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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: 346

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: 424

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: 248

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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Although Mars' soloar cap survives each warm summer season, it is constantly changing its shape due to sublimation of carbon dioxide from steep slopes and deposition onto flat areas as seen in this image from NASA's Mars Reconnaissance Orbiter.
Although Mars' soloar cap survives each warm summer season, it is constantly changing its shape due to sublimation of carbon dioxide from steep slopes and deposition onto flat areas as seen in this image from NASA's Mars Reconnaissance Orbiter.

Honey, I Shrunk the Mesas

Although Mars' soloar cap survives each warm summer season, it is constantly changing its shape due to sublimation of carbon dioxide from steep slopes and deposition onto flat areas 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#: PIA18560
Added: 2015-05-20

Views: 376

Honey, I Shrunk the Mesas

Although Mars' soloar cap survives each warm summer season, it is constantly changing its shape due to sublimation of carbon dioxide from steep slopes and deposition onto flat areas as seen in this image from NASA's Mars Reconnaissance Orbiter.

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This image from NASA's 2001 Mars Odyssey spacecraft shows numerous gullies dissect the rim of this unnamed crater in Terra Sirenum.
This image from NASA's 2001 Mars Odyssey spacecraft shows numerous gullies dissect the rim of this unnamed crater in Terra Sirenum.

Crater Rim Gullies

This image from NASA's 2001 Mars Odyssey spacecraft shows numerous gullies dissect the rim of this unnamed crater in Terra Sirenum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19466
Added: 2015-05-20

Views: 371

Crater Rim Gullies

This image from NASA's 2001 Mars Odyssey spacecraft shows numerous gullies dissect the rim of this unnamed crater in Terra Sirenum.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive flow field called Daedalia Planum. The lava flows originated at Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive flow field called Daedalia Planum. The lava flows originated at Arsia Mons.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive flow field called Daedalia Planum. The lava flows originated at Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19465
Added: 2015-05-19

Views: 230

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive flow field called Daedalia Planum. The lava flows originated at Arsia Mons.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks in Noachis Terra. The dark tracks show where the whirlwind was in contact with the surface and removed dust to expose the darker rocky surface.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks in Noachis Terra. The dark tracks show where the whirlwind was in contact with the surface and removed dust to expose the darker rocky surface.

Dust Devil Tracks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks in Noachis Terra. The dark tracks show where the whirlwind was in contact with the surface and removed dust to expose the darker rocky surface.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19464
Added: 2015-05-18

Views: 234

Dust Devil Tracks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks in Noachis Terra. The dark tracks show where the whirlwind was in contact with the surface and removed dust to expose the darker rocky surface.

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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 image from NASA's 2001 Mars Odyssey spacecraft shows the margin of the polar cap in Promethei Chasma.
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 image from NASA's 2001 Mars Odyssey spacecraft shows the margin of the polar cap in Promethei Chasma.

South Polar Layers - 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 image from NASA's 2001 Mars Odyssey spacecraft shows the margin of the polar cap in Promethei Chasma.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19462
Added: 2015-05-15

Views: 317

South Polar Layers - 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 image from NASA's 2001 Mars Odyssey spacecraft shows the margin of the polar cap in Promethei Chasma.

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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 image from NASA's 2001 Mars Odyssey spacecraft shows the surface of the south polar cap during springtime.
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 image from NASA's 2001 Mars Odyssey spacecraft shows the surface of the south polar cap during springtime.

Southern Spring - 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 image from NASA's 2001 Mars Odyssey spacecraft shows the surface of the south polar cap during springtime.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19461
Added: 2015-05-14

Views: 320

Southern Spring - 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 image from NASA's 2001 Mars Odyssey spacecraft shows the surface of the south polar cap during springtime.

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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 image from NASA's 2001 Mars Odyssey spacecraft shows a highland surrounded by the lava flows of Daedalia Planum.
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 image from NASA's 2001 Mars Odyssey spacecraft shows a highland surrounded by the lava flows of Daedalia Planum.

