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B96 (BRIXIIS)







156P/RUSSELL-LINEAR - (P/2000 QD_181 = 2000 XV_43 = 1986 R1 = 1993 WU (Russell- LINEAR))

Photometric data obtained with FOCAS-II software


COD B96

OBS BRIXIIS Observatory

CATALOG: Gaia DR2 - BAND: G


                                   10x10  20x20  30x30  40x40  50x50  60x60   SNR   SB   COD

COMET         UTC                    +/-    +/-    +/-    +/-    +/-    +/-     N  FWHM  CAT

------------  -------------------  -----  -----  -----  -----  -----  -----  ----  ----  ---

156P          02/11/2020 21:35:21  12.91  12.48  12.33  12.23  12.15  12.08  47.2  16.4  B96

156P          02/11/2020 21:35:21*  0.01   0.03   0.03   0.04   0.04   0.05    12   3.9  Gai

156P          04/11/2020 20:31:16  12.87  12.45  12.29  12.19  12.11  12.04  58.3  17.1  B96

156P          04/11/2020 20:31:16*  0.01   0.01   0.00   0.00   0.00   0.01     3   3.9  Gai

156P          06/11/2020 20:25:51  12.80  12.25  12.08  11.97  11.88  11.81  43.1  17.5  B96

156P          06/11/2020 20:25:51*  0.00   0.02   0.01   0.01   0.02   0.02     2   3.5  Gai

156P          19/11/2020 18:16:06  12.44  11.89  11.70  11.59  11.49  11.42  51.6  17.5  B96

156P          19/11/2020 18:16:06*  0.01   0.02   0.02   0.02   0.02   0.02    22   3.8  Gai

156P          20/11/2020 19:48:32  12.43  11.92  11.72  11.61  11.51  11.44  52.8  17.4  B96

156P          20/11/2020 19:48:32*  0.00   0.01   0.01   0.00   0.00   0.00     3   3.6  Gai

156P          26/02/2021 19:53:32  15.36  14.48  14.13  13.91  13.75  13.64  14.7  17.6  B96

156P          26/02/2021 19:53:32*  0.00   0.01   0.01   0.00   0.03   0.02     2   3.4  Gai

156P          02/03/2021 20:34:13  15.41  14.59  14.22  13.96  13.76  13.62   9.7  17.5  B96

156P          02/03/2021 20:34:13*  0.03   0.05   0.05   0.05   0.04   0.04     4   3.7  Gai

156P          19/03/2021 20:28:27  15.84  15.06  14.71  14.46  14.31  14.21   9.8  18.1  B96

156P          19/03/2021 20:28:27*  0.07   0.04   0.01   0.02   0.01   0.02     2   3.3  Gai

156P          25/03/2021 21:40:04  16.07  15.20  14.74  14.47  14.29  14.19   9.9  17.4  B96

156P          25/03/2021 21:40:04*  0.02   0.01   0.05   0.03   0.00   0.01     2   3.9  Gai

                                                                     AFRHO         LOG

COMET         UTC                   DELTA    r    BOX "   MAG   RSR    CM    +/-  AFRHO  OBS

------------  -------------------   -----  -----  -----  -----  ---  -----  ----  -----  ---

156P          02/11/2020 21:35:21    0.49   1.34  56.53  12.08   47     61     1  1.786  B96

156P          04/11/2020 20:31:16    0.49   1.34  56.17  12.04   58     64     1  1.804  B96

156P          06/11/2020 20:25:51    0.49   1.34  55.75  11.80   43     81     2  1.906  B96

156P          19/11/2020 18:16:06    0.53   1.33  51.77  11.45   52    127     2  2.105  B96

156P          20/11/2020 19:48:32    0.54   1.33  51.37  11.48   53    126     2  2.101  B96

156P          26/02/2021 19:53:32    1.47   1.75  18.82  14.65   15     87     6  1.938  B96

156P          02/03/2021 20:34:13    1.52   1.77  18.11  14.76   10     87     9  1.942  B96

156P          19/03/2021 20:28:27    1.78   1.89  15.52  15.36   10     77     8  1.889  B96

156P          25/03/2021 21:40:04    1.87   1.93  14.74  15.58   10     74     7  1.867  B96

156P on Kronk’s cometography

Discovery:

 

The story of this comet officially began in September of 1986. K. S. Russell (Siding Spring Observatory, Australia) was examining a 90-min exposure taken by F. G. Watson on September 3.64 with the U.K. Schmidt Telescope. The comet appeared as a diffuse trail, since it moved during the exposure, and the magnitude was estimated as 17. M. Hartley obtained a 30-minute exposure with the same telescope on September 25.63, but independent examination by Russell and, later, R. H. McNaught revealed no trace of the comet. No formal announcement was ever made by the Central Bureau for Astronomical Telegrams.


Recovery:


     The story continued in 1993, when C. S. Shoemaker (Palomar Observatory, California, USA) discovered a minor planet on plates exposed with the 46-cm Palomar Schmidt telescope and gave positions for November 19.40, November 19.44, and November 20.44. It received the designation "1993 WU", but it was not followed further.

     The object was found a third time in 2000. The LINEAR survey obtained five images of a minor planet during the period of August 31.42 to August 31.47. It received the designation 2000 QD181. LINEAR obtained three more positions during the period of September 5.44 to September 5.46. Another minor planet was found by LINEAR on November 6.41, which was designated 2000 XV43. Three additional images were obtained on November 6, and additional images were obtained on December 5 and 7.


     T. B. Spahr announced on 2001 January 20 (MPEC 2001-B13) that minor planet 2000 QD181 was identical to minor planet 2000 XV43 and, also, minor planet 1993 WU.


Last updated: 2020-11-02