[Iaude] CBET 5422: COMET P/2024 N5 = P/2012 US_27

quai at eps.harvard.edu quai at eps.harvard.edu
Sat Jul 27 01:55:39 EDT 2024


                                                  Electronic Telegram No. 5422
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/2024 N5 = P/2012 US_27 (SIDING SPRING)
     Martin Masek reports the recovery of comet P/2012 US27 (cf. CBET 3310)
on CCD images taken on July 5 and 6 UT at the Pierre Auger Observatory at
Malarguee, Mendoza, Argentina, using a 0.3-m f/6.8 reflector ("Fotometric
Robotic Atmospheric Monitor").  The object appears essentially stellar, but
Masek measured the head of the comet to have a size of 5".6 (full-width-at-
half-maximum) in 4".7-5".2 seeing in the July 5 images.  The astrometry is
tabulated below.

     2024 UT             R.A. (2000) Decl.       Mag.   Observer
     July  5.35240    2 54 48.76   -11 16 30.1   19.1   Masek
           5.35959    2 54 49.50   -11 16 24.8   19.3     "
           5.38126    2 54 51.67   -11 16 08.0   19.2     "
           5.40239    2 54 53.78   -11 15 51.2   19.2     "
           5.40960    2 54 54.52   -11 15 45.5   19.2     "
           6.37942    2 56 32.90   -11 03 15.9   19.6     "
           6.41497    2 56 36.45   -11 02 48.3   19.5     "
          11.39605    3 04 56.93   - 9 58 33.4   19.2     "
          11.41760    3 04 59.07   - 9 58 16.9   19.2     "

The object was posted on the Minor Planet Center's NEOCP webpage, and
additional astrometry appears on MPEC 2024-O57.  Twelve stacked 60-s CCD
exposures taken remotely by H. Sato (Bunkyo-ku, Tokyo, Japan) on 2024 July
25.4 UT with a "Deep Sky Chile" 0.51-m f/6.8 astrograph located in Rio
Hurtado, Chile, shows a strongly condensed coma 5" in diameter and no tail;
the magnitude was 18.5 as measured within a circular aperture of radius 2".8.
     S. Deen (Simi Valley, CA, USA), writes that he has identified apparent
images of this comet in publicly available images obtained with the 3.5-m
telescope at Apache Point in the course of the Sloan Digital Sky Survey on
2002 Feb. 13.4 UT; Deen notes an essentially stellar nuclear condensation of
size 0".9 (FWHM) but with a clearly detached tail separated from the head by
5".5 and with a length of about 50" in p.a. 304 degrees.  Deen's astrometry
is provided below.

     2002 UT             R.A. (2000) Decl.       Mag.
     Feb. 13.44440   12 17 10.00   +58 57 09.6   21.5
          13.44523   12 17 09.91   +58 57 10.0   21.5
          13.44688   12 17 09.78   +58 57 10.3   20.7
          13.44771   12 17 09.74   +58 57 10.7   22.1

The residuals for the recovery observations were +7'.7 in R.A. and +13'.1 in
Decl. from the prediction in NK 2665 (and ICQ Comet Handbook 2023), with a
corresponding correction of Delta(T) = -0.67 day.  The 2002 observations were
only 4" off the predicted position from an orbit covering only the 2013 and
2024 apparitions.  The following linked orbital elements by S. Nakano (Central
Bureau) are from 339 observations spanning 2002 Feb. 13-2024 July 25 (mean
residual 0".5).  There are no close approaches to major planets.

                    Epoch = 1989 July 13.0 TT
     T = 1989 July  3.78184 TT        Peri. =   2.01673
     e = 0.6480828                    Node  =  49.21843 2000.0
     q = 1.8394203 AU                 Incl. =  39.07255
       a =  5.2268552 AU   n = 0.08247900   P =  11.95 years

                    Epoch = 2001 May  11.0 TT
     T = 2001 May   6.76063 TT        Peri. =   1.65553
     e = 0.6485331                    Node  =  49.20961 2000.0
     q = 1.8283189 AU                 Incl. =  39.19627
       a =  5.2019655 AU   n = 0.08307166   P =  11.86 years

                    Epoch = 2013 Jan. 28.0 TT
     T = 2013 Feb.  8.55790 TT        Peri. =   1.27008
     e = 0.6485996                    Node  =  49.20691 2000.0
     q = 1.8208299 AU                 Incl. =  39.29238
       a =  5.1816391 AU   n = 0.08356094   P =  11.80 years

                    Epoch = 2024 Oct. 17.0 TT
     T = 2024 Oct. 20.65464 TT        Peri. =   0.86597
     e = 0.6486278                    Node  =  49.21139 2000.0
     q = 1.8149783 AU                 Incl. =  39.36973
       a =  5.1654008 AU   n = 0.08395528   P =  11.74 years

