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Rover Curiosity on March, 12 May 2019.

Rover Curiosity on March, 12 May 2019.

PIX5940237

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

PIX4606652

Full Moon and Mars views from ISS - Full Moon with Mars - Mars (small point on the right) from the International Space Station on September 9, 2003. This view of a full Moon was photographed by one of the Expedition 7 crewmembers aboard the International Space Station (ISS) on September 9, 2003. The view also includes Mars, which appears as a small dot

Full Moon and Mars views from ISS - Full Moon with Mars - Mars (small point on the right) from the International Space Station on September 9, 2003. This view of a full Moon was photographed by one of the Expedition 7 crewmembers aboard the International Space Station (ISS) on September 9, 2003. The view also includes Mars, which appears as a small dot

PIX4588149

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

D. Ducros

PIX4606641

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

PIX4580080

Mars Science Laboratory - Artist view - Mars Science Laboratory - Artist view - Artist view of the Mars Science Laboratory (MSL) probe, approaching the surface of Mars. In August 2012 this probe should deposit a rover named Curiosity on the surface of the planet Mars. This is an artist's concept of Nasa's Mars Science Laboratory spacecraft approaching Mars. The Curiosity rover is safely tucked inside the spacecraft's aeroshell. The mission's approach phase begins 45 minutes before the spacecraft enters the Martian atmosphere. It lasts until the spacecraft enters the atmosphere. For navigation purposes, the atmospheric entry point is (2,188 miles (3,522 kilometers) above the center of the planet. This illustration depicts a scene after the spacecraft's cruise stage has been jettisoned, which will occur 10 minutes before atmospheric entry. The Mars Science Laboratory spacecraft is being prepared for launch during Nov. 25 to Dec. 18, 2011. Landing on Mars is in early August 2012. In a pri

Mars Science Laboratory - Artist view - Mars Science Laboratory - Artist view - Artist view of the Mars Science Laboratory (MSL) probe, approaching the surface of Mars. In August 2012 this probe should deposit a rover named Curiosity on the surface of the planet Mars. This is an artist's concept of Nasa's Mars Science Laboratory spacecraft approaching Mars. The Curiosity rover is safely tucked inside the spacecraft's aeroshell. The mission's approach phase begins 45 minutes before the spacecraft enters the Martian atmosphere. It lasts until the spacecraft enters the atmosphere. For navigation purposes, the atmospheric entry point is (2,188 miles (3,522 kilometers) above the center of the planet. This illustration depicts a scene after the spacecraft's cruise stage has been jettisoned, which will occur 10 minutes before atmospheric entry. The Mars Science Laboratory spacecraft is being prepared for launch during Nov. 25 to Dec. 18, 2011. Landing on Mars is in early August 2012. In a pri

PIX4606783

Total Eclipse of Moon and March, 27 July 2018.

Total Eclipse of Moon and March, 27 July 2018.

Alex Conu

PIX5940210

Permanent station between Mars and Earth - Artist view - Mars lander departs cycler - Artist view - A landing ship (top left) leaves the Mars Cycler to land on the red planet. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. A manned Mars lander/return vehicle, upper left, disembarks from a Mars cycler for the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a large and well-equipped Mars cycler would off

Permanent station between Mars and Earth - Artist view - Mars lander departs cycler - Artist view - A landing ship (top left) leaves the Mars Cycler to land on the red planet. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. A manned Mars lander/return vehicle, upper left, disembarks from a Mars cycler for the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a large and well-equipped Mars cycler would off

Walter B Myers

PIX4639544

Mars Recognition Orbiter and the Comet, Artist view (photo)

Mars Recognition Orbiter and the Comet, Artist view (photo)

Steven Hobbs

PIX6039537

Martian Base - Illustration

Martian Base - Illustration

PIX5940231

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

PIX4615099

Conjunction Mars Jupiter - Jupiter - Mars conjunction: Landscape seen at dawn with in the sky, Jupiter, very bright, and Mars (just below). January 7, 2018. Very close conjunction between Jupiter and Mars above misty plains in Southern Romania

Conjunction Mars Jupiter - Jupiter - Mars conjunction: Landscape seen at dawn with in the sky, Jupiter, very bright, and Mars (just below). January 7, 2018. Very close conjunction between Jupiter and Mars above misty plains in Southern Romania

Alex Conu

PIX4588267

Rover Curiosity on Mars - Curiosity Mars rover selfie - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of images taken by the robot on August 5, 2015. This low-angle self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the site from which it reached down to drill into a rock target called “” Buckskin”” on lower Mount Sharp. The selfie combines several component images taken by Curiosity's Mars Hand Lens Imager (MAHLI) on Aug. 5, 2015, during the 1,065th Martian day, or sol, of the rover's work on Mars. For scale, the rover's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide

