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NASA's Dawn spacecraft views Abellio Crater (20 miles, 32 kilometers wide) on Ceres in this image. Dawn took this image on June 2, 2016, from its low-altitude mapping orbit, at a distance of about 240 miles (385 kilometers) above the surface.
NASA's Dawn spacecraft views Abellio Crater (20 miles, 32 kilometers wide) on Ceres in this image. Dawn took this image on June 2, 2016, from its low-altitude mapping orbit, at a distance of about 240 miles (385 kilometers) above the surface.

Dawn LAMO Image 178

NASA's Dawn spacecraft views Abellio Crater (20 miles, 32 kilometers wide) on Ceres in this image. Dawn took this image on June 2, 2016, from its low-altitude mapping orbit, at a distance of about 240 miles (385 kilometers) above the surface.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20940
Added: 2016-09-23

Views: 46

Dawn LAMO Image 178

NASA's Dawn spacecraft views Abellio Crater (20 miles, 32 kilometers wide) on Ceres in this image. Dawn took this image on June 2, 2016, from its low-altitude mapping orbit, at a distance of about 240 miles (385 kilometers) above the surface.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.

Daedalia Planum Windstreaks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20995
Added: 2016-09-23

Views: 29

Daedalia Planum Windstreaks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.

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This view from NASA's Dawn spacecraft shows terrain in the northern hemisphere of Ceres, near Jarovit Crater. This image was taken on June 2, 2016, at a distance of about 240 miles (385 kilometers) above the surface.
This view from NASA's Dawn spacecraft shows terrain in the northern hemisphere of Ceres, near Jarovit Crater. This image was taken on June 2, 2016, at a distance of about 240 miles (385 kilometers) above the surface.

Dawn LAMO Image 177

This view from NASA's Dawn spacecraft shows terrain in the northern hemisphere of Ceres, near Jarovit Crater. This image was taken on June 2, 2016, at a distance of about 240 miles (385 kilometers) above the surface.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20939
Added: 2016-09-22

Views: 53

Dawn LAMO Image 177

This view from NASA's Dawn spacecraft shows terrain in the northern hemisphere of Ceres, near Jarovit Crater. This image was taken on June 2, 2016, at a distance of about 240 miles (385 kilometers) above the surface.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a depression (or trough) on the polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a depression (or trough) on the polar cap.

South Polar Cap

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a depression (or trough) on the polar cap.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20994
Added: 2016-09-22

Views: 42

South Polar Cap

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a depression (or trough) on the polar cap.

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This image from NASA's Mars Reconnaissance Orbiter shows a complicated area containing various types of channels, pits and fractures near Olympica Fossae.
This image from NASA's Mars Reconnaissance Orbiter shows a complicated area containing various types of channels, pits and fractures near Olympica Fossae.

Intersecting Channels near Olympica Fossae

This image from NASA's Mars Reconnaissance Orbiter shows a complicated area containing various types of channels, pits and fractures near Olympica Fossae.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA21066
Added: 2016-09-21

Views: 113

Intersecting Channels near Olympica Fossae

This image from NASA's Mars Reconnaissance Orbiter shows a complicated area containing various types of channels, pits and fractures near Olympica Fossae.

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This image captured by NASA's Mars Reconnaissance Orbiter shows viscous flow features. Currently, water-ice is stable on the Martian surface only in the polar regions.
This image captured by NASA's Mars Reconnaissance Orbiter shows viscous flow features. Currently, water-ice is stable on the Martian surface only in the polar regions.

What Lies Beneath: Surface Patterns of Glacier-Like Landforms

This image captured by NASA's Mars Reconnaissance Orbiter shows viscous flow features. Currently, water-ice is stable on the Martian surface only in the polar regions.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA21065
Added: 2016-09-21

Views: 53

What Lies Beneath: Surface Patterns of Glacier-Like Landforms

This image captured by NASA's Mars Reconnaissance Orbiter shows viscous flow features. Currently, water-ice is stable on the Martian surface only in the polar regions.

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This image from NASA's Mars Reconnaissance Orbiter shows a circular impact crater and an oval volcanic caldera on the southern flank of a large volcano on Mars called Pavonis Mons.
This image from NASA's Mars Reconnaissance Orbiter shows a circular impact crater and an oval volcanic caldera on the southern flank of a large volcano on Mars called Pavonis Mons.

