2500-15-large satellites

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ZEUS and Io Io was a priestess of Hera in Argo, a nymph who was seduced by Zeus, who changed her into a heifer to escape detection. Her mistress Hera set everwatchful Argus Panoptes to guard her, but Hermes was sent to distract the guardian and slay him. Heifer Io was loosed to roam the world, stung by a maddening gadfly sent by Hera, and wandered to Egypt Zeus and Io c. <strong>15</strong>30 by Antonio Allegri da Correggio 1489 - <strong>15</strong>34 Rococo
ZEUS and EUROPA Zeus was enamored of Europa and decided to seduce or ravish her. He transformed himself into a tame white bull and mixed in with her father's herds. While Europa and her female attendants were gathering flowers, she saw the bull, caressed his flanks, and eventually got onto his back. Zeus took that opportunity and ran to the sea and swam, with her on his back, to the island of Crete. He then revealed his true identity, and Europa became the first queen of Crete. The Abduction of Europa 1632 by Rembrandt 1606-1669 Dutch Golden Age
Page 1 and 2: Worlds of Fire and Ice: The Large S
Page 3: JUPITER JUPITER’S Four Largest Mo
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 and 28: Ganymede: A Moon with a History •
Page 29 and 30: Ganymede • Old, Dark Terrains and
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:
Page 99 and 100:
Page 101 and 102:
Page 103 and 104:
Page 105 and 106:
Page 107 and 108:
Page 109 and 110:
Page 111 and 112:
1994 Galileo Spacecraft Launched To
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