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This image, taken by NASA's Mars Reconnaissance Orbiter, shows the transition between the 'Murray Formation,' in which layers are poorly expressed and difficult to trace from orbit, and the hematite ridge, which is made up of continuous layers.
This image, taken by NASA's Mars Reconnaissance Orbiter, shows the transition between the 'Murray Formation,' in which layers are poorly expressed and difficult to trace from orbit, and the hematite ridge, which is made up of continuous layers.

Geological Transition

This image, taken by NASA's Mars Reconnaissance Orbiter, shows the transition between the 'Murray Formation,' in which layers are poorly expressed and difficult to trace from orbit, and the hematite ridge, which is made up of continuous layers.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO), Mars Science Laboratory (MSL)
Spacecraft: Curiosity, Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18785
Added: 2014-09-11

Views: 278

Geological Transition

This image, taken by NASA's Mars Reconnaissance Orbiter, shows the transition between the 'Murray Formation,' in which layers are poorly expressed and difficult to trace from orbit, and the hematite ridge, which is made up of continuous layers.

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This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.
This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.

Bands on the 'Murray Formation'

This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO), Mars Science Laboratory (MSL)
Spacecraft: Curiosity, Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18784
Added: 2014-09-11

Views: 254

Bands on the 'Murray Formation'

This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.

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This image, taken by NASA's Mars Reconnaissance Orbiter, shows a mesa within the 'Murray Buttes' area on Mars showing a complex fracture pattern (black arrow) protruding from the eroding rock.
This image, taken by NASA's Mars Reconnaissance Orbiter, shows a mesa within the 'Murray Buttes' area on Mars showing a complex fracture pattern (black arrow) protruding from the eroding rock.

'Murray Buttes' Mesa

This image, taken by NASA's Mars Reconnaissance Orbiter, shows a mesa within the 'Murray Buttes' area on Mars showing a complex fracture pattern (black arrow) protruding from the eroding rock.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO), Mars Science Laboratory (MSL)
Spacecraft: Curiosity, Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18783
Added: 2014-09-11

Views: 286

'Murray Buttes' Mesa

This image, taken by NASA's Mars Reconnaissance Orbiter, shows a mesa within the 'Murray Buttes' area on Mars showing a complex fracture pattern (black arrow) protruding from the eroding rock.

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This is a map of lower Mount Sharp on Mars, showing the major geologic units identified from orbit. The rocks of the 'Murray Formation,' mapped in green, likely represent the oldest layers of Mount Sharp that NASA's Curiosity rover will explore.
This is a map of lower Mount Sharp on Mars, showing the major geologic units identified from orbit. The rocks of the 'Murray Formation,' mapped in green, likely represent the oldest layers of Mount Sharp that NASA's Curiosity rover will explore.

Map of Lower Mount Sharp

This is a map of lower Mount Sharp on Mars, showing the major geologic units identified from orbit. The rocks of the 'Murray Formation,' mapped in green, likely represent the oldest layers of Mount Sharp that NASA's Curiosity rover will explore.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO), Mars Science Laboratory (MSL)
Spacecraft: Curiosity, Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18781
Added: 2014-09-11

Views: 265

Map of Lower Mount Sharp

This is a map of lower Mount Sharp on Mars, showing the major geologic units identified from orbit. The rocks of the 'Murray Formation,' mapped in green, likely represent the oldest layers of Mount Sharp that NASA's Curiosity rover will explore.

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Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.
Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.

Overlapping Lobate Lava Flows in Daedalia Planum

Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. 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#: PIA18807
Added: 2014-09-10

Views: 53

Overlapping Lobate Lava Flows in Daedalia Planum

Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.

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The tropics of Mars are commonly littered with small bright ripples that were somehow shaped by the wind. NASA's Mars Reconnaissance Orbiter might provide a valuable clue to the formation of transverse aeolian ridges (TARs) elsewhere on Mars.
The tropics of Mars are commonly littered with small bright ripples that were somehow shaped by the wind. NASA's Mars Reconnaissance Orbiter might provide a valuable clue to the formation of transverse aeolian ridges (TARs) elsewhere on Mars.

Banded TARs in Iapygia

The tropics of Mars are commonly littered with small bright ripples that were somehow shaped by the wind. NASA's Mars Reconnaissance Orbiter might provide a valuable clue to the formation of transverse aeolian ridges (TARs) elsewhere on Mars.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18806
Added: 2014-09-10

Views: 79

Banded TARs in Iapygia

The tropics of Mars are commonly littered with small bright ripples that were somehow shaped by the wind. NASA's Mars Reconnaissance Orbiter might provide a valuable clue to the formation of transverse aeolian ridges (TARs) elsewhere on Mars.

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This image from NASA's Mars Reconnaissance Orbiter shows Vinogradov, an old, 224-kilometer diameter, heavily degraded impact crater in southern Margaritifer Terra.
This image from NASA's Mars Reconnaissance Orbiter shows Vinogradov, an old, 224-kilometer diameter, heavily degraded impact crater in southern Margaritifer Terra.

Mysterious Light-Toned Deposit in Vinogradov Crater

This image from NASA's Mars Reconnaissance Orbiter shows Vinogradov, an old, 224-kilometer diameter, heavily degraded impact crater in southern Margaritifer Terra.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18805
Added: 2014-09-10

Views: 60

Mysterious Light-Toned Deposit in Vinogradov Crater

This image from NASA's Mars Reconnaissance Orbiter shows Vinogradov, an old, 224-kilometer diameter, heavily degraded impact crater in southern Margaritifer Terra.

