[Iaude] CBET 5405: COMET C/2024 L2

quai at eps.harvard.edu quai at eps.harvard.edu
Wed Jun 19 13:28:41 EDT 2024


                                                  Electronic Telegram No. 5405
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/2024 L2 (PANSTARRS)
     R. Weryk, Department of Physics and Astronomy, University of Western
Ontario, reports the discovery of another comet in images obtained on June 13
with the Pan-STARRS1 1.8-m Ritchey-Chretien reflector at Haleakala (discovery
observations tabulated below).  Four 45-s stacked w-band survey images taken
on June 13.5 UT in 1".2 seeing show the condensed head with size 2".0 (full-
width-at-half-maximum) and no tail.  Four 60-s stacked w-band follow-up images
taken on June 14.5 in 1".7-1".9 seeing show a condensed head of size 2".4
(FWHM) and no tail.

     2024 UT             R.A. (2000) Decl.       Mag.
     June 13.52926   20 29 17.40   -43 58 25.4   20.4
          13.53705   20 29 17.02   -43 58 26.5   20.0
          13.54481   20 29 16.65   -43 58 27.4   20.1
          13.55256   20 29 16.26   -43 58 28.7   20.0
          14.54728   20 28 28.09   -44 00 41.0   19.6
          14.54811   20 28 28.06   -44 00 41.2   19.4
          14.54892   20 28 28.02   -44 00 41.0   19.4
          14.54974   20 28 27.98   -44 00 41.3   19.6

Weryk adds that he then found this comet in Pan-STARRS1 images from June 1.6
UT; four 45-s w-band survey images taken in 1".8-2".3 seeing show a condensed
head of size 2".9 (FWHM) and magnitude 19.4-19.5, again with no tail.  After
the comet was posted on the Minor Planet Center's PCCP, T. Prystavski (Lviv,
Ukraine) found that CCD exposures taken remotely with a 0.51-m f/4.4 reflector
at Siding Spring, NSW, Australia, on June 18.8 show a very condensed coma
about 9".9 in diameter (total mag 19.0) with a straight tail 0'.3 long in p.a.
98 degrees.
     The Minor Planet Center found three single-night observations from 2023
July 15 in its "isolated tracklet file", which were obtained using the 4-m
reflector (+ DECam) at Cerro Tololo, as tabulated below.  Following a request
by the Central Bureau, S. Deen (Simi Valley, CA, USA) has examined the DECam
images and finds the comet to be clearly cometary therein, with a tail about
20" long in p.a. 85 degrees.  Deen adds that DECam images were also obtained
of the area around the comet's predicted position in August 2023, but those
data will not be publicly available until Aug. 2024.

     2023 UT             R.A. (2000) Decl.       Mag.
     July 15.23005   21 57 41.03   -48 58 09.5   19.5
          15.24530   21 57 40.26   -48 58 13.0   19.6
          15.26052   21 57 39.48   -48 58 16.6   19.5

     The available astrometry from June 2024 appears on MPEC 2024-M24.  The
following parabolic orbital elements by S. Nakano (Central Bureau) are from 20
observations spanning 2024 June 1-18 (mean residual 0".2).

     T = 2025 June 14.95019 TT        Peri. = 345.72169
                                      Node  = 266.18737 2000.0
     q = 8.3312117 AU                 Incl. = 139.57930

Nakano notes that the residuals for the 2023 July 15 observations with respect
to the above parabolic elements are only +6" in R.A. and +16" in Decl.  Nakano
supplies the following linked orbital elements from 23 observations spanning
2023 July 15-2024 June 18 (mean residual 0".2), with corresponding "original"
and "future" values of 1/a being -0.000076 and -0.000042 (+/- 0.000028)
AU**-1, respectively.  There are no close approaches to major planets.