                    Epoch = 2036 May  27.0 TT
     T = 2036 June 14.70921 TT        Peri. =   0.47686
     e = 0.6488411                    Node  =  49.22199 2000.0
     q = 1.8091809 AU                 Incl. =  39.43187
       a =  5.1520295 AU   n = 0.08428234   P =  11.69 years

                    Epoch = 2048 Jan.  5.0 TT
     T = 2048 Jan. 21.39838 TT        Peri. =   0.14974
     e = 0.6512972                    Node  =  49.20698 2000.0
     q = 1.7909369 AU                 Incl. =  39.53111
       a =  5.1359973 AU   n = 0.08467728   P =  11.64 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.  The 2002 and 2024 apparitions have observed magnitudes that
are both about 1.5 mag fainter than those at the 2013 apparition (where
H_10 was around 12.5).

Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase  Mag.
2024 06 19    02 26.60   -14 47.8    2.465    2.196    62.9    24.3  19.4
2024 06 29    02 43.97   -12 38.5    2.339    2.144    66.4    25.7  19.2
2024 07 09    03 00.95   -10 29.5    2.211    2.094    70.0    27.1  18.9
2024 07 19    03 17.43   -08 20.0    2.081    2.047    73.9    28.5  18.7
2024 07 29    03 33.30   -06 08.2    1.951    2.004    78.0    29.7  18.5
2024 08 08    03 48.43   -03 52.2    1.820    1.964    82.4    30.8  18.2
2024 08 18    04 02.60   -01 28.5    1.690    1.928    87.3    31.6  18.0
2024 08 28    04 15.59   +01 07.2    1.560    1.896    92.6    32.2  17.7
2024 09 07    04 27.07   +04 00.5    1.433    1.869    98.5    32.2  17.5
2024 09 17    04 36.58   +07 18.9    1.310    1.848   105.1    31.7  17.3
2024 09 27    04 43.59   +11 11.2    1.194    1.831   112.7    30.3  17.0
2024 10 07    04 47.31   +15 46.4    1.089    1.820   121.2    28.0  16.8
2024 10 17    04 46.81   +21 10.9    1.000    1.815   130.8    24.6  16.6
2024 10 27    04 41.05   +27 22.2    0.933    1.816   141.0    20.2  16.4
2024 11 06    04 29.03   +34 00.8    0.893    1.823   150.5    15.5  16.4
2024 11 16    04 10.66   +40 28.0    0.886    1.835   156.2    12.6  16.4
2024 11 26    03 47.48   +45 59.0    0.912    1.853   154.6    13.2  16.5
2024 12 06    03 23.09   +50 05.2    0.969    1.876   147.5    16.4  16.7
2024 12 16    03 02.01   +52 48.2    1.050    1.904   138.7    19.9  16.9
2024 12 26    02 47.52   +54 29.7    1.151    1.937   130.1    22.8  17.2
2025 01 05    02 40.89   +55 34.3    1.266    1.974   122.2    24.9  17.5
2025 01 15    02 41.83   +56 21.0    1.390    2.015   115.1    26.2  17.8
2025 01 25    02 49.38   +56 59.9    1.522    2.060   108.6    26.9  18.0
2025 02 04    03 02.52   +57 35.1    1.658    2.107   102.7    27.2  18.3
2025 02 14    03 20.32   +58 07.5    1.797    2.158    97.3    27.0  18.6
2025 02 24    03 41.97   +58 35.3    1.939    2.211    92.2    26.6  18.9
2025 03 06    04 06.79   +58 56.1    2.082    2.266    87.4    25.9  19.1
2025 03 16    04 34.07   +59 07.1    2.225    2.323    82.9    25.1  19.4
2025 03 26    05 03.11   +59 05.9    2.369    2.381    78.6    24.2  19.6
2025 04 05    05 33.23   +58 50.7    2.513    2.441    74.3    23.2  19.9
2025 04 15    06 03.74   +58 20.7    2.656    2.502    70.3    22.2  20.1
2025 04 25    06 34.03   +57 35.7    2.798    2.564    66.3    21.0  20.3
2025 05 05    07 03.60   +56 36.5    2.939    2.627    62.3    19.9  20.5
2025 05 15    07 32.09   +55 24.6    3.077    2.690    58.5    18.7  20.7
2025 05 25    07 59.26   +54 01.8    3.213    2.754    54.7    17.5  20.9
2025 06 04    08 25.03   +52 29.9    3.345    2.818    50.9    16.2  21.1
2025 06 14    08 49.35   +50 51.3    3.472    2.882    47.3    15.0  21.3


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

                         (C) Copyright 2024 CBAT
2024 July 27                     (CBET 5422)              Daniel W. E. Green




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