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Recurring slope lineae are active flows on warm Martian slopes that might be caused by seeping water. One of the most active sites known is in the central peaks of Hale Crater as seen by NASA's Mars Reconnaissance Orbiter.
Recurring slope lineae are active flows on warm Martian slopes that might be caused by seeping water. One of the most active sites known is in the central peaks of Hale Crater as seen by NASA's Mars Reconnaissance Orbiter.

Seasonal Flows in the Central Mountains of Hale Crater

Recurring slope lineae are active flows on warm Martian slopes that might be caused by seeping water. One of the most active sites known is in the central peaks of Hale Crater 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#: PIA19359
Added: 2015-04-08

Views: 2050

Seasonal Flows in the Central Mountains of Hale Crater

Recurring slope lineae are active flows on warm Martian slopes that might be caused by seeping water. One of the most active sites known is in the central peaks of Hale Crater as seen by NASA's Mars Reconnaissance Orbiter.

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The target of this observation as seen by ASA's Mars Reconnaissance Orbiter is a circular depression in a dark-toned unit associated with a field of cones to the northeast.
The target of this observation as seen by ASA's Mars Reconnaissance Orbiter is a circular depression in a dark-toned unit associated with a field of cones to the northeast.

Layers and Dark Dunes

The target of this observation as seen by ASA's Mars Reconnaissance Orbiter is a circular depression in a dark-toned unit associated with a field of cones to the northeast.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19358
Added: 2015-04-08

Views: 311

Layers and Dark Dunes

The target of this observation as seen by ASA's Mars Reconnaissance Orbiter is a circular depression in a dark-toned unit associated with a field of cones to the northeast.

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Coprates Chasma is located in the huge canyon system, Vallis Marineris. NASA's Mars Reconnaissance Orbiter finds indications of high thermal inertia.
Coprates Chasma is located in the huge canyon system, Vallis Marineris. NASA's Mars Reconnaissance Orbiter finds indications of high thermal inertia.

What on Mars is a High Thermal-Inertia Surface?

Coprates Chasma is located in the huge canyon system, Vallis Marineris. NASA's Mars Reconnaissance Orbiter finds indications of high thermal inertia.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19357
Added: 2015-04-08

Views: 214

What on Mars is a High Thermal-Inertia Surface?

Coprates Chasma is located in the huge canyon system, Vallis Marineris. NASA's Mars Reconnaissance Orbiter finds indications of high thermal inertia.

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There are some interesting erosional signs in this observation from NASA's Mars Reconnaissance Orbiter, which will make for a good comparison with other intracrater fans and fluvial sedimentary landforms.
There are some interesting erosional signs in this observation from NASA's Mars Reconnaissance Orbiter, which will make for a good comparison with other intracrater fans and fluvial sedimentary landforms.

Sinuous Ridge Materials in Reuyl Crater

There are some interesting erosional signs in this observation from NASA's Mars Reconnaissance Orbiter, which will make for a good comparison with other intracrater fans and fluvial sedimentary landforms.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19356
Added: 2015-04-08

Views: 187

Sinuous Ridge Materials in Reuyl Crater

There are some interesting erosional signs in this observation from NASA's Mars Reconnaissance Orbiter, which will make for a good comparison with other intracrater fans and fluvial sedimentary landforms.

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This frame from a sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.
This frame from a sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

Changes in Scars From 2012 Mars Landing

This frame from a sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO), Mars Science Laboratory (MSL)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19159
Added: 2015-03-27

Views: 14722

Changes in Scars From 2012 Mars Landing

This frame from a sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

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This observation from NASA's Mars Reconnaissance Orbiter shows an interesting crater floor with what appear to be inverted channels, rounded lobe-like landforms, and light-toned layered deposits along the southern portion of the crater wall.
This observation from NASA's Mars Reconnaissance Orbiter shows an interesting crater floor with what appear to be inverted channels, rounded lobe-like landforms, and light-toned layered deposits along the southern portion of the crater wall.

