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This oblique view of Gale Crater shows the landing site and the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The landing site is in the smooth area in front of the mound.
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11.10.2011

Canyons on Mountain Inside Gale Crater, Annotated

This oblique view of Gale Crater shows the landing site and the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The landing site is in the smooth area in front of the mound.

Gale Crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor.

The landing site contains material washed down from the wall of the crater, which will provide scientists with the opportunity to investigate the rocks that form the bedrock in this area. The landing ellipse also contains a rock type that is very dense and very bright colored; it is unlike any rock type previously investigated on Mars. It may be an ancient playa lake deposit, and it will likely be the mission's first target in checking for the presence of organic molecules.

The area of top scientific interest for Mars Science Laboratory is at the base of the mound, just at the edge of the landing ellipse and beyond a dark dune field. Here, orbiting instruments have detected signatures of both clay minerals and sulfate salts. Scientists studying Mars have several important hypotheses about how these minerals reflect changes in the Martian environment, particularly changes in the amount of water on the surface of Mars. The Mars Science Laboratory rover, Curiosity, will use its full instrument suite to study these minerals and how they formed to give us insights into those ancient Martian environments. These rocks are also a prime target in checking for organic molecules, since these environments may have been habitable -- able to support microbial life.

Canyons were cut in the mound through the layers containing the clay minerals and sulfate salts after deposition of the layers. These canyons, much like the Grand Canyon in Arizona, expose layers of rock representing tens or hundreds of millions of years of environmental change. Over its two-year primary mission, the rover may be able to investigate these layers in a canyon close to the landing ellipse (shown by an example rover path), gaining access to a long history of environmental change on the planet. Above this region, the material on the mound has spectroscopic characteristics similar to dusty areas of Mars, indicating it may be composed of dust that has been cemented into rock.

This three-dimensional perspective view was created using visible-light imaging by the Thermal Emission Imaging System camera on NASA's Mars Odyssey orbiter. Three-dimensional information was derived from observations by the Mars Orbiter Laser Altimeter, which flew on NASA's Mars Global Surveyor orbiter. Color information is derived from color imaging of portions of the scene by the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter. The vertical dimension is not exaggerated.

The Mars Science Laboratory spacecraft is being prepared for launch during the period Nov. 25 to Dec. 18, 2011. In a prime mission lasting one Martian year -- nearly two Earth years -- after landing, researchers will use the rover's tools to study whether the landing region has had environmental conditions favorable for supporting microbial life and for preserving clues about whether life existed.

NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Science Laboratory Project for NASA's Science Mission Directorate in Washington. Arizona State University, Tempe, operates the Thermal Emission Imaging System. The Mars Orbiter Laser Altimeter was operated by NASA Goddard Space Flight Center, Greenbelt, Md. The University of Arizona, Tucson, operates the High Resolution Science Imaging Experiment. JPL manages Mars Odyssey and Mars Reconnaissance Orbiter for NASA's Science Mission Directorate.

Image Credit: NASA/JPL-Caltech/ASU/UA

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