Daedalia Planum - 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 image from NASA's 2001 Mars Odyssey spacecraft shows a highland surrounded by the lava flows of Daedalia Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19460
Added: 2015-05-13

Views: 392

Daedalia Planum - 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 image from NASA's 2001 Mars Odyssey spacecraft shows a highland surrounded by the lava flows of Daedalia Planum.

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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 image from NASA's 2001 Mars Odyssey spacecraft shows a crater within a crater on the floor of Hadley Crater.
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 image from NASA's 2001 Mars Odyssey spacecraft shows a crater within a crater on the floor of Hadley Crater.

Hadley Crater - 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 image from NASA's 2001 Mars Odyssey spacecraft shows a crater within a crater on the floor of Hadley Crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19455
Added: 2015-05-12

Views: 520

Hadley Crater - 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 image from NASA's 2001 Mars Odyssey spacecraft shows a crater within a crater on the floor of Hadley Crater.

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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 craters in 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 craters in 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 craters in Terra Cimmeria.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19454
Added: 2015-05-11

Views: 3177

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 craters in Terra Cimmeria.

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This frame is from sequence of views NASA's Curiosity Mars rover recorded of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.
This frame is from sequence of views NASA's Curiosity Mars rover recorded of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

Sunset Sequence in Mars' Gale Crater (Animation)

This frame is from sequence of views NASA's Curiosity Mars rover recorded of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA19401
Added: 2015-05-08

Views: 35923

Sunset Sequence in Mars' Gale Crater (Animation)

This frame is from sequence of views NASA's Curiosity Mars rover recorded of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

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NASA's Curiosity Mars rover recorded this view of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.
NASA's Curiosity Mars rover recorded this view of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

Sunset in Mars' Gale Crater

NASA's Curiosity Mars rover recorded this view of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA19400
Added: 2015-05-08

Views: 42135

Sunset in Mars' Gale Crater

NASA's Curiosity Mars rover recorded this view of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

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This map shows the route on lower Mount Sharp that NASA's Curiosity followed in April and early May 2015, in the context of the surrounding terrain. Numbers along the route identify the sol, or Martian day, on which it completed the drive.
This map shows the route on lower Mount Sharp that NASA's Curiosity followed in April and early May 2015, in the context of the surrounding terrain. Numbers along the route identify the sol, or Martian day, on which it completed the drive.

Curiosity's Path to Some Spring 2015 Study Sites

This map shows the route on lower Mount Sharp that NASA's Curiosity followed in April and early May 2015, in the context of the surrounding terrain. Numbers along the route identify the sol, or Martian day, on which it completed the drive.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19399
Added: 2015-05-08

Views: 1161

Curiosity's Path to Some Spring 2015 Study Sites

This map shows the route on lower Mount Sharp that NASA's Curiosity followed in April and early May 2015, in the context of the surrounding terrain. Numbers along the route identify the sol, or Martian day, on which it completed the drive.

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This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.
This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.

Looking Toward Curiosity Study Areas, Spring 2015

This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA19398
Added: 2015-05-08

Views: 2997

Looking Toward Curiosity Study Areas, Spring 2015

This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.

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A sweeping panorama combining 33 telephoto images into one Martian vista presents details of several types of terrain visible on Mount Sharp from a location along the route of NASA's Curiosity Mars rover.
A sweeping panorama combining 33 telephoto images into one Martian vista presents details of several types of terrain visible on Mount Sharp from a location along the route of NASA's Curiosity Mars rover.

Diverse Terrain Types on Mount Sharp, Mars

A sweeping panorama combining 33 telephoto images into one Martian vista presents details of several types of terrain visible on Mount Sharp from a location along the route of NASA's Curiosity Mars rover.

Target: Mars
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: Mastcam
ID#: PIA19397
Added: 2015-05-08

Views: 967

Diverse Terrain Types on Mount Sharp, Mars

A sweeping panorama combining 33 telephoto images into one Martian vista presents details of several types of terrain visible on Mount Sharp from a location along the route of NASA's Curiosity Mars rover.

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This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.

