Memphis Facula
Memphis Facula /ˈmɛmfɪs ˈfækjʊlə/ is a palimpsest, or "ghost crater", on Ganymede, the largest of the Jovian satellites.
About 360 km across, it is situated in the southwestern part of Galileo Regio, a huge almost circular dark region in Ganymede's northern hemisphere. Although almost level today, it is a relic of a massive impact and once was a deep impact crater whose walls have slumped and its floor has risen isostatically, smoothing out the remaining topography with slush.
The morphology of the larger palimpsests like Memphis Facula suggests that Ganymede's icy crust at the time of impact was about 10 km thick and was penetrated by the impact, allowing the slush and fluid beneath to fill and level out the crater.
See also
References
- ^ "Ganymede: Nidaba". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2014-06-21.
- ^ "Ganymede: Memphis Facula". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2012-03-12.
- ^ Harland, D. M. (1 October 2000). Jupiter Odyssey: The Story of NASA's Galileo Mission. Springer. p. 136. ISBN 978-1-85233-301-0. OCLC 44461919.
 | This article about an extraterrestrial geological feature is a stub. You can help Wikipedia by expanding it. |
| Geology |
|  | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Exploration |
| |||||||||||||
| Other | ||||||||||||||
