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The linear feature in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Cyane Fossae. The circular collapse features are bounded by linear faults.
The linear feature in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Cyane Fossae. The circular collapse features are bounded by linear faults.

Cyane Fossae

The linear feature in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Cyane Fossae. The circular collapse features are bounded by linear faults.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18548
Added: 2014-07-31

Views: 4

Cyane Fossae

The linear feature in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Cyane Fossae. The circular collapse features are bounded by linear faults.

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Schiaparelli Crater is a 460 kilometer (286 mile) wide multi-ring structure. However, it is a very shallow crater, apparently filled by younger materials such as lava and/or fluvial and aeolian sediments as seen by NASA's Mars Reconnaissance Orbiter.
Schiaparelli Crater is a 460 kilometer (286 mile) wide multi-ring structure. However, it is a very shallow crater, apparently filled by younger materials such as lava and/or fluvial and aeolian sediments as seen by NASA's Mars Reconnaissance Orbiter.

Layers and Sand on the Floor of Schiaparelli Crater

Schiaparelli Crater is a 460 kilometer (286 mile) wide multi-ring structure. However, it is a very shallow crater, apparently filled by younger materials such as lava and/or fluvial and aeolian sediments 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#: PIA18635
Added: 2014-07-30

Views: 6

Layers and Sand on the Floor of Schiaparelli Crater

Schiaparelli Crater is a 460 kilometer (286 mile) wide multi-ring structure. However, it is a very shallow crater, apparently filled by younger materials such as lava and/or fluvial and aeolian sediments as seen by NASA's Mars Reconnaissance Orbiter.

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Monitoring by NASA's Mars Reconnaissance Orbiter HiRISE has shown that gully formation on Mars occurs in winter and early spring in times and places with frost on the ground.
Monitoring by NASA's Mars Reconnaissance Orbiter HiRISE has shown that gully formation on Mars occurs in winter and early spring in times and places with frost on the ground.

Frosty Gullies

Monitoring by NASA's Mars Reconnaissance Orbiter HiRISE has shown that gully formation on Mars occurs in winter and early spring in times and places with frost on the ground.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18634
Added: 2014-07-30

Views: 6

Frosty Gullies

Monitoring by NASA's Mars Reconnaissance Orbiter HiRISE has shown that gully formation on Mars occurs in winter and early spring in times and places with frost on the ground.

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This image from NASA's Mars Reconnaissance Orbiter shows what is termed a pedestal crater, so-called because the level of the surface adjacent to the crater is elevated relative to the surface of the surrounding terrain.
This image from NASA's Mars Reconnaissance Orbiter shows what is termed a pedestal crater, so-called because the level of the surface adjacent to the crater is elevated relative to the surface of the surrounding terrain.

Preserving Ice from a Vanished Terrain

This image from NASA's Mars Reconnaissance Orbiter shows what is termed a pedestal crater, so-called because the level of the surface adjacent to the crater is elevated relative to the surface of the surrounding terrain.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18633
Added: 2014-07-30

Views: 6

Preserving Ice from a Vanished Terrain

This image from NASA's Mars Reconnaissance Orbiter shows what is termed a pedestal crater, so-called because the level of the surface adjacent to the crater is elevated relative to the surface of the surrounding terrain.

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Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, as seen by NASA's Mars Reconnaissance Orbiter.
Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, as seen by NASA's Mars Reconnaissance Orbiter.

Water-Bearing Rocks in Noctis Labyrinthus

Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, 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#: PIA18632
Added: 2014-07-30

Views: 4

Water-Bearing Rocks in Noctis Labyrinthus

Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, as seen by NASA's Mars Reconnaissance Orbiter.

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The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.
The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.

Hyperboreae Undae

The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18550
Added: 2014-07-30

Views: 22

Hyperboreae Undae

The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.

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The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.
The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.

Hrad Vallis

The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18549
Added: 2014-07-29

Views: 23

Hrad Vallis

The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.

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This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.
This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

'Lunokhod 2' Crater on Mars

This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18416
Added: 2014-07-28

Views: 935

'Lunokhod 2' Crater on Mars

This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

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This stereo view from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.
This stereo view from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

'Lunokhod 2' Crater on Mars (Stereo)

This stereo view from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18415
Added: 2014-07-28

Views: 261

'Lunokhod 2' Crater on Mars (Stereo)

This stereo view from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

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This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.
This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

'Lunokhod 2 Crater' on Mars (False Color)

This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

Target: Mars
Mission: Mars Exploration Rover (MER)
Spacecraft: Opportunity
Instrument: Panoramic Camera
ID#: PIA18414
Added: 2014-07-28

Views: 26

'Lunokhod 2 Crater' on Mars (False Color)

This scene from NASA's Opportunity rover shows 'Lunokhod 2 Crater,' which lies south of 'Solander Point' on the west rim of Endeavour Crater. Lunokhod 2 Crater is approximately 20 feet (6 meters) in diameter.

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NASA's Opportunity rover, working on Mars since January 2004, passed 25 miles of total driving on the July 27, 2014. The gold line on this map shows Opportunity's route from the landing site inside Eagle Crater, in upper left.
NASA's Opportunity rover, working on Mars since January 2004, passed 25 miles of total driving on the July 27, 2014. The gold line on this map shows Opportunity's route from the landing site inside Eagle Crater, in upper left.

