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Layered Fill

The floor of this unnamed crater in Aonia Terra has been filled with multiple layers of material.

June 25, 2007

The floor of this unnamed crater in Aonia Terra has been filled with multiple layers of material.

Credits

NASA/JPL-Caltech/ASU

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Martian surface frost, made up largely of carbon dioxide, appears blueish-white in these images from the Thermal Emission Imaging System (THEMIS) camera aboard NASA’s 2001 Odyssey orbiter. THEMIS t...
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Martian surface frost, made up largely of carbon dioxide, appears blueish-white in these images from the Thermal Emission Imaging System (THEMIS) camera aboard NASA’s 2001 Odyssey orbiter. THEMIS takes images in both visible light perceptible to the human eye and heat-sensitive infrared.
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The annotated area of Mars in this illustration holds near-surface water ice that would be easily accessible for astronauts to dig up. The water ice was identified as part of a map using data from ...
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The annotated area of Mars in this illustration holds near-surface water ice that would be easily accessible for astronauts to dig up. The water ice was identified as part of a map using data from NASA orbiters.
Water Ice Marked on Mars Globe
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Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture.
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Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 270 miles in diameter, almost 12 mi...
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Morning clouds fill Coprates Chasma on Mars in this Nov. 25, 2015, image from the THEMIS camera on NASA's Mars Odyssey. No orbiter systematically observed Mars in morning sunlight before 2015. The clouds appear blue because ice particles in them scatter blue light more strongly than other colors.
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A small basin (center foreground) lies below the southern rim of Melas Chasma, part of Valles Marineris.
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A small basin (center foreground) lies below the southern rim of Melas Chasma, part of Valles Marineris.
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If a meteorite breaks in two shortly before hitting the ground, the typical bowl shape of a single impact crater becomes doubled.
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The dunes and dust devil tracks in this VIS image are located on the plains of Planum Chronium.
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The dunes and dust devil tracks in this VIS image are located on the plains of Planum Chronium.
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Artist rendering of commercial Mars satellites providing communications back to Earth.
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This image is located near the boundary between Syrtis Major and Isidis Planitia. The top of the image shows rough material that has eroded away from the lower portion of the image, revealing an un...
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This image is located near the boundary between Syrtis Major and Isidis Planitia. The top of the image shows rough material that has eroded away from the lower portion of the image, revealing an underlying surface that has many small craters. It also reveals an ancient flow lobe that is barely discernable, crossing the southern part of the image (this flow lobe is much easier to see as a smooth region in the context image).
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This is an image of ice-rich clouds in false color, taken by the Odyssey satellite orbiting Mars.
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This image from NASA's Mars Odyssey shows a crater from a double impact - two meteors hitting simultaneously. The two meteors would have started as a single object and, at some point prior to impact, separated into two parts.
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Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike.
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This image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
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This image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
Acidalia Planitia Crater
This image from NASAs Mars Odyssey shows lava flows from Alba Mons, and a tectonic graben called Cyane Fossae.
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This image from NASAs Mars Odyssey shows lava flows from Alba Mons, and a tectonic graben called Cyane Fossae.
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Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture. The frame is about 14 kilometers (9 miles) wide.
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Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from five instruments on three different NASA Mars orbiters, including physical properties from THEMIS (left) and mineral information from CRISM (right).
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