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Circular No. 2711
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Cable Address: SATELLITES, NEWYORK
Western Union: RAPID SATELLITE CAMBMASS
JUPITER XIII
Dr. M. Schmidt, Hale Observatories, telegraphs the following
positions, obtained by C. Kowal with the 122-cm Schmidt telescope:
1974 UT R. A. (1950) Decl. mpv
Oct. 17.23472 22 37 17.3 - 9 53 47 20
18.24236 22 37 07.3 - 9 54 04
The following jovicentric orbit, by K. Aksnes, Center for
Astrophysics, Harvard and Smithsonian Observatories, satisfies the
seven available observations (cf. IAUC 2702, 2703) within 1".5:
T = 1974 July 16.88 ET
Peri. = 267.96 e = 0.1053
Node = 249.18 1950.0 a = 0.0829 AU
Incl. = 24.95 n = 1.2764
q = 0.074 AU P = 282.0 days
Solar perturbations were ignored, and the observations may be satisfied
equally well with an orbit having e = 0.3. The above orbit is
similar to those of Jupiter VI, VII and X. A retrograde orbit does
not give a satisfactory fit to the observations, and the least-squares
heliocentric orbit - determined by the undersigned - gives
e = 1.19 +/- 0.06. Further observations at the November (and if
possible at the December) dark run will be essential if a reliable
ephemeris is to be provided for the 1975 opposition.
1974 ET R. A. (1950) Decl.
Oct. 30 22 36.18 - 9 52.2
Nov. 4 22 36.35 - 9 48.5
9 22 36.85 - 9 43.2
14 22 37.68 - 9 36.1
19 22 38.83 - 9 27.5
24 22 40.29 - 9 17.3
29 22 42.04 - 9 05.7
Dec. 4 22 44.06 - 8 52.6
9 22 46.35 - 8 38.2
14 22 48.89 - 8 22.6
19 22 51.65 - 8 05.7
24 22 54.63 - 7 47.6
29 22 57.81 - 7 28.5
1974 October 24 (2711) Brian G. Marsden
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