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Images of 'Valles Marineris' found, 46

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The Valles Marineris Canyon, 2005

The Valles Marineris Canyon, 2005

UIG1580018

Mars: Valles Marineris - Mosaic of 20 images obtained by the European probe Mars Express. This image shows the eastern part of Valles Marineris, a canyon about 4500 km long and 8 km deep. This mosaic image of eastern part of Valles Marineris - colored to resemble the martian surface - comes from Esa's Mars Express spacecraft, which repeatedly crosses the Martian equator from north to south or south to north. The High Resolution Stereo Camera (HRSC) on board Mars Express, has been taking image strips of the valley system since 2004 as it passes overhead. The individual HRSC image strips are each between 50 and 200 kilometers wide, depending on Mars Express' orbit, so this view of Valles Marineris has only been made possible by creating a mosaic using 20 separate images. To improve the presentation here, the altitudes have been exaggerated fourfold, so that the slopes and mountainsides appear steeper than they are in reality. The colours in this image are slightly false as well. By incre

Mars: Valles Marineris - Mosaic of 20 images obtained by the European probe Mars Express. This image shows the eastern part of Valles Marineris, a canyon about 4500 km long and 8 km deep. This mosaic image of eastern part of Valles Marineris - colored to resemble the martian surface - comes from Esa's Mars Express spacecraft, which repeatedly crosses the Martian equator from north to south or south to north. The High Resolution Stereo Camera (HRSC) on board Mars Express, has been taking image strips of the valley system since 2004 as it passes overhead. The individual HRSC image strips are each between 50 and 200 kilometers wide, depending on Mars Express' orbit, so this view of Valles Marineris has only been made possible by creating a mosaic using 20 separate images. To improve the presentation here, the altitudes have been exaggerated fourfold, so that the slopes and mountainsides appear steeper than they are in reality. The colours in this image are slightly false as well. By incre

PIX4616253

Mars view of Deimos - Illustration - Mars seen from Deimos - Illustration - Mars seen from Deimos satellite. A view of Mars from its moon Deimos

Mars view of Deimos - Illustration - Mars seen from Deimos - Illustration - Mars seen from Deimos satellite. A view of Mars from its moon Deimos

Miller, Ron (b.1947)

PIX4616808

This canyon system, Valles Marineris, was named in honor of its discoverer, Mariner 9. Melas Chasma is shown in the image.

This canyon system, Valles Marineris, was named in honor of its discoverer, Mariner 9. Melas Chasma is shown in the image.

UIG866522

Mars and Phobos - Illustration - Mars and Phobos - Illustration - Mars seen from its nearest satellite, Phobos. A view of Mars from its nearest moon, Phobo

Mars and Phobos - Illustration - Mars and Phobos - Illustration - Mars seen from its nearest satellite, Phobos. A view of Mars from its nearest moon, Phobo

Steven Hobbs

PIX4616806

Coprates Chasma comprises the central portion of the Valles Marineris canyon system complex. THEMIS.

Coprates Chasma comprises the central portion of the Valles Marineris canyon system complex. THEMIS.

UIG866526

Ius Chasma is one of several canyons that make up Valles Marineris, the largest canyon system in the Solar System.

Ius Chasma is one of several canyons that make up Valles Marineris, the largest canyon system in the Solar System.

UIG866541

West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured. As faults opened, they released subsurface ice and water, causing the ground to collapse.

West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured. As faults opened, they released subsurface ice and water, causing the ground to collapse.

