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This enhanced-color image from NASA's Mars Reconnaissance Orbiter shows gullies in the northern wall of an unnamed crater in Utopia Planitia. The banked, sinuous shape of the gully channels suggest that water was involved in their formation.
This enhanced-color image from NASA's Mars Reconnaissance Orbiter shows gullies in the northern wall of an unnamed crater in Utopia Planitia. The banked, sinuous shape of the gully channels suggest that water was involved in their formation.

Gullies on the Wall of an Unnamed Crater in Utopia Planitia

This enhanced-color image from NASA's Mars Reconnaissance Orbiter shows gullies in the northern wall of an unnamed crater in Utopia Planitia. The banked, sinuous shape of the gully channels suggest that water was involved in their formation.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19862
Added: 2015-07-29

Views: 141

Gullies on the Wall of an Unnamed Crater in Utopia Planitia

This enhanced-color image from NASA's Mars Reconnaissance Orbiter shows gullies in the northern wall of an unnamed crater in Utopia Planitia. The banked, sinuous shape of the gully channels suggest that water was involved in their formation.

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This image from NASA's Mars Reconnaissance Orbiter shows a portion of a long valley system in northern Arabia Terra.
This image from NASA's Mars Reconnaissance Orbiter shows a portion of a long valley system in northern Arabia Terra.

A Fresh Shallow Valley Transitions to an Inverted Channel

This image from NASA's Mars Reconnaissance Orbiter shows a portion of a long valley system in northern Arabia Terra.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19861
Added: 2015-07-29

Views: 96

A Fresh Shallow Valley Transitions to an Inverted Channel

This image from NASA's Mars Reconnaissance Orbiter shows a portion of a long valley system in northern Arabia Terra.

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This scene captured by NASA's Mars Reconnaissance Orbiter includes chaotic deposits with a wide range of colors. The deposits are distinctive with both unique colors and small-scale textures such as fracture patterns.
This scene captured by NASA's Mars Reconnaissance Orbiter includes chaotic deposits with a wide range of colors. The deposits are distinctive with both unique colors and small-scale textures such as fracture patterns.

Diverse Deposits in Melas Chasma

This scene captured by NASA's Mars Reconnaissance Orbiter includes chaotic deposits with a wide range of colors. The deposits are distinctive with both unique colors and small-scale textures such as fracture patterns.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19860
Added: 2015-07-29

Views: 108

Diverse Deposits in Melas Chasma

This scene captured by NASA's Mars Reconnaissance Orbiter includes chaotic deposits with a wide range of colors. The deposits are distinctive with both unique colors and small-scale textures such as fracture patterns.

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This image from NASA's Mars Reconnaissance Orbiter is part of a proposed landing site in Aram Dorsum for the ExoMars Rover, planned for launch in 2018. Upper layers of light toned sediments have been eroded, leaving a lower surface which appears dark.
This image from NASA's Mars Reconnaissance Orbiter is part of a proposed landing site in Aram Dorsum for the ExoMars Rover, planned for launch in 2018. Upper layers of light toned sediments have been eroded, leaving a lower surface which appears dark.

A Possible Landing Site for the ExoMars Rover in Aram Dorsum

This image from NASA's Mars Reconnaissance Orbiter is part of a proposed landing site in Aram Dorsum for the ExoMars Rover, planned for launch in 2018. Upper layers of light toned sediments have been eroded, leaving a lower surface which appears dark.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19859
Added: 2015-07-29

Views: 68

A Possible Landing Site for the ExoMars Rover in Aram Dorsum

This image from NASA's Mars Reconnaissance Orbiter is part of a proposed landing site in Aram Dorsum for the ExoMars Rover, planned for launch in 2018. Upper layers of light toned sediments have been eroded, leaving a lower surface which appears dark.

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This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.
This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.

Volunteers Help Decide Where to Point Mars Camera

This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: Context Camera (CTX), High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19823
Added: 2015-07-22

Views: 741

Volunteers Help Decide Where to Point Mars Camera

This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.

