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A grid of small polygons on the Martian rock surface near the right edge of this view may have originated as cracks in drying mud more than 3 billion years ago. Multiple images of this view were combined for this view from NASA's Curiosity Mars rover.
A grid of small polygons on the Martian rock surface near the right edge of this view may have originated as cracks in drying mud more than 3 billion years ago. Multiple images of this view were combined for this view from NASA's Curiosity Mars rover.

Possible Signs of Ancient Drying in Martian Rock

A grid of small polygons on the Martian rock surface near the right edge of this view may have originated as cracks in drying mud more than 3 billion years ago. Multiple images of this view were combined for this view from NASA's Curiosity Mars rover.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA21263
Added: 2017-01-17

Views: 760

Possible Signs of Ancient Drying in Martian Rock

A grid of small polygons on the Martian rock surface near the right edge of this view may have originated as cracks in drying mud more than 3 billion years ago. Multiple images of this view were combined for this view from NASA's Curiosity Mars rover.

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This view of a Martian rock slab called 'Old Soaker,' which has a network of cracks that may have originated in drying mud, comes from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover.
This view of a Martian rock slab called 'Old Soaker,' which has a network of cracks that may have originated in drying mud, comes from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover.

Mars Rover's Mastcam View of Possible Mud Cracks

This view of a Martian rock slab called 'Old Soaker,' which has a network of cracks that may have originated in drying mud, comes from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA21262
Added: 2017-01-17

Views: 1246

Mars Rover's Mastcam View of Possible Mud Cracks

This view of a Martian rock slab called 'Old Soaker,' which has a network of cracks that may have originated in drying mud, comes from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover.

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The network of cracks in this Martian rock slab called 'Old Soaker' may have formed from the drying of a mud layer more than 3 billion years ago. The view combines three images taken by NASA's Curiosity Mars rover on Dec. 31, 2016.
The network of cracks in this Martian rock slab called 'Old Soaker' may have formed from the drying of a mud layer more than 3 billion years ago. The view combines three images taken by NASA's Curiosity Mars rover on Dec. 31, 2016.

Possible Mud Cracks Preserved in Martian Rock

The network of cracks in this Martian rock slab called 'Old Soaker' may have formed from the drying of a mud layer more than 3 billion years ago. The view combines three images taken by NASA's Curiosity Mars rover on Dec. 31, 2016.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mars Hand Lens Imager (MAHLI)
ID#: PIA21261
Added: 2017-01-17

Views: 1656

Possible Mud Cracks Preserved in Martian Rock

The network of cracks in this Martian rock slab called 'Old Soaker' may have formed from the drying of a mud layer more than 3 billion years ago. The view combines three images taken by NASA's Curiosity Mars rover on Dec. 31, 2016.

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Impact craters form when an asteroid, meteoroid, or comet crashes into a planet's surface, causing an explosion. This impact crater is a little less than 3 kilometers in diameter as seen by NASA's Mars Reconnaissance Orbiter.
Impact craters form when an asteroid, meteoroid, or comet crashes into a planet's surface, causing an explosion. This impact crater is a little less than 3 kilometers in diameter as seen by NASA's Mars Reconnaissance Orbiter.

Crater with Exposed Layers

Impact craters form when an asteroid, meteoroid, or comet crashes into a planet's surface, causing an explosion. This impact crater is a little less than 3 kilometers in diameter 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#: PIA12328
Added: 2017-01-17

Views: 155

Crater with Exposed Layers

Impact craters form when an asteroid, meteoroid, or comet crashes into a planet's surface, causing an explosion. This impact crater is a little less than 3 kilometers in diameter as seen by NASA's Mars Reconnaissance Orbiter.

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The THEMIS camera contains 5 filters. The 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 interior of Coprates Chasma.
The THEMIS camera contains 5 filters. The 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 interior of Coprates Chasma.

Coprates Chasma - False Color

The THEMIS camera contains 5 filters. The 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 interior of Coprates Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21290
Added: 2017-01-17

Views: 129

Coprates Chasma - False Color

The THEMIS camera contains 5 filters. The 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 interior of Coprates Chasma.

