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<DIV><FONT size=2 face=Arial>Helen / Denis,</FONT></DIV>
<DIV><FONT size=2 face=Arial></FONT> </DIV>
<DIV><FONT size=2 face=Arial>Unfortunately the current solar elongation of about
40 degrees makes it unobservable from all of the Las Cumbres Observatory
telescopes. Looks like the elongation may be decreasing as well.</FONT></DIV>
<DIV><FONT size=2 face=Arial></FONT> </DIV>
<DIV><FONT size=2 face=Arial>Here's an example of the utility of having your own
scope in the back garden. It's a morning object visible around 5.30 UT from the
UK.</FONT></DIV>
<DIV><FONT size=2 face=Arial></FONT> </DIV>
<DIV><FONT size=2 face=Arial>Discovery of a bright comet is exceedingly
difficult so this is testimony to Don Macholz's near superhuman efforts to do
just this: something that deserves a hearty congratulations from us
all.</FONT></DIV>
<DIV><FONT size=2 face=Arial></FONT> </DIV>
<DIV><FONT size=2 face=Arial>Looking at images posted to the Web makes me think
that the object has recently undergone a significant outburst, given its
'spherical halo' appearance. The last discovery by a visual observer of a comet
occurred in almost the same scenario back on 2010 Nov 02.83 when Kaoru Ikeya
and Shigeki Murakami spotted P/2010 V1 (Ikeya-Murakami) from their respective
observatories in Japan. It was because that object had had an outburst close to
perihelion that precipitated its discovery. We may be witnesssing a similar
event here now.</FONT></DIV>
<DIV><FONT size=2 face=Arial></FONT> </DIV>
<DIV><FONT size=2 face=Arial>Richard Miles</FONT></DIV>
<DIV><FONT size=2 face=Arial>BAA</FONT></DIV>
<BLOCKQUOTE
style="BORDER-LEFT: #000000 2px solid; PADDING-LEFT: 5px; PADDING-RIGHT: 0px; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px">
<DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
<DIV
style="FONT: 10pt arial; BACKGROUND: #e4e4e4; font-color: black"><B>From:</B>
<A title=helen.usher@yahoo.co.uk href="mailto:helen.usher@yahoo.co.uk">Helen
Usher</A> </DIV>
<DIV style="FONT: 10pt arial"><B>To:</B> <A
title=comets-disc@lists.britastro.org
href="mailto:comets-disc@lists.britastro.org">BAA Comets discussion list</A> ;
<A title=buczynski8166@btinternet.com
href="mailto:buczynski8166@btinternet.com">denis buczynski</A> </DIV>
<DIV style="FONT: 10pt arial"><B>Sent:</B> Friday, November 09, 2018 2:33
PM</DIV>
<DIV style="FONT: 10pt arial"><B>Subject:</B> Re: [BAA Comets] DM001
EPHEMERIS</DIV>
<DIV><BR></DIV>
<DIV style="FONT-FAMILY: verdana, helvetica, sans-serif; FONT-SIZE: 16px"
class=ydpe6a12238yahoo-style-wrap>
<DIV></DIV>
<DIV>Thanks Jon. The field of view of the FT 2m telescopes is quite
small - 10.5 x 10.5 arcmin. So it sounds like it would be good to
resubmit after a couple of days. The FT have access to 2 2m scopes, one
in Hawaii and one in Siding Springs, so the comet will be much better
positioned that from here! It might also be worth utilising their small
scopes (1m or 0.4m) to get a bigger FOV and so a greater margin for
divergence.</DIV>
<DIV><BR></DIV>
<DIV>Helen</DIV>
<DIV><BR></DIV></DIV>
<DIV id=ydpa7adea12yahoo_quoted_2024378786 class=ydpa7adea12yahoo_quoted>
<DIV
style="FONT-FAMILY: 'Helvetica Neue', Helvetica, Arial, sans-serif; COLOR: #26282a; FONT-SIZE: 13px">
<DIV>On Friday, 9 November 2018, 14:21:26 GMT, Shanklin, Jonathan D.