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Most larger chasmata contain kilometer-thick light-toned layered deposits composed of sulfates. However, some of the chasmata, like Ius Chasma shown in this image from NASA's Mars Reconnaissance Orbiter, lack these deposits or have much thinner deposits.
Most larger chasmata contain kilometer-thick light-toned layered deposits composed of sulfates. However, some of the chasmata, like Ius Chasma shown in this image from NASA's Mars Reconnaissance Orbiter, lack these deposits or have much thinner deposits.

Sedimentary Deposits within Ius Chasma

Most larger chasmata contain kilometer-thick light-toned layered deposits composed of sulfates. However, some of the chasmata, like Ius Chasma shown in this image from NASA's Mars Reconnaissance Orbiter, lack these deposits or have much thinner deposits.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19855
Added: 2015-07-15

Views: 76

Sedimentary Deposits within Ius Chasma

Most larger chasmata contain kilometer-thick light-toned layered deposits composed of sulfates. However, some of the chasmata, like Ius Chasma shown in this image from NASA's Mars Reconnaissance Orbiter, lack these deposits or have much thinner deposits.

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NASA's Mars Reconnaissance Orbite observed this image of an isolated mountain in the Southern highlands reveals a large exposure of 'purplish' bedrock.
NASA's Mars Reconnaissance Orbite observed this image of an isolated mountain in the Southern highlands reveals a large exposure of 'purplish' bedrock.

Purple Mountain's Majesty

NASA's Mars Reconnaissance Orbite observed this image of an isolated mountain in the Southern highlands reveals a large exposure of 'purplish' bedrock.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19854
Added: 2015-07-15

Views: 62

Purple Mountain's Majesty

NASA's Mars Reconnaissance Orbite observed this image of an isolated mountain in the Southern highlands reveals a large exposure of 'purplish' bedrock.

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This image from NASA's Mars Reconnaissance Orbiter shows the central peak in Porter Crater. Southward on the slopes below the peak is a large dune field.
This image from NASA's Mars Reconnaissance Orbiter shows the central peak in Porter Crater. Southward on the slopes below the peak is a large dune field.

Potential Active Processes in Porter Crater

This image from NASA's Mars Reconnaissance Orbiter shows the central peak in Porter Crater. Southward on the slopes below the peak is a large dune field.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19853
Added: 2015-07-15

Views: 65

Potential Active Processes in Porter Crater

This image from NASA's Mars Reconnaissance Orbiter shows the central peak in Porter Crater. Southward on the slopes below the peak is a large dune field.

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Seasonal frost commonly forms at middle and high latitudes on Mars, much like winter snow on Earth. However, on Mars most frost is carbon dioxide (dry ice) rather than water ice. This image is from NASA's Mars Reconnaissance Orbiter.
Seasonal frost commonly forms at middle and high latitudes on Mars, much like winter snow on Earth. However, on Mars most frost is carbon dioxide (dry ice) rather than water ice. This image is from NASA's Mars Reconnaissance Orbiter.

Frosty Gullies on the Northern Plains

Seasonal frost commonly forms at middle and high latitudes on Mars, much like winter snow on Earth. However, on Mars most frost is carbon dioxide (dry ice) rather than water ice. 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#: PIA19852
Added: 2015-07-15

Views: 71

Frosty Gullies on the Northern Plains

Seasonal frost commonly forms at middle and high latitudes on Mars, much like winter snow on Earth. However, on Mars most frost is carbon dioxide (dry ice) rather than water ice. This image is from NASA's Mars Reconnaissance Orbiter.

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Oxia Planum is an ancient (Noachian epoch) terrain situated to the east of Chryse Planitia at about 18 degrees north. This image from NASA's Mars Reconnaissance Orbiteris of a proposed ExoMars Landing Site.
Oxia Planum is an ancient (Noachian epoch) terrain situated to the east of Chryse Planitia at about 18 degrees north. This image from NASA's Mars Reconnaissance Orbiteris of a proposed ExoMars Landing Site.