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This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater in Terra Sirenum. There are gullies dissecting part of the crater rim, and small dunes on the crater floor.
This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater in Terra Sirenum. There are gullies dissecting part of the crater rim, and small dunes on the crater floor.

Terra Sirenum

This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater in Terra Sirenum. There are gullies dissecting part of the crater rim, and small dunes on the crater floor.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21289
Added: 2017-01-16

Views: 155

Terra Sirenum

This image from NASA's 2001 Mars Odyssey spacecraft is of an unnamed crater in Terra Sirenum. There are gullies dissecting part of the crater rim, and small dunes on the crater floor.

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This image captured by NASA's Mars Reconnaissance Orbiter shows ancient highland channels in Eridania Valley.
This image captured by NASA's Mars Reconnaissance Orbiter shows ancient highland channels in Eridania Valley.

Smooth and Fractured Deposits in Eridania Valleys

This image captured by NASA's Mars Reconnaissance Orbiter shows ancient highland channels in Eridania Valley.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA12968
Added: 2017-01-13

Views: 228

Smooth and Fractured Deposits in Eridania Valleys

This image captured by NASA's Mars Reconnaissance Orbiter shows ancient highland channels in Eridania Valley.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows graben called Claritas Fossae.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows graben called Claritas Fossae.

Claritas Fossae

This image captured by NASA's 2001 Mars Odyssey spacecraft shows graben called Claritas Fossae.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21288
Added: 2017-01-13

Views: 160

Claritas Fossae

This image captured by NASA's 2001 Mars Odyssey spacecraft shows graben called Claritas Fossae.

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This image of a well-preserved unnamed elliptical crater in Terra Sabaea, captured by NASA's Mars Reconnaissance Orbiter, shows the complexity of ejecta deposits forming as a by-product of the impact process that shapes much of the surface of Mars.
This image of a well-preserved unnamed elliptical crater in Terra Sabaea, captured by NASA's Mars Reconnaissance Orbiter, shows the complexity of ejecta deposits forming as a by-product of the impact process that shapes much of the surface of Mars.

Well-Preserved Impact Ejecta and Impact Melt-Rich Deposits in Terra Sabaea

This image of a well-preserved unnamed elliptical crater in Terra Sabaea, captured by NASA's Mars Reconnaissance Orbiter, shows the complexity of ejecta deposits forming as a by-product of the impact process that shapes much of the surface of Mars.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA13078
Added: 2017-01-12

Views: 357

Well-Preserved Impact Ejecta and Impact Melt-Rich Deposits in Terra Sabaea

This image of a well-preserved unnamed elliptical crater in Terra Sabaea, captured by NASA's Mars Reconnaissance Orbiter, shows the complexity of ejecta deposits forming as a by-product of the impact process that shapes much of the surface of Mars.

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The linear depressions in this image from NASA's 2001 Mars Odyssey spacecraft are graben. Graben are formed from tectonic activity with large blocks of material moving downward between paired faults.
The linear depressions in this image from NASA's 2001 Mars Odyssey spacecraft are graben. Graben are formed from tectonic activity with large blocks of material moving downward between paired faults.

Sirenum Fossae

The linear depressions in this image from NASA's 2001 Mars Odyssey spacecraft are graben. Graben are formed from tectonic activity with large blocks of material moving downward between paired faults.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21287
Added: 2017-01-12

Views: 182

Sirenum Fossae

The linear depressions in this image from NASA's 2001 Mars Odyssey spacecraft are graben. Graben are formed from tectonic activity with large blocks of material moving downward between paired faults.

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Southern spring on Mars brings sublimation of the seasonal dry ice polar cap as seen by NASA's Mars Reconnaissance Orbiter.
Southern spring on Mars brings sublimation of the seasonal dry ice polar cap as seen by NASA's Mars Reconnaissance Orbiter.