<jdsh@bas.ac.uk> wrote: </DIV>
<DIV><BR></DIV>
<DIV><BR></DIV>
<DIV>
<DIV id=ydpa7adea12yiv9330807525>
<DIV>
<DIV class=ydpa7adea12yiv9330807525WordSection1>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt">Although the designation is likely to be 2018 V1, this
is not guaranteed, hence the use of DM001 as a preliminary
designation.</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN style="FONT-SIZE: 11pt">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.</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt">Regards,</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN style="FONT-SIZE: 11pt">Jon
Shanklin</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt">Visual Co-ordinator, BAA Comet Section</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt">http://www.ast.cam.ac.uk/~jds/</SPAN></P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 11pt"></SPAN> </P>
<DIV>
<DIV
style="BORDER-BOTTOM: medium none; BORDER-LEFT: medium none; PADDING-BOTTOM: 0cm; PADDING-LEFT: 0cm; PADDING-RIGHT: 0cm; BORDER-TOP: #e1e1e1 1pt solid; BORDER-RIGHT: medium none; PADDING-TOP: 3pt">
<P class=ydpa7adea12yiv9330807525MsoNormal><B><SPAN style="FONT-SIZE: 11pt"
lang=EN-US>From:</SPAN></B><SPAN style="FONT-SIZE: 11pt" lang=EN-US>
Comets-disc <comets-disc-bounces@lists.britastro.org> <B>On Behalf Of
</B>Helen Usher<BR clear=none><B>Sent:</B> 09 November 2018 14:03<BR
clear=none><B>To:</B> denis buczynski <buczynski8166@btinternet.com>;
BAA Comets discussion list <comets-disc@lists.britastro.org><BR
clear=none><B>Subject:</B> Re: [BAA Comets] DM001
EPHEMERIS</SPAN></P></DIV></DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal> </P>
<DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN>Hi Jon,</SPAN></P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN></SPAN> </P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN>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?</SPAN></P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN></SPAN> </P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN>Thanks</SPAN></P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN>Helen</SPAN></P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN></SPAN> </P></DIV></DIV>
<DIV id=ydpa7adea12yiv9330807525ydpa878fed4yahoo_quoted_2031119615>
<DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN style="FONT-SIZE: 10pt">On
Friday, 9 November 2018, 13:57:57 GMT, Shanklin, Jonathan D. <<A
href="mailto:jdsh@bas.ac.uk" shape=rect rel=nofollow
target=_blank>jdsh@bas.ac.uk</A>> wrote: </SPAN></P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 10pt"></SPAN> </P></DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525MsoNormal><SPAN
style="FONT-SIZE: 10pt"></SPAN> </P></DIV>
<DIV>
<DIV id=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404>
<DIV>
<DIV>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">The orbit is still rather fluid, but the ephemeris
from Nakano on the CBET is probably no longer valid.</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">This ephemeris uses the latest PCCP orbit:</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Ephemeris for
DM001 DM001</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Omega= 80.0525 OMEGA=125.3290 i=149.1079 q= 0.429752
a= 51.051556</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">e=0.991582 P= 364.765 T= 2018
December 2.9708 Equinox= 2000</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Magnitudes calculated from
m=10.9+5.0*Log(d)+15.0*Log(r)+0.000*Beta</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Station: Cambridge</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Latitude: 52.213
Longitude: 0.000 Magnetic variation:
0.0</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Observing constraints: Sun below -13.
deg Object above***** deg</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">November
2018
Positions for 00:00 ET, Times in UT</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">
Elong
Moon Comet</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Day R.A. B1950 Dec
R.A. J2000 Dec Mag
D R Trans
Observable Sun Moon Phase Tail pA d RA
dDec</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"> 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</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">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</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">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</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">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</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">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</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">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</SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">It will almost certainly change further as more
observations come in and the observational arc is extended.</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Regards,</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Jon Shanklin</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt">Visual Co-ordinator, BAA Comet Section</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"><A href="http://www.ast.cam.ac.uk/~jds/" shape=rect
rel=nofollow target=_blank>http://www.ast.cam.ac.uk/~jds/</A></SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 11pt"></SPAN><SPAN style="FONT-SIZE: 10pt"></SPAN> </P>
<DIV>
<DIV
style="BORDER-BOTTOM: medium none; BORDER-LEFT: medium none; PADDING-BOTTOM: 0cm; PADDING-LEFT: 0cm; PADDING-RIGHT: 0cm; BORDER-TOP: #e1e1e1 1pt solid; BORDER-RIGHT: medium none; PADDING-TOP: 3pt">
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><B><SPAN
style="FONT-SIZE: 11pt" lang=EN-US>From:</SPAN></B><SPAN
style="FONT-SIZE: 11pt" lang=EN-US> Comets-disc <<A
href="mailto:comets-disc-bounces@lists.britastro.org" shape=rect rel=nofollow
target=_blank>comets-disc-bounces@lists.britastro.org</A>> <B>On Behalf Of
</B>denis buczynski<BR clear=none><B>Sent:</B> 09 November 2018 13:40<BR
clear=none><B>To:</B> BAA Comets Discussion List <<A
href="mailto:comets-disc@lists.britastro.org" shape=rect rel=nofollow
target=_blank>comets-disc@lists.britastro.org</A>><BR
clear=none><B>Subject:</B> [BAA Comets] DM001 EPHEMERIS</SPAN><SPAN
style="FONT-SIZE: 10pt"></SPAN></P></DIV></DIV>
<P class=ydpa7adea12yiv9330807525ydpa878fed4yiv9399587404msonormal><SPAN
style="FONT-SIZE: 10pt"></SPAN> </P>
<DIV><PRE><SPAN style="COLOR: #26282a">On CBET 4569 <BR clear=none> Nakano provides the following preliminary ephemeris for the comet:</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> </SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 2018 TT R.A. (2000) Decl. Delta r</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> Nov. 5 12 06.22 -02 26.5 1.549 1.013</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 6 12 10.91 -02 21.2 1.549 1.012</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 7 12 15.60 -02 15.7 1.550 1.011</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 8 12 20.29 -02 10.2 1.550 1.011</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 9 12 24.97 -02 04.6 1.551 1.012</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 10 12 29.64 -01 59.0 1.552 1.012</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 11 12 34.30 -01 53.3 1.553 1.013</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 12 12 38.95 -01 47.6 1.555 1.014</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 13 12 43.59 -01 41.8 1.556 1.015</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 14 12 48.22 -01 36.0 1.558 1.017</SPAN></PRE><PRE><SPAN style="COLOR: #26282a"> 15 12 52.84 -01 30.2 1.560 1.019</SPAN></PRE></DIV></DIV>
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