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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the border between Chandor and Melas Chasmata. The entire image is landslide deposits.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the border between Chandor and Melas Chasmata. The entire image is landslide deposits.

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the border between Chandor and Melas Chasmata. The entire image is landslide deposits.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22167
Added: 2018-01-16

Views: 15

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the border between Chandor and Melas Chasmata. The entire image is landslide deposits.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of western Candor Chasma. Near the bottom of the image is an impact crater. Impact craters are relatively rare within all the canyons of Valles Marineria.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of western Candor Chasma. Near the bottom of the image is an impact crater. Impact craters are relatively rare within all the canyons of Valles Marineria.

Investigating Mars: Candor Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows part of western Candor Chasma. Near the bottom of the image is an impact crater. Impact craters are relatively rare within all the canyons of Valles Marineria.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22166
Added: 2018-01-15

Views: 41

Investigating Mars: Candor Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows part of western Candor Chasma. Near the bottom of the image is an impact crater. Impact craters are relatively rare within all the canyons of Valles Marineria.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. In the middle of the image is a set of linear ridges and valleys.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. In the middle of the image is a set of linear ridges and valleys.

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. In the middle of the image is a set of linear ridges and valleys.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22165
Added: 2018-01-12

Views: 197

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. In the middle of the image is a set of linear ridges and valleys.

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At this wedge-shaped pit on Mars, the steep slope (or scarp) at the northern edge exposes a cross-section of a thick sheet of underground water ice in this image from NASA's Mars Reconnaissance Orbiter.
At this wedge-shaped pit on Mars, the steep slope (or scarp) at the northern edge exposes a cross-section of a thick sheet of underground water ice in this image from NASA's Mars Reconnaissance Orbiter.

Pit Where a Scarp Exposes an Underground Deposit of Martian Ice

At this wedge-shaped pit on Mars, the steep slope (or scarp) at the northern edge exposes a cross-section of a thick sheet of underground water ice in this image from NASA's Mars Reconnaissance Orbiter.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA22078
Added: 2018-01-11

Views: 1116

Pit Where a Scarp Exposes an Underground Deposit of Martian Ice

At this wedge-shaped pit on Mars, the steep slope (or scarp) at the northern edge exposes a cross-section of a thick sheet of underground water ice in this image from NASA's Mars Reconnaissance Orbiter.

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A cross-section of a thick sheet of underground ice is exposed at the steep slope (or scarp) that appears bright blue in this enhanced-color view from NASA's Mars Reconnaissance Orbiter.
A cross-section of a thick sheet of underground ice is exposed at the steep slope (or scarp) that appears bright blue in this enhanced-color view from NASA's Mars Reconnaissance Orbiter.

Underground Martian Ice Deposit Exposed at Scarp

A cross-section of a thick sheet of underground ice is exposed at the steep slope (or scarp) that appears bright blue in this enhanced-color view from NASA's Mars Reconnaissance Orbiter.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA22077
Added: 2018-01-11

Views: 2454

Underground Martian Ice Deposit Exposed at Scarp

A cross-section of a thick sheet of underground ice is exposed at the steep slope (or scarp) that appears bright blue in this enhanced-color view from NASA's Mars Reconnaissance Orbiter.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22163
Added: 2018-01-11

Views: 102

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the bottom of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the bottom of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

Investigating Mars: Candor Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the bottom of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22162
Added: 2018-01-10

Views: 51

Investigating Mars: Candor Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the bottom of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa. Layered materials are visible throughout the image.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa. Layered materials are visible throughout the image.

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa. Layered materials are visible throughout the image.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22161
Added: 2018-01-09

Views: 54

Investigating Mars: Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa. Layered materials are visible throughout the image.

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Candor Chasma is one of the largest canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa.
Candor Chasma is one of the largest canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa.

Investigating Mars: Candor Chasma

Candor Chasma is one of the largest canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22160
Added: 2018-01-08

Views: 96

Investigating Mars: Candor Chasma

Candor Chasma is one of the largest canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of western Candor and the erosion of a large mesa.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern margin of the summit caldera. This image contains a variety of features representing the major events related to the formation of the volcano.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern margin of the summit caldera. This image contains a variety of features representing the major events related to the formation of the volcano.

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern margin of the summit caldera. This image contains a variety of features representing the major events related to the formation of the volcano.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22159
Added: 2018-01-05

Views: 76

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern margin of the summit caldera. This image contains a variety of features representing the major events related to the formation of the volcano.

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The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern flank of Arsia Mons, along the center of the aligned fracture system.
The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern flank of Arsia Mons, along the center of the aligned fracture system.

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern flank of Arsia Mons, along the center of the aligned fracture system.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22158
Added: 2018-01-04

Views: 138

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southern flank of Arsia Mons, along the center of the aligned fracture system.

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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 miles high, and the summit caldera is 72 miles wide.
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 miles high, and the summit caldera is 72 miles wide.

Investigating Mars: Arsia Mons

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 miles high, and the summit caldera is 72 miles wide.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22157
Added: 2018-01-03

Views: 91

Investigating Mars: Arsia Mons

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 miles high, and the summit caldera is 72 miles wide.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. It is not uncommon for calderas to have 'flat' floors after the final explosive eruption that empties the subsurface magma chamber.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. It is not uncommon for calderas to have 'flat' floors after the final explosive eruption that empties the subsurface magma chamber.

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. It is not uncommon for calderas to have 'flat' floors after the final explosive eruption that empties the subsurface magma chamber.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22156
Added: 2018-01-02

Views: 94

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. It is not uncommon for calderas to have 'flat' floors after the final explosive eruption that empties the subsurface magma chamber.