Wide, Branching Channels

Southern spring on Mars brings sublimation of the seasonal dry ice polar cap 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#: PIA13151
Added: 2017-01-11

Views: 377

Wide, Branching Channels

Southern spring on Mars brings sublimation of the seasonal dry ice polar cap as seen by NASA's Mars Reconnaissance Orbiter.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows several channels in and around unnamed craters in Noachis Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows several channels in and around unnamed craters in Noachis Terra.

Noachis Terra Channels

This image captured by NASA's 2001 Mars Odyssey spacecraft shows several channels in and around unnamed craters in Noachis Terra.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21286
Added: 2017-01-11

Views: 95

Noachis Terra Channels

This image captured by NASA's 2001 Mars Odyssey spacecraft shows several channels in and around unnamed craters in Noachis Terra.

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NASA's Mars Reconnaissance Orbiter spied this small 2 kilometer-wide crater when a meteoroid struck the ground just to the west and created a new, larger crater (not shown).
NASA's Mars Reconnaissance Orbiter spied this small 2 kilometer-wide crater when a meteoroid struck the ground just to the west and created a new, larger crater (not shown).

Muddy Ejecta Flow

NASA's Mars Reconnaissance Orbiter spied this small 2 kilometer-wide crater when a meteoroid struck the ground just to the west and created a new, larger crater (not shown).

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA13181
Added: 2017-01-10

Views: 179

Muddy Ejecta Flow

NASA's Mars Reconnaissance Orbiter spied this small 2 kilometer-wide crater when a meteoroid struck the ground just to the west and created a new, larger crater (not shown).

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Noachis Terra, including several large dunes on the floor of an unnamed crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Noachis Terra, including several large dunes on the floor of an unnamed crater.

Noachis Terra Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Noachis Terra, including several large dunes on the floor of an unnamed crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21285
Added: 2017-01-10

Views: 89

Noachis Terra Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Noachis Terra, including several large dunes on the floor of an unnamed crater.

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The western Utopia Planitia in the Northern mid-latitudes of Mars is marked by a peculiar type of depression with scalloped edges and by a network of polygonal fractures as seen by NASA's Mars Reconnaissance Orbiter.
The western Utopia Planitia in the Northern mid-latitudes of Mars is marked by a peculiar type of depression with scalloped edges and by a network of polygonal fractures as seen by NASA's Mars Reconnaissance Orbiter.

Eroded Scallops with Layers

The western Utopia Planitia in the Northern mid-latitudes of Mars is marked by a peculiar type of depression with scalloped edges and by a network of polygonal fractures 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#: PIA13485
Added: 2017-01-09

Views: 465

Eroded Scallops with Layers

The western Utopia Planitia in the Northern mid-latitudes of Mars is marked by a peculiar type of depression with scalloped edges and by a network of polygonal fractures as seen by NASA's Mars Reconnaissance Orbiter.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive wind etched terrain in Memnonia Sulci, located south west of Olympus Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive wind etched terrain in Memnonia Sulci, located south west of Olympus Mons.

Memnonia Sulci

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive wind etched terrain in Memnonia Sulci, located south west of Olympus Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21283
Added: 2017-01-09

Views: 414

Memnonia Sulci

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive wind etched terrain in Memnonia Sulci, located south west of Olympus Mons.

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The THEMIS camera contains 5 filters. The 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 interior deposits and floor of Firsoff Crater.
The THEMIS camera contains 5 filters. The 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 interior deposits and floor of Firsoff Crater.

Firsoff Crater - False Color

The THEMIS camera contains 5 filters. The 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 interior deposits and floor of Firsoff Crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21282
Added: 2017-01-06

Views: 2017

Firsoff Crater - False Color

The THEMIS camera contains 5 filters. The 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 interior deposits and floor of Firsoff Crater.

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Large impact craters have central hills or mountains, because the tremendous shock waves from the impact first compresses the ground, then causes a rebound when it becomes uncompressed. This image is from NASA's Mars Reconnaissance Orbiter.
Large impact craters have central hills or mountains, because the tremendous shock waves from the impact first compresses the ground, then causes a rebound when it becomes uncompressed. This image is from NASA's Mars Reconnaissance Orbiter.