Rover Curiosity on Mars - Curiosity Mars rover selfie - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of images taken by the robot on August 5, 2015. This low-angle self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the site from which it reached down to drill into a rock target called “” Buckskin”” on lower Mount Sharp. The selfie combines several component images taken by Curiosity's Mars Hand Lens Imager (MAHLI) on Aug. 5, 2015, during the 1,065th Martian day, or sol, of the rover's work on Mars. For scale, the rover's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide

PIX4643615

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Walter B Myers

PIX4629809

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

PIX4615036

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

D. Ducros

PIX4606610

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

D. Ducros

PIX4606614

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

D. Ducros

PIX4606616

Mars - Volcano Olympus Mons - Olympus Mons volcano on Mars - Image made from black and white photos obtained by Viking probes. This image shows Olympus Mons, a volcano 600 km in diameter and 27 km high. This painting, based on a mosaic of black - and - white Viking Orbiter images of Olympus Mons, shows the volcano's flanks and complex caldera above thin clouds of water ice

Mars - Volcano Olympus Mons - Olympus Mons volcano on Mars - Image made from black and white photos obtained by Viking probes. This image shows Olympus Mons, a volcano 600 km in diameter and 27 km high. This painting, based on a mosaic of black - and - white Viking Orbiter images of Olympus Mons, shows the volcano's flanks and complex caldera above thin clouds of water ice

PIX4615147

Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for stereo color viewing of surrounding terrain and material collected by the arm; and, the ChemCam instrument, which is a laser that vaporizes material from rocks up to about 9 meters (30 feet) away and determines what elements the rocks are made of

Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for stereo color viewing of surrounding terrain and material collected by the arm; and, the ChemCam instrument, which is a laser that vaporizes material from rocks up to about 9 meters (30 feet) away and determines what elements the rocks are made of

PIX4606945

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

D. Ducros

PIX4606646

March -View of the south pole - Mars South Pole: Image of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. Mars Express imaged this area of March on 17 December 2012, in infrared, green and blue light, using its High Resolution Stereo Camera.

March -View of the south pole - Mars South Pole: Image of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. Mars Express imaged this area of March on 17 December 2012, in infrared, green and blue light, using its High Resolution Stereo Camera.

PIX4616213

Tsunami on Mars - Artist's view - Mars tsunami: More than three billion years ago, oceans existed on Mars. It is likely that the planet has experienced gigantic tsunamis caused by meteorite impacts on the planet - 3.5 billion years ago Mars had oceans. Huge Tsunamis probably occured most likely caused by meteors colliding with the planet

Tsunami on Mars - Artist's view - Mars tsunami: More than three billion years ago, oceans existed on Mars. It is likely that the planet has experienced gigantic tsunamis caused by meteorite impacts on the planet - 3.5 billion years ago Mars had oceans. Huge Tsunamis probably occured most likely caused by meteors colliding with the planet

Miller, Ron (b.1947)

PIX4616903

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606969

Mars (Greek Ares) Roman god of war. A male planet, hot and fiery. Those born under Mars had a choleric temperament. The planet's metal was iron, its season Summer, its day Tuesday and its night Saturday. From Solensis Aratus Phaenomena et Prognostica, Cologne, 1569, Woodcut

Mars (Greek Ares) Roman god of war. A male planet, hot and fiery. Those born under Mars had a choleric temperament. The planet's metal was iron, its season Summer, its day Tuesday and its night Saturday. From Solensis Aratus Phaenomena et Prognostica, Cologne, 1569, Woodcut

UIG542243

From Earth to Moon, then March -Illustration - Aurora program - Illustration - Aurora Programme is part of Europe's strategy for space, endorsed by the European Union Council of Research and the ESA Council in 2001. The objective of the Aurora is first to formulate and then to implement a European long-term plan for the robotic and human exploration of solar system, with Mars, the Moon and the asteroids as the most likely targets

From Earth to Moon, then March -Illustration - Aurora program - Illustration - Aurora Programme is part of Europe's strategy for space, endorsed by the European Union Council of Research and the ESA Council in 2001. The objective of the Aurora is first to formulate and then to implement a European long-term plan for the robotic and human exploration of solar system, with Mars, the Moon and the asteroids as the most likely targets

P. Carril

PIX4639717

An automatic cargo ship en route to Mars - Unmanned cargo capsule departs Mars cycler - An automatic cargo ship separates from the Mars Cycler to bring equipment to Mars. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. With small bursts from its reaction control thrusters, an automated cargo capsule begins its one-way journey from a Mars cycler to the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a la