Clay-Rich Terrain in Oxia Planum: A Proposed ExoMars Landing Site

Oxia Planum is an ancient (Noachian epoch) terrain situated to the east of Chryse Planitia at about 18 degrees north. This image from NASA's Mars Reconnaissance Orbiteris of a proposed ExoMars Landing Site.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19851
Added: 2015-07-01

Views: 59

Clay-Rich Terrain in Oxia Planum: A Proposed ExoMars Landing Site

Oxia Planum is an ancient (Noachian epoch) terrain situated to the east of Chryse Planitia at about 18 degrees north. This image from NASA's Mars Reconnaissance Orbiteris of a proposed ExoMars Landing Site.

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This image from NASA's Mars Reconnaissance Orbiter shows the southwestern floor of a 50-kilometer diameter unnamed crater, about 100 kilometers northeast of Hellas Basin.
This image from NASA's Mars Reconnaissance Orbiter shows the southwestern floor of a 50-kilometer diameter unnamed crater, about 100 kilometers northeast of Hellas Basin.

A Channel System and Patterned Ground near Hellas Basin

This image from NASA's Mars Reconnaissance Orbiter shows the southwestern floor of a 50-kilometer diameter unnamed crater, about 100 kilometers northeast of Hellas Basin.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19850
Added: 2015-07-01

Views: 53

A Channel System and Patterned Ground near Hellas Basin

This image from NASA's Mars Reconnaissance Orbiter shows the southwestern floor of a 50-kilometer diameter unnamed crater, about 100 kilometers northeast of Hellas Basin.

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A pedestal crater is when the ejecta from an impact settles around the new crater and is more erosion-resistant than the surrounding terrain as seen in this image from NASA's Mars Reconnaissance Orbiter.
A pedestal crater is when the ejecta from an impact settles around the new crater and is more erosion-resistant than the surrounding terrain as seen in this image from NASA's Mars Reconnaissance Orbiter.

Pedestal Crater Development

A pedestal crater is when the ejecta from an impact settles around the new crater and is more erosion-resistant than the surrounding terrain as seen in this image from NASA's Mars Reconnaissance Orbiter.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19849
Added: 2015-07-01

Views: 46

Pedestal Crater Development

A pedestal crater is when the ejecta from an impact settles around the new crater and is more erosion-resistant than the surrounding terrain as seen in this image from NASA's Mars Reconnaissance Orbiter.

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A delta is a pile of sediment dumped by a river where it enters a standing body of water. Evidence for deltas that formed billions of years ago on Mars has been mounting in recent years. This image is from NASA's Mars Reconnaissance Orbiter.
A delta is a pile of sediment dumped by a river where it enters a standing body of water. Evidence for deltas that formed billions of years ago on Mars has been mounting in recent years. This image is from NASA's Mars Reconnaissance Orbiter.

Searching for Clinoforms in a Possible Delta

A delta is a pile of sediment dumped by a river where it enters a standing body of water. Evidence for deltas that formed billions of years ago on Mars has been mounting in recent years. 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#: PIA19848
Added: 2015-07-01

Views: 52

Searching for Clinoforms in a Possible Delta

A delta is a pile of sediment dumped by a river where it enters a standing body of water. Evidence for deltas that formed billions of years ago on Mars has been mounting in recent years. This image is from NASA's Mars Reconnaissance Orbiter.

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This observation from NASA's Mars Reconnaissance Orbite shows a candidate 2018 European Space Agency ExoMars landing site in Hypanis Vallis.
This observation from NASA's Mars Reconnaissance Orbite shows a candidate 2018 European Space Agency ExoMars landing site in Hypanis Vallis.

Cloudy Skies over Hypanis Vallis

This observation from NASA's Mars Reconnaissance Orbite shows a candidate 2018 European Space Agency ExoMars landing site in Hypanis Vallis.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19846
Added: 2015-06-17

Views: 33

Cloudy Skies over Hypanis Vallis

This observation from NASA's Mars Reconnaissance Orbite shows a candidate 2018 European Space Agency ExoMars landing site in Hypanis Vallis.

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The focus of this image from NASA's Mars Reconnaissance Orbiter is on the western end of a fan-shaped landform, located at the end point of a sinuous valley.
The focus of this image from NASA's Mars Reconnaissance Orbiter is on the western end of a fan-shaped landform, located at the end point of a sinuous valley.

