2500-15-large satellites

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Ganymede - Indications of Internal Activity Several Diverse Terrains Appear in This Galileo Image • Oldest Area (right) Consists of Rolling Hills with Many Craters • Intermediate Age (Left) Displays a Dense Pattern of Folded Mountains (Not Tectonic Compression – Rather Uplift-Downdrop Along Faults - Valleys Flooded by Waters from the Interior) • Youngest (Center) Displays Smooth Terrain with Numerous Craters (Craters Suggest that Surface Is at Least 2 Billion Years Old) Note: This Is a Single Picture – Not a Montage of Three Separate Images
Ganymede • Old, Dark Terrains and Young, Light Terrains - Both Contain Water Ice Mixed with “Dirty Contaminants” • Young Areas Are Brighter (40% Albedo) - Less Contaminated - Just Reverse of Lunar Surface (25% Albedo) • A Few Bright Craters with Crater Rays (Pure Water Splash)
Page 1 and 2: Worlds of Fire and Ice: The Large S
Page 3 and 4: JUPITER JUPITER’S Four Largest Mo
Page 5 and 6: ZEUS and EUROPA Zeus was enamored o
Page 7 and 8: JUPITER and CALLISTO Callisto took
Page 9 and 10: The Large Moons Characteristics •
Page 11 and 12: Impacts and Cratering in the Outer
Page 13 and 14: Crater-Retention Ages on the Satell
Page 15 and 16: Crater-Retention Ages on the Satell
Page 17 and 18: Callisto: Basic Facts • Diameter
Page 19 and 20: First Look at Callisto Voyager
Page 21 and 22: Geology of Callisto • Very Little
Page 23 and 24: • High-Resolution View of the Sur
Page 25 and 26: Ganymede 3rd Closest Moon to Jupite
Page 27: Ganymede: A Moon with a History •
Page 31 and 32: Ganymede Indications of Internal Ac
Page 33 and 34: Anatomy of a Torn Comet Crater Chai
Page 35 and 36: • Smallest Galilean Satellite 3,1
Page 37 and 38: • Little Topographic Relief • S
Page 39 and 40: Europa • Scalloped Arc Shaped Pat
Page 41 and 42: Europa Close-Up of Chaotic Surface
Page 43 and 44: • Magnetic Field Indicates a Coup
Page 45 and 46: Io Density - 3.3 g/cm3 • Higher t
Page 47 and 48: 15.4 Io The Volcanic Moon • Surfa
Page 49 and 50: Io • About Same Distance as Moon
Page 51 and 52: Io • Water, Other Ices, Carbon, N
Page 53 and 54: Geology of Io High Resolution View
Page 55 and 56: Volcanic Eruption on JUPITERR’S M
Page 57 and 58: IO Plume Eruptions • 10 Tons/Sec
Page 59 and 60: Volcanic Eruption on JUPITERR’S M
Page 61 and 62: Io Infrared Emissions from Hot Spot
Page 63 and 64: Dione - Foreground, Tethys and Mima
Page 65 and 66: • Infrared Spectrum of Titan (top
Page 67 and 68: Titan Composition of the Atmosphere
Page 69 and 70: Photochemical Smog • Detached Lay
Page 71 and 72: Voyager Ultraviolet Spectrometer Re
Page 73 and 74: Evolution of the Atmosphere • Met
Page 75 and 76: SATURN Cassini Orbiter Remained in
Page 77 and 78: TITAN Huygens Lander September 2004
Page 79 and 80:
NEPTUNE by Itself - Proved to Be
Page 81 and 82:
Triton (in Foreground) Large Moon
Page 83 and 84:
Triton (in Foreground) Retrograde O
Page 85 and 86:
Triton’s Surface Unique Surface A
Page 87 and 88:
Triton Nitrogen Atmosphere
Page 89 and 90:
• Calculations Based Upon the App
Page 91 and 92:
Evolution of the Atmosphere Geyser
Page 93 and 94:
Triton Moon of NEPTUNE Nitrogen Gey
Page 95 and 96:
15.7 Comparing the Large Satellites
Page 97 and 98:
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Page 109 and 110:
Page 111 and 112:
1994 Galileo Spacecraft Launched To
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2500-15-large satellites

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