Possible Fluvial Features in Golden Crater

This observation from NASA's Mars Reconnaissance Orbiter shows an interesting crater floor with what appear to be inverted channels, rounded lobe-like landforms, and light-toned layered deposits along the southern portion of the crater wall.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19353
Added: 2015-03-25

Views: 234

Possible Fluvial Features in Golden Crater

This observation from NASA's Mars Reconnaissance Orbiter shows an interesting crater floor with what appear to be inverted channels, rounded lobe-like landforms, and light-toned layered deposits along the southern portion of the crater wall.

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Osuga Valles lies around 170 kilometers to the south of Eos Chasma, which is at the eastern end of the vast Valles Marineris canyon system as seen by NASA's Mars Reconnaissance Orbiter.
Osuga Valles lies around 170 kilometers to the south of Eos Chasma, which is at the eastern end of the vast Valles Marineris canyon system as seen by NASA's Mars Reconnaissance Orbiter.

The Lowest Point of Osuga Valles

Osuga Valles lies around 170 kilometers to the south of Eos Chasma, which is at the eastern end of the vast Valles Marineris canyon system 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#: PIA19352
Added: 2015-03-25

Views: 274

The Lowest Point of Osuga Valles

Osuga Valles lies around 170 kilometers to the south of Eos Chasma, which is at the eastern end of the vast Valles Marineris canyon system as seen by NASA's Mars Reconnaissance Orbiter.

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This observation from NASA's Mars Reconnaissance Orbiter shows samples of bedrock lithologies which give us a measure of the post-flood erosion and modification history for the floor of Kasei Valles.
This observation from NASA's Mars Reconnaissance Orbiter shows samples of bedrock lithologies which give us a measure of the post-flood erosion and modification history for the floor of Kasei Valles.

At the Head of a Kasei Valles Cataract

This observation from NASA's Mars Reconnaissance Orbiter shows samples of bedrock lithologies which give us a measure of the post-flood erosion and modification history for the floor of Kasei Valles.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19351
Added: 2015-03-25

Views: 164

At the Head of a Kasei Valles Cataract

This observation from NASA's Mars Reconnaissance Orbiter shows samples of bedrock lithologies which give us a measure of the post-flood erosion and modification history for the floor of Kasei Valles.

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This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed by NASA's Mars Reconnaissance Orbiter.
This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed by NASA's Mars Reconnaissance Orbiter.

Pitted Landforms in Southern Hellas Planitia

This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed 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#: PIA19350
Added: 2015-03-25

Views: 168

Pitted Landforms in Southern Hellas Planitia

This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed by NASA's Mars Reconnaissance Orbiter.

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Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers).
Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers).

Opportunity Rover Surpasses Marathon Distance

Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers).

Target: Mars
Mission: Mars Exploration Rover (MER), Mars Reconnaissance Orbiter (MRO)
Spacecraft: Opportunity
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19157
Added: 2015-03-24

Views: 557

Opportunity Rover Surpasses Marathon Distance

Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers).

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This image from NASA's Mars Reconnaissance Orbiter covers Raga Crater, the location of well-studied recurring slope lineae (RSL). RSL are dark flows that disappear and re-form every Mars year at certain locations.
This image from NASA's Mars Reconnaissance Orbiter covers Raga Crater, the location of well-studied recurring slope lineae (RSL). RSL are dark flows that disappear and re-form every Mars year at certain locations.

Recurring Slope Lineae in Raga Crater

This image from NASA's Mars Reconnaissance Orbiter covers Raga Crater, the location of well-studied recurring slope lineae (RSL). RSL are dark flows that disappear and re-form every Mars year at certain locations.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19309
Added: 2015-03-11

Views: 123

Recurring Slope Lineae in Raga Crater

This image from NASA's Mars Reconnaissance Orbiter covers Raga Crater, the location of well-studied recurring slope lineae (RSL). RSL are dark flows that disappear and re-form every Mars year at certain locations.

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Gullies are commonly found in the southern mid-latitudes of Mars. In this image from NASA's Mars Reconnaissance Orbiter they start near top of a long ridge, and descend into an impact crater that lies at the bottom of the ridge.
Gullies are commonly found in the southern mid-latitudes of Mars. In this image from NASA's Mars Reconnaissance Orbiter they start near top of a long ridge, and descend into an impact crater that lies at the bottom of the ridge.

