This image shows relatively bright mounds, hundreds of meters in size, scattered throughout darker and diverse surfaces in Chryse Planitia. The largest shows a central pit, similar to the collapsed craters in some Earth volcanoes.

September 4, 2018

Map Projected Browse Image
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This image was acquired on May 15, 2018, by NASA's Mars Reconnaissance Orbiter. This observation shows relatively bright mounds scattered throughout darker and diverse surfaces in Chryse Planitia. These mounds are hundreds of meters in size. The largest of the mounds shows a central pit, similar to the collapsed craters found at the summit of some volcanoes on Earth. The origins of these pitted mounds or cratered cones are uncertain. They could be the result of the interaction of lava and water, or perhaps formed from the eruption of hot mud originating from beneath the surface.

These features are very interesting to scientists who study Mars, especially to those involved in the ExoMars Trace Gas Orbiter mission. If these mounds are indeed mud-related, they may be one of the long sought-after sources for transient methane on Mars.

The map is projected here at a scale of 50 centimeters (19.7 inches) per pixel. [The original image scale is 60.5 centimeters (23.8 inches) per pixel (with 2 x 2 binning); objects on the order of 181 centimeters (71.3 inches) across are resolved.] North is up.

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Credit

NASA/JPL-Caltech/Univ. of Arizona

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