UIG866561

Mars: Valles Marineris - Illustration - Artist's view of the Martian canyon filled with haze. Artwork showing the great martian canyon filled with fog

Mars: Valles Marineris - Illustration - Artist's view of the Martian canyon filled with haze. Artwork showing the great martian canyon filled with fog

Steven Hobbs

PIX4616971

Mars: Valles Marineris - Illustration - Artist's view of the grand martian canyon Valles Marineris. Valles Marineris on Mars, the largest canyon in the solar system could swallow the Grand Canyon many times over

Mars: Valles Marineris - Illustration - Artist's view of the grand martian canyon Valles Marineris. Valles Marineris on Mars, the largest canyon in the solar system could swallow the Grand Canyon many times over

Steven Hobbs

PIX4616978

Mars: Noctis Labyrinthus - Illustration - Artist's view of Noctis Labyrinthus, a Martian canyon located in the western part of Valles Marineris. Panorama of Noctis Labyrinthus, a giant fault system on Mar

Mars: Noctis Labyrinthus - Illustration - Artist's view of Noctis Labyrinthus, a Martian canyon located in the western part of Valles Marineris. Panorama of Noctis Labyrinthus, a giant fault system on Mar

Steven Hobbs

PIX4616993

Mars: artist's view of Valles Marineris - Mars: artist's view of Valles Marineri

Mars: artist's view of Valles Marineris - Mars: artist's view of Valles Marineri

Dixon, Don (b.1951)

PIX4616927

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows the central region of Valles Marineris, Ophir Chasma and Candor Chasma

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows the central region of Valles Marineris, Ophir Chasma and Candor Chasma

PIX4615132

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows the central region of Valles Marineris, Candor Chasma

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows the central region of Valles Marineris, Candor Chasma

PIX4615137

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows the central region of Valles Marineris, Ophir Chasma and Candor Chasma

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows the central region of Valles Marineris, Ophir Chasma and Candor Chasma

PIX4615183

Part of the Valles Marineris, the Martian 'Grand Canyon', 1976

Part of the Valles Marineris, the Martian 'Grand Canyon', 1976

UIS5071542

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep

PIX4615125

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows a detail of Valles Marineris, Candor Chasma. The cliffs along this canyon are about 7000m high

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows a detail of Valles Marineris, Candor Chasma. The cliffs along this canyon are about 7000m high

PIX4615151

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep

PIX4615124

Mars - Valles Marineris - Mosaic of 102 images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep. On the left, the volcanoes of Tharsis

Mars - Valles Marineris - Mosaic of 102 images obtained by the Viking probe 1. This image shows Valles Marineris, a canyon more than 3000 km long and 8 km deep. On the left, the volcanoes of Tharsis

PIX4615065

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows a detail of Valles Marineris, Ophir Chasma. These eroded cliffs measure 4000m high

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1 put into perspective. This image shows a detail of Valles Marineris, Ophir Chasma. These eroded cliffs measure 4000m high

PIX4615138

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image, deformed by a fish-eye effect, shows Valles Marineris, a canyon more than 3000 km long and 8 km deep. On the left, the volcanoes of Tharsis

Mars - Valles Marineris - Mosaic of images obtained by the Viking probe 1. This image, deformed by a fish-eye effect, shows Valles Marineris, a canyon more than 3000 km long and 8 km deep. On the left, the volcanoes of Tharsis

PIX4615087

Spacecraft, USA, Viking Part ofÊ Valles Marineris, the ÔGrand CanyonÕ of Mars, 1976

Spacecraft, USA, Viking Part ofÊ Valles Marineris, the ÔGrand CanyonÕ of Mars, 1976

UIS5071693

Mars - Valles Marineris - Mosaic of 500 infrared images obtained by the Mars Odyssey probe. This image shows Valles Marineris, a canyon about 4500 km long and 8 km deep. Image covers an area of 3000 km Faux colors

Mars - Valles Marineris - Mosaic of 500 infrared images obtained by the Mars Odyssey probe. This image shows Valles Marineris, a canyon about 4500 km long and 8 km deep. Image covers an area of 3000 km Faux colors

PIX4616291

Coprates Chasma - This image shows a detail of Valles Marineris, Coprates Chasma. Image obtained by the Mars Global Surveyor probe

Coprates Chasma - This image shows a detail of Valles Marineris, Coprates Chasma. Image obtained by the Mars Global Surveyor probe

PIX4615270

This THEMIS visible image shows the effects of erosion on a beautiful sequence of dramatically layered rocks within Candor Chasma, which is part of the Valles Marineris.