                    Epoch = 2025 June 14.0 TT
     T = 2025 June 17.44235 TT        Peri. = 345.88681
     e = 1.0043848                    Node  = 266.17945 2000.0
     q = 8.3262340 AU                 Incl. = 139.58690

The following ephemeris by the undersigned from the linked orbital elements
above 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.
2024 05 10    20 49.76   -42 33.6    8.348    8.666   105.1     6.5  19.1
2024 05 20    20 45.36   -42 57.9    8.179    8.650   114.7     6.1  19.1
2024 05 30    20 39.71   -43 23.2    8.024    8.634   124.2     5.6  19.0
2024 06 09    20 32.81   -43 47.9    7.888    8.619   133.5     4.9  19.0
2024 06 19    20 24.75   -44 10.1    7.776    8.604   142.4     4.1  18.9
2024 06 29    20 15.72   -44 27.5    7.693    8.589   150.1     3.4  18.9
2024 07 09    20 05.96   -44 38.6    7.641    8.575   155.3     2.8  18.9
2024 07 19    19 55.82   -44 41.9    7.621    8.561   156.2     2.8  18.9
2024 07 29    19 45.68   -44 36.6    7.635    8.547   152.3     3.2  18.9
2024 08 08    19 35.90   -44 22.7    7.681    8.534   145.2     3.9  18.9
2024 08 18    19 26.83   -44 00.9    7.758    8.521   136.5     4.7  18.9
2024 08 28    19 18.76   -43 32.3    7.860    8.508   127.1     5.4  18.9
2024 09 07    19 11.87   -42 58.5    7.986    8.496   117.4     6.0  18.9
2024 09 17    19 06.26   -42 21.1    8.128    8.485   107.5     6.5  19.0
2024 09 27    19 01.97   -41 41.5    8.281    8.474    97.7     6.7  19.0
2024 10 07    18 58.95   -41 01.1    8.440    8.463    87.9     6.8  19.1
2024 10 17    18 57.13   -40 20.9    8.600    8.452    78.2     6.6  19.1
2024 10 27    18 56.40   -39 41.7    8.754    8.442    68.6     6.3  19.1
2024 11 06    18 56.62   -39 04.0    8.899    8.433    59.1     5.8  19.2
2024 11 16    18 57.67   -38 28.0    9.028    8.423    49.8     5.1  19.2
2024 11 26    18 59.40   -37 54.2    9.139    8.415    40.7     4.4  19.2

2025 02 14    19 21.28   -34 43.9    9.093    8.359    39.9     4.3  19.2
2025 02 24    19 23.07   -34 30.7    8.969    8.354    49.1     5.1  19.1
2025 03 06    19 24.23   -34 19.9    8.825    8.349    58.5     5.8  19.1
2025 03 16    19 24.63   -34 11.5    8.666    8.345    68.0     6.3  19.1
2025 03 26    19 24.18   -34 05.4    8.495    8.341    77.8     6.7  19.0
2025 04 05    19 22.76   -34 01.3    8.317    8.338    87.8     6.9  19.0
2025 04 15    19 20.30   -33 58.7    8.138    8.335    97.9     6.8  18.9
2025 04 25    19 16.73   -33 57.2    7.964    8.332   108.1     6.6  18.9
2025 05 05    19 12.02   -33 55.8    7.800    8.330   118.6     6.1  18.8
2025 05 15    19 06.22   -33 53.7    7.653    8.329   129.2     5.4  18.8
2025 05 25    18 59.39   -33 49.8    7.527    8.327   139.9     4.5  18.7
2025 06 04    18 51.68   -33 43.1    7.429    8.327   150.5     3.4  18.7
2025 06 14    18 43.32   -33 32.6    7.361    8.326   160.7     2.3  18.7
2025 06 24    18 34.57   -33 17.6    7.327    8.326   168.8     1.4  18.7
2025 07 04    18 25.73   -32 58.1    7.328    8.327   168.4     1.4  18.7
2025 07 14    18 17.13   -32 34.0    7.365    8.328   160.0     2.4  18.7
2025 07 24    18 09.04   -32 06.2    7.436    8.329   149.8     3.5  18.7


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

                         (C) Copyright 2024 CBAT
2024 June 19                     (CBET 5405)              Daniel W. E. Green




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