Gullies and Layers in a Crater Near Mariner Crater

Gullies are commonly found in the southern mid-latitudes of Mars. In this image from NASA's Mars Reconnaissance Orbiter they start near top of a long ridge, and descend into an impact crater that lies at the bottom of the ridge.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19308
Added: 2015-03-11

Views: 150

Gullies and Layers in a Crater Near Mariner Crater

Gullies are commonly found in the southern mid-latitudes of Mars. In this image from NASA's Mars Reconnaissance Orbiter they start near top of a long ridge, and descend into an impact crater that lies at the bottom of the ridge.

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This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.
This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.

Cracks in a Debris Apron

This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19307
Added: 2015-03-11

Views: 128

Cracks in a Debris Apron

This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.

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This image from NASA's Mars Reconnaissance Orbiter shows a region of Acidalia Planitia which is covered by dense fields of boulders up to several meters high.
This image from NASA's Mars Reconnaissance Orbiter shows a region of Acidalia Planitia which is covered by dense fields of boulders up to several meters high.

Ares 3 and The Martian

This image from NASA's Mars Reconnaissance Orbiter shows a region of Acidalia Planitia which is covered by dense fields of boulders up to several meters high.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19306
Added: 2015-03-11

Views: 163

Ares 3 and The Martian

This image from NASA's Mars Reconnaissance Orbiter shows a region of Acidalia Planitia which is covered by dense fields of boulders up to several meters high.

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This image from NASA's Mars Reconnaissance Orbiter shows sand avalanches in Meroe Patera.
This image from NASA's Mars Reconnaissance Orbiter shows sand avalanches in Meroe Patera.

Sand Avalanches in Meroe Patera

This image from NASA's Mars Reconnaissance Orbiter shows sand avalanches in Meroe Patera.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19305
Added: 2015-03-04

Views: 281

Sand Avalanches in Meroe Patera

This image from NASA's Mars Reconnaissance Orbiter shows sand avalanches in Meroe Patera.

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This image from NASA's Mars Reconnaissance Orbiter of craters near Nilokeras Scopulus shows two pits partially filled with lumpy material, probably trapped dust that blew in from the atmosphere.
This image from NASA's Mars Reconnaissance Orbiter of craters near Nilokeras Scopulus shows two pits partially filled with lumpy material, probably trapped dust that blew in from the atmosphere.

Craters Near Nilokeras Scopulus

This image from NASA's Mars Reconnaissance Orbiter of craters near Nilokeras Scopulus shows two pits partially filled with lumpy material, probably trapped dust that blew in from the atmosphere.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19304
Added: 2015-03-04

Views: 223

Craters Near Nilokeras Scopulus

This image from NASA's Mars Reconnaissance Orbiter of craters near Nilokeras Scopulus shows two pits partially filled with lumpy material, probably trapped dust that blew in from the atmosphere.

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This image shows a possible landing site for the 2020 Mission: Jezero Crater, as seen by NASA's Mars Reconnaissance Orbiter.
This image shows a possible landing site for the 2020 Mission: Jezero Crater, as seen by NASA's Mars Reconnaissance Orbiter.

A Possible Landing Site for the 2020 Mission: Jezero Crater

This image shows a possible landing site for the 2020 Mission: Jezero Crater, 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#: PIA19303
Added: 2015-03-04

Views: 231

A Possible Landing Site for the 2020 Mission: Jezero Crater

This image shows a possible landing site for the 2020 Mission: Jezero Crater, as seen by NASA's Mars Reconnaissance Orbiter.

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This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.
This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.

Dunes in Western Medusae Fossae Formation

This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19302
Added: 2015-03-04

Views: 301

Dunes in Western Medusae Fossae Formation

This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.

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Bigbee is a 21 kilometer-diameter impact crater located on the northern rim of Holden crater in southern Margaritifer Terra, a region on Mars that is well known for its long record of water-rich activity as seen by NASA's Mars Reconnaissance Orbiter.
Bigbee is a 21 kilometer-diameter impact crater located on the northern rim of Holden crater in southern Margaritifer Terra, a region on Mars that is well known for its long record of water-rich activity as seen by NASA's Mars Reconnaissance Orbiter.

