Media Information

 
 
 
Collection:
NASA Astronomy Picture of the Day Collection
Title:
Young Martian Terrain
Explanation:
What caused the pits, ridges, and gullies on otherwise smooth Martian terrain? One hypothesis [ http://www.brown.ed…] is water. The lack of craters [ http://antwrp.gsfc.…] at this mid-latitude location indicates that the terrain is quite young by geological standards, perhaps only 100,000 years old. Were the terrain since saturated by water ice, that ice would soon evaporate into the thin Martian air [ http://www.pbs.org/…]. Left over, however, might be fragile cake [ http://www.cakereci…]-like sand [ http://www.paccd.cc…] that can be broken up by wind into pits and ridges. Consequences of this hypothesis [ http://news.bbc.co.…] include that even the Martian equator [ http://antwrp.gsfc.…] undergoes epochs of relative wet and dry, and that future spacefarers might be able to find water [ http://antwrp.gsfc.…] (ice) in a relatively mild climate near the Martian [ http://www.marsdail…] equator. Pictured above [ http://ida.wr.usgs.…] is young-ridged terrain that also shows evidence of a downhill flow [ http://antwrp.gsfc.…].
Credit and Copyright:
keyword:
Jupiter
keyword:
Callisto
keyword:
life
facet_where:
Mars
facet_where:
Jupiter
facet_where:
Callisto
facet_where:
Goddard Space Flight Center (GSFC)
facet_where:
Jet Propulsion Laboratory (JPL)
facet_what:
Mars
facet_what:
Jupiter
facet_what:
Callisto
facet_what:
Mars Global Surveyor Orbiter (MGS)
original url:
UID:
SPD-APOD-ap010801

Young Martian Terrain