Opportunity's Journey Exceeds 25 Miles

NASA's Opportunity rover, working on Mars since January 2004, passed 25 miles of total driving on the July 27, 2014. The gold line on this map shows Opportunity's route from the landing site inside Eagle Crater, in upper left.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO), Opportunity
Instrument: Context Camera (CTX)
ID#: PIA18404
Added: 2014-07-28

Views: 1480

Opportunity's Journey Exceeds 25 Miles

NASA's Opportunity rover, working on Mars since January 2004, passed 25 miles of total driving on the July 27, 2014. The gold line on this map shows Opportunity's route from the landing site inside Eagle Crater, in upper left.

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The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.
The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.

Colles

The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18547
Added: 2014-07-28

Views: 23

Colles

The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.

Rubicon Valles

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18546
Added: 2014-07-25

Views: 39

Rubicon Valles

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.

Plains Layers

This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18545
Added: 2014-07-24

Views: 45

Plains Layers

This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.

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The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.

Lyot Crater Dunes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18544
Added: 2014-07-23

Views: 49

Lyot Crater Dunes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.

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The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.

Coloe Fossae

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18543
Added: 2014-07-22

Views: 53

Coloe Fossae

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field called Olympia Undae. There are hills in this region, and the dunes are concentrated in the lower elevations.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field called Olympia Undae. There are hills in this region, and the dunes are concentrated in the lower elevations.

More Polar Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field called Olympia Undae. There are hills in this region, and the dunes are concentrated in the lower elevations.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18542
Added: 2014-07-21

Views: 69

More Polar Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field called Olympia Undae. There are hills in this region, and the dunes are concentrated in the lower elevations.

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This image from NASA's 2001 Mars Odyssey spacecraft shows Lonar Crater. This crater has undergone very little modification since it formed, and so is one of the younger features in this region.
This image from NASA's 2001 Mars Odyssey spacecraft shows Lonar Crater. This crater has undergone very little modification since it formed, and so is one of the younger features in this region.

Lonar Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows Lonar Crater. This crater has undergone very little modification since it formed, and so is one of the younger features in this region.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18541
Added: 2014-07-18

Views: 98

Lonar Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows Lonar Crater. This crater has undergone very little modification since it formed, and so is one of the younger features in this region.

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This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.
This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.

Olympia Undae

This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18540
Added: 2014-07-17

Views: 66

Olympia Undae

This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.

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This image from NASA's Mars Reconnaissance Orbiter shows some interesting fractured materials on the floor of an impact crater in Arabia Terra.
This image from NASA's Mars Reconnaissance Orbiter shows some interesting fractured materials on the floor of an impact crater in Arabia Terra.

Ancient Lake Sediments in a Crater

This image from NASA's Mars Reconnaissance Orbiter shows some interesting fractured materials on the floor of an impact crater in Arabia Terra.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18625
Added: 2014-07-16

Views: 70

Ancient Lake Sediments in a Crater

This image from NASA's Mars Reconnaissance Orbiter shows some interesting fractured materials on the floor of an impact crater in Arabia Terra.

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At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.
At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.

The Icy Surface of the North Polar Cap

At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is 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#: PIA18624
Added: 2014-07-16

Views: 49

The Icy Surface of the North Polar Cap

At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.

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Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is from NASA's Mars Reconnaissance Orbiter.
Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

Ridges in Eridania Basin

Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is 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#: PIA18623
Added: 2014-07-16

Views: 60

Ridges in Eridania Basin

Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

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NASA's Curiosity Mars rover used the Mars Hand Lens Imager (MAHLI) camera on its arm to catch the first images of sparks produced by the rover's laser being shot at a rock on Mars. The left image is from before the laser zapped this rock, called 'Nova'.
NASA's Curiosity Mars rover used the Mars Hand Lens Imager (MAHLI) camera on its arm to catch the first images of sparks produced by the rover's laser being shot at a rock on Mars. The left image is from before the laser zapped this rock, called 'Nova'.

First Imaging of Laser-Induced Spark on Mars

NASA's Curiosity Mars rover used the Mars Hand Lens Imager (MAHLI) camera on its arm to catch the first images of sparks produced by the rover's laser being shot at a rock on Mars. The left image is from before the laser zapped this rock, called 'Nova'.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mars Hand Lens Imager (MAHLI)
ID#: PIA18401
Added: 2014-07-16

Views: 876

First Imaging of Laser-Induced Spark on Mars

NASA's Curiosity Mars rover used the Mars Hand Lens Imager (MAHLI) camera on its arm to catch the first images of sparks produced by the rover's laser being shot at a rock on Mars. The left image is from before the laser zapped this rock, called 'Nova'.

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A Martian target rock called 'Nova,' shown here, displayed an increasing concentration of aluminum as a series of laser shots from NASA's Curiosity Mars rover penetrated through dust on the rock's surface.
A Martian target rock called 'Nova,' shown here, displayed an increasing concentration of aluminum as a series of laser shots from NASA's Curiosity Mars rover penetrated through dust on the rock's surface.

Curiosity's ChemCam Examines Mars Rock Target 'Nova'

A Martian target rock called 'Nova,' shown here, displayed an increasing concentration of aluminum as a series of laser shots from NASA's Curiosity Mars rover penetrated through dust on the rock's surface.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Chemistry and Camera (ChemCam), Mars Hand Lens Imager (MAHLI)
ID#: PIA18388
Added: 2014-07-16

Views: 265

Curiosity's ChemCam Examines Mars Rock Target 'Nova'

A Martian target rock called 'Nova,' shown here, displayed an increasing concentration of aluminum as a series of laser shots from NASA's Curiosity Mars rover penetrated through dust on the rock's surface.

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The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae, a huge dune field near the north polar cap.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae, a huge dune field near the north polar cap.

Polar Dunes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae, a huge dune field near the north polar cap.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA18509
Added: 2014-07-16

Views: 65

Polar Dunes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae, a huge dune field near the north polar cap.

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