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The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons at the summit caldera.
The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons at the summit caldera.

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons at the summit caldera.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22155
Added: 2018-01-01

Views: 550

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons at the summit caldera.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southeastern flank of Arsia Mons, including the flat lying flows around the base of the volcano. These flows are located at the bottom of the image.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southeastern flank of Arsia Mons, including the flat lying flows around the base of the volcano. These flows are located at the bottom of the image.

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southeastern flank of Arsia Mons, including the flat lying flows around the base of the volcano. These flows are located at the bottom of the image.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22154
Added: 2017-12-29

Views: 124

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southeastern flank of Arsia Mons, including the flat lying flows around the base of the volcano. These flows are located at the bottom of the image.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northwestern margin of the summit caldera. This image illustrates the many processes that occurred in the formation of the volcano.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northwestern margin of the summit caldera. This image illustrates the many processes that occurred in the formation of the volcano.

Investigating Mars: Arsia Mons

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northwestern margin of the summit caldera. This image illustrates the many processes that occurred in the formation of the volcano.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22153
Added: 2017-12-28

Views: 133

Investigating Mars: Arsia Mons

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northwestern margin of the summit caldera. This image illustrates the many processes that occurred in the formation of the volcano.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern margin of the summit caldera of Arsia Mons. The arcuate features are the faults created by collapse of summit materials.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern margin of the summit caldera of Arsia Mons. The arcuate features are the faults created by collapse of summit materials.

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern margin of the summit caldera of Arsia Mons. The arcuate features are the faults created by collapse of summit materials.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22152
Added: 2017-12-27

Views: 140

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern margin of the summit caldera of Arsia Mons. The arcuate features are the faults created by collapse of summit materials.

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The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons.
The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons.

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22151
Added: 2017-12-26

Views: 148

Investigating Mars: Arsia Mons

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons.

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This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of the western wall of the caldera, revealing the steep walls and linear features associated with the collapse that formed the caldera.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of the western wall of the caldera, revealing the steep walls and linear features associated with the collapse that formed the caldera.

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of the western wall of the caldera, revealing the steep walls and linear features associated with the collapse that formed the caldera.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22150
Added: 2017-12-25

Views: 137

Investigating Mars: Arsia Mons

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of the western wall of the caldera, revealing the steep walls and linear features associated with the collapse that formed the caldera.

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This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.
This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22148
Added: 2017-12-22

Views: 208

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

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This false color image from NASA's 2001 Mars Odyssey spacecraft crosses the entire crater and demonstrates how extensive the dunes are on the floor of Rabe Crater. In this combination of filters 'blue' typically means basaltic sand.
This false color image from NASA's 2001 Mars Odyssey spacecraft crosses the entire crater and demonstrates how extensive the dunes are on the floor of Rabe Crater. In this combination of filters 'blue' typically means basaltic sand.

Investigating Mars: Rabe Crater

This false color image from NASA's 2001 Mars Odyssey spacecraft crosses the entire crater and demonstrates how extensive the dunes are on the floor of Rabe Crater. In this combination of filters 'blue' typically means basaltic sand.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22147
Added: 2017-12-21

Views: 132

Investigating Mars: Rabe Crater

This false color image from NASA's 2001 Mars Odyssey spacecraft crosses the entire crater and demonstrates how extensive the dunes are on the floor of Rabe Crater. In this combination of filters 'blue' typically means basaltic sand.

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This is a false color image of Rabe Crater from NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across. Craters of similar size often have flat floors.
This is a false color image of Rabe Crater from NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across. Craters of similar size often have flat floors.

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater from NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across. Craters of similar size often have flat floors.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22146
Added: 2017-12-20

Views: 197

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater from NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across. Craters of similar size often have flat floors.

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This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.
This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22145
Added: 2017-12-19

Views: 127

Investigating Mars: Rabe Crater

This is a false color image of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft. In this combination of filters 'blue' typically means basaltic sand. Rabe Crater is 108 km (67 miles) across.

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This image from NASA's 2001 Mars Odyssey spacecraft shows Rabe Crater. The majority of the dune field in Rabe Crater consists of a sand sheet with dune forms on the surface. The sand sheet is where a thick layer of sand has been concentrated.
This image from NASA's 2001 Mars Odyssey spacecraft shows Rabe Crater. The majority of the dune field in Rabe Crater consists of a sand sheet with dune forms on the surface. The sand sheet is where a thick layer of sand has been concentrated.

Investigating Mars: Rabe Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows Rabe Crater. The majority of the dune field in Rabe Crater consists of a sand sheet with dune forms on the surface. The sand sheet is where a thick layer of sand has been concentrated.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22144
Added: 2017-12-18

Views: 103

Investigating Mars: Rabe Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows Rabe Crater. The majority of the dune field in Rabe Crater consists of a sand sheet with dune forms on the surface. The sand sheet is where a thick layer of sand has been concentrated.

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This image captured by NASA's 2001 Mars Odyssey spacecraft provides another instance where the topography of the upper floor material affects the winds and dune formation.
This image captured by NASA's 2001 Mars Odyssey spacecraft provides another instance where the topography of the upper floor material affects the winds and dune formation.

Investigating Mars: Rabe Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft provides another instance where the topography of the upper floor material affects the winds and dune formation.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22143
Added: 2017-12-15

Views: 166

Investigating Mars: Rabe Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft provides another instance where the topography of the upper floor material affects the winds and dune formation.

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