A Fan-Shaped Landform and Nearby Light-Toned Material

The focus of this image from NASA's Mars Reconnaissance Orbiter is on the western end of a fan-shaped landform, located at the end point of a sinuous valley.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19845
Added: 2015-06-17

Views: 36

A Fan-Shaped Landform and Nearby Light-Toned Material

The focus of this image from NASA's Mars Reconnaissance Orbiter is on the western end of a fan-shaped landform, located at the end point of a sinuous valley.

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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.' Some shapes suggest erosion by a fluid moving north and south.
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.' Some shapes suggest erosion by a fluid moving north and south.

A Light Toned Deposit in Aureum 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.' Some shapes suggest erosion by a fluid moving north and south.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19844
Added: 2015-06-17

Views: 41

A Light Toned Deposit in Aureum 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.' Some shapes suggest erosion by a fluid moving north and south.

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Gully and defrosting activity have been visible here along the edge of a dune field, along with blocks of frost. Observations from NASA's Mars Reconnaissance Orbiter of the same area help check for repeat activity.
Gully and defrosting activity have been visible here along the edge of a dune field, along with blocks of frost. Observations from NASA's Mars Reconnaissance Orbiter of the same area help check for repeat activity.

Active High-Latitude Dune-Gullies

Gully and defrosting activity have been visible here along the edge of a dune field, along with blocks of frost. Observations from NASA's Mars Reconnaissance Orbiter of the same area help check for repeat activity.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19843
Added: 2015-06-17

Views: 43

Active High-Latitude Dune-Gullies

Gully and defrosting activity have been visible here along the edge of a dune field, along with blocks of frost. Observations from NASA's Mars Reconnaissance Orbiter of the same area help check for repeat activity.

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Researchers have found deposits of impact glass preserved in Martian craters, including Alga Crater, shown here. The detection is based on data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on NASA's Mars Reconnaissance Orbiter.
Researchers have found deposits of impact glass preserved in Martian craters, including Alga Crater, shown here. The detection is based on data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on NASA's Mars Reconnaissance Orbiter.

Spectral Signals Indicating Impact Glass on Mars

Researchers have found deposits of impact glass preserved in Martian craters, including Alga Crater, shown here. The detection is based on data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on NASA's Mars Reconnaissance Orbiter.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: Compact Reconnaissance Imaging Spectrometer for Mars (CRISM)
ID#: PIA19673
Added: 2015-06-08

Views: 1800

Spectral Signals Indicating Impact Glass on Mars

Researchers have found deposits of impact glass preserved in Martian craters, including Alga Crater, shown here. The detection is based on data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on NASA's Mars Reconnaissance Orbiter.

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This observation from NASA's Mars Reconnaissance Orbiter locates what appears to be a graben (a fault-bounded valley) on a large scale, and locally became a vent region for lava flows.
This observation from NASA's Mars Reconnaissance Orbiter locates what appears to be a graben (a fault-bounded valley) on a large scale, and locally became a vent region for lava flows.

Gigas Sulci

This observation from NASA's Mars Reconnaissance Orbiter locates what appears to be a graben (a fault-bounded valley) on a large scale, and locally became a vent region for lava flows.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA11778
Added: 2015-06-03

Views: 181

Gigas Sulci

This observation from NASA's Mars Reconnaissance Orbiter locates what appears to be a graben (a fault-bounded valley) on a large scale, and locally became a vent region for lava flows.

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This impact crater, as seen by NASA's Mars Reconnaissance Orbiter, appears relatively recent as it has a sharp rim and well-preserved ejecta.
This impact crater, as seen by NASA's Mars Reconnaissance Orbiter, appears relatively recent as it has a sharp rim and well-preserved ejecta.

A Fresh Crater near Sirenum Fossae

This impact crater, as seen by NASA's Mars Reconnaissance Orbiter, appears relatively recent as it has a sharp rim and well-preserved ejecta.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA11777
Added: 2015-06-03

Views: 476

A Fresh Crater near Sirenum Fossae

This impact crater, as seen by NASA's Mars Reconnaissance Orbiter, appears relatively recent as it has a sharp rim and well-preserved ejecta.

