[BAA Comets] DM001 EPHEMERIS

Shanklin, Jonathan D. jdsh at bas.ac.uk
Fri Nov 9 14:20:44 GMT 2018


Although the designation is likely to be 2018 V1, this is not guaranteed, hence the use of DM001 as a preliminary designation.

I’m not sure what the field of view of the Faulkes Telescope is, but the Nakano ephemeris and that based on the latest observations diverge by at least 6 minutes by November 15.  You should be OK for a couple of days, but it might then be worth a resubmission.  Also the comet will be quite low – I think around 20 degrees altitude at the start of twilight.

Regards,

Jon Shanklin
Visual Co-ordinator, BAA Comet Section
http://www.ast.cam.ac.uk/~jds/



From: Comets-disc <comets-disc-bounces at lists.britastro.org> On Behalf Of Helen Usher
Sent: 09 November 2018 14:03
To: denis buczynski <buczynski8166 at btinternet.com>; BAA Comets discussion list <comets-disc at lists.britastro.org>
Subject: Re: [BAA Comets] DM001 EPHEMERIS

Hi Jon,

Thanks for this.  I've just submitted an observation run request to the Faulkes Telescope and have used their MPC lookup using the designation 2018 V1.  I've asked for one image a day for 6 days.  Do you think the elements will be robust enough to last 6 days, or should I resubmit each day in case the elements get refined?

Thanks
Helen

On Friday, 9 November 2018, 13:57:57 GMT, Shanklin, Jonathan D. <jdsh at bas.ac.uk<mailto:jdsh at bas.ac.uk>> wrote:



The orbit is still rather fluid, but the ephemeris from Nakano on the CBET is probably no longer valid.



This ephemeris uses the latest PCCP orbit:



Ephemeris for   DM001     DM001



Omega= 80.0525 OMEGA=125.3290 i=149.1079 q= 0.429752 a= 51.051556

e=0.991582  P=  364.765  T= 2018 December   2.9708    Equinox= 2000

Magnitudes calculated from m=10.9+5.0*Log(d)+15.0*Log(r)+0.000*Beta



Station: Cambridge

Latitude:  52.213  Longitude:    0.000   Magnetic variation:   0.0

Observing constraints:   Sun below -13. deg  Object above***** deg



November  2018                 Positions for 00:00 ET, Times in UT

                                                                                       Elong  Moon  Comet

Day     R.A. B1950 Dec   R.A. J2000 Dec   Mag    D      R    Trans    Observable    Sun Moon Phase Tail  pA d RA dDec



  9/10  12 25.1   -2.02  12 27.6   -2.18   8.8   1.08   0.71   9.12   4.42 to  5.47   40   69    5   19  294    0    0

10/11  12 30.4   -1.54  12 32.9   -2.10   8.6   1.04   0.69   9.14   4.38 to  5.48   40   80   11   22  295   32    3

11/12  12 36.1   -1.46  12 38.7   -2.03   8.4   1.00   0.68   9.15   4.35 to  5.50   40   91   18   26  295   35    3

12/13  12 42.4   -1.38  12 44.9   -1.55   8.1   0.97   0.66   9.18   4.32 to  5.51   39  102   26   30  296   39    3

13/14  12 49.2   -1.31  12 51.8   -1.47   7.8   0.93   0.64   9.21   4.31 to  5.53   39  112   35   35  297   42    3

14/15  12 56.7   -1.23  12 59.3   -1.39   7.6   0.90   0.62   9.24   4.30 to  5.54   38  122   44   41  298   46    3



It will almost certainly change further as more observations come in and the observational arc is extended.



Regards,



Jon Shanklin

Visual Co-ordinator, BAA Comet Section

http://www.ast.cam.ac.uk/~jds/





From: Comets-disc <comets-disc-bounces at lists.britastro.org<mailto:comets-disc-bounces at lists.britastro.org>> On Behalf Of denis buczynski
Sent: 09 November 2018 13:40
To: BAA Comets Discussion List <comets-disc at lists.britastro.org<mailto:comets-disc at lists.britastro.org>>
Subject: [BAA Comets] DM001 EPHEMERIS



On CBET 4569
  Nakano provides the following preliminary ephemeris for the comet:



   2018 TT    R.A. (2000) Decl.    Delta     r

   Nov.  5    12 06.22  -02 26.5   1.549   1.013

         6    12 10.91  -02 21.2   1.549   1.012

         7    12 15.60  -02 15.7   1.550   1.011

         8    12 20.29  -02 10.2   1.550   1.011

         9    12 24.97  -02 04.6   1.551   1.012

        10    12 29.64  -01 59.0   1.552   1.012

        11    12 34.30  -01 53.3   1.553   1.013

        12    12 38.95  -01 47.6   1.555   1.014

        13    12 43.59  -01 41.8   1.556   1.015

        14    12 48.22  -01 36.0   1.558   1.017

        15    12 52.84  -01 30.2   1.560   1.019

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