Portal:Jupiter/Moon/4

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Ganymede[edit]

A true color image of Ganymede is acquired by the Galileo spacecraft on June 26, 1996. Credit: NASA/JPL.
This is global pictoral map of Ganymede. Credit: National Oceanic and Atmospheric Administration/USGS.

"If Ganymede rotated around the Sun rather than around Jupiter, it would be classified as a planet."[1]

The Galilean Moons is a "name given to Jupiter's four largest moons, Io, Europa, Callisto & Ganymede. They were discovered independently by Galileo Galilei and Simon Marius."Cite error: Invalid <ref> tag; invalid names, e.g. too many

"Ganymede has a very distinct surface with bright and dark regions. The surface includes mountains, valleys, craters and lava flows. The darker regions are more heavily littered with craters implying that those regions are older. The largest dark region is named Galileo Regio and is almost 2000 miles [3200 km] in diameter. The lighter regions display extensive series of troughs and ridges, thought to be a result of tectonic movement."[1]

"A notable attribute of the craters on Ganymede is that they are not very deep and don’t have mountains around the edges of them as can normally be seen around craters on other moons and planets. The reason for this is that the crust of Ganymede is relatively soft and over a geological time frame has flattened out the extreme elevation changes."[1]

References[edit]

  1. 1.0 1.1 1.2 Bjorn Jonsson and Steve Albers (October 17, 2000). Ganymede (Jupiter moon). NOAA. Retrieved 2012-07-01.