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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: 132

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: 117

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: 117

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: 136

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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The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Cimmeria.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Cimmeria.

Terra Cimmeria - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Cimmeria.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19725
Added: 2015-07-15

Views: 173

Terra Cimmeria - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Cimmeria.

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The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra north of the Argyre basin.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra north of the Argyre basin.

Noachis Terra - False Color

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra north of the Argyre basin.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19724
Added: 2015-07-14

Views: 198

Noachis Terra - False Color

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra north of the Argyre basin.

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The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Terra Sabaea.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Terra Sabaea.

Terra Sabaea - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Terra Sabaea.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19723
Added: 2015-07-13

Views: 238

Terra Sabaea - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Terra Sabaea.

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The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Daedalia Planum, a huge lava field that originates from Arsia Mons.
The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Daedalia Planum, a huge lava field that originates from Arsia Mons.

Daedalia Planum

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Daedalia Planum, a huge lava field that originates from Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19722
Added: 2015-07-10

Views: 220

Daedalia Planum

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Daedalia Planum, a huge lava field that originates from Arsia Mons.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Cavi Angusti, a region of depressions near the south polar cap. The linear ridges in the image were likely formed by tectonic activity.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Cavi Angusti, a region of depressions near the south polar cap. The linear ridges in the image were likely formed by tectonic activity.

Cavi Angusti

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Cavi Angusti, a region of depressions near the south polar cap. The linear ridges in the image were likely formed by tectonic activity.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19721
Added: 2015-07-09

Views: 223

Cavi Angusti

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Cavi Angusti, a region of depressions near the south polar cap. The linear ridges in the image were likely formed by tectonic activity.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows depressions near the south polar cap. All surface ice in this region has been removed by the relative warmth of summer, revealing subtle features of the surface.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows depressions near the south polar cap. All surface ice in this region has been removed by the relative warmth of summer, revealing subtle features of the surface.

Summer's End

This image captured by NASA's 2001 Mars Odyssey spacecraft shows depressions near the south polar cap. All surface ice in this region has been removed by the relative warmth of summer, revealing subtle features of the surface.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19720
Added: 2015-07-08

Views: 203

Summer's End

This image captured by NASA's 2001 Mars Odyssey spacecraft shows depressions near the south polar cap. All surface ice in this region has been removed by the relative warmth of summer, revealing subtle features of the surface.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of Tugaske Crater. The northern margin of this crater has been modified from a circular form, most likely related to the tectonic activity of Claritas Fossae, where this crater is located.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of Tugaske Crater. The northern margin of this crater has been modified from a circular form, most likely related to the tectonic activity of Claritas Fossae, where this crater is located.

Tugaske Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows part of Tugaske Crater. The northern margin of this crater has been modified from a circular form, most likely related to the tectonic activity of Claritas Fossae, where this crater is located.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19505
Added: 2015-07-07

Views: 185

Tugaske Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows part of Tugaske Crater. The northern margin of this crater has been modified from a circular form, most likely related to the tectonic activity of Claritas Fossae, where this crater is located.

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This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater located on the floor of the much larger Newton Crater. This crater had a central peak, gullies on the inner rim and dunes on the northern part of the crater floor.
This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater located on the floor of the much larger Newton Crater. This crater had a central peak, gullies on the inner rim and dunes on the northern part of the crater floor.

Crater Features

This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater located on the floor of the much larger Newton Crater. This crater had a central peak, gullies on the inner rim and dunes on the northern part of the crater floor.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19504
Added: 2015-07-06

Views: 231

Crater Features

This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater located on the floor of the much larger Newton Crater. This crater had a central peak, gullies on the inner rim and dunes on the northern part of the crater floor.

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The linear features in this image from NASA's 2001 Mars Odyssey spacecraft are faults. Where depressions are formed bounded by faulting the feature is called a graben. These faults and graben are part of a large region of faulting called Sirenum Fossae.
The linear features in this image from NASA's 2001 Mars Odyssey spacecraft are faults. Where depressions are formed bounded by faulting the feature is called a graben. These faults and graben are part of a large region of faulting called Sirenum Fossae.

Sirenum Fossae

The linear features in this image from NASA's 2001 Mars Odyssey spacecraft are faults. Where depressions are formed bounded by faulting the feature is called a graben. These faults and graben are part of a large region of faulting called Sirenum Fossae.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19503
Added: 2015-07-03

Views: 269

Sirenum Fossae

The linear features in this image from NASA's 2001 Mars Odyssey spacecraft are faults. Where depressions are formed bounded by faulting the feature is called a graben. These faults and graben are part of a large region of faulting called Sirenum Fossae.

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This image captured by NASA's 2001 Mars Odyssey spacecraft show long term winds have etched the surface in Memnonia Sulci. Partial cemented surface materials are easily eroded by the wind, forming linear ridges called yardangs.
This image captured by NASA's 2001 Mars Odyssey spacecraft show long term winds have etched the surface in Memnonia Sulci. Partial cemented surface materials are easily eroded by the wind, forming linear ridges called yardangs.

Wind Erosion

This image captured by NASA's 2001 Mars Odyssey spacecraft show long term winds have etched the surface in Memnonia Sulci. Partial cemented surface materials are easily eroded by the wind, forming linear ridges called yardangs.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19502
Added: 2015-07-02

Views: 267

Wind Erosion

This image captured by NASA's 2001 Mars Odyssey spacecraft show long term winds have etched the surface in Memnonia Sulci. Partial cemented surface materials are easily eroded by the wind, forming linear ridges called yardangs.