This THEMIS visible image shows the effects of erosion on a beautiful sequence of dramatically layered rocks within Candor Chasma, which is part of the Valles Marineris.

UIG866521

Mars, February 1980

Mars, February 1980

UIS5104642

Mars - Candor Chasma - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

Mars - Candor Chasma - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

PIX4616382

Ocean sur Mars - Region of Tharsis et Valles Marineris - Mars with ocean - looking at Valles Marineris - Reconstructed view of Mars at the time when it had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

Ocean sur Mars - Region of Tharsis et Valles Marineris - Mars with ocean - looking at Valles Marineris - Reconstructed view of Mars at the time when it had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

PIX4616858

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Image obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is an approximately 100 km long and 10 km wide incision in the Lunae Planum high plateau north of Valles Marineris, the 'Grand Canyon' of Mars. Etus Chasma is the water source region of Kasei Valles, which extends thousands of kilometres to the north, and its southern - most part. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Image obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is an approximately 100 km long and 10 km wide incision in the Lunae Planum high plateau north of Valles Marineris, the 'Grand Canyon' of Mars. Etus Chasma is the water source region of Kasei Valles, which extends thousands of kilometres to the north, and its southern - most part. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

PIX4616094

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

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March: Detail of the region of Candor Chasma. - Detail of the region of Candor Chasma, in Valles Marineris, obtained in September 2006 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. The white cretes visible in the lower part of the image would have been formed by the passage of water through the basement of the planet millions of years ago

March: Detail of the region of Candor Chasma. - Detail of the region of Candor Chasma, in Valles Marineris, obtained in September 2006 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. The white cretes visible in the lower part of the image would have been formed by the passage of water through the basement of the planet millions of years ago

PIX4616419

Clouds on Mars - Clouds over Tharsis volcanoes (left) and around Valles Marineris, below. The three volcanoes of Tharsis form a diagonal; from top to bottom are Ascraeus Mons, Pavonis Mons and Arsia Mons. Top left is the volcano Olympus Mons. Image obtained by the Mars Global Surveyor probe in May 2003

Clouds on Mars - Clouds over Tharsis volcanoes (left) and around Valles Marineris, below. The three volcanoes of Tharsis form a diagonal; from top to bottom are Ascraeus Mons, Pavonis Mons and Arsia Mons. Top left is the volcano Olympus Mons. Image obtained by the Mars Global Surveyor probe in May 2003

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March: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Perspective image obtained by the Mars Express probe in 2005. Perspective view of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars, where water is believed to have flowed. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel

March: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Perspective image obtained by the Mars Express probe in 2005. Perspective view of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars, where water is believed to have flowed. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel

PIX4616076

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Perspective image obtained by the Mars Express probe in 2005. Perspective view of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars, where water is believed to have flowed. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Perspective image obtained by the Mars Express probe in 2005. Perspective view of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars, where water is believed to have flowed. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel

PIX4616055

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

Mars seen by the Hubble Space Telescope - 1997 - Images obtained on March 30, 1997. Between each image, Mars rotated 90 degrees. At the top left, the image is centered on Ares Vallis, the or Mars Pathfinder landed on July 4, 1997. At the top right you can see Valles Marineris and the volcanoes of Tharsis. Lower left, Cerberus and Elysium region, lower right, Syris Major

Mars seen by the Hubble Space Telescope - 1997 - Images obtained on March 30, 1997. Between each image, Mars rotated 90 degrees. At the top left, the image is centered on Ares Vallis, the or Mars Pathfinder landed on July 4, 1997. At the top right you can see Valles Marineris and the volcanoes of Tharsis. Lower left, Cerberus and Elysium region, lower right, Syris Major

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A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky

