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Images de ' Martian' médias trouvés, 1,027

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Martian Base - Illustration

Martian Base - Illustration

PIX5940231

Martian base - Illustration - Martian base - Illustration - Artist's view of a first European Martian base with a pressurised mobile laboratory. An european martian base with a mobile pressurized laboratory

Martian base - Illustration - Martian base - Illustration - Artist's view of a first European Martian base with a pressurised mobile laboratory. An european martian base with a mobile pressurized laboratory

D. Ducros

PIX4639847

European astronauts on Mars - Illustration - European astronauts on Mars - Illustration - View of European astronauts artist near their Martian base and a mobile pressurised laboratory. European astronauts near their martian base with a mobile presurized laboratory

European astronauts on Mars - Illustration - European astronauts on Mars - Illustration - View of European astronauts artist near their Martian base and a mobile pressurised laboratory. European astronauts near their martian base with a mobile presurized laboratory

D. Ducros

PIX4639851

Martian base - Illustration - Martian base - Illustratio

Martian base - Illustration - Martian base - Illustratio

S. Numazawa

PIX4639900

Martian Landscape: March -Illustration - Martian surface Artwork

Martian Landscape: March -Illustration - Martian surface Artwork

S. Numazawa

PIX4616929

Martian base - Illustration - Martian base - Illustratio

Martian base - Illustration - Martian base - Illustratio

S. Numazawa

PIX4639906

Experience Mars500 - Mars500 experiment facility in Moscow - Installed at the Russian Institute of Bio-Medical Problems (IBMP) in Moscow, the 550 m Seal Simulator consists of an interplanetary spacecraft and a Martian lander, and features a Martian landscape. The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500, the first full-length simulated mission to Mars, started on June 3 2010 when the six-man crew entered their 'spacecraft' and the hatch was closed. The experiment will run until November 2011. Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China face a mission that is as close as possible to a real space voyage without leavi

Experience Mars500 - Mars500 experiment facility in Moscow - Installed at the Russian Institute of Bio-Medical Problems (IBMP) in Moscow, the 550 m Seal Simulator consists of an interplanetary spacecraft and a Martian lander, and features a Martian landscape. The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500, the first full-length simulated mission to Mars, started on June 3 2010 when the six-man crew entered their 'spacecraft' and the hatch was closed. The experiment will run until November 2011. Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China face a mission that is as close as possible to a real space voyage without leavi

S. Corvaja

PIX4640078

Experience Mars500 - Mars500 experiment facility in Moscow - Installed at the Russian Institute of Bio-Medical Problems (IBMP) in Moscow, the 550 m Seal Simulator consists of an interplanetary spacecraft and a Martian lander, and features a Martian landscape. The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500, the first full-length simulated mission to Mars, started on June 3 2010 when the six-man crew entered their 'spacecraft' and the hatch was closed. The experiment will run until November 2011. Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China face a mission that is as close as possible to a real space voyage without leavi

Experience Mars500 - Mars500 experiment facility in Moscow - Installed at the Russian Institute of Bio-Medical Problems (IBMP) in Moscow, the 550 m Seal Simulator consists of an interplanetary spacecraft and a Martian lander, and features a Martian landscape. The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500, the first full-length simulated mission to Mars, started on June 3 2010 when the six-man crew entered their 'spacecraft' and the hatch was closed. The experiment will run until November 2011. Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China face a mission that is as close as possible to a real space voyage without leavi

PIX4640069

European Astronaut on Mars - Illustration - European Astronaut on Mars - Illustration - A European astronaut robs the soil of March in 2030. Artist's view. An european spacewoman walking on the martian surface in 2030

European Astronaut on Mars - Illustration - European Astronaut on Mars - Illustration - A European astronaut robs the soil of March in 2030. Artist's view. An european spacewoman walking on the martian surface in 2030

P. Carril

PIX4639704

Crew of the Mars500 experience - Mars500 experiment crew - The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500 520-day isolation crew (Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China) photographed just before the entry to the facility at 13:49 local time in Moscow (11:49 CET) on 3 June 2010. They will stay in the facility for more than 17 months simulating a mission to Mars