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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: 119

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: 100

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: 106

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: 114

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 360-degree panorama from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the surroundings of a site on lower Mount Sharp where the rover spent its 1,000th Martian day, or sol, on Mars.
This 360-degree panorama from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the surroundings of a site on lower Mount Sharp where the rover spent its 1,000th Martian day, or sol, on Mars.

Panorama from Curiosity's Sol 1000 Location

This 360-degree panorama from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the surroundings of a site on lower Mount Sharp where the rover spent its 1,000th Martian day, or sol, on Mars.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Mars Science Laboratory (MSL)
Instrument: Navigation Camera (MSL)
ID#: PIA19679
Added: 2015-07-01

Views: 705

Panorama from Curiosity's Sol 1000 Location

This 360-degree panorama from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the surroundings of a site on lower Mount Sharp where the rover spent its 1,000th Martian day, or sol, on Mars.

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This 3-D stereo view from NASA's Curiosity Mars rover shows a 360-degree panorama around the location where the rover spent its 1,000th Martian day, or sol, on Mars. The site is a valley just below 'Marias Pass' on lower Mount Sharp.
This 3-D stereo view from NASA's Curiosity Mars rover shows a 360-degree panorama around the location where the rover spent its 1,000th Martian day, or sol, on Mars. The site is a valley just below 'Marias Pass' on lower Mount Sharp.

Panorama from Curiosity's Sol 1000 Location (Stereo)

This 3-D stereo view from NASA's Curiosity Mars rover shows a 360-degree panorama around the location where the rover spent its 1,000th Martian day, or sol, on Mars. The site is a valley just below 'Marias Pass' on lower Mount Sharp.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Mars Science Laboratory (MSL)
Instrument: Navigation Camera (MSL)
ID#: PIA19678
Added: 2015-07-01

Views: 1159

Panorama from Curiosity's Sol 1000 Location (Stereo)

This 3-D stereo view from NASA's Curiosity Mars rover shows a 360-degree panorama around the location where the rover spent its 1,000th Martian day, or sol, on Mars. The site is a valley just below 'Marias Pass' on lower Mount Sharp.

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This view of a sandstone target called 'Big Arm' covers an area about 1.3 inches (33 millimeters) wide in detail that shows differing shapes and colors of sand grains in the stone.
This view of a sandstone target called 'Big Arm' covers an area about 1.3 inches (33 millimeters) wide in detail that shows differing shapes and colors of sand grains in the stone.

Diverse Grains in Mars Sandstone Target 'Big Arm'

This view of a sandstone target called 'Big Arm' covers an area about 1.3 inches (33 millimeters) wide in detail that shows differing shapes and colors of sand grains in the stone.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Mars Science Laboratory (MSL)
Instrument: Mars Hand Lens Imager (MAHLI)
ID#: PIA19677
Added: 2015-07-01

Views: 841

Diverse Grains in Mars Sandstone Target 'Big Arm'

This view of a sandstone target called 'Big Arm' covers an area about 1.3 inches (33 millimeters) wide in detail that shows differing shapes and colors of sand grains in the stone.

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This view from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover shows a site where two different types of bedrock meet on lower Mount Sharp.
This view from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover shows a site where two different types of bedrock meet on lower Mount Sharp.

Geological Contact Zone Near 'Marias Pass' on Mars

This view from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover shows a site where two different types of bedrock meet on lower Mount Sharp.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Mars Science Laboratory (MSL)
Instrument: Mastcam
ID#: PIA19676
Added: 2015-07-01

Views: 1202

Geological Contact Zone Near 'Marias Pass' on Mars

This view from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover shows a site where two different types of bedrock meet on lower Mount Sharp.

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This image from NASA's 2001 Mars Odyssey spacecraft shows two channels. The channel in the center of the image ends in a crater, where it has created a delta deposit. These craters and channels are located on the northeastern margin of Icaria Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows two channels. The channel in the center of the image ends in a crater, where it has created a delta deposit. These craters and channels are located on the northeastern margin of Icaria Planum.

Channel and Delta

This image from NASA's 2001 Mars Odyssey spacecraft shows two channels. The channel in the center of the image ends in a crater, where it has created a delta deposit. These craters and channels are located on the northeastern margin of Icaria Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19500
Added: 2015-07-01

Views: 195

Channel and Delta

This image from NASA's 2001 Mars Odyssey spacecraft shows two channels. The channel in the center of the image ends in a crater, where it has created a delta deposit. These craters and channels are located on the northeastern margin of Icaria Planum.

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This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel draining from the highlands of Promethei Terra to lowlands of the Hellas Basin.
This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel draining from the highlands of Promethei Terra to lowlands of the Hellas Basin.

Channel

This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel draining from the highlands of Promethei Terra to lowlands of the Hellas Basin.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19499
Added: 2015-06-30

Views: 240

Channel

This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel draining from the highlands of Promethei Terra to lowlands of the Hellas Basin.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the lava flows of Daedalia Planum. The 'tail' behind the crater indicates winds blew from east to west.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the lava flows of Daedalia Planum. The 'tail' behind the crater indicates winds blew from east to west.

Windstreaks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the lava flows of Daedalia Planum. The 'tail' behind the crater indicates winds blew from east to west.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19498
Added: 2015-06-29

Views: 215

Windstreaks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the lava flows of Daedalia Planum. The 'tail' behind the crater indicates winds blew from east to west.

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