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THE ASTRONOMER Electronic Circular No 847 1994 June 3 20.05UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke,
Hants, RG22 4PP,England. Telephone/FAX(0256)471074 Int:+44256471074
INTERNET: GMH at AST.STAR.RL.AC.UK or GMH at GXVG.AST.CAM.AC.UK
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PERIODIC COMET SHOEMAKER 4 (1994k)
Improved elements for this comet (cf E842) confirm it is of short
period:
T 1994 Oct 31.2310 TT w 196.52100 )
e 0.52851000 O 92.60300 ) 2000.0
q 2.9250300 A.U. i 25.34500 )
Source: IAUC 5998 Positions are geocentric
Ephemeris by Hurst using EPH.EXE by N.James:
m = 10.0 + 5.0 log R + 10.0 log r
Date R.A. (2000) Dec. R r Elong Mag. Motion
h m o ' (AU) (AU) o "/hr P.A.
1994 May
28.00 17 14.11 -10 47.8 2.152 3.135 163.0 16.6 28 241
1994 June
2.00 17 10.64 -11 16.5 2.127 3.123 166.8 16.6 30 240
7.00 17 6.99 -11 47.8 2.109 3.111 168.9 16.5 32 239
12.00 17 3.25 -12 21.5 2.097 3.099 168.5 16.5 33 238
17.00 16 59.52 -12 57.4 2.093 3.087 165.7 16.5 33 236
22.00 16 55.90 -13 35.3 2.095 3.076 161.5 16.5 32 233
27.00 16 52.48 -14 14.7 2.104 3.065 156.8 16.5 31 230
1994 July
2.00 16 49.36 -14 55.5 2.120 3.055 151.9 16.5 30 226
7.00 16 46.59 -15 37.4 2.142 3.044 146.9 16.5 28 221
12.00 16 44.27 -16 19.9 2.170 3.035 141.9 16.5 26 215
17.00 16 42.45 -17 3.0 2.203 3.025 136.9 16.5 24 207
22.00 16 41.17 -17 46.3 2.240 3.016 132.0 16.5 23 198
27.00 16 40.45 -18 29.6 2.283 3.008 127.2 16.6 22 188
1994 Aug
1.00 16 40.31 -19 12.7 2.329 3.000 122.5 16.6 22 177
6.00 16 40.76 -19 55.5 2.379 2.992 118.0 16.6 22 166
11.00 16 41.80 -20 37.8 2.431 2.984 113.5 16.7 23 156
16.00 16 43.44 -21 19.6 2.486 2.977 109.2 16.7 25 147
21.00 16 45.64 -22 0.6 2.544 2.971 105.0 16.8 27 140
26.00 16 48.40 -22 40.8 2.602 2.965 100.9 16.8 29 134
31.00 16 51.70 -23 20.0 2.663 2.959 96.9 16.8 31 128
PERIODIC COMET SHOEMAKER-LEVY 9 (1993e)
D. Jewitt and N. Trentham, University of Hawaii, communicate:
"New observations from the University of Hawaii 2.2-m telescope
show that nucleus 15 (= G) is double. On May 7 UT, the fainter
component (15b) appears 3".5 east and 3".7 north of the brighter
(15a). The red magnitude difference measured in a 1"-radius
aperture is 3.8. The fainter component is not evident in
observations taken in previous months under similar observing
conditions."
IAUC 5999
UV PERSEI
Bill Worraker, Didcot, England reports that he also confirmed this
outburst but apparently the original e-mail message to TA HQ
went astray:
1994 May 30.971UT, 12.6 (BAAVSS sequence, 0.26-m reflector)
31.008UT, 12.4 (ditto)
Guy M Hurst
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Date: Fri, 3 Jun 1994 21:38:46 +0100 (BST)