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This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows near Arsia Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows near Arsia Mons.

Lava Flows

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows near Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18751
Added: 2014-10-17

Views: 468

Lava Flows

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows near Arsia Mons.

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This stereo vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look. You will need 3-D glasses to view this image.
This stereo vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look. You will need 3-D glasses to view this image.

Opportunity's Northward View of 'Wdowiak Ridge' (Stereo)

This stereo vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look. You will need 3-D glasses to view this image.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18616
Added: 2014-10-16

Views: 1117

Opportunity's Northward View of 'Wdowiak Ridge' (Stereo)

This stereo vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look. You will need 3-D glasses to view this image.

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This north-looking vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center. This version is presented in false color, which enhances visibility of the rover's wheel tracks at right.
This north-looking vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center. This version is presented in false color, which enhances visibility of the rover's wheel tracks at right.

Opportunity's Northward View of 'Wdowiak Ridge' (False Color)

This north-looking vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center. This version is presented in false color, which enhances visibility of the rover's wheel tracks at right.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18615
Added: 2014-10-16

Views: 2239

Opportunity's Northward View of 'Wdowiak Ridge' (False Color)

This north-looking vista from NASA's Mars Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center. This version is presented in false color, which enhances visibility of the rover's wheel tracks at right.

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This vista from NASA's Mars Exploration Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look with the rover's tracks visible at right.
This vista from NASA's Mars Exploration Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look with the rover's tracks visible at right.

Opportunity's Northward View of 'Wdowiak Ridge'

This vista from NASA's Mars Exploration Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look with the rover's tracks visible at right.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18614
Added: 2014-10-16

Views: 5110

Opportunity's Northward View of 'Wdowiak Ridge'

This vista from NASA's Mars Exploration Rover Opportunity shows 'Wdowiak Ridge,' from left foreground to center, as part of a northward look with the rover's tracks visible at right.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Candor Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Candor Chasma.

Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Candor Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18750
Added: 2014-10-16

Views: 385

Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Candor Chasma.

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Most surface ice on Mars is temporary. The polar layered deposits are thick stacks of permanent water ice at each pole, and the South Polar residual cap may be a permanent (although dynamic) layer of carbon dioxide ice as seen by NASA's Mars Reconnaissanc
Most surface ice on Mars is temporary. The polar layered deposits are thick stacks of permanent water ice at each pole, and the South Polar residual cap may be a permanent (although dynamic) layer of carbon dioxide ice as seen by NASA's Mars Reconnaissanc

Perennial Frost in a Crater on the Northern Plains

Most surface ice on Mars is temporary. The polar layered deposits are thick stacks of permanent water ice at each pole, and the South Polar residual cap may be a permanent (although dynamic) layer of carbon dioxide ice as seen by NASA's Mars Reconnaissanc

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18832
Added: 2014-10-15

Views: 809

Perennial Frost in a Crater on the Northern Plains

Most surface ice on Mars is temporary. The polar layered deposits are thick stacks of permanent water ice at each pole, and the South Polar residual cap may be a permanent (although dynamic) layer of carbon dioxide ice as seen by NASA's Mars Reconnaissanc

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In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.
In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.

A Collection of Landforms in Eastern Elysium Planitia

In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18831
Added: 2014-10-15

Views: 589

A Collection of Landforms in Eastern Elysium Planitia

In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.

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Melas Chasma is the widest segment of the Valles Marineris canyon, and is an area where NASA's Mars Reconnaissance Orbiter has detected the presence of sulfates.
Melas Chasma is the widest segment of the Valles Marineris canyon, and is an area where NASA's Mars Reconnaissance Orbiter has detected the presence of sulfates.

Mounds of Layered Material on the West Edge of Melas Chasma

Melas Chasma is the widest segment of the Valles Marineris canyon, and is an area where NASA's Mars Reconnaissance Orbiter has detected the presence of sulfates.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18830
Added: 2014-10-15

Views: 541

Mounds of Layered Material on the West Edge of Melas Chasma

Melas Chasma is the widest segment of the Valles Marineris canyon, and is an area where NASA's Mars Reconnaissance Orbiter has detected the presence of sulfates.

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The objective of this observation from NASA's Mars Reconnaissance Orbiter is to examine a light-toned deposit in a region of what is called 'chaotic terrain' at the base of the Valles Marineris canyon system.
The objective of this observation from NASA's Mars Reconnaissance Orbiter is to examine a light-toned deposit in a region of what is called 'chaotic terrain' at the base of the Valles Marineris canyon system.