Crew of the Mars500 experience - Mars500 experiment crew - The Mars500 experience is a Martian mission simulation that began on June 3, 2010. The crew locked up for 520 days consists of six people. They are Italian-Colombian Diego Urbina (27) and Frenchman Roman Charles (31) selected by ESA, Russian Sukhrob Kamolov (32), Alexey Sitev (38), Alexandr Smoleevskiy (33) and Chinese Wang Yue (26). March 500 520-day isolation crew (Diego Urbina and Romain Charles from Europe, Sukhrob Kamolov, Alexey Sitev, Alexandr Smoleevskiy and Wang Yue from China) photographed just before the entry to the facility at 13:49 local time in Moscow (11:49 CET) on 3 June 2010. They will stay in the facility for more than 17 months simulating a mission to Mars

PIX4640067

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Walter B Myers

PIX4616961

Sol de Mars by Viking 2 - High resolution Viking image of Martian rocks - Image of the Mars surface obtained by the Viking 2 probe on September 5, 1976. Image of martian soil taken by the Viking 2 Lander on september 5 1976

Sol de Mars by Viking 2 - High resolution Viking image of Martian rocks - Image of the Mars surface obtained by the Viking 2 probe on September 5, 1976. Image of martian soil taken by the Viking 2 Lander on september 5 1976

Steven Hobbs

PIX4615200

The Colonization of Mars - Illustration - Mars Colony: Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

The Colonization of Mars - Illustration - Mars Colony: Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

PIX4640022

Martian base-illustration - Martian base - Illustratio

Martian base-illustration - Martian base - Illustratio

L. Bret

PIX4639673

Mars surface seen by the rover Curiosity 09/2015 - Martian surface seen from the rover Curiosity 09/2015: Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity on September 9, 2015. This composite image looking toward the higher regions of Mount Sharp was taken on September 9, 2015, by Nasa's Curiosity rover. In the foreground - about 2 miles (3 kilometers) from the rover - is a long ridge teeming with hematite, an iron oxide. Just beyond is an undulating plain rich in clay minerals. And just beyond that are a multitude of rounded buttes, all high in sulfate minerals. The changing mineralogy in these layers of Mount Sharp suggests a changing environment in early Mars, though all involve exposure to water billions of years ago. Further back in the image are striking, light-toned cliffs in rock that may have formed in drier times and now is heavily eroded by winds. The colors are adjusted so that rocks look approximately as they would if they we

Mars surface seen by the rover Curiosity 09/2015 - Martian surface seen from the rover Curiosity 09/2015: Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity on September 9, 2015. This composite image looking toward the higher regions of Mount Sharp was taken on September 9, 2015, by Nasa's Curiosity rover. In the foreground - about 2 miles (3 kilometers) from the rover - is a long ridge teeming with hematite, an iron oxide. Just beyond is an undulating plain rich in clay minerals. And just beyond that are a multitude of rounded buttes, all high in sulfate minerals. The changing mineralogy in these layers of Mount Sharp suggests a changing environment in early Mars, though all involve exposure to water billions of years ago. Further back in the image are striking, light-toned cliffs in rock that may have formed in drier times and now is heavily eroded by winds. The colors are adjusted so that rocks look approximately as they would if they we

PIX4616695

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Landing sequence of a mini - station. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Mini - landing sequence stations. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Landing sequence of a mini - station. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Mini - landing sequence stations. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606463

Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander

Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander

Steven Hobbs

PIX4615194

European astronaut on Mars - Illustration - European female astronaut on Mars - Illustration - A European astronaut finds the Rover Pasteur of the EXOMARS mission. Artist's view. An european astronaut finds the Rover Pasteur of the EXOMARS mission

European astronaut on Mars - Illustration - European female astronaut on Mars - Illustration - A European astronaut finds the Rover Pasteur of the EXOMARS mission. Artist's view. An european astronaut finds the Rover Pasteur of the EXOMARS mission

