Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-20T10:43:33.003Z Has data issue: false hasContentIssue false
  • English
  • Français

New constants for Sampson-Lieske theory of the Galilean satellites of Jupiter from mutual occultation data

Published online by Cambridge University Press:  25 May 2016

R. Vasundhara ,
J.E. Arlot  and
P. Descamps
R. Vasundhara
Affiliation:
Indian Institute of Astrophysics, Bangalore 560034, India
J.E. Arlot
Affiliation:
Bureau des Longitudes, URA 0707 CNRS, 77 avenue Denfert-Rochereau, 75014 Paris, France
P. Descamps
Affiliation:
Bureau des Longitudes, URA 0707 CNRS, 77 avenue Denfert-Rochereau, 75014 Paris, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

New constants for Sampson-Lieske theory of the Galilean Satellites have been derived using 6360 individual photographic positions (1891–1990) and 438 pseudo astrometric positions from mutual occultations during 1973, 1979, 1985 and 1991. Using these new sets of constants, significant improvement is noticed in the O-C values of the sky plane coordinates of the mutual event data set and residuals in longitude for Io and Europa are found to improve. Problems concerning the inclusion of mutual event data in attempting evaluation of secular variations of the mean motions of the satellites are discussed.

Type
Part III - Satellites: Theory and Ephemerides
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 145 - 150
Copyright
Copyright © Kluwer 1996 

References

Aksnes, K., Franklin, F. 1976, Astron. J., 81, 464.Google Scholar
Aksnes, K., Franklin, F., Millis, R., Birch, P., Blanco, C., Catalano, S., Piironen, J. 1984, Astron. J., 89, 280.Google Scholar
Aksnes, K., Franklin, F., Magnusson, P. 1986, Astron. J., 92, 1436.Google Scholar
Arlot, J.E. 1982, Astron. Astrophys., 107, 305.Google Scholar
Arlot, J.E. et al., 1992, Astron. Astrophys. Supp. Series, 92, 151.Google Scholar
Arlot, J.E. et al., 1996, to be published in Astron. Astrophys. Supp. Series..Google Scholar
Brouwer, D., Clemence, G.M. 1961, in Planets and Satellites, Kuiper, and Middlehurst, ed., Chicago University Piers, p. 88.Google Scholar
Descamps, P., Thuillot, W. 1993, Icarus, in press.Google Scholar
de Sitter, W., 1928, Leiden Annals, 16, 92.Google Scholar
GSO and Franklin, F., 1991, Astrophys. 102, 806.Google Scholar
Goldstein, S.J., Jacobs, K.C. 1996, On the Evolution of the galilean satellites, in press.Google Scholar
Goldstein, S.J., Jacobs, K.C. 1996, A recalculation of the secular acceleration of IO, in press.Google Scholar
Greenberg, R., Goldstein, S.J., Jacobs, K.C. 1986, Nature, 323, 789.Google Scholar
Hapke, B.W. 1984, Icarus 59, 41.Google Scholar
Lieske, J.H., 1974, Astron. Astrophys. 31, 137.Google Scholar
Lieske, J.H., 1977, Astron. Astrophys. 56, 333.Google Scholar
Lieske, J.H., 1978, Astron. Astrophys. 65, 83.Google Scholar
Lieske, J.H., 1980, Astron. Astrophys. 82, 340.Google Scholar
Lieske, J.H., 1987, Astron. Astrophys. 176, 146.Google Scholar
Vasundhara, R. 1993, .Google Scholar
Vasundhara, R. 1994, Astron. Astrophys. 281, 565.Google Scholar