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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the Nili Patera dune field. Winds are blowing the dunes across a rough surface of regional volcanic lava flows.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the Nili Patera dune field. Winds are blowing the dunes across a rough surface of regional volcanic lava flows.

Investigating Mars: Nili and Meroe Paterae

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the Nili Patera dune field. Winds are blowing the dunes across a rough surface of regional volcanic lava flows.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22001
Added: 2017-10-09

Views: 154

Investigating Mars: Nili and Meroe Paterae

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the Nili Patera dune field. Winds are blowing the dunes across a rough surface of regional volcanic lava flows.

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This diagram illustrates an interpretation for the origin of some deposits in the Eridania basin of southern Mars as resulting from seafloor hydrothermal activity more than 3 billion years ago.
This diagram illustrates an interpretation for the origin of some deposits in the Eridania basin of southern Mars as resulting from seafloor hydrothermal activity more than 3 billion years ago.

A Geologic Model for Eridania Basin on Ancient Mars

This diagram illustrates an interpretation for the origin of some deposits in the Eridania basin of southern Mars as resulting from seafloor hydrothermal activity more than 3 billion years ago.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
ID#: PIA22060
Added: 2017-10-06

Views: 986

A Geologic Model for Eridania Basin on Ancient Mars

This diagram illustrates an interpretation for the origin of some deposits in the Eridania basin of southern Mars as resulting from seafloor hydrothermal activity more than 3 billion years ago.

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The Eridania basin of southern Mars is believed to have held a sea about 3.7 billion years ago, with seafloor deposits likely resulting from underwater hydrothermal activity.
The Eridania basin of southern Mars is believed to have held a sea about 3.7 billion years ago, with seafloor deposits likely resulting from underwater hydrothermal activity.

Estimated Water Depths in Ancient Martian Sea

The Eridania basin of southern Mars is believed to have held a sea about 3.7 billion years ago, with seafloor deposits likely resulting from underwater hydrothermal activity.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
ID#: PIA22059
Added: 2017-10-06

Views: 881

Estimated Water Depths in Ancient Martian Sea

The Eridania basin of southern Mars is believed to have held a sea about 3.7 billion years ago, with seafloor deposits likely resulting from underwater hydrothermal activity.

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This image from NASA's Mars Reconnaisance Orbiter shows a portion of the Eridania region of southern Mars with fractured, dismembered blocks of deep-basin deposits that have been surrounded and partially buried by younger volcanic deposits.
This image from NASA's Mars Reconnaisance Orbiter shows a portion of the Eridania region of southern Mars with fractured, dismembered blocks of deep-basin deposits that have been surrounded and partially buried by younger volcanic deposits.

Possible Floor of an Ancient Martian Sea

This image from NASA's Mars Reconnaisance Orbiter shows a portion of the Eridania region of southern Mars with fractured, dismembered blocks of deep-basin deposits that have been surrounded and partially buried by younger volcanic deposits.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: Context Camera (CTX)
ID#: PIA22058
Added: 2017-10-06

Views: 1917

Possible Floor of an Ancient Martian Sea

This image from NASA's Mars Reconnaisance Orbiter shows a portion of the Eridania region of southern Mars with fractured, dismembered blocks of deep-basin deposits that have been surrounded and partially buried by younger volcanic deposits.

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This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. The brighter materials at the bottom of the image are layered deposits. It is unknown how deep these canyon deposits were when they formed.
This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. The brighter materials at the bottom of the image are layered deposits. It is unknown how deep these canyon deposits were when they formed.

Investigating Mars: Coprates Chasma

This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. The brighter materials at the bottom of the image are layered deposits. It is unknown how deep these canyon deposits were when they formed.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22000
Added: 2017-10-06

Views: 142

Investigating Mars: Coprates Chasma

This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. The brighter materials at the bottom of the image are layered deposits. It is unknown how deep these canyon deposits were when they formed.

