Electronic Telegram No. 5497
Central Bureau for Astronomical Telegrams
Mailing address:  Hoffman Lab 209; Harvard University;
 20 Oxford St.; Cambridge, MA  02138; U.S.A.
e-mail:  cbatiau@eps.harvard.edu (alternate cbat@iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network


COMET C/2025 B1 (PANSTARRS)
     Y. Ramanjooloo, Institute for Astronomy, University of Hawaii, reports
the discovery of another comet in images taken on Jan. 20 UT with the
Pan-STARRS2 1.8-m Ritchey-Chretien reflector at Haleakala (discovery
observations tabulated below).  Four stacked 45-s w-band survey images taken
in 1".2-1".3 seeing show a condensed head of size 2".4 (full-width-at-half-
maximum) with a straight tail 7" long in p.a. 220 degrees.

     2025 UT             R.A. (2000) Decl.       Mag.
     Jan. 20.24040    5 56 04.37   +16 53 17.8   20.7
          20.25124    5 56 04.03   +16 53 24.4   20.6
          20.26212    5 56 03.68   +16 53 30.7   20.7
          20.27295    5 56 03.33   +16 53 37.3   20.6
          20.38375    5 55 59.82   +16 54 42.5   21.5
          20.38440    5 55 59.81   +16 54 42.7   20.1

After the comet was posted to the Minor Planet Center's PCCP webpage, S. Deen
(Simi Valley, CA, USA) found archival observations taken with the Mt. Lemmon
Survey's 1.5-m reflector on 2024 Dec. 24.35-24.37 (mag 20.4) and 2025 Jan.
3.28-3.30 UT (mag 20.3).  On Dec. 24, the object does not appear obviously
cometary (but a star to the southeast, towards the anti-solar vector, may be
hiding any tail); its nuclear condensation may be slightly less than stellar,
but not confidently so.  On Jan. 3, the comet showed a fairly condensed coma
about 3" (FWHM) in size and a 9" tail pointing towards p.a. 230 degrees.
     M. Jaeger writes that twenty-nine 90-s CMOS images taken on 2025 Jan.
21.86 UT with a 0.30-m f/4 reflector at Martinsberg, Austria, shows a
possible coma of size 7" of total magnitude 20.0; he notes that the comet's
head appears softer than the images of nearby stars of similar brightness.
     The available astrometry appears on MPEC 2025-B77.  The following
parabolic orbital elements by S. Nakano (Central Bureau) are from 35
observations spanning 2024 Dec. 24-2025 Jan. 23 (mean residual 0".6); they
indicate that the comet passed 1.74 AU from Jupiter on 2024 Nov. 10 UT.

     T = 2025 June 26.19686 TT        Peri. =  23.40132
                                      Node  = 102.85251 2000.0
     q = 3.5313557 AU                 Incl. =  39.62111

The following ephemeris by the undersigned from the above orbital elements
uses photometric power-law parameters H = 12.5 and 2.5n = 8 for the
magnitudes.

Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase  Mag.
2025 01 05    06 05.04   +14 26.3    2.908    3.862   164.0     4.0  19.5
2025 01 10    06 01.88   +15 13.8    2.909    3.844   159.2     5.2  19.5
2025 01 15    05 58.91   +16 02.2    2.918    3.827   154.0     6.5  19.5
2025 01 20    05 56.19   +16 50.9    2.935    3.810   148.6     7.7  19.5
2025 01 25    05 53.80   +17 39.9    2.959    3.793   143.2     8.9  19.5
2025 01 30    05 51.79   +18 28.5    2.989    3.777   137.8    10.1  19.5
2025 02 04    05 50.21   +19 16.8    3.025    3.761   132.5    11.1  19.5
2025 02 09    05 49.09   +20 04.2    3.066    3.746   127.2    12.1  19.5
2025 02 14    05 48.46   +20 50.7    3.112    3.731   122.1    13.0  19.5
2025 02 19    05 48.33   +21 36.2    3.162    3.717   117.0    13.7  19.6
2025 02 24    05 48.71   +22 20.4    3.215    3.703   112.1    14.3  19.6
2025 03 01    05 49.60   +23 03.3    3.272    3.690   107.3    14.9  19.6
2025 03 06    05 51.01   +23 44.9    3.330    3.677   102.6    15.3  19.6
2025 03 11    05 52.91   +24 25.1    3.390    3.664    98.1    15.6  19.7
2025 03 16    05 55.30   +25 03.7    3.452    3.653    93.6    15.8  19.7
2025 03 21    05 58.15   +25 40.9    3.514    3.641    89.3    15.9  19.7
2025 03 26    06 01.46   +26 16.6    3.577    3.630    85.1    15.9  19.7
2025 03 31    06 05.19   +26 50.8    3.639    3.620    81.0    15.8  19.8
2025 04 05    06 09.34   +27 23.4    3.701    3.610    77.0    15.7  19.8
2025 04 10    06 13.88   +27 54.4    3.762    3.601    73.1    15.4  19.8
2025 04 15    06 18.78   +28 23.9    3.822    3.593    69.3    15.1  19.9
2025 04 20    06 24.03   +28 51.7    3.881    3.584    65.6    14.8  19.9
2025 04 25    06 29.60   +29 18.0    3.938    3.577    62.0    14.4  19.9
2025 04 30    06 35.48   +29 42.6    3.993    3.570    58.4    13.9  19.9
2025 05 05    06 41.65   +30 05.7    4.046    3.564    55.0    13.4  19.9
2025 05 10    06 48.09   +30 27.0    4.096    3.558    51.6    12.8  20.0
2025 05 15    06 54.77   +30 46.8    4.144    3.552    48.3    12.3  20.0
2025 05 20    07 01.68   +31 04.9    4.190    3.548    45.0    11.6  20.0
2025 05 25    07 08.81   +31 21.4    4.233    3.544    41.9    11.0  20.0


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

                         (C) Copyright 2025 CBAT
2025 January 23                  (CBET 5497)              Daniel W. E. Green