P. Carril

PIX4639716

March: gullies in the crater Gale (photo)

March: gullies in the crater Gale (photo)

Steven Hobbs

PIX6039529

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of landing of a penetrator. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Penetrator landing sequence. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of landing of a penetrator. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Penetrator landing sequence. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606471

Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays

Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays

Walter B Myers

PIX4639821

Lander of the probe Mars 96 - Mars 96 surface station - Artist view - Artist view of the lander of the probe Mars 96 poses on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing a March 96 surface station. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

Lander of the probe Mars 96 - Mars 96 surface station - Artist view - Artist view of the lander of the probe Mars 96 poses on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing a March 96 surface station. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606441

Astronaut on Mars-Artist's view - Astronaut on Mars - Illustratio

Astronaut on Mars-Artist's view - Astronaut on Mars - Illustratio

S. Numazawa

PIX4639697

Detail of the 1st color panorama of the Martian soil obtained by Spirit. The Rover Spirit landed on Mars in the area of the crater Gusev, July 4, 2004 - Detail of the first panorama taken by Spirit.: Surface de Mars: detail of the first panorama obtained by Spirit - The martian surface seen by Spirit. 07/2004

Detail of the 1st color panorama of the Martian soil obtained by Spirit. The Rover Spirit landed on Mars in the area of the crater Gusev, July 4, 2004 - Detail of the first panorama taken by Spirit.: Surface de Mars: detail of the first panorama obtained by Spirit - The martian surface seen by Spirit. 07/2004

PIX4615535

March: Spherule seen by Opportunity - Mars: hematite - rich berry seen by Opportunity - Spherule of a few millimetres in diameter, rich in hematite, seen on the surface of a Martian rock by the microscope camera of the rover Opportunity on March 4, 2004. Recolorized image. Opportunity micrograph of Martian soil taken on Sol 39 (march 4 2004), showing the blueberries of hematite, indicators of evidence of past water activity. Recolorized picture

March: Spherule seen by Opportunity - Mars: hematite - rich berry seen by Opportunity - Spherule of a few millimetres in diameter, rich in hematite, seen on the surface of a Martian rock by the microscope camera of the rover Opportunity on March 4, 2004. Recolorized image. Opportunity micrograph of Martian soil taken on Sol 39 (march 4 2004), showing the blueberries of hematite, indicators of evidence of past water activity. Recolorized picture

Steven Hobbs

PIX4615783

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606673

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut crowds the soil of March. Artist's view. In some distant future, astronauts amble about on Mars. The hardware designs are based on the Lunar spacecraft being imagined by NASA

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut crowds the soil of March. Artist's view. In some distant future, astronauts amble about on Mars. The hardware designs are based on the Lunar spacecraft being imagined by NASA

PIX4639858

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

PIX4616735

Snow on Mars - Illustration - Snow at the martian pole: Snow Tempete at the martian pole

Snow on Mars - Illustration - Snow at the martian pole: Snow Tempete at the martian pole

Miller, Ron (b.1947)

PIX4617063

Mars surface seen by the rover Curiosity 03/2014: The formation “” Kimberley “” seen by Curiosity on March 25, 2014. The strata indicate a flow of water towards Mount Sharp (in the background). A view from the “” Kimberley”” formation on Mars taken by Nasa's Curiosity rover. The strata in the foreground dip towards the base of Mount Sharp, indicating flow of water toward a basin that existed before the larger bulk of the mountain formed. The colors are adjusted so that rocks look approximately as they would if they were on Earth, to help geologists interpret the rocks. This “” white balancing”” to adjust for the lighting on Mars overly compensates for the absence of blue on Mars, making the sky appear light blue and sometimes giving dark, black rocks a blue cast.

