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Perturbation of an orbiter of a Galilean satellite by the other satellites

Acta Astronautica, 1983
In 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 ...
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Rotation models for the Galilean satellites

Planetary and Space Science, 2022
Bruce 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 orbit
Marie Yseboodt, Rose-Marie Baland
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The Galilean Satellites of Jupiter

Scientific American, 1976
Dale 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, 2002
Harald Krüger   +2 more
exaly  

Galilean satellite eclipse studies

Icarus, 1980
Dale W. Smith, Thomas F. Greene
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New evidence of precision premium for Galilean satellites from CCD imaging

Planetary and Space Science, 2008
Benoît Noyelles, A Vienne
exaly  

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