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PIA05154: Targeting a Hematite-rich Terrain
Target Name: Mars
Is a satellite of: Sol (our sun)
Mission: 2001 Mars Odyssey
Mars Global Surveyor (MGS)
Mars Exploration Rover (MER)
Spacecraft: 2001 Mars Odyssey
Mars Global Surveyor Orbiter
Opportunity
Instrument: Thermal Emission Imaging System
Thermal Emission Spectrometer
Product Size: 640 samples x 480 lines
Produced By: Arizona State University
Full-Res TIFF: PIA05154.tif (922.8 kB)
Full-Res JPEG: PIA05154.jpg (52.31 kB)

Click on the image to download a moderately sized image in JPEG format (possibly reduced in size from original).

Original Caption Released with Image:
This image shows the abundance and location of the mineral grey hematite at the Mars Exploration Rover Opportunity's landing site, Meridiani Planum, Mars. Opportunity is targeted to land somewhere inside the oval, approximately 71 kilometers (45 miles) long, on January 24, 2004 Pacific Standard Time. The background surface image of Meridiani Planum is a mosaic of daytime infrared images acquired by the thermal emission imaging system instrument on NASA's Mars Odyssey Orbiter. Superimposed on this image mosaic is a rainbow-colored map showing the abundance and location of grey hematite, as mapped by the thermal emission spectrometer on NASA's Mars Global Surveyor orbiter. Red and yellow indicates higher concentrations, whereas green and blue areas denote lower levels. On Earth, grey hematite is an iron oxide mineral that typically forms in the presence of liquid water. The rover Opportunity will study the martian terrain to determine whether liquid water was present in the past when rocks were being formed, and ultimately will address whether that past environment was favorable for life.
Image Credit:
NASA/JPL/ASU


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