Media Information

 
 
 
Collection:
NASA Solarsystem Collection
title:
Ganymede Topography
description:
This perspective view, simulating a low altitude flight over the surface of Ganymede, was made possible by topographic analysis of stereo images of the Sippar Sulcus region. Such a view was made possible when Galileo passed Ganymede in May 1997, providing a virtual second "eye" to Voyager's first view in 1979.

Because this view covers a large area, it reveals that younger, smoother terrains are low-lying relative to older, heavily faulted terrains. The consistently low elevations of these smooth deposits has been cited as evidence for flooding of parts of Ganymede by low-viscosity lavas, most likely liquid water or water-ice slush.

This view is centered at 35 degrees south, 180 degrees west. The smallest features visible are roughly 350 to 400 meters (1,150 to 1,300 feet) across.

This image was prepared by the Lunar and Planetary Institute, Houston, and included in a report by Dr. Paul Schenk et al. in the March 1, 2001, edition of the journal Nature.

*Image Credit*: NASA and Lunar and Planetary Institute
keywords:
Solar System Exploration
keywords:
SSE
keywords:
Space
keywords:
NASA
keywords:
National Aeronautics and Space Administration
keywords:
JPL
keywords:
Jet Propulsion Laboratory
keywords:
Planets
facet_what:
Voyager
facet_what:
Galileo
facet_what:
STEREO
facet_what:
Ganymede
facet_what:
Ganymede (Jupiter Moon)
facet_where:
Jet Propulsion Laboratory
facet_where:
Ganymede
facet_where:
Jet Propulsion Laboratory (JPL)
facet_when:
1979
facet_when:
May 1997
facet_when:
March 1, 2001
facet_when_year:
2001
facet_when_year:
1979
facet_when_year:
1997
UID:
SPD-SLRSY-2006
original url:

Ganymede Topography