Mars surface seen by the rover Curiosity 03/2014: The formation “” Kimberley “” seen by Curiosity on March 25, 2014. The strata indicate a flow of water towards Mount Sharp (in the background). A view from the “” Kimberley”” formation on Mars taken by Nasa's Curiosity rover. The strata in the foreground dip towards the base of Mount Sharp, indicating flow of water toward a basin that existed before the larger bulk of the mountain formed. The colors are adjusted so that rocks look approximately as they would if they were on Earth, to help geologists interpret the rocks. This “” white balancing”” to adjust for the lighting on Mars overly compensates for the absence of blue on Mars, making the sky appear light blue and sometimes giving dark, black rocks a blue cast.

PIX4616687

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606454

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

PIX4616696

What humans hope to eventually find on the surface of Mars - the fossilised remains of organic life. The fossil models used in ths scene are a species of trilobites, whichcompletely dominated the Earth after the Cambrian explosion, some 500 million years ago: Trilobite fossils on the surface of Mars - Fossil on Mars. Artwork

What humans hope to eventually find on the surface of Mars - the fossilised remains of organic life. The fossil models used in ths scene are a species of trilobites, whichcompletely dominated the Earth after the Cambrian explosion, some 500 million years ago: Trilobite fossils on the surface of Mars - Fossil on Mars. Artwork

PIX4617060

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606678

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606690

Martian Roche seen by Opportunity - Water action on Mars rock seen by Opportunity - Small cavites (“vugs”) observed on the surface of the Martian rock nicknamed “El Capitan””. These voids were created by the disappearance of crystals of salts included in the rock dissolved or eroded by water. Image obtained by the microscope camera of the rover Opportunity on February 23, 2004 (Sol 29). Recolorized image. Opportunity micrograph of Martian soil, located on the region dubbed “El Capitan”” showing regions where mineral crystals have been dissolved by water action. Image taken on February 23 2004 (Sol 29). Recolorized picture

Martian Roche seen by Opportunity - Water action on Mars rock seen by Opportunity - Small cavites (“vugs”) observed on the surface of the Martian rock nicknamed “El Capitan””. These voids were created by the disappearance of crystals of salts included in the rock dissolved or eroded by water. Image obtained by the microscope camera of the rover Opportunity on February 23, 2004 (Sol 29). Recolorized image. Opportunity micrograph of Martian soil, located on the region dubbed “El Capitan”” showing regions where mineral crystals have been dissolved by water action. Image taken on February 23 2004 (Sol 29). Recolorized picture

Steven Hobbs

PIX4615765

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606692

Probe Penetrator Mars 96 - Penetrator of the Mars 96 spacecraft - Cross-section view of one of the two penetrators of the Mars 96 probe. Numerous measuring instruments were incorporated. The lower part was to sink several metres into the Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Cutaway of a penetrator deployed on the martian surface showing the different experiments in the forebody and in the afterbody. The forebody should be separated from the afterbody and dive several meters into the martian soil. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

Probe Penetrator Mars 96 - Penetrator of the Mars 96 spacecraft - Cross-section view of one of the two penetrators of the Mars 96 probe. Numerous measuring instruments were incorporated. The lower part was to sink several metres into the Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Cutaway of a penetrator deployed on the martian surface showing the different experiments in the forebody and in the afterbody. The forebody should be separated from the afterbody and dive several meters into the martian soil. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606433

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines hundreds exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view is in approximately true color. The landing site is at 68.22 degrees north latitude, 234.25

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines hundreds exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view is in approximately true color. The landing site is at 68.22 degrees north latitude, 234.25

PIX4616671

La conquete de Mars-Illustration - Mars outpost near mesa - Artist's view of an inhabited base on Mars. A manned habitat rests on the rocky and desolate surface of Mars. In the background is a mesa and on the right a manned rover

La conquete de Mars-Illustration - Mars outpost near mesa - Artist's view of an inhabited base on Mars. A manned habitat rests on the rocky and desolate surface of Mars. In the background is a mesa and on the right a manned rover