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This image from NASA's Mars Reconnaissance Orbiter shows a lacy network of many fine channels associated with jets in the subliming carbon dioxide of the springtime.
This image from NASA's Mars Reconnaissance Orbiter shows a lacy network of many fine channels associated with jets in the subliming carbon dioxide of the springtime.

A Mysterious Bright Streak on the South Polar Layered Deposits

This image from NASA's Mars Reconnaissance Orbiter shows a lacy network of many fine channels associated with jets in the subliming carbon dioxide of the springtime.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA11776
Added: 2015-06-03

Views: 165

A Mysterious Bright Streak on the South Polar Layered Deposits

This image from NASA's Mars Reconnaissance Orbiter shows a lacy network of many fine channels associated with jets in the subliming carbon dioxide of the springtime.

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This observation from NASA's Mars Reconnaissance Orbiter targets some unknown fill or mantling material within valleys on a crater floor and within a central pit.
This observation from NASA's Mars Reconnaissance Orbiter targets some unknown fill or mantling material within valleys on a crater floor and within a central pit.

Fill or Mantling Material in a Crater

This observation from NASA's Mars Reconnaissance Orbiter targets some unknown fill or mantling material within valleys on a crater floor and within a central pit.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA11775
Added: 2015-06-03

Views: 204

Fill or Mantling Material in a Crater

This observation from NASA's Mars Reconnaissance Orbiter targets some unknown fill or mantling material within valleys on a crater floor and within a central pit.

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This image from NASA's Mars Reconnaissance Orbiter shows a landscape that is pervasively eroded, right up to the tops of the ridges, with channels extending down into depositional fans much like alluvial fans in the Mojave Desert.
This image from NASA's Mars Reconnaissance Orbiter shows a landscape that is pervasively eroded, right up to the tops of the ridges, with channels extending down into depositional fans much like alluvial fans in the Mojave Desert.

Alluvial Fans in Mojave Crater

This image from NASA's Mars Reconnaissance Orbiter shows a landscape that is pervasively eroded, right up to the tops of the ridges, with channels extending down into depositional fans much like alluvial fans in the Mojave Desert.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18563
Added: 2015-05-20

Views: 408

Alluvial Fans in Mojave Crater

This image from NASA's Mars Reconnaissance Orbiter shows a landscape that is pervasively eroded, right up to the tops of the ridges, with channels extending down into depositional fans much like alluvial fans in the Mojave Desert.

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This image from NASA's Mars Reconnaissance Orbiter covers layered sedimentary rocks on the floor of an impact crater north of Eberswalde Crater. There may have been a lake in this crater billions of years ago.
This image from NASA's Mars Reconnaissance Orbiter covers layered sedimentary rocks on the floor of an impact crater north of Eberswalde Crater. There may have been a lake in this crater billions of years ago.

Sedimentary Rock Layers on a Crater Floor

This image from NASA's Mars Reconnaissance Orbiter covers layered sedimentary rocks on the floor of an impact crater north of Eberswalde Crater. There may have been a lake in this crater billions of years ago.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA18562
Added: 2015-05-20

Views: 468

Sedimentary Rock Layers on a Crater Floor

This image from NASA's Mars Reconnaissance Orbiter covers layered sedimentary rocks on the floor of an impact crater north of Eberswalde Crater. There may have been a lake in this crater billions of years ago.

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Seasonal flows called recurring slope lineae (RSL) grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA's Mars Reconnaissance Orbiter
Seasonal flows called recurring slope lineae (RSL) grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA's Mars Reconnaissance Orbiter

Seasonal Flows in Asimov Crater

Seasonal flows called recurring slope lineae (RSL) grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation 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#: PIA18561
Added: 2015-05-20

Views: 283

Seasonal Flows in Asimov Crater

Seasonal flows called recurring slope lineae (RSL) grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA's Mars Reconnaissance Orbiter

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