The Wind-Scoured Lava Flows of Pavonis Mons

This image from NASA's Mars Reconnaissance Orbiter shows a circular impact crater and an oval volcanic caldera on the southern flank of a large volcano on Mars called Pavonis Mons.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: High Resolution Imaging Science Experiment (HiRISE)
ID#: PIA21064
Added: 2016-09-21

Views: 47

The Wind-Scoured Lava Flows of Pavonis Mons

This image from NASA's Mars Reconnaissance Orbiter shows a circular impact crater and an oval volcanic caldera on the southern flank of a large volcano on Mars called Pavonis Mons.

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Cerberus Fossae are a series of discontinuous fissures along dusty plains in the southeastern region of Elysium Planitia as seen by NASA's Mars Reconnaissance Orbiter.
Cerberus Fossae are a series of discontinuous fissures along dusty plains in the southeastern region of Elysium Planitia as seen by NASA's Mars Reconnaissance Orbiter.

River of Sand

Cerberus Fossae are a series of discontinuous fissures along dusty plains in the southeastern region of Elysium Planitia 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#: PIA21063
Added: 2016-09-21

Views: 122

River of Sand

Cerberus Fossae are a series of discontinuous fissures along dusty plains in the southeastern region of Elysium Planitia as seen by NASA's Mars Reconnaissance Orbiter.

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This view from NASA's Dawn spacecraft shows the rim of Dantu Crater (78 miles, 125 kilometers wide). This image was taken on June 2, 2016.
This view from NASA's Dawn spacecraft shows the rim of Dantu Crater (78 miles, 125 kilometers wide). This image was taken on June 2, 2016.

Dawn LAMO Image 176

This view from NASA's Dawn spacecraft shows the rim of Dantu Crater (78 miles, 125 kilometers wide). This image was taken on June 2, 2016.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20938
Added: 2016-09-21

Views: 58

Dawn LAMO Image 176

This view from NASA's Dawn spacecraft shows the rim of Dantu Crater (78 miles, 125 kilometers wide). This image was taken on June 2, 2016.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.

Polar Textures

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20993
Added: 2016-09-21

Views: 47

Polar Textures

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.

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This graphic depicts the Asteroid Redirect Vehicle conducting a flyby of its target asteroid. The robotic segment of the Asteroid Redirect Mission will demonstrate advanced, high-power, high-throughput solar electric propulsion.
This graphic depicts the Asteroid Redirect Vehicle conducting a flyby of its target asteroid. The robotic segment of the Asteroid Redirect Mission will demonstrate advanced, high-power, high-throughput solar electric propulsion.

ARM Spacecraft (Illustration)

This graphic depicts the Asteroid Redirect Vehicle conducting a flyby of its target asteroid. The robotic segment of the Asteroid Redirect Mission will demonstrate advanced, high-power, high-throughput solar electric propulsion.

Mission: Asteroid Redirect Mission (ARM)
ID#: PIA21062
Added: 2016-09-20

Views: 69

ARM Spacecraft (Illustration)

This graphic depicts the Asteroid Redirect Vehicle conducting a flyby of its target asteroid. The robotic segment of the Asteroid Redirect Mission will demonstrate advanced, high-power, high-throughput solar electric propulsion.

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NASA's Dawn spacecraft obtained this view of Laukumate Crater (19 miles, 30 kilometers wide) on Ceres on June 2, 2016. Laukumate is named for a Latvian goddess of agriculture.
NASA's Dawn spacecraft obtained this view of Laukumate Crater (19 miles, 30 kilometers wide) on Ceres on June 2, 2016. Laukumate is named for a Latvian goddess of agriculture.

Dawn LAMO Image 175

NASA's Dawn spacecraft obtained this view of Laukumate Crater (19 miles, 30 kilometers wide) on Ceres on June 2, 2016. Laukumate is named for a Latvian goddess of agriculture.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20937
Added: 2016-09-20

Views: 70

Dawn LAMO Image 175

NASA's Dawn spacecraft obtained this view of Laukumate Crater (19 miles, 30 kilometers wide) on Ceres on June 2, 2016. Laukumate is named for a Latvian goddess of agriculture.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit from the cliffside along Tiu Valles.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit from the cliffside along Tiu Valles.

Tiu Valles Landslide

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit from the cliffside along Tiu Valles.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20992
Added: 2016-09-20

Views: 85

Tiu Valles Landslide

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit from the cliffside along Tiu Valles.

