Results 201 to 210 of about 1,104 (222)

The Galilean Satellites of Jupiter

Scientific American, 1976
Dale P. Cruikshank, David Morrison
openaire   +1 more source

Rotation models for the Galilean satellites

Planetary and Space Science, 2022
Bruce G. Bills, Bryan R. Scott
openaire   +1 more source

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
openaire   +1 more source

A tenuous dust ring of Jupiter formed by escaping ejecta from the Galilean satellites

Journal of Geophysical Research, 2002
Alexander V Krivov, Harald Kruger, Eberhard Grün   +2 more
exaly  

Polarimetry of the Galilean satellites and Jupiter near opposition

Journal of Quantitative Spectroscopy and Radiative Transfer, 2009
Vera Rosenbush
exaly  

Atlas of the Galilean satellites

Choice Reviews Online, 2011
openaire   +1 more source

New evidence of precision premium for Galilean satellites from CCD imaging

Planetary and Space Science, 2008
Q Y Peng, A Vienne, V Lainey
exaly  

Galilean satellites

2011
openaire   +1 more source

Astrometric results of the mutual events between the Galilean satellites during 2014–15

Planetary and Space Science, 2019
Chuan-Jun Wang, Jinming Bai
exaly  

Galilean Satellites

2014
openaire   +1 more source