Walter B Myers

PIX4639947

The Phoenix probe on its landing site - Phoenix landing site, cylindrical projection - Mosaic of images in cylindrical projection showing the Phoenix probe placed on Mars. The location of the ground through the probe arm is visible in the right part of the image. The probe landed on a vast plain north of the planet in the Vastitas Borealis region on 25 May 2008. She took and analyzed samples of Martian soil and confirmed the presence of water on Mars. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth. The center of the image is the westward part of the scene. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible in the right half of t

The Phoenix probe on its landing site - Phoenix landing site, cylindrical projection - Mosaic of images in cylindrical projection showing the Phoenix probe placed on Mars. The location of the ground through the probe arm is visible in the right part of the image. The probe landed on a vast plain north of the planet in the Vastitas Borealis region on 25 May 2008. She took and analyzed samples of Martian soil and confirmed the presence of water on Mars. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth. The center of the image is the westward part of the scene. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible in the right half of t

PIX4616660

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

PIX4616646

Vegetable Garden on Mars-Illustration - Mars Exploration - Illustration: Nasa develops the idea of growing food on other planets. NASA plans to grow food on future spacecraft and on other planets as a food supplement for astronauts. Fresh food, such as vegetables, provide essential vitamins and nutrients that will help enable sustainable deep space pioneering.

Vegetable Garden on Mars-Illustration - Mars Exploration - Illustration: Nasa develops the idea of growing food on other planets. NASA plans to grow food on future spacecraft and on other planets as a food supplement for astronauts. Fresh food, such as vegetables, provide essential vitamins and nutrients that will help enable sustainable deep space pioneering.

PIX4639992

Based on an asteroid-Artist's view - Base on an asteroid - Illustratio

Based on an asteroid-Artist's view - Base on an asteroid - Illustratio

S. Numazawa

PIX4639693

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut robs the soil of March as a dust storm comes up. Artist's view. Astronaut walking on Mars soil with a dust storm approaching

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut robs the soil of March as a dust storm comes up. Artist's view. Astronaut walking on Mars soil with a dust storm approaching

PIX4639949

Astronauts on Mars - Illustration - Astronauts on Mars - Illustration - Astronauts explore the surface of Mars. Artist's view. Human exploration of the martian surface

Astronauts on Mars - Illustration - Astronauts on Mars - Illustration - Astronauts explore the surface of Mars. Artist's view. Human exploration of the martian surface

PIX4639920

Sedimentary depots on Mars seen by Curiosity 02/2013 - Martian surface seen from the rover Curiosity 02/2013 - Sedimentary depots in the crater Gale sur Mars. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on February 14, 2013. This mosaic of images from the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west - northwest. Mastcam took the images for this mosaic during the 188th Martian day, or sol, of Curiosity's work on Mars (Feb. 14, 2013). The image has been white - balanced to show what the rocks would look like if ther were on Earth

Sedimentary depots on Mars seen by Curiosity 02/2013 - Martian surface seen from the rover Curiosity 02/2013 - Sedimentary depots in the crater Gale sur Mars. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on February 14, 2013. This mosaic of images from the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west - northwest. Mastcam took the images for this mosaic during the 188th Martian day, or sol, of Curiosity's work on Mars (Feb. 14, 2013). The image has been white - balanced to show what the rocks would look like if ther were on Earth

PIX4616681

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

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Scenario of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Scenario of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606457

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The 500 clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view in approximately true color covers an area about 30 meters by 30 meters (a

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The 500 clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view in approximately true color covers an area about 30 meters by 30 meters (a

PIX4616661

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 surface seen by the rover Curiosity 01/2014 - Martian surface seen from the rover Curiosity 01/2014 - Panorama of the surface of Mars in the crater Gale. A small sand dune one metre high is visible in the center of the image. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on January 28, 2014. This scene combines images taken by the left - eye camera of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover during the midafternoon, local Mars solar time, of the mission's 526th Martian day, or sol (Jan. 28, 2014). The sand dune in the upper center of the image spans a gap, called “” Dingo Gap,””” between two short scarps. The dune is about 3 feet (1 meter) high. The nearer edge of it is about 115 feet (35 meters) away from the top's position when the component images were taken, just after a Sol 526 drive of 49 feet (15 meters). The image has been white - balanced to show what the rocks would look like if they were on Earth

