This image was acquired by the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter on April 18, 2017, at 14:04 local Mars time. It reminded the HiRISE team of the rugged and open terrain of a stark shore-line, perhaps of the British Isles. A close-up in enhanced color produces a striking effect, giving the impression of a cloud-covered cliff edge with foamy waves crashing against it.
The reality is that the surface of Mars is much dryer than our imaginations might want to suggest. This is only a tiny part of a much larger structure; an inverted crater—a crater that has been infilled by material that is more resistant to erosion than the rocks around it—surrounded by bluish basaltic dunes. The edge of these elevated light-toned deposits are degraded, irregular and cliff-forming.
Dunes visible below the cliff, give the impression of an ocean surface, complete with foam capped waves crashing against the “shore line,” demonstrating the abstract similarity between the nature of a turbulent ocean and a Martian dune field.
Meridiani Planum has an overall smooth terrain, which starkly contrasts with the more common boulder- and crater-laden landscapes observed over much of the rest of Mars. This makes it relatively younger in character than many other areas of the planet. Meridiani is one of the Mars Exploration Rover landing sites, and, is known for its layers and sediments. The orbital detection of hematite was one of the main reasons for sending Opportunity to this area.
Salt-bearing rocks—also called sulphates—were observed in the very first image from Opportunity, so perhaps it’s apt that this HiRISE image reminds us of the turmoil and rugged beauty of a cliff-face, a coastline, being worn down by a relentless sea.
The reality is that the surface of Mars is much dryer than our imaginations might want to suggest. This is only a tiny part of a much larger structure; an inverted crater—a crater that has been infilled by material that is more resistant to erosion than the rocks around it—surrounded by bluish basaltic dunes. The edge of these elevated light-toned deposits are degraded, irregular and cliff-forming.
Dunes visible below the cliff, give the impression of an ocean surface, complete with foam capped waves crashing against the “shore line,” demonstrating the abstract similarity between the nature of a turbulent ocean and a Martian dune field.
Meridiani Planum has an overall smooth terrain, which starkly contrasts with the more common boulder- and crater-laden landscapes observed over much of the rest of Mars. This makes it relatively younger in character than many other areas of the planet. Meridiani is one of the Mars Exploration Rover landing sites, and, is known for its layers and sediments. The orbital detection of hematite was one of the main reasons for sending Opportunity to this area.
Salt-bearing rocks—also called sulphates—were observed in the very first image from Opportunity, so perhaps it’s apt that this HiRISE image reminds us of the turmoil and rugged beauty of a cliff-face, a coastline, being worn down by a relentless sea.
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.
Image Credit: NASA/JPL/University of Arizona
Caption: Jon Kissi, Livio L. Tornabene, Zach Morse, Eric Pilles and Gavin Tolometti
Caption: Jon Kissi, Livio L. Tornabene, Zach Morse, Eric Pilles and Gavin Tolometti
Last Updated: June 22, 2017
Editor: Sarah Loff
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