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This view from NASA's Dawn spacecraft shows cratered terrain on the edge of the giant crater Yalode. This image was taken on June 1, 2016.
This view from NASA's Dawn spacecraft shows cratered terrain on the edge of the giant crater Yalode. This image was taken on June 1, 2016.

Dawn LAMO Image 174

This view from NASA's Dawn spacecraft shows cratered terrain on the edge of the giant crater Yalode. This image was taken on June 1, 2016.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20936
Added: 2016-09-19

Views: 92

Dawn LAMO Image 174

This view from NASA's Dawn spacecraft shows cratered terrain on the edge of the giant crater Yalode. This image was taken on June 1, 2016.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive lava flows that comprise Solis Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive lava flows that comprise Solis Planum.

Solis Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive lava flows that comprise Solis Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20991
Added: 2016-09-19

Views: 101

Solis Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the extensive lava flows that comprise Solis Planum.

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This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows Rongo Crater, located near Ceres' equator.
This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows Rongo Crater, located near Ceres' equator.

Dawn LAMO Image 173

This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows Rongo Crater, located near Ceres' equator.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20935
Added: 2016-09-16

Views: 123

Dawn LAMO Image 173

This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows Rongo Crater, located near Ceres' equator.

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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 Terby 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 Terby Crater.

Terby 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 Terby Crater.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20990
Added: 2016-09-16

Views: 150

Terby 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 Terby Crater.

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This map of an area within the Arabia Terra region on Mars shows where hydrologic modeling predicts locations of depressions that would have been lakes (black), overlaid with a map of the preserved valleys (blue lines) that would have been streams.
This map of an area within the Arabia Terra region on Mars shows where hydrologic modeling predicts locations of depressions that would have been lakes (black), overlaid with a map of the preserved valleys (blue lines) that would have been streams.

Hydrologic Modeling of Relatively Recent Martian Streams and Lake

This map of an area within the Arabia Terra region on Mars shows where hydrologic modeling predicts locations of depressions that would have been lakes (black), overlaid with a map of the preserved valleys (blue lines) that would have been streams.

Target: Mars
Mission: 2001 Mars Odyssey, Mars Global Surveyor (MGS)
Spacecraft: 2001 Mars Odyssey, Mars Global Surveyor Orbiter
Instrument: Mars Orbiter Laser Altimeter, Thermal Emission Imaging System
ID#: PIA20839
Added: 2016-09-15

Views: 408

Hydrologic Modeling of Relatively Recent Martian Streams and Lake

This map of an area within the Arabia Terra region on Mars shows where hydrologic modeling predicts locations of depressions that would have been lakes (black), overlaid with a map of the preserved valleys (blue lines) that would have been streams.

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Valleys much younger than well-known ancient valley networks on Mars are evident near the informally named 'Heart Lake' on Mars. This map based on NASA's MGS data presents color-coded topographical information overlaid onto a photo mosaic.
Valleys much younger than well-known ancient valley networks on Mars are evident near the informally named 'Heart Lake' on Mars. This map based on NASA's MGS data presents color-coded topographical information overlaid onto a photo mosaic.

Landscape of Former Lakes and Streams on Northern Mars

Valleys much younger than well-known ancient valley networks on Mars are evident near the informally named 'Heart Lake' on Mars. This map based on NASA's MGS data presents color-coded topographical information overlaid onto a photo mosaic.

Target: Mars
Mission: 2001 Mars Odyssey, Mars Global Surveyor (MGS)
Spacecraft: 2001 Mars Odyssey, Mars Global Surveyor Orbiter
Instrument: Mars Orbiter Laser Altimeter, Thermal Emission Imaging System
ID#: PIA20838
Added: 2016-09-15

Views: 1076

Landscape of Former Lakes and Streams on Northern Mars

Valleys much younger than well-known ancient valley networks on Mars are evident near the informally named 'Heart Lake' on Mars. This map based on NASA's MGS data presents color-coded topographical information overlaid onto a photo mosaic.

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This image taken by NASA's Mars Reconnaissance Orbiter covers an area about 8 miles wide in the northern Arabia Terra region of Mars. Researchers estimate the stream and the lakes it linked held water at some time in the range of 2-3 billion years ago.
This image taken by NASA's Mars Reconnaissance Orbiter covers an area about 8 miles wide in the northern Arabia Terra region of Mars. Researchers estimate the stream and the lakes it linked held water at some time in the range of 2-3 billion years ago.