Raised Bedrock in Terra Cimmeria

Large impact craters have central hills or mountains, because the tremendous shock waves from the impact first compresses the ground, then causes a rebound when it becomes uncompressed. 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#: PIA15149
Added: 2017-01-05

Views: 425

Raised Bedrock in Terra Cimmeria

Large impact craters have central hills or mountains, because the tremendous shock waves from the impact first compresses the ground, then causes a rebound when it becomes uncompressed. This image is from NASA's Mars Reconnaissance Orbiter.

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The THEMIS camera contains 5 filters. The 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 some of the extensive plains that comprise Terra Sabaea.
The THEMIS camera contains 5 filters. The 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 some of the extensive plains that comprise Terra Sabaea.

Terra Sabaea - False Color

The THEMIS camera contains 5 filters. The 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 some of the extensive plains that comprise Terra Sabaea.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21281
Added: 2017-01-05

Views: 222

Terra Sabaea - False Color

The THEMIS camera contains 5 filters. The 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 some of the extensive plains that comprise Terra Sabaea.

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The THEMIS camera contains 5 filters. The 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 some of the floor of Newton Crater.
The THEMIS camera contains 5 filters. The 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 some of the floor of Newton Crater.

Newton Crater - False Color

The THEMIS camera contains 5 filters. The 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 some of the floor of Newton Crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21280
Added: 2017-01-04

Views: 196

Newton Crater - False Color

The THEMIS camera contains 5 filters. The 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 some of the floor of Newton Crater.

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Over 300 meters of layered beds are exposed in this trough of Noctis Labyrinthus, at the western edge of Valles Marineris, as observed by NASA's Mars Reconnaissance Orbiter.
Over 300 meters of layered beds are exposed in this trough of Noctis Labyrinthus, at the western edge of Valles Marineris, as observed by NASA's Mars Reconnaissance Orbiter.

Light-Toned Layering in a Labyrinthus Noctis Pit

Over 300 meters of layered beds are exposed in this trough of Noctis Labyrinthus, at the western edge of Valles Marineris, 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#: PIA14455
Added: 2017-01-03

Views: 338

Light-Toned Layering in a Labyrinthus Noctis Pit

Over 300 meters of layered beds are exposed in this trough of Noctis Labyrinthus, at the western edge of Valles Marineris, as observed by NASA's Mars Reconnaissance Orbiter.

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The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.
The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

Gorgonum Chaos - False Color

The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21279
Added: 2017-01-03

Views: 165

Gorgonum Chaos - False Color

The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

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Impact craters expose the subsurface materials on steep slopes in this image observed by NASA's Mars Reconnaissance Orbiter.
Impact craters expose the subsurface materials on steep slopes in this image observed by NASA's Mars Reconnaissance Orbiter.

Hues in a Crater Slope

Impact craters expose the subsurface materials on steep slopes in this image 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#: PIA14454
Added: 2017-01-02

Views: 264

Hues in a Crater Slope

Impact craters expose the subsurface materials on steep slopes in this image observed by NASA's Mars Reconnaissance Orbiter.

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The THEMIS camera contains 5 filters. The 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 several wind streaks in Syrtis Major Planum.
The THEMIS camera contains 5 filters. The 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 several wind streaks in Syrtis Major Planum.

Syrtis Major Planum - False Color

The THEMIS camera contains 5 filters. The 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 several wind streaks in Syrtis Major Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21278
Added: 2017-01-02

Views: 221

Syrtis Major Planum - False Color

The THEMIS camera contains 5 filters. The 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 several wind streaks in Syrtis Major Planum.

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The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.
The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

Gorgonum Chaos - False Color

The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA21277
Added: 2016-12-30

Views: 356

Gorgonum Chaos - False Color

The THEMIS camera contains 5 filters. The 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 Gorgonum Chaos.

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Currently displaying images 51-75 of 4178
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