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Satellites Chapter 14
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Opener
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Fig. 14.1 Tidal Heating of Io
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Fig. 14.2 Orbital Resonance
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Tab. 14.1
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Fig. 14.3 Phobos, Martian Satellite
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Phobos, Martian Satellite
Fig. 14.4 Phobos, Martian Satellite
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Fig. 14.5 Deimos (Mars)
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Fig. 14.6 Deimos, close up view
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Tab. 14.2
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Sulfur and sulfuric compounds
Fig. 14.7 Io Sulfur and sulfuric compounds Volcanic activity
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Fig. 14.8 Plume on the Limb of Io
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Fig. 14.9
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Volcanic eruption on Io
Fig Volcanic eruption on Io
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Two different images of Io 17 years apart (Voyager and Galileo)
Fig Two different images of Io 17 years apart (Voyager and Galileo)
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Model for the sufrace of Io
Fig Model for the sufrace of Io
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Europa (from Galileo) Smooth, highly reflective surface
Fig Europa (from Galileo) Smooth, highly reflective surface crisscrossed by dark lines. Water ice. Liquid water underneath? Evidence of tidal forces from Jupiter.
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Europa’s Interior Structure
Fig Europa’s Interior Structure
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Fig Europa
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Fig Ice Rafts on Europa
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Fig
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Ganymede Ancient dark terrain separated By light-colored terrain
Fig Ganymede Ancient dark terrain separated By light-colored terrain
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Fig Faulting on Ganymede
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Fig A view across Ganymede
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Fig Callisto
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Fig Callisto
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Fig A scarp on Callisto
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Fig Rhea (1530 km)
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Fig Tethys, (1050 km)
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Fig Iapetus (1440 km)
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Fig Enceladus (500 km)
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Icy material from Enceladus
Fig Icy material from Enceladus
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Fig Titan (5150 km)
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Panoramic view of Titan
Fig Panoramic view of Titan
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Fig At the surface of Titan (From Huygens)
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Fig Umbriel (Uranus)
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Fig Oberon (Uranus)
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Fig Titania (Uranus)
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Fig Ariel (Uranus)
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Fig Miranda, Uranus)
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Fig Coronae on Miranda (Uranus)
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Fig
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Fig
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Fig Triton
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Fig Triton
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Fig Plumes on Triton
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