in 1".5 seeing show a diffuse coma of size 2".0 (FWHM)
with a straight 10" tail in p.a. 300 degrees.
     Twelve stacked 60-s exposures taken remotely by Hidetaka Sato (Bunkyo-ku,
Tokyo, Japan) with a 0.51-m f/6.8 astrograph on 2023 Dec. 17.7 UT show a
poorly condensed coma 12" in diameter with a faint 3'.0 tail toward p.a. 295
degrees; the magnitude was 19.6 as measured within a circular aperture of
radius 6".5.  Twenty stacked 90-s exposures taken by T. Ikemura with a 0.38-m
f/4.2 reflector at Shinshiro, Japan, on 2024 Jan. 11.7 (and measured by
Hirohisa Sato) show a condensed coma about 9" in diameter and a hint of a tail
about 13" long toward p.a. 297 degrees; the total magnitude was measured to be
19.4.  One-hundred-ninety-nine stacked 30-s exposures taken by A. Aletti with
a 0.36-m f/7.5 reflector at Varese, Italy, on 2024 Jan. 4.2 (and measured with
M. Auteri) show a diffuse 7" coma with a broad, fan-shaped tail at least 25"
long centered around p.a. 300 degrees.
     Additional astrometry of the comet, imaged as an apparently stellar
object, was found in the MPC's "isolated tracklet file" for 2022 Oct. 23 UT
(Pan-STARRS2 reflector; mag 21.9-22.2) and 2022 Dec. 20 (Mt. Lemmon Survey
reflector; mag 20.8-21.4).  The available astrometry appears on MPEC 2024-A148.
     The following elliptical orbital elements by S. Nakano (Central Bureau)
are from 56 observations spanning 2022 Oct. 23-2024 Jan. 12 (mean residual
0".6), which indicate that the comet passed 0.030 AU from Jupiter in 1973
January and 0.15 AU from Jupiter on 2020 Feb. 28.  Orbital elements prior to
the 1973 encounter suggest e = 0.32, q = 2.63 AU, i = 9.6 deg, and P = 7.6 yr.
The 2022 observations show residuals of -0.19 deg in R.A. and -0.09 deg in
Decl. from an orbit computed only with the available 2023-2024 observations.

                    Epoch = 2015 June 27.0 TT
     T = 2015 June 28.54390 TT        Peri. =   2.55022
     e = 0.1535860                    Node  = 102.60233 2000.0
     q = 3.7743195 AU                 Incl. =  14.49583
       a =  4.4591882 AU   n = 0.10466956   P =   9.42 years

                    Epoch = 2023 Aug.  4.0 TT
     T = 2023 Aug.  9.79773 TT        Peri. =  16.78813
     e = 0.3920926                    Node  =  79.23106 2000.0
     q = 2.2758828 AU                 Incl. =   6.99276
       a =  3.7437986 AU   n = 0.13606153   P =   7.24 years

                    Epoch = 2030 Oct. 26.0 TT
     T = 2030 Nov. 13.66151 TT        Peri. =  16.91369
     e = 0.3907447                    Node  =  79.19469 2000.0
     q = 2.2862654 AU                 Incl. =   6.98616
       a =  3.7525572 AU   n = 0.13558545   P =   7.27 years

                    Epoch = 2038 Feb. 26.0 TT
     T = 2038 Feb. 12.28766 TT        Peri. =  16.81147
     e = 0.3922982                    Node  =  79.20341 2000.0
     q = 2.2766310 AU                 Incl. =   6.99038
       a =  3.7462965 AU   n = 0.13592547   P =   7.25 years

The following ephemeris by the undersigned from the above orbital elements
uses photometric power-law parameters H = 14.0 and 2.5n = 10 for the
magnitudes.

Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase  Mag.
2023 12 02    10 45.25   +14 42.0    2.169    2.414    92.0    24.1  19.5
2023 12 12    10 55.18   +14 22.3    2.070    2.438    99.7    23.5  19.4
2023 12 22    11 02.92   +14 17.2    1.974    2.463   108.0    22.3  19.4
2024 01 01    11 08.24   +14 28.1    1.884    2.489   116.9    20.6  19.3
2024 01 11    11 10.91   +14 55.3    1.805    2.517   126.5    18.3  19.3
2024 01 21    11 10.78   +15 37.9    1.739    2.546   136.7    15.4  19.3
2024 01 31    11 07.93   +16 32.0    1.692    2.576   147.3    11.9  19.3
2024 02 10    11 02.71   +17 32.3    1.667    2.608   157.8     8.2  19.3
2024 02 20    10 55.78   +18 31.1    1.667    2.640   166.9     4.9  19.3
2024 03 01    10 48.11   +19 20.9    1.695    2.673   168.3     4.3  19.4
2024 03 11    10 40.73   +19 55.9    1.750    2.706   160.5     7.0  19.5
2024 03 21    10 34.59   +20 12.9    1.830    2.741   150.4    10.3  19.7
2024 03 31    10 30.36   +20 11.3    1.933    2.776   140.3    13.3  19.9
2024 04 10    10 28.36   +19 52.8    2.056    2.812   130.5    15.7  20.1
2024 04 20    10 28.66   +19 19.6    2.194    2.848   121.2    17.6  20.3
2024 04 30    10 31.11   +18 34.4    2.345    2.884   112.5    18.8  20.5
2024 05 10    10 35.46   +17 39.3    2.504    2.921   104.2    19.6  20.6
2024 05 20    10 41.45   +16 36.3    2.669    2.958    96.4    19.9  20.8
2024 05 30    10 48.80   +15 26.8    2.837    2.995    89.0    19.8  21.0
2024 06 09    10 57.25   +14 12.2    3.006    3.033    81.8    19.3  21.2
2024 06 19    11 06.61   +12 53.3    3.174    3.071    74.9    18.6  21.4
2024 06 29    11 16.68   +11 31.2    3.338    3.109    68.3    17.7  21.5
2024 07 09    11 27.32   +10 06.4    3.498    3.146    61.7    16.5  21.7
2024 07 19    11 38.43   +08 39.8    3.651    3.184    55.3    15.2  21.8
2024 07 29    11 49.88   +07 12.0    3.796    3.222    49.0    13.8  22.0


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2021 CBAT
2021 January 13                  (CBET 5329)              Daniel W. E. Green




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