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This view is located in eastern Coprates Chasma. The plateau above the chasma is visible in this image from NASA's 2001 Mars Odyssey spacecraft. The cliff face is very steep, with the elevation dropping over 3 miles from the plateau to the canyon floor.
This view is located in eastern Coprates Chasma. The plateau above the chasma is visible in this image from NASA's 2001 Mars Odyssey spacecraft. The cliff face is very steep, with the elevation dropping over 3 miles from the plateau to the canyon floor.

Investigating Mars: Coprates Chasma

This view is located in eastern Coprates Chasma. The plateau above the chasma is visible in this image from NASA's 2001 Mars Odyssey spacecraft. The cliff face is very steep, with the elevation dropping over 3 miles from the plateau to the canyon floor.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21999
Added: 2017-10-05

Views: 132

Investigating Mars: Coprates Chasma

This view is located in eastern Coprates Chasma. The plateau above the chasma is visible in this image from NASA's 2001 Mars Odyssey spacecraft. The cliff face is very steep, with the elevation dropping over 3 miles from the plateau to the canyon floor.

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This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017.
This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017.

Temperature Gradient on Martian Moon Phobos

This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017.

Target: Phobos
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22057
Added: 2017-10-04

Views: 1155

Temperature Gradient on Martian Moon Phobos

This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017.

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This image of Phobos is one product of the first pointing at the Martian moon by the THEMIS camera on NASA's Mars Odyssey orbiter. The Sept. 29, 2017, observation also provided information about temperatures on different areas of Phobos.
This image of Phobos is one product of the first pointing at the Martian moon by the THEMIS camera on NASA's Mars Odyssey orbiter. The Sept. 29, 2017, observation also provided information about temperatures on different areas of Phobos.

Martian Moon Phobos Observed by NASA's Odyssey

This image of Phobos is one product of the first pointing at the Martian moon by the THEMIS camera on NASA's Mars Odyssey orbiter. The Sept. 29, 2017, observation also provided information about temperatures on different areas of Phobos.

Target: Phobos
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA22056
Added: 2017-10-04

Views: 457

Martian Moon Phobos Observed by NASA's Odyssey

This image of Phobos is one product of the first pointing at the Martian moon by the THEMIS camera on NASA's Mars Odyssey orbiter. The Sept. 29, 2017, observation also provided information about temperatures on different areas of Phobos.

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This frame from an animation was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017.
This frame from an animation was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017.

Series of Images from THEMIS Scanning Phobos

This frame from an animation was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017.

Target: Phobos
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21859
Added: 2017-10-04

Views: 350

Series of Images from THEMIS Scanning Phobos

This frame from an animation was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017.

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Colors in this image of the Martian moon Phobos indicate a range of surface temperatures detected by observing the moon on Sept. 29, 2017, with the Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey orbiter.
Colors in this image of the Martian moon Phobos indicate a range of surface temperatures detected by observing the moon on Sept. 29, 2017, with the Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey orbiter.

Martian Moon Phobos in Thermal Infrared Image

Colors in this image of the Martian moon Phobos indicate a range of surface temperatures detected by observing the moon on Sept. 29, 2017, with the Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey orbiter.

Target: Phobos
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21858
Added: 2017-10-04

Views: 352

Martian Moon Phobos in Thermal Infrared Image

Colors in this image of the Martian moon Phobos indicate a range of surface temperatures detected by observing the moon on Sept. 29, 2017, with the Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey orbiter.

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This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma. The branching features near the bottom of the image are spurs of rock in the cliff face.
This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma. The branching features near the bottom of the image are spurs of rock in the cliff face.

Investigating Mars: Coprates Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma. The branching features near the bottom of the image are spurs of rock in the cliff face.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21998
Added: 2017-10-04

Views: 116

Investigating Mars: Coprates Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma. The branching features near the bottom of the image are spurs of rock in the cliff face.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. In this view, there is a landslide deposit at the bottom of the image.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. In this view, there is a landslide deposit at the bottom of the image.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. In this view, there is a landslide deposit at the bottom of the image.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21996
Added: 2017-10-03

Views: 126

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma. In this view, there is a landslide deposit at the bottom of the image.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21995
Added: 2017-10-02

Views: 178

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in eastern Coprates Chasma.