Dust Devil Tracks

This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19453
Added: 2015-05-08

Views: 278

Dust Devil Tracks

This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Terra Sirenum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Terra Sirenum.

Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Terra Sirenum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19452
Added: 2015-05-07

Views: 227

Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Terra Sirenum.

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This image was acquired by NASA's Mars Reconnaissance Orbiter to complete a stereo pair over sinuous ridges in Argyre Planitia, but dust clouds kicked up, obscuring most of the surface.
This image was acquired by NASA's Mars Reconnaissance Orbiter to complete a stereo pair over sinuous ridges in Argyre Planitia, but dust clouds kicked up, obscuring most of the surface.

Darn Dust!

This image was acquired by NASA's Mars Reconnaissance Orbiter to complete a stereo pair over sinuous ridges in Argyre Planitia, but dust clouds kicked up, obscuring most of the surface.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19459
Added: 2015-05-06

Views: 300

Darn Dust!

This image was acquired by NASA's Mars Reconnaissance Orbiter to complete a stereo pair over sinuous ridges in Argyre Planitia, but dust clouds kicked up, obscuring most of the surface.

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Ravines (or very large gullies) are actively forming on Mars during the coldest times of year, when carbon dioxide frost aids mass wasting as seen by NASA's Mars Reconnaissance Orbiter.
Ravines (or very large gullies) are actively forming on Mars during the coldest times of year, when carbon dioxide frost aids mass wasting as seen by NASA's Mars Reconnaissance Orbiter.

Warm-Season Flows in Cold-Season Ravines

Ravines (or very large gullies) are actively forming on Mars during the coldest times of year, when carbon dioxide frost aids mass wasting 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#: PIA19458
Added: 2015-05-06

Views: 303

Warm-Season Flows in Cold-Season Ravines

Ravines (or very large gullies) are actively forming on Mars during the coldest times of year, when carbon dioxide frost aids mass wasting as seen by NASA's Mars Reconnaissance Orbiter.

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The long straight ridges seen in this image from NASA's Mars Reconnaissance Orbiter are called yardangs and they form on Mars (and Earth) when the wind strips away the inter-ridge material.
The long straight ridges seen in this image from NASA's Mars Reconnaissance Orbiter are called yardangs and they form on Mars (and Earth) when the wind strips away the inter-ridge material.

On the Beauty of Yardangs

The long straight ridges seen in this image from NASA's Mars Reconnaissance Orbiter are called yardangs and they form on Mars (and Earth) when the wind strips away the inter-ridge material.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19457
Added: 2015-05-06

Views: 229

On the Beauty of Yardangs

The long straight ridges seen in this image from NASA's Mars Reconnaissance Orbiter are called yardangs and they form on Mars (and Earth) when the wind strips away the inter-ridge material.

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This image from NASA's Mars Reconnaissance Orbiter shows a dusty area of Mars. The dark streaks on the slopes are locations where the dust has slumped downhill revealing a less dusty surface underneath.
This image from NASA's Mars Reconnaissance Orbiter shows a dusty area of Mars. The dark streaks on the slopes are locations where the dust has slumped downhill revealing a less dusty surface underneath.

Slope Streaks on a Dusty Planet

This image from NASA's Mars Reconnaissance Orbiter shows a dusty area of Mars. The dark streaks on the slopes are locations where the dust has slumped downhill revealing a less dusty surface underneath.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA19456
Added: 2015-05-06

Views: 210

Slope Streaks on a Dusty Planet

This image from NASA's Mars Reconnaissance Orbiter shows a dusty area of Mars. The dark streaks on the slopes are locations where the dust has slumped downhill revealing a less dusty surface underneath.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum. These flows originated at Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum. These flows originated at Arsia Mons.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum. These flows originated at Arsia Mons.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19451
Added: 2015-05-06

Views: 242

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum. These flows originated at Arsia Mons.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Samara Valles.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Samara Valles.

Samara Valles

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Samara Valles.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA19447
Added: 2015-05-05

Views: 259

Samara Valles

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Samara Valles.

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Currently displaying images 51-75 of 3341
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