Refiner of Gold Creations'

Solar System -- Ganymede

Third Galilean Moon
of the Fifth Planet
Ganymede: A Wrinkle in Jupiter's system
  • Jupiter's largest satellite.
  • Largest moon and 8th largest body in Solar System
  • Average distance from Jupiter is 1,070,400 km.
  • Revolution is 7 days 3 hours.
  • Diamter is 5,280 km
  • Composed of ice and carbonaceous silicates.
  • One face pointing toward planet (synchronous).
  • View from Earthbound telescopes is as a pinhead with vague markings.
  • Geology of this ice-dominated moon revealed by Voyagers 1 & @ in 1979.
    • Ice and water assume geologic roles similar to Earth's rock and lava.
    • A "magma" of watery materiall erupts from internal heat.
    • WHen the "magma" freezes, the fresh surface appears as bright ice.
    • Dark with heavily cratered areas, grooved terrain and a system of faults.
  • Mean density higher than density of pure ice.
    • Density lower than most rock types.
    • Indicative of a rock component, but not pure rock or ice.
    • Most rock has probably shifted toward the moon's center.
    • Core is likely to be rocky with an ice mantle.
  • Earthbound scientists expected Voyager probes to reveal and ancient static surface pocked with impact craters.
    • Ganymede does have large regions of ancient craters.
    • Crater regions broken by swaths of young furrows.
    • Younger formations believed to be youthful flows and ice squeeze-ups.
    • Older terrain is dark, suggesting that the ice component has been vaporized by meteor impact.
  • Giant arcs of parallel furrows cross the cratered surface.
    • Furrows are few kilometers wide and hundreds of kilometers long.
    • Appear to be fragments of giant, ancient impact craters.
    • Known as "multi-ring" basins, created by the largest impacts.
    • Such impacts leave behind multiple concentric rings of cliffs hundreds of kilometers across.
    • Resemble a bull-eye of a target.
    • Similar, more complete, multi-ring systems appear on Mercury, our Moon and Callisto.
  • Ganymede's surface resembles a giant jigsaw puzzle.
    • Ancient craters have been broken or shifted by resurfacing processes.
    • Most of the original picture is preserved.
    • Some parts replaced by swaths of fresher ice.
    • Newer regions appear as lighter, wandering bands among dark polygonal regions of craters.
    • Lighter regions traverse by intricate systems of narrow fissures.
    • Narrow fissures arranged as parallel streaks, in turn broken by craters.
  • Appearance of surface pattern suggestive of an original dark crust.
    • This crust appears to have been broken apart by expansion.
    • Ganymede's equivalent of lava, water, was allowed to flow onto the surface.
    • The water then froze into ice floes.
    • Further eruptions along fissures squeezed out new parallel ridges of ice.
    • The same phenomenon also occurs in Earth's Acrtic ice floes.
    • Ganymede displays the process of plate tectonics, not as dynamic as on Earth.
    • Ganymede's interior may be warm, but not as hot as Earth's.
    • The ice "lithosphere" at the surface may have broken into "plates," but the plates have only jostled one another.
    • Little scattered pieces hseem to have moved tens of kilometers, offsetting craters and faults.
    • No large-scale motions or collisions and no folded mountain ranges like the ones found on Earth.
  • Other interesting features of Ganymede:
    • Whitish polar caps extend down to latitudes about 40 degrees.
    • Caps may mark condensation of water vapor escaping from fractures around the planet.
    • Most fresh craters display bright radiating rays of ejecta blown onto the surrounding surface.
    • These craters probably blew away the darkish surface soil to expose fresher ice.
    • Occasional small craters, typically 10 to 20 kilometers (6 to 12 miles) across and a few kilometers deep, have dark rays.
    • Small craters may reflect a layered structure beneath Ganymede's surface.
    • Should surface layers melt or if "volcanic water" gushes out along with soil, the soil would sink before the resulting oceans froze.
    • Therefore craters need penetrate a few kilometers to tap layers of blackish soil.
    • Ganymede's surface may contain intricate sedimentary layers of ice and rock.
  • Ganymede provides a simple model in which ice, one of the prime geologic constituents, interacts with rocky material.
  • Remnants of cratered "plates," partially erased by fractures and ice flows, testify to the forces that shape all worlds.

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Refiner of Gold Creations
1998 Solar System Facts
Created by EMC on 6/23/1997. Updated 5/4/2005.