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These profiles show the brightness of aurora emission in Mars' atmosphere at different altitudes. The data are from observations by the Imaging Ultraviolet Spectrograph instrument (IUVS) on NASA's Mars Atmosphere and Volatile Evolution orbiter, or MAVEN.
These profiles show the brightness of aurora emission in Mars' atmosphere at different altitudes. The data are from observations by the Imaging Ultraviolet Spectrograph instrument (IUVS) on NASA's Mars Atmosphere and Volatile Evolution orbiter, or MAVEN.

Martian Aurora 25 Times Brighter Than Prior Brightest

These profiles show the brightness of aurora emission in Mars' atmosphere at different altitudes. The data are from observations by the Imaging Ultraviolet Spectrograph instrument (IUVS) on NASA's Mars Atmosphere and Volatile Evolution orbiter, or MAVEN.

Target: Mars
Mission: Mars Atmosphere and Volatile Evolution MissioN (MAVEN)
ID#: PIA21857
Added: 2017-09-29

Views: 358

Martian Aurora 25 Times Brighter Than Prior Brightest

These profiles show the brightness of aurora emission in Mars' atmosphere at different altitudes. The data are from observations by the Imaging Ultraviolet Spectrograph instrument (IUVS) on NASA's Mars Atmosphere and Volatile Evolution orbiter, or MAVEN.

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Energetic particles from a large solar storm in September 2017 were seen both in Mars orbit by NASA's MAVEN orbiter, and on the surface of Mars by NASA's Curiosity Mars rover.
Energetic particles from a large solar storm in September 2017 were seen both in Mars orbit by NASA's MAVEN orbiter, and on the surface of Mars by NASA's Curiosity Mars rover.

Solar Storm's Radiation at Martian Orbit and Surface

Energetic particles from a large solar storm in September 2017 were seen both in Mars orbit by NASA's MAVEN orbiter, and on the surface of Mars by NASA's Curiosity Mars rover.

Target: Mars
Mission: Mars Atmosphere and Volatile Evolution MissioN (MAVEN)
ID#: PIA21856
Added: 2017-09-29

Views: 505

Solar Storm's Radiation at Martian Orbit and Surface

Energetic particles from a large solar storm in September 2017 were seen both in Mars orbit by NASA's MAVEN orbiter, and on the surface of Mars by NASA's Curiosity Mars rover.

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These images show the sudden appearance of a bright aurora on Mars during a solar storm in September 2017. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side before (left) and during (right) the event.
These images show the sudden appearance of a bright aurora on Mars during a solar storm in September 2017. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side before (left) and during (right) the event.

Solar Storm Triggers Whole-Planet Aurora at Mars

These images show the sudden appearance of a bright aurora on Mars during a solar storm in September 2017. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side before (left) and during (right) the event.

Target: Mars
Mission: Mars Atmosphere and Volatile Evolution MissioN (MAVEN)
ID#: PIA21855
Added: 2017-09-29

Views: 892

Solar Storm Triggers Whole-Planet Aurora at Mars

These images show the sudden appearance of a bright aurora on Mars during a solar storm in September 2017. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side before (left) and during (right) the event.

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This image shows the sudden appearance of a bright aurora on Mars during a solar storm as observed by NASA's Maven orbiter. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side over the course of the event.
This image shows the sudden appearance of a bright aurora on Mars during a solar storm as observed by NASA's Maven orbiter. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side over the course of the event.

Solar Storm Triggers Whole-Planet Aurora at Mars (Video)

This image shows the sudden appearance of a bright aurora on Mars during a solar storm as observed by NASA's Maven orbiter. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side over the course of the event.

