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30th Anniversary of The Planetary Society
 

Space Topics: Mars Reconnaissance Orbiter

The Year in Pictures: 2007

Mars Reconnaissance Orbiter: Nili Fossae Trough

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Nili Fossae Trough from CRISM and HiRISE
Credit: NASA / JPL / U. Arizona / JHUAPL

The blooming purples and greens in this image of the west wall of Nili Fossae, northwest of Mars' Isidis basin, map the signatures of minerals in the Martian bedrock that scientists hope to sample with a future rover. The image represents the best that two of Mars Reconnaissance Orbiter's instruments—CRISM and HiRISE—have to offer. Together, these instruments are performing detailed mapping of all the potential landing sites for the 2009 Mars Science Laboratory. Nili Fossae Trough is just one of half a dozen sites being considered.

The HiRISE camera is taking photos of Mars with resolutions as high as 25 centimeters (about 10 inches) per pixel. With such sharp images, planners for future landed missions can name every large rock in their landing site before they even arrive at Mars. This image reveals the floor of Nili Fossae (lower right) paved with volcanic materials; "shark's-tooth" dunes of dark basaltic sand march parallel to the northwest wall of the trough. An ancient flooding event cut into that wall, carving a landscape of mesas and buttes and exposing ancient bedrock.

At the same time, the CRISM imaging spectrometer is slicing the colors of Mars into an unprecedented 544 different bands of the electromagnetic spectrum. Because of such high spectral resolution, CRISM workers can search for the fingerprints of specific minerals on the Martian surface. For instance, in this image, the blues and magentas map locations where CRISM sees the spectral signature of phyllosilicates, minerals that form when igneous minerals such as pyroxene are altered in the presence of water. Greenish colors imply the presence of low-calcium pyroxene, a mineral that formed very early in Mars' history with the hottest volcanic activity. A lander sent to one of these greenish areas has the potential to sample Mars' youth.