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One of the most spectacular results of the Mars Global Surveyor
(MGS) Mars Orbiter Camera (MOC) mission thus far has been the observation
of many layered outcrops in various locations across the surface
of the red planet. On Earth, layered rocks are used by geologists
to decipher the history of the planet's surface over time scales
of billions of years. Layered rock on Mars might one day offer the
same opportunity for intense examination by geologists working "in
the field."
The thickest sequences of layered material are exposed in the deepest
canyons--that is, in the walls of the Valles Marineris--a system
of canyons and troughs that would stretch from Los Angeles to New
York if it occurred on Earth. MOC image 8003 (above) shows a flat-topped
ridge in the middle of Coprates Chasma in the eastern Valles Marineris
system. The highest terrain in the image is the relatively smooth
plateau near the center of the frame. Slopes descend to the north
and south (upper and lower part of image, respectively) in broad,
debris-filled gullies with intervening, rocky spurs. Multiple rock
layers, varying from a few to a few tens of meters thick, are visible
in the steep slopes on the spurs and gullies. Layered rocks on Earth
form from sedimentary processes (such as those that formed the layered
rocks now seen in Arizona's Grand Canyon) and volcanic processes
(such as layering seen in the Waimea Canyon on the island of Kauai).
Both origins are possible for the martian layered rocks seen in
this image. In either case, the total thickness of the layered rocks
seen in this image implies a complex and extremely active early
history for geologic processes on Mars.
Photo information and credit: MOC image 8003
was taken on January 1, 1998. The image was also the subject of
two earlier MGS MOC releases, the first on February 2, 1998 and
the second on March 13, 1998. The image was taken as a monochrome
(black and white) picture; color was derived from lower spatial-resoluion
Viking images taken during the 1970s. The image center is near 14.5°S,
55.8°W, and the scene covers an area approximately 9.8 km by 17.3
km (6.1 mi by 10.7 mi). North is up, illumination is from the left.
Caption and image courtesy of Malin Space Science Systems.
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