An automatic cargo ship en route to Mars - Unmanned cargo capsule departs Mars cycler - An automatic cargo ship separates from the Mars Cycler to bring equipment to Mars. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. With small bursts from its reaction control thrusters, an automated cargo capsule begins its one-way journey from a Mars cycler to the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a la

Walter B Myers

PIX4639566

Mars and the M35 cluster in the Gemeaux - Mars meets M35 in Gemini - The planet Mars shines above the cluster of stars M35 in the constellation Gemeaux. December 19, 2007. Mars is shining above the star cluster M35 in the constellation of Gemini. December 19, 2007

Mars and the M35 cluster in the Gemeaux - Mars meets M35 in Gemini - The planet Mars shines above the cluster of stars M35 in the constellation Gemeaux. December 19, 2007. Mars is shining above the star cluster M35 in the constellation of Gemini. December 19, 2007

Sebastian Voltmer

PIX4587748

Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history

Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history

Steven Hobbs

PIX4616896

Mars and the open cluster M44 - Planet Mars and the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. Bright Mars above M44 stars; this cluster is located about 600 light year away in Cancer

Mars and the open cluster M44 - Planet Mars and the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. Bright Mars above M44 stars; this cluster is located about 600 light year away in Cancer

Sebastian Voltmer

PIX4588249

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

PIX4640029

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

PIX4615396

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

Mars XIII, 1971 (steel)

Mars XIII, 1971 (steel)

Gabino, Amadeo (1922-2004)

XKH151915

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 23, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 23, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587634

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. October 23, 1990. - Photo series showing the retrograde movement of Mars in the Taurus. October 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. October 23, 1990. - Photo series showing the retrograde movement of Mars in the Taurus. October 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587645

Orion, the Taurus, Venus, the Moon and Mars - Orion, Taurus, Venus, Moon and Mars - Venus in conjunction with the Moon, on the right. Visible also the Mars planet near the Pleiades cluster. 24 March 2004, Quimper Moon Venus conjunction (right). Also visible, Mars near the Pleiades star cluster. March 24 2004

Orion, the Taurus, Venus, the Moon and Mars - Orion, Taurus, Venus, Moon and Mars - Venus in conjunction with the Moon, on the right. Visible also the Mars planet near the Pleiades cluster. 24 March 2004, Quimper Moon Venus conjunction (right). Also visible, Mars near the Pleiades star cluster. March 24 2004

Laurent Laveder

PIX4586529

Exploration of Mars-Illustration - Exploring Mars - Artist view - Astronauts explore an ancient river bed on Mars. In the sky the satellites of Mars, Phobos and Deimos. Astronauts set up Mars base at edge of ancient river valley

Exploration of Mars-Illustration - Exploring Mars - Artist view - Astronauts explore an ancient river bed on Mars. In the sky the satellites of Mars, Phobos and Deimos. Astronauts set up Mars base at edge of ancient river valley

Dixon, Don (b.1951)

PIX4639763

Rover Opportunity sur Mars - Artist view - Rover Opportunity on martian surface - Artist view - Photograph showing the rover Opportunity on the edge of the Victoria crater on Mars. This image superimposes an artist's concept of the Mars Exploration Rover Opportunity on the rim of Victoria Crater. It is done to give a sense of scale

Rover Opportunity sur Mars - Artist view - Rover Opportunity on martian surface - Artist view - Photograph showing the rover Opportunity on the edge of the Victoria crater on Mars. This image superimposes an artist's concept of the Mars Exploration Rover Opportunity on the rim of Victoria Crater. It is done to give a sense of scale

PIX4606589

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

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars en route vers Mars, en 2016. Artist view of the european spacecraft ExoMars leaving the Earth in 2016 to study planet Mars

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars en route vers Mars, en 2016. Artist view of the european spacecraft ExoMars leaving the Earth in 2016 to study planet Mars

D. Ducros

PIX4606951

Mars, 1990 (neon)

Mars, 1990 (neon)

Paik, Nam June (1932-2006)

Wolfgang Neeb

WNB242936

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

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

PIX4616532

March - Arabia Terra - Mars Express probe on June 17, 2019.

March - Arabia Terra - Mars Express probe on June 17, 2019.