Outflow Stream from Relatively Recent Martian Lake

This image taken by NASA's Mars Reconnaissance Orbiter covers an area about 8 miles wide in the northern Arabia Terra region of Mars. Researchers estimate the stream and the lakes it linked held water at some time in the range of 2-3 billion years ago.

Target: Mars
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: Context Camera (CTX)
ID#: PIA20837
Added: 2016-09-15

Views: 381

Outflow Stream from Relatively Recent Martian Lake

This image taken by NASA's Mars Reconnaissance Orbiter covers an area about 8 miles wide in the northern Arabia Terra region of Mars. Researchers estimate the stream and the lakes it linked held water at some time in the range of 2-3 billion years ago.

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This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows terrain on Ceres directly south of Kupalo Crater. The area is blanketed by smooth ejecta from Kupalo.
This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows terrain on Ceres directly south of Kupalo Crater. The area is blanketed by smooth ejecta from Kupalo.

Dawn LAMO Image 172

This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows terrain on Ceres directly south of Kupalo Crater. The area is blanketed by smooth ejecta from Kupalo.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20934
Added: 2016-09-15

Views: 137

Dawn LAMO Image 172

This view from NASA's Dawn spacecraft, captured on June 1, 2016, shows terrain on Ceres directly south of Kupalo Crater. The area is blanketed by smooth ejecta from Kupalo.

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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 plains of Terra Cimmeria.
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 plains of Terra Cimmeria.

Terra Cimmeria - 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 plains of Terra Cimmeria.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20989
Added: 2016-09-15

Views: 125

Terra Cimmeria - 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 plains of Terra Cimmeria.

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As NASA's New Horizons approached Pluto in late 2014 and then flew by the planet during the summer of 2015, NASA's Chandra obtained data during four separate observations. During each observation, Chandra detected low-energy X-rays from the small planet.
As NASA's New Horizons approached Pluto in late 2014 and then flew by the planet during the summer of 2015, NASA's Chandra obtained data during four separate observations. During each observation, Chandra detected low-energy X-rays from the small planet.

X-Rays from Pluto

As NASA's New Horizons approached Pluto in late 2014 and then flew by the planet during the summer of 2015, NASA's Chandra obtained data during four separate observations. During each observation, Chandra detected low-energy X-rays from the small planet.

Target: Pluto
Mission: Chandra X-ray Observatory, New Horizons
Spacecraft: New Horizons
Instrument: Long Range Reconnaissance Imager (LORRI), Solar Wind Around Pluto (SWAP)
ID#: PIA21061
Added: 2016-09-14

Views: 232

X-Rays from Pluto

As NASA's New Horizons approached Pluto in late 2014 and then flew by the planet during the summer of 2015, NASA's Chandra obtained data during four separate observations. During each observation, Chandra detected low-energy X-rays from the small planet.

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This view from NASA's Dawn spacecraft, taken on June 6, 2016, shows Takel Crater (at top left) on Ceres. Takel is 14 miles (22 kilometers) wide and exhibits streaks of bright material on its walls.
This view from NASA's Dawn spacecraft, taken on June 6, 2016, shows Takel Crater (at top left) on Ceres. Takel is 14 miles (22 kilometers) wide and exhibits streaks of bright material on its walls.

Dawn LAMO Image 171

This view from NASA's Dawn spacecraft, taken on June 6, 2016, shows Takel Crater (at top left) on Ceres. Takel is 14 miles (22 kilometers) wide and exhibits streaks of bright material on its walls.

Target: Ceres
Mission: Dawn
Spacecraft: Dawn
Instrument: Framing Camera
ID#: PIA20933
Added: 2016-09-14

Views: 146

Dawn LAMO Image 171

This view from NASA's Dawn spacecraft, taken on June 6, 2016, shows Takel Crater (at top left) on Ceres. Takel is 14 miles (22 kilometers) wide and exhibits streaks of bright material on its walls.

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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 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 part of 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 part of Syrtis Major Planum.

Target: Mars
Mission: 2001 Mars Odyssey
Spacecraft: 2001 Mars Odyssey
Instrument: Thermal Emission Imaging System
ID#: PIA20988
Added: 2016-09-14

Views: 159

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 part of Syrtis Major Planum.

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