A Light Toned Deposit in Arsinoes Chaos

The objective of this observation from NASA's Mars Reconnaissance Orbiter is to examine a light-toned deposit in a region of what is called 'chaotic terrain' at the base of the Valles Marineris canyon system.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18829
Added: 2014-10-15

Views: 550

A Light Toned Deposit in Arsinoes Chaos

The objective of this observation from NASA's Mars Reconnaissance Orbiter is to examine a light-toned deposit in a region of what is called 'chaotic terrain' at the base of the Valles Marineris canyon system.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the north wall of Valles Marineris near Melas Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the north wall of Valles Marineris near Melas Chasma.

Valles Marineris

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the north wall of Valles Marineris near Melas Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18745
Added: 2014-10-15

Views: 385

Valles Marineris

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the north wall of Valles Marineris near Melas Chasma.

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Three views of an escaping atmosphere around Mars, obtained by NASA's MAVEN's Imaging Ultraviolet Spectrograph, are shown here.
Three views of an escaping atmosphere around Mars, obtained by NASA's MAVEN's Imaging Ultraviolet Spectrograph, are shown here.

Ultraviolet Views of Martian Atmosphere

Three views of an escaping atmosphere around Mars, obtained by NASA's MAVEN's Imaging Ultraviolet Spectrograph, are shown here.

Target: Mars
Spacecraft: MAVEN
Instrument: Imaging Ultraviolet Spectrograph
ID#: PIA18613
Added: 2014-10-14

Views: 812

Ultraviolet Views of Martian Atmosphere

Three views of an escaping atmosphere around Mars, obtained by NASA's MAVEN's Imaging Ultraviolet Spectrograph, are shown here.

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This image from NASA's 2001 Mars Odyssey spacecraft shows a region of plateaus and depressions near the south polar cap.
This image from NASA's 2001 Mars Odyssey spacecraft shows a region of plateaus and depressions near the south polar cap.

South Polar Features

This image from NASA's 2001 Mars Odyssey spacecraft shows a region of plateaus and depressions near the south polar cap.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18744
Added: 2014-10-14

Views: 391

South Polar Features

This image from NASA's 2001 Mars Odyssey spacecraft shows a region of plateaus and depressions near the south polar cap.

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This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.
This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.

Yardangs

This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18743
Added: 2014-10-13

Views: 471

Yardangs

This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.

Arsia Mons

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18742
Added: 2014-10-10

Views: 422

Arsia Mons

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.

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Comet Siding Spring will have a close approach to Mars on Oct. 19, 2014. This artist's concept shows people in the Southern Hemisphere where to look for Mars in the night sky. Mars and the comet may be visible with binoculars.
Comet Siding Spring will have a close approach to Mars on Oct. 19, 2014. This artist's concept shows people in the Southern Hemisphere where to look for Mars in the night sky. Mars and the comet may be visible with binoculars.

View of Comet Siding Spring from Southern Hemisphere (Artist's Concept)

Comet Siding Spring will have a close approach to Mars on Oct. 19, 2014. This artist's concept shows people in the Southern Hemisphere where to look for Mars in the night sky. Mars and the comet may be visible with binoculars.

Target: Mars
ID#: PIA18612
Added: 2014-10-09

Views: 1084

View of Comet Siding Spring from Southern Hemisphere (Artist's Concept)

Comet Siding Spring will have a close approach to Mars on Oct. 19, 2014. This artist's concept shows people in the Southern Hemisphere where to look for Mars in the night sky. Mars and the comet may be visible with binoculars.

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This artist's concept shows NASA's Mars orbiters lining up behind the Red Planet for their 'duck and cover' maneuver to shield them from comet dust that may result from the close flyby of comet Siding Spring (C/2013 A1) on Oct. 19, 2014.
This artist's concept shows NASA's Mars orbiters lining up behind the Red Planet for their 'duck and cover' maneuver to shield them from comet dust that may result from the close flyby of comet Siding Spring (C/2013 A1) on Oct. 19, 2014.

Mars Orbiters 'Duck and Cover' for Comet Siding Spring Flyby (Artist's Concept)

This artist's concept shows NASA's Mars orbiters lining up behind the Red Planet for their 'duck and cover' maneuver to shield them from comet dust that may result from the close flyby of comet Siding Spring (C/2013 A1) on Oct. 19, 2014.

Target: Mars
ID#: PIA18611
Added: 2014-10-09

Views: 2083

Mars Orbiters 'Duck and Cover' for Comet Siding Spring Flyby (Artist's Concept)

This artist's concept shows NASA's Mars orbiters lining up behind the Red Planet for their 'duck and cover' maneuver to shield them from comet dust that may result from the close flyby of comet Siding Spring (C/2013 A1) on Oct. 19, 2014.