Mars surface seen by the rover Curiosity 01/2014 - Martian surface seen from the rover Curiosity 01/2014 - Panorama of the surface of Mars in the crater Gale. A small sand dune one metre high is visible in the center of the image. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on January 28, 2014. This scene combines images taken by the left - eye camera of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover during the midafternoon, local Mars solar time, of the mission's 526th Martian day, or sol (Jan. 28, 2014). The sand dune in the upper center of the image spans a gap, called “” Dingo Gap,””” between two short scarps. The dune is about 3 feet (1 meter) high. The nearer edge of it is about 115 feet (35 meters) away from the top's position when the component images were taken, just after a Sol 526 drive of 49 feet (15 meters). The image has been white - balanced to show what the rocks would look like if they were on Earth

PIX4616684

Midnight Sun on Mars seen by Phoenix - Midnight Sun on Mars seen by Phoenix - Panorama obtained by Phoenix probe showing the sun's race in the sky of Mars. The foreground image was taken on the 54th day of the mission (Ground 54, July 20, 2008). The different images of the Sun were taken between 10 pm and 2 am (local time) during soils 46 to 56 (12 to 22 July 2008 on Earth). The Phoenix probe landed on May 25, 2008 in the Vastitas Borealis region in the polar circle of Mars. This panorama mosaic of images was taken by the Surface Stereo Imager on board Nasa's Phoenix Mars Lander. This mosaic documents the midnight sun during several days of the mission. The foreground and sky images were taken on Sol 54, or the 54th Martian day of the mission (July 20, 2008). The solar images were taken between 10 p.m. and 2 a.m., local solar time, during the nights of sols 46 to 56. During this period of 11 sols, the sun's path got slightly lower over the northern horizon, causing the lack of smoothne

Midnight Sun on Mars seen by Phoenix - Midnight Sun on Mars seen by Phoenix - Panorama obtained by Phoenix probe showing the sun's race in the sky of Mars. The foreground image was taken on the 54th day of the mission (Ground 54, July 20, 2008). The different images of the Sun were taken between 10 pm and 2 am (local time) during soils 46 to 56 (12 to 22 July 2008 on Earth). The Phoenix probe landed on May 25, 2008 in the Vastitas Borealis region in the polar circle of Mars. This panorama mosaic of images was taken by the Surface Stereo Imager on board Nasa's Phoenix Mars Lander. This mosaic documents the midnight sun during several days of the mission. The foreground and sky images were taken on Sol 54, or the 54th Martian day of the mission (July 20, 2008). The solar images were taken between 10 p.m. and 2 a.m., local solar time, during the nights of sols 46 to 56. During this period of 11 sols, the sun's path got slightly lower over the northern horizon, causing the lack of smoothne

PIX4616625

The Phoenix probe on its landing site - Phoenix landing site, polar projection - Mosaic of polar projection images showing the Phoenix probe on Mars. The south is towards the top of the image, the place of the ground hollow through the probe arm is visible in the lower part of the image. The probe landed on a vast plain north of the planet in the Vastitas Borealis region on 25 May 2008. She took and analyzed samples of Martian soil and confirmed the presence of water on Mars. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth. South is towards the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible in the lower half of the image

The Phoenix probe on its landing site - Phoenix landing site, polar projection - Mosaic of polar projection images showing the Phoenix probe on Mars. The south is towards the top of the image, the place of the ground hollow through the probe arm is visible in the lower part of the image. The probe landed on a vast plain north of the planet in the Vastitas Borealis region on 25 May 2008. She took and analyzed samples of Martian soil and confirmed the presence of water on Mars. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth. South is towards the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible in the lower half of the image

PIX4616665

Geysers sur Mars - Illustration - Mars polar sand geysers - Illustration: Carbon gas jets melees a du sable on the southern pole of Mars during the spring degel - These jets are carbon dioxide gas with sand and dust emerging from solid carbon dioxide ice on the southern Martian polar ice cap

