Polar cap formation on Ganymede

• Main Authors: Pilcher, C. B., Shaya, E. J.
• Format: Other/Unknown Material
• Language: unknown
• Published: 1985
• Subjects: 91; Ganymede; Ice Sheet
• Online Access: http://ntrs.nasa.gov/search.jsp?R=19850015175

Since thermal migration is not an effective mechanism for water transport in the polar regions at the Galilean satellites, some other process must be responsible for the formation of Ganymede's polar caps. It is proposed that Ganymede's polar caps are the optical manifestation of a process that began with the distribution of an ice sheet over the surface of Ganymede. The combined processes of impact gardening and thermal migration led, in regions at latitudes less than 40 to 45 deg., to the burial of some fraction of this ice, the migration of some to the polar caps margins, and a depletion of free ice in the optical surface. At higher latitudes, no process was effective in removing ice from the optical surface, so the remanants of the sheet are visible today.