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This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Angustus Labyrinthus

This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18741
Added: 2014-10-09

Views: 322

Angustus Labyrinthus

This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, a huge region of volcanic flows south of Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, a huge region of volcanic flows south of Arsia Mons.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, a huge region of volcanic flows south of Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18740
Added: 2014-10-08

Views: 87

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, a huge region of volcanic flows south of Arsia Mons.

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While yesterday's image showed a texture of oval depressions (swiss cheese), this image from NASA's 2001 Mars Odyssey spacecraft shows a linear surface texture of the south polar cap. This texture is described as looking like a thumbprint.
While yesterday's image showed a texture of oval depressions (swiss cheese), this image from NASA's 2001 Mars Odyssey spacecraft shows a linear surface texture of the south polar cap. This texture is described as looking like a thumbprint.

South Polar Textures

While yesterday's image showed a texture of oval depressions (swiss cheese), this image from NASA's 2001 Mars Odyssey spacecraft shows a linear surface texture of the south polar cap. This texture is described as looking like a thumbprint.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18736
Added: 2014-10-07

Views: 836

South Polar Textures

While yesterday's image showed a texture of oval depressions (swiss cheese), this image from NASA's 2001 Mars Odyssey spacecraft shows a linear surface texture of the south polar cap. This texture is described as looking like a thumbprint.

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This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.
This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.

South Polar Textures

This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18733
Added: 2014-10-06

Views: 927

South Polar Textures

This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.

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This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.
This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.

Apollinaris Mons

This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18732
Added: 2014-10-03

Views: 496

Apollinaris Mons

This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.

Hebes Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18731
Added: 2014-10-02

Views: 348

Hebes Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.

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This observation from NASA's Mars Reconnaissance Orbiter shows both dome and barchan dunes in a small sand dune field on the floor of Newton Crater, an approximately 300 kilometer (130 mile) wide crater in the Southern hemisphere of Mars.
This observation from NASA's Mars Reconnaissance Orbiter shows both dome and barchan dunes in a small sand dune field on the floor of Newton Crater, an approximately 300 kilometer (130 mile) wide crater in the Southern hemisphere of Mars.

Dome and Barchan Dunes in Newton Crater

This observation from NASA's Mars Reconnaissance Orbiter shows both dome and barchan dunes in a small sand dune field on the floor of Newton Crater, an approximately 300 kilometer (130 mile) wide crater in the Southern hemisphere of Mars.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18820
Added: 2014-10-01

Views: 336

Dome and Barchan Dunes in Newton Crater

This observation from NASA's Mars Reconnaissance Orbiter shows both dome and barchan dunes in a small sand dune field on the floor of Newton Crater, an approximately 300 kilometer (130 mile) wide crater in the Southern hemisphere of Mars.

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This observation from NASA's Mars Reconnaissance Orbiter shows bright and dark slope streaks in craters in the Arabia Terra region.
This observation from NASA's Mars Reconnaissance Orbiter shows bright and dark slope streaks in craters in the Arabia Terra region.

Bright Slope Streaks in Arabia Terra

This observation from NASA's Mars Reconnaissance Orbiter shows bright and dark slope streaks in craters in the Arabia Terra region.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18819
Added: 2014-10-01

Views: 298

Bright Slope Streaks in Arabia Terra

This observation from NASA's Mars Reconnaissance Orbiter shows bright and dark slope streaks in craters in the Arabia Terra region.

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Nili Patera is a region on Mars in which dunes and ripples are moving rapidly. HiRISE continues to monitor this area every couple of months to see changes over seasonal and annual time scales as seen by NASA's Mars Reconnaissance Orbiter.
Nili Patera is a region on Mars in which dunes and ripples are moving rapidly. HiRISE continues to monitor this area every couple of months to see changes over seasonal and annual time scales as seen by NASA's Mars Reconnaissance Orbiter.

Continual Dune and Ripple Migration in Nili Patera

Nili Patera is a region on Mars in which dunes and ripples are moving rapidly. HiRISE continues to monitor this area every couple of months to see changes over seasonal and annual time scales as seen by 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#: PIA18818
Added: 2014-10-01

Views: 345

Continual Dune and Ripple Migration in Nili Patera

Nili Patera is a region on Mars in which dunes and ripples are moving rapidly. HiRISE continues to monitor this area every couple of months to see changes over seasonal and annual time scales as seen by NASA's Mars Reconnaissance Orbiter.

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