A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky

Steven Hobbs

PIX4617044

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

PIX4616128

Mars seen by the Hubble Space Telescope - 1999 - Images obtained between 27 April and 6 May 1999 during the opposition of Mars when the planet was only 87 million km away from Earth. Between each image, Mars rotated 90 degrees. At the top left, the image is centered on Ares Vallis, the or Mars Pathfinder landed on July 4, 1997. At the top right you can see Valles Marineris and the volcanoes of Tharsis. Lower left, Cerberus and Elysium region, lower right, Syris Major

Mars seen by the Hubble Space Telescope - 1999 - Images obtained between 27 April and 6 May 1999 during the opposition of Mars when the planet was only 87 million km away from Earth. Between each image, Mars rotated 90 degrees. At the top left, the image is centered on Ares Vallis, the or Mars Pathfinder landed on July 4, 1997. At the top right you can see Valles Marineris and the volcanoes of Tharsis. Lower left, Cerberus and Elysium region, lower right, Syris Major

PIX4614949

Mars seen by the Hubble Space Telescope - 2003 - Images obtained in August 2003 during the opposition of Mars when the planet was only 56 million km away from Earth. These images were taken 11 hours apart, showing the two opposing hemispheres of Mars. On the left, image taken August 26, 2003, hemisphere of Syrtis Major with the Hellas basin. On the right, image taken on 27 August 2003, the region of the volcano Olympus Mons, at the top in the center, the volcanoes of Tharsis, below the right, and Valles Marineris in the middle of the image

Mars seen by the Hubble Space Telescope - 2003 - Images obtained in August 2003 during the opposition of Mars when the planet was only 56 million km away from Earth. These images were taken 11 hours apart, showing the two opposing hemispheres of Mars. On the left, image taken August 26, 2003, hemisphere of Syrtis Major with the Hellas basin. On the right, image taken on 27 August 2003, the region of the volcano Olympus Mons, at the top in the center, the volcanoes of Tharsis, below the right, and Valles Marineris in the middle of the image

PIX4614968

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel. The dark material shows a network of light - coloured, incised valleys that look similar to drainage networks known on Earth. It is still debated whether the valleys originate from precipitation, groundwater springs or liquid or magma flows on the surface

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel. The dark material shows a network of light - coloured, incised valleys that look similar to drainage networks known on Earth. It is still debated whether the valleys originate from precipitation, groundwater springs or liquid or magma flows on the surface

PIX4616125

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

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Mars: Noctis Labyrinthus - Mars: Noctis Labyrinthus - Perspective view of Noctis Labyrinthus, located in the western part of the great Martian canyon Valles Marineris. This heavily eroded canyon is here 5000 meters deep. Image obtained by the Mars Express probe on June 25, 2006. On 25 June 2006 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 16 meters per pixel. The data were acquired in the region of Noctis Labyrinthus at approximately 6.5* southern latitude and 260* eastern longitude. The region Noctis Labyrinthus, the Labyrinth of the Night”” is located directly on the western edge of Valles Marineris, the “Grand Canyon of Mars””. It is part of the complex graben system which is associated with the up - arching of Tharsis. Eye - catching is the high density of deeply incised, smaller, maze - like fractures. The scene exhibits parts of those graben structures which are incised up to 5000

Mars: Noctis Labyrinthus - Mars: Noctis Labyrinthus - Perspective view of Noctis Labyrinthus, located in the western part of the great Martian canyon Valles Marineris. This heavily eroded canyon is here 5000 meters deep. Image obtained by the Mars Express probe on June 25, 2006. On 25 June 2006 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 16 meters per pixel. The data were acquired in the region of Noctis Labyrinthus at approximately 6.5* southern latitude and 260* eastern longitude. The region Noctis Labyrinthus, the Labyrinth of the Night”” is located directly on the western edge of Valles Marineris, the “Grand Canyon of Mars””. It is part of the complex graben system which is associated with the up - arching of Tharsis. Eye - catching is the high density of deeply incised, smaller, maze - like fractures. The scene exhibits parts of those graben structures which are incised up to 5000

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Water ice clouds over Mars, 1976

Water ice clouds over Mars, 1976

UIS5071554

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Walter B Myers

PIX4616824

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