Geysers sur Mars - Illustration - Mars polar sand geysers - Illustration: Carbon gas jets melees a du sable on the southern pole of Mars during the spring degel - These jets are carbon dioxide gas with sand and dust emerging from solid carbon dioxide ice on the southern Martian polar ice cap

Miller, Ron (b.1947)

PIX4617118

The Colonization of Mars-Illustration - Mars Colony - Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

The Colonization of Mars-Illustration - Mars Colony - Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

Steven Hobbs

PIX4639993

Detail of the panorama obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater of 200m in diameter. Far right, Columbia Hills. The Rover Spirit landed on Mars in the crater region Gusev, July 4, 2004 - The rim and interior of a 200m diameter impact crater nicknamed “” Bonneville”” dominate this image. The Mars Exploration Rover Spirit acquired this panoramic camera image mosaic on the 68th martian day, or sol, of its mission (March 12, 2004): March: Cratere Bonneville seen by Spirit - March: impact crater Bonneville seen by Spirit

Detail of the panorama obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater of 200m in diameter. Far right, Columbia Hills. The Rover Spirit landed on Mars in the crater region Gusev, July 4, 2004 - The rim and interior of a 200m diameter impact crater nicknamed “” Bonneville”” dominate this image. The Mars Exploration Rover Spirit acquired this panoramic camera image mosaic on the 68th martian day, or sol, of its mission (March 12, 2004): March: Cratere Bonneville seen by Spirit - March: impact crater Bonneville seen by Spirit

PIX4615572

March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

PIX4615799

Geysers sur Mars - Illustration - Mars polar sand geysers - Illustration: Carbon gas jets melees a du sable on the southern pole of Mars during the spring degel - These jets are carbon dioxide gas with sand and dust emerging from solid carbon dioxide ice on the southern Martian polar ice cap

Geysers sur Mars - Illustration - Mars polar sand geysers - Illustration: Carbon gas jets melees a du sable on the southern pole of Mars during the spring degel - These jets are carbon dioxide gas with sand and dust emerging from solid carbon dioxide ice on the southern Martian polar ice cap

Miller, Ron (b.1947)

PIX4617128

Base sur Mars - Illustration - Mars Ice Home concept - Artist's view of an inhabited base on Mars. Inflatable housing concept surrounded by a layer of ice. The “” Mars Ice Home”” is a large inflatable torus, a shape similar to an inner tube, that is surrounded by a shell of water ice. The Mars Ice Home design has several advantages that make it an appealing concept. It is lightweight and can be transported and deployed with simple robotics, then filled with water before the crew arrives. It incorporates materials extracted from Mars, and because water in the Ice Home could potentially be converted to rocket fuel for the Mars Ascent Vehicle, the structure itself doubles as a storage tank that can be refilled for the next crew. Another critical benefit is that water, a hydrogen-rich material, is an excellent shielding material for galactic cosmic rays - and many areas of Mars have abundant water ice just below the surface. Galactic cosmic rays are one of the biggest risks of long stays o

Base sur Mars - Illustration - Mars Ice Home concept - Artist's view of an inhabited base on Mars. Inflatable housing concept surrounded by a layer of ice. The “” Mars Ice Home”” is a large inflatable torus, a shape similar to an inner tube, that is surrounded by a shell of water ice. The Mars Ice Home design has several advantages that make it an appealing concept. It is lightweight and can be transported and deployed with simple robotics, then filled with water before the crew arrives. It incorporates materials extracted from Mars, and because water in the Ice Home could potentially be converted to rocket fuel for the Mars Ascent Vehicle, the structure itself doubles as a storage tank that can be refilled for the next crew. Another critical benefit is that water, a hydrogen-rich material, is an excellent shielding material for galactic cosmic rays - and many areas of Mars have abundant water ice just below the surface. Galactic cosmic rays are one of the biggest risks of long stays o

PIX4640020

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