C 2018 V1 MACHHOLZ-FUJIKAWA-IWAMOTO
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COMET C/2018 V1 (MACHHOLZ-FUJIKAWA-IWAMOTO)
Further to CBET 4569, additional physical observations have been reported
by CCD astrometrists. J.-F. Soulier writes that unfiltered images taken by A.
Maury, J.-B. Vanssay, and himself with a 0.4-m f/5 Ritchey-Chretien reflector
at San Pedro de Atacama, Chile, on Nov. 9.35-9.37 UT show a diffuse coma of
size 2'.4 x 3'.5 with no tail, and they measured magnitude 11.5 in an aperture
of radius 0'.56; follow-up observations taken during Nov. 10.34-10.36 show a
4'.2 x 5'.2 coma with a tail more than 12' long in p.a. 300 degrees, and
the magnitude was 10.2 in the same-sized photometric aperture; similar
exposures taken on Nov. 11.35-11.37 show a 5' x 6' coma with a 13' tail in
p.a. 300 deg (and mag 10.1 in the same-sized photometric aperture). K.
Kadota, Ageo, Japan, reports that images taken with a 0.25-m f/5 reflector on
Nov. 9.84 UT show a strong central condensation and a coma of diameter 4'.4
and magnitude 10.3, with no tail.
Visual total-magnitude and coma-diameter estimates: Nov. 9.22 UT, 9.9,
4' (J. J. Gonzalez, Collada del Fresno, Sierra del Aramo, near Asturias,
Spain, 0.20-m reflector; near-stellar central condensation of mag about 12.5;
altitude 17 degrees with zodiacal light); 10.49, 9.4, 2'.5 (A. Hale,
Cloudcroft, NM, USA, 10x50 binoculars).
Additional astrometry were published on MPEC 2018-V151. The following
preliminary parabolic orbital elements by S. Nakano, Sumoto, Japan, are from
313 observations spanning Nov. 7-11:
T = 2018 Dec. 3.5142 TT Peri. = 88.8051
Node
= 128.7214 2000.0
q = 0.386827 AU Incl. = 143.9742
The following ephemeris is from the above elements, with power-law
photometric parameters H = 10.5 and 2.5n = 7.5:
2018 TT R. A. (2000) Decl. Delta r Elong. Phase Mag.
Nov.
11 12 35.75 -01 46.3 1.069
0.698 39.4 64.2 9.5
12 12 41.75 -01 38.1 1.034
0.679 39.1 66.9 9.3
13 12 48.25 -01 29.9
0.999 0.660 38.7 69.8
9.1
14 12 55.31 -01 21.8
0.965 0.641 38.2
73.0 9.0
15 13 03.00
-01 13.8 0.931 0.621 37.6
76.3 8.8
16 13 11.39
-01 06.2 0.898 0.603 36.9
79.9 8.6
17 13 20.55
-00 59.2 0.865 0.584 35.9
83.6 8.4
18 13 30.58
-00 53.1 0.834 0.566 34.9
87.7 8.2
19 13 41.53
-00 48.1 0.804 0.548 33.6
91.9 8.1
20 13 53.50
-00 44.7 0.777 0.530 32.2
96.5 7.9
21 14 06.54
-00 43.4 0.751 0.513 30.6
101.2 7.7
22 14 20.68 -00
44.7 0.728 0.496 28.9
106.0 7.5
23 14 35.92 -00
49.3 0.708 0.480 27.0
111.0 7.4
24 14 52.21 -00
57.8 0.691 0.465 25.1
115.8 7.2
25 15 09.42 -01
10.7 0.679 0.451 23.2
120.4 7.1
26 15 27.37 -01
28.5 0.671 0.438 21.5
124.4 6.9
27 15 45.79 -01
51.5 0.668 0.426 20.0
127.5 6.8
28 16 04.37 -02
19.6 0.670 0.415 19.0
129.3 6.8
29 16 22.76 -02
52.6 0.677 0.406 18.5
129.5 6.7
30 16 40.62 -03
30.0 0.689 0.399 18.6
128.0 6.7
Dec. 1 16 57.66 -04 11.2
0.707 0.393 19.0 125.0
6.7
2 17 13.63 -04
55.3 0.728 0.389 19.8
120.8 6.7
3 17 28.37
-05 41.5 0.754 0.387 20.7
115.7 6.8
4 17 41.82
-06 29.0 0.784 0.387 21.7
110.0 6.9
5 17 53.96
-07 17.2 0.816 0.389 22.5
104.0 7.0
6 18 04.82
-08 05.6 0.851 0.393 23.3
97.9 7.1
7 18 14.50
-08 53.5 0.888 0.399 23.8
91.9 7.2
8 18
23.09 -09 40.7 0.926 0.406
24.3 86.1 7.4
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2018 CBAT
2018
November 11
(CBET 4572) Daniel W.
E. Green