Volcanic Terrain on Mercury
Explanation:
Why are many large craters on Mercury relatively smooth inside?
Recent images from the robotic
MESSENGER
spacecraft that flew by Mercury last October show previously uncharted regions
of
Mercury that have large craters with an internal smoothness similar to the
maria on Earth's own Moon.
Therefore, like
our Moon's maria, these
craters on Mercury are thought to have been flooded by
lava floes that are old but not as old as the surrounding more highly cratered surface.
The
above image mosaic
of the western limb of Mercury was created by MESSENGER as it approached the Solar
System's innermost planet last October.
Old and heavily textured terrain runs across much of the image bottom, while across
the middle left lies comparatively smooth
impact basins
where small craters may appear similar at first to protruding hills.
MESSENGER will buzz
past Mercury
again next year before entering orbit in 2011.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
