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On the Migration of the Galilean Satellites
2014Topic 67: Solar System ...
Lee, MH, Li, WY
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Perturbation of an orbiter of a Galilean satellite by the other satellites
Acta Astronautica, 1983In this paper the perturbation of an orbiter of one of the Galilean satellites by the other Galilean satellites of Jupiter is investigated. The attraction of a perturbing satellite is averaged over one revolution assuming a circular orbit. The perturbation can then easily be represented by elliptic integrals.
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The Galilean Satellites: An Overview
Abstract The four largest moons of Jupiter—Io, Europa, Ganymede, and Callisto—are known as the Galilean satellites, named after Galileo Galilei, who discovered them in 1610. Early 19th-century observations revealed that the three inner moons are locked in a 4:2:1 Laplacian orbital resonance, a relationship that has had significant ...openaire +1 more source
Rotation models for the Galilean satellites
Planetary and Space Science, 2022Bruce G. Bills, Bryan R. Scott
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Spin Orientation of the Galilean Satellites
The four Galilean satellites (Io, Europa, Ganymede, and Callisto) are locked in a 1:1 spin-orbit resonance. Their rotation axis is assumed to be in a Cassini state, meaning that the rotation axis follows the long-term precession of the orbit normal. The obliquity of the satellites, which is the angular separation between the rotation axis and the orbitMarie Yseboodt, Rose-Marie Baland
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The Galilean Satellites of Jupiter
Scientific American, 1976Dale P. Cruikshank, David Morrison
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A tenuous dust ring of Jupiter formed by escaping ejecta from the Galilean satellites
Journal of Geophysical Research E: Planets, 2002Harald Krüger +2 more
exaly
Galilean satellite eclipse studies
Icarus, 1980Dale W. Smith, Thomas F. Greene
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New evidence of precision premium for Galilean satellites from CCD imaging
Planetary and Space Science, 2008Benoît Noyelles, A Vienne
exaly

