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Ocean Lurks Deep in Ganymede, Galileo Finds
Galileo Swoops In Close to Jupiter's Moon Ganymede
Auroras Shed Light on Jupiter's Moon Ganymede
Io's Volcanoes Revealed in Sharp Detail
Two-Faced Moon: Did Ice Volcanoes Pave Ganymede?
By Robert Roy Brittt
Senior Science Writer
posted: 07:00 am ET
01 March 2001

Ice Volcanoes Give Craggy Ganymede a Partial Baby Face

Jupiter's moon Ganymede, the largest moon in the solar system, has two faces. One is dark, craggy and ancient; the other is bright, presumably younger, and long thought to be smooth as baby's skin.

Scientists have been puzzled by the difference for 22 years, since the first Voyager spacecraft images were returned.

New research, which combined the Voyager images with some recent Galileo probe photographs to create fresh "stereo" views, shows that the brightest, smoothest areas of Ganymede may have been created by ice volcanoes.

These eruptions of presumably water lava, made of melted ice and pulled to the surface as the giant moon gravitationally wrestled with Jupiter's other satellites, have filled in low-lying areas.

"This result seems to confirm that molten crustal and mantle material [in the form of water] was fairly plentiful and that Ganymede must have undergone a period of partial melting," said Paul Schenk of the Lunar and Planetary Institute in Houston. Schenk and his colleagues present the findings in the March 1 issue of the journal Nature.

Previous Galileo images suggest that Ganymede, like its sibling Jovian moons Callisto and Europa, is covered by a crust of frozen ocean. Some scientists say those crusts harbor water beneath. Data returned last year by the Galileo spacecraft indicated that Ganymede's icy outer shell may cover less water ice than some have expected, but the evidence for at least a global layer is strong.

Ice volcanoes?

The volcanoes are not the same as the typical terrestrial variety, but they operate similarly. "Volcanism involves the melting of solid crust or mantle," Schenk told SPACE.com. "In this case, the crust happens to be ice."

Though the ice volcanoes spew melted water, they are unlike Yellowstone's Old Faithful or an undersea hydrothermal vent, both of which recycle surface water that is heated by hot rocks. Water magma on Ganymede originates deep within the moon, in the same way that molten volcanic rock, called magma, does on Earth.

This image, showing an area roughly 44 miles (70 kilometers) wide, shows how flowing material from an ice volcano seems to have butted up against higher, rugged terrain.

Schenk described the resulting smooth structures as looking something like the lunar mare. A visitor standing on Ganymede's surface would see vast flats that would appear virtually unblemished. One trough extends an estimated 600 miles (900 kilometers), roughly the distance between St. Louis and New Orleans. The features, though younger than much of the surface, are estimated to be a billion years old.

"This is the most persuasive evidence yet that there is volcanism on Ganymede," said Louise Prockter, a Johns Hopkins University researcher who was not involved in the study. "I think [the researchers] are definitely onto something."

But Prockter said in a telephone interview that the smooth areas appear very well confined -- uncharacteristic for lava flows. And, she said, she would have expected to see more evidence of volcanism in more places than the researchers uncovered.

The Nature paper discusses two areas that appear to have been resurfaced by volcanism, and Schenk said another extensive region was spotted at Ganymede's south pole. Several other areas suggest similar topography, he said. Volcanism typifies the surface of another Jovian moon -- Io.

Next page: Stereo images and dancing moons

1 2    | >> Continue with this story >

 

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