Fan-Shaped Deposits in Bigbee Crater

Bigbee is a 21 kilometer-diameter impact crater located on the northern rim of Holden crater in southern Margaritifer Terra, a region on Mars that is well known for its long record of water-rich activity 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#: PIA19296
Added: 2015-02-11

Views: 876

Fan-Shaped Deposits in Bigbee Crater

Bigbee is a 21 kilometer-diameter impact crater located on the northern rim of Holden crater in southern Margaritifer Terra, a region on Mars that is well known for its long record of water-rich activity as seen by NASA's Mars Reconnaissance Orbiter.

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The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.
The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

Boulders in Gully Alcoves

The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19295
Added: 2015-02-11

Views: 391

Boulders in Gully Alcoves

The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

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The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.
The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

Gullies and Bedrock in Nirgal Vallis

The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19294
Added: 2015-02-11

Views: 347

Gullies and Bedrock in Nirgal Vallis

The gullies observed in this image from NASA's Mars Reconnaissance Orbiter are within the valley wall of an ancient channel-Nirgal Vallis-a testament to flowing water in Mars' ancient past.

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Taken in late southern spring and when Mars is near perihelion (closest distance to the Sun), this image from NASA's Mars Reconnaissance Orbiter shows the effects of dry ice sublimation on a longitudinal dune in the far Southern hemisphere.
Taken in late southern spring and when Mars is near perihelion (closest distance to the Sun), this image from NASA's Mars Reconnaissance Orbiter shows the effects of dry ice sublimation on a longitudinal dune in the far Southern hemisphere.

A Large, Longitudinal Dune

Taken in late southern spring and when Mars is near perihelion (closest distance to the Sun), this image from NASA's Mars Reconnaissance Orbiter shows the effects of dry ice sublimation on a longitudinal dune in the far Southern hemisphere.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19293
Added: 2015-02-11

Views: 266

A Large, Longitudinal Dune

Taken in late southern spring and when Mars is near perihelion (closest distance to the Sun), this image from NASA's Mars Reconnaissance Orbiter shows the effects of dry ice sublimation on a longitudinal dune in the far Southern hemisphere.

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NASA's Curiosity Mars rover can be seen at the 'Pahrump Hills' area of Gale Crater in this view from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
NASA's Curiosity Mars rover can be seen at the 'Pahrump Hills' area of Gale Crater in this view from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

Curiosity Rover at 'Pahrump Hills'

NASA's Curiosity Mars rover can be seen at the 'Pahrump Hills' area of Gale Crater in this view from the High Resolution Imaging Science Experiment (HiRISE) camera on 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#: PIA19114
Added: 2015-02-04

Views: 7374

Curiosity Rover at 'Pahrump Hills'

NASA's Curiosity Mars rover can be seen at the 'Pahrump Hills' area of Gale Crater in this view from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

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The dark fans in this image are made up of small particles from the surface deposited on top of the seasonal layer of ice; carbon dioxide ice still covers much of the surface at this high latitude site observed by NASA's Mars Reconnaissance Orbiter.
The dark fans in this image are made up of small particles from the surface deposited on top of the seasonal layer of ice; carbon dioxide ice still covers much of the surface at this high latitude site observed by NASA's Mars Reconnaissance Orbiter.

Icy Wonderland

The dark fans in this image are made up of small particles from the surface deposited on top of the seasonal layer of ice; carbon dioxide ice still covers much of the surface at this high latitude site observed 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#: PIA19292
Added: 2015-02-04

Views: 472

Icy Wonderland

The dark fans in this image are made up of small particles from the surface deposited on top of the seasonal layer of ice; carbon dioxide ice still covers much of the surface at this high latitude site observed by NASA's Mars Reconnaissance Orbiter.

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Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.
Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.

Yardangs in Arsinoes Chaos, Mars

Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19291
Added: 2015-02-04

Views: 917

Yardangs in Arsinoes Chaos, Mars

Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.

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