Target: Mars
Mission: Mars Atmosphere and Volatile Evolution MissioN (MAVEN)
ID#: PIA21854
Added: 2017-09-29

Views: 753

Solar Storm Triggers Whole-Planet Aurora at Mars (Video)

This image shows the sudden appearance of a bright aurora on Mars during a solar storm as observed by NASA's Maven orbiter. The purple-white color scheme shows the intensity of ultraviolet light seen on Mars' night side over the course of the event.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21994
Added: 2017-09-29

Views: 147

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

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Re-analysis of data from a hydrogen-finding instrument on NASA's Mars Odyssey orbiter increased the resolution of maps of hydrogen abundance. The reprocessed data shows more 'water-equivalent hydrogen'in some parts of this equatorial region of Mars.
Re-analysis of data from a hydrogen-finding instrument on NASA's Mars Odyssey orbiter increased the resolution of maps of hydrogen abundance. The reprocessed data shows more 'water-equivalent hydrogen'in some parts of this equatorial region of Mars.

Analysis Sharpens Mars Hydrogen Map, Hinting Equatorial Water Ice

Re-analysis of data from a hydrogen-finding instrument on NASA's Mars Odyssey orbiter increased the resolution of maps of hydrogen abundance. The reprocessed data shows more 'water-equivalent hydrogen'in some parts of this equatorial region of Mars.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Neutron Spectrometer
ID#: PIA21848
Added: 2017-09-28

Views: 555

Analysis Sharpens Mars Hydrogen Map, Hinting Equatorial Water Ice

Re-analysis of data from a hydrogen-finding instrument on NASA's Mars Odyssey orbiter increased the resolution of maps of hydrogen abundance. The reprocessed data shows more 'water-equivalent hydrogen'in some parts of this equatorial region of Mars.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows a relatively smooth floor, with a group of sand dune forms located against the wall of the chasma (bottom of image).
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows a relatively smooth floor, with a group of sand dune forms located against the wall of the chasma (bottom of image).

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows a relatively smooth floor, with a group of sand dune forms located against the wall of the chasma (bottom of image).

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21993
Added: 2017-09-28

Views: 139

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows a relatively smooth floor, with a group of sand dune forms located against the wall of the chasma (bottom of image).

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21992
Added: 2017-09-27

Views: 155

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located in central Coprates Chasma.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located on the eastern side of Coprates Chasma, near Capri Chasma.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located on the eastern side of Coprates Chasma, near Capri Chasma.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located on the eastern side of Coprates Chasma, near Capri Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21991
Added: 2017-09-26

Views: 198

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image captured by NASA's 2001 Mars Odyssey spacecraft is located on the eastern side of Coprates Chasma, near Capri Chasma.

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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows multiple landslide features, which form lobed shaped deposits at the bottom of the canyon cliff face.
Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows multiple landslide features, which form lobed shaped deposits at the bottom of the canyon cliff face.

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows multiple landslide features, which form lobed shaped deposits at the bottom of the canyon cliff face.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21990
Added: 2017-09-25

Views: 215

Investigating Mars: Coprates Chasma

Coprates Chasma is one of the numerous canyons that make up Valles Marineris. This image from NASA's 2001 Mars Odyssey spacecraft shows multiple landslide features, which form lobed shaped deposits at the bottom of the canyon cliff face.

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Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft crosses the center of the dune field and was collected in early spring.
Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft crosses the center of the dune field and was collected in early spring.

Investigating Mars: Siton Undae

Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft crosses the center of the dune field and was collected in early spring.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21989
Added: 2017-09-22

Views: 257

Investigating Mars: Siton Undae

Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft crosses the center of the dune field and was collected in early spring.

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Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft shows a cross section of the dune field.
Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft shows a cross section of the dune field.

Investigating Mars: Siton Undae

Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft shows a cross section of the dune field.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21988
Added: 2017-09-21

Views: 278

Investigating Mars: Siton Undae

Siton Undae is a large dune field located in the northern plains near Escorial Crater. This image from NASA's 2001 Mars Odyssey spacecraft shows a cross section of the dune field.

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Currently displaying images 51-75 of 4807
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