Abstract
The second zonal and second sectorial Stokes parameters of Ganymede determined on the basis of Galileo spacecraft orbit dynamics (June and September 1996) are used to determine the triaxial level ellipsoid of Ganymede. The polar and the equatorial flattening are of the same order in magnitude, about 5 × 10−4, the secular Love and tidal numbers amount 0.80 and they clarify the equilibrium state of Ganymede. The tidal rotational and orbital dynamics and tidal evolution of the Jupiter-Ganymede system differ significantly from those of the Earth-Moon system.
Similar content being viewed by others
References
Anderson J D, Lau E L, Sjogren W L, Schubert G, Moore W B 1996: Nature, 384, 541–543.
Burns J A 1986: In: Satellites, J A Burns, M S Mathews eds, The University of Arizona Press, Tucson, 1–38.
Bursa M 1994: Studia geoph. et geod., 38, 7–22.
Campbell J K, Synnott S P 1985: Astron J., 90, 364–372.
Davies M E, Abalakin V K, Bursa M, Lieske J H, Morando B, Morrison D, Scidelmann P K, Sinclair A T, Yallop B, Tjuflin Y S 1996: Celestial Mechanics and Dynamical Astronomy, 63, 127–148.
Greenberg R 1982: In: Satellites of Jupiter, D Morrison ed., The University of Arizona Press, Tucson, Arizona, 65.
Kopal Z 1966: An introduction to the study of the Moon. D Reidel Publishing Company, Dordrecht
Kopal Z 1978: Dynamics of close binary systems. D Reidel Publishing Company, Dordrecht
McCarthy D D ed. 1992: IERS Standards. Observatoire de Paris
Yoder C F 1979: Nature, 279, 767.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Burša, M. Figure Parameters of Ganymede. Acta Geod. Geoph. Hung 32, 225–233 (1997). https://doi.org/10.1007/BF03325489
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF03325489