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Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or inland sea. This image is from NASA's Mars Reconnaissance Orbiter.
Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

Chaos in Eridania Basin

Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or 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#: PIA18804
Added: 2014-09-10

Views: 59

Chaos in Eridania Basin

Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

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This recent image from NASA's Mars Reconnaissance Orbiter, acquired to certify a landing site for NASA'a InSight mission, shows a distinctive crater with a very sharp rim and ejecta.
This recent image from NASA's Mars Reconnaissance Orbiter, acquired to certify a landing site for NASA'a InSight mission, shows a distinctive crater with a very sharp rim and ejecta.

A New Impact Crater Near NASA's InSight Landing Region

This recent image from NASA's Mars Reconnaissance Orbiter, acquired to certify a landing site for NASA'a InSight mission, shows a distinctive crater with a very sharp rim and ejecta.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18776
Added: 2014-08-27

Views: 138

A New Impact Crater Near NASA's InSight Landing Region

This recent image from NASA's Mars Reconnaissance Orbiter, acquired to certify a landing site for NASA'a InSight mission, shows a distinctive crater with a very sharp rim and ejecta.

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This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.
This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.

Mantled Terrain in the Southern Mid-Latitudes

This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18775
Added: 2014-08-27

Views: 108

Mantled Terrain in the Southern Mid-Latitudes

This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.

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This crater captured by NASA's Mars Reconnaissance Orbiter has a strange appearance, as if the crater has feet with toes sticking out of two sides, likely caused by a highly oblique impact event.
This crater captured by NASA's Mars Reconnaissance Orbiter has a strange appearance, as if the crater has feet with toes sticking out of two sides, likely caused by a highly oblique impact event.

Weird Crater

This crater captured by NASA's Mars Reconnaissance Orbiter has a strange appearance, as if the crater has feet with toes sticking out of two sides, likely caused by a highly oblique impact event.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18774
Added: 2014-08-27

Views: 138

Weird Crater

This crater captured by NASA's Mars Reconnaissance Orbiter has a strange appearance, as if the crater has feet with toes sticking out of two sides, likely caused by a highly oblique impact event.

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This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.
This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.

A Possible Landing Site in Aram Dorsum for the ExoMars Rover

This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18773
Added: 2014-08-27

Views: 80

A Possible Landing Site in Aram Dorsum for the ExoMars Rover

This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.

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Puppis A, around 7,000 light-years away, is seen in this image from NASA's Spitzer Space Telescope and Chandra X-Ray Observatory, and the European Space Agency's XMM-Newton.
Puppis A, around 7,000 light-years away, is seen in this image from NASA's Spitzer Space Telescope and Chandra X-Ray Observatory, and the European Space Agency's XMM-Newton.

Supernova Seen In Two Lights

Puppis A, around 7,000 light-years away, is seen in this image from NASA's Spitzer Space Telescope and Chandra X-Ray Observatory, and the European Space Agency's XMM-Newton.

Mission: Chandra X-Ray Observatory, Spitzer Space Telescope, XMM-Newton
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: Multiband Imaging Photometer (MIPS), XMM-Newton X-ray
ID#: PIA18468
Added: 2014-08-21

Views: 976

Supernova Seen In Two Lights

Puppis A, around 7,000 light-years away, is seen in this image from NASA's Spitzer Space Telescope and Chandra X-Ray Observatory, and the European Space Agency's XMM-Newton.

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The track left by an oblong boulder as it tumbled down a slope on Mars runs from upper left to right center of this image taken by NASA's Mars Reconnaissance Orbiter.
The track left by an oblong boulder as it tumbled down a slope on Mars runs from upper left to right center of this image taken by NASA's Mars Reconnaissance Orbiter.

An Irregular, Upright Boulder on Mars

The track left by an oblong boulder as it tumbled down a slope on Mars runs from upper left to right center of this image taken 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#: PIA18594
Added: 2014-08-13

Views: 5222

An Irregular, Upright Boulder on Mars

The track left by an oblong boulder as it tumbled down a slope on Mars runs from upper left to right center of this image taken by NASA's Mars Reconnaissance Orbiter.

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Hellas Crater in the ancient highlands contains some of the clearest evidence on Mars for glacial processes. This image from NASA's Mars Reconnaissance Orbiter shows a number of features consistent with glaciation.
Hellas Crater in the ancient highlands contains some of the clearest evidence on Mars for glacial processes. This image from NASA's Mars Reconnaissance Orbiter shows a number of features consistent with glaciation.

Glaciation at the Eastern Hellas Margin

Hellas Crater in the ancient highlands contains some of the clearest evidence on Mars for glacial processes. This image from NASA's Mars Reconnaissance Orbiter shows a number of features consistent with glaciation.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18647
Added: 2014-08-13

Views: 159

Glaciation at the Eastern Hellas Margin

Hellas Crater in the ancient highlands contains some of the clearest evidence on Mars for glacial processes. This image from NASA's Mars Reconnaissance Orbiter shows a number of features consistent with glaciation.

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The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.
The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

The Side of Chasma Boreale

The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18646
Added: 2014-08-13

Views: 182

The Side of Chasma Boreale

The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

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The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.
The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

Strange Cones and Flows

The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18645
Added: 2014-08-13

Views: 167

Strange Cones and Flows

The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

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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: 246

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: 240

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: 206

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: 230

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

Views: 2548

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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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: 258

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: 203

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

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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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