PIX5940214

Phobos and Mars

Phobos and Mars

P. Carril

PIX4616760

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of 57 images taken by the robot on January 19, 2016. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at “” Namib Dune,””” where the rover's activities included scuffing into the dune with a wheel and scooping samples of sand for laboratory analysis. The scene combines 57 images taken on Jan. 19, 2016, during the 1,228th Martian day, or sol, of Curiosity's work on Mars. The camera used for this is the Mars Hand Lens Imager (MAHLI) at the end of the rover's robotic arm. The view does not include the rover's arm. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. For scale, the rover's wheels are 20 inches (50 centimeters) in diamet

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of 57 images taken by the robot on January 19, 2016. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at “” Namib Dune,””” where the rover's activities included scuffing into the dune with a wheel and scooping samples of sand for laboratory analysis. The scene combines 57 images taken on Jan. 19, 2016, during the 1,228th Martian day, or sol, of Curiosity's work on Mars. The camera used for this is the Mars Hand Lens Imager (MAHLI) at the end of the rover's robotic arm. The view does not include the rover's arm. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. For scale, the rover's wheels are 20 inches (50 centimeters) in diamet

PIX4643637

Nine kinds of Bali representing the planets, from 'The History and Doctrine of Buddhism' by Edward Upham, 1829 (colour litho)

Nine kinds of Bali representing the planets, from 'The History and Doctrine of Buddhism' by Edward Upham, 1829 (colour litho)

English School, (19th century)

STC414240

Exploration of Mars-Illustration - Exploring Mars - Artist view - Astronauts explore an ancient river bed on Mars. In the sky the satellites of Mars, Phobos and Deimos. Astronauts survey site for base in ancient river valley on Mars

Exploration of Mars-Illustration - Exploring Mars - Artist view - Astronauts explore an ancient river bed on Mars. In the sky the satellites of Mars, Phobos and Deimos. Astronauts survey site for base in ancient river valley on Mars

Dixon, Don (b.1951)

PIX4639778

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

PIX4580071

Ice Towers on Mars - Illustration - Martian ice towers - Illustration: The Hellas basin on Mars would house ice towers several tens of metres high in which a geothermale activity was discovered - Unusual warm spots on Mars might represent “” ice towers””” similar to those seen in Antarctica, say researchers. ♪ They could even harbour life ♪

Ice Towers on Mars - Illustration - Martian ice towers - Illustration: The Hellas basin on Mars would house ice towers several tens of metres high in which a geothermale activity was discovered - Unusual warm spots on Mars might represent “” ice towers””” similar to those seen in Antarctica, say researchers. ♪ They could even harbour life ♪

Miller, Ron (b.1947)

PIX4617116

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

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Walter B Myers

PIX4639664

Observation night - Saturn Mars and Venus - Observing night - Saturn Mars and Venus - Starry sky observation in the Alps. The planets Saturn Mars and Venus are visible. July 19, 2010. Planets Saturn Mars and Venus shine above observers. Alps, july 19, 2010

Observation night - Saturn Mars and Venus - Observing night - Saturn Mars and Venus - Starry sky observation in the Alps. The planets Saturn Mars and Venus are visible. July 19, 2010. Planets Saturn Mars and Venus shine above observers. Alps, july 19, 2010

Stefan Seip

PIX4588130

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars en route vers Mars, en 2016. Artist view of the european spacecraft ExoMars leaving the Earth in 2016 to study planet Mars

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars en route vers Mars, en 2016. Artist view of the european spacecraft ExoMars leaving the Earth in 2016 to study planet Mars

D. Ducros

PIX4606940

Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum

Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum

Steven Hobbs

PIX4606584

Mars - View of the north pole - Mars north pole - Image of a portion of the northern polar cap of Mars obtained by the Mars Express probe on May 17, 2010. This image was acquired by the Mars Express High - Resolution Stereo Camera on 17 May 2010 and shows a part of the northern polar region of Mars at the northern hemisphere summer solstice. The polar ice deposits follow the seasonal cycles. Studies made by Mars Express's OMEGA instrument shows that the cap is covered by frozen water and carbon dioxide ice in winter and spring but by this point in the martian year all of the carbon dioxide ice has warmed and evaporated into the planet's atmosphere. Only water ice is left behind, which shows up as bright white areas in this picture. From these layers, large bursts of water vapour are occasionally released into the atmosphere. In winter, part of the atmosphere recondenses as frost and snow on the northern cap. These seasonal deposits can extend as far south as 45* N latitude and be up to

Mars - View of the north pole - Mars north pole - Image of a portion of the northern polar cap of Mars obtained by the Mars Express probe on May 17, 2010. This image was acquired by the Mars Express High - Resolution Stereo Camera on 17 May 2010 and shows a part of the northern polar region of Mars at the northern hemisphere summer solstice. The polar ice deposits follow the seasonal cycles. Studies made by Mars Express's OMEGA instrument shows that the cap is covered by frozen water and carbon dioxide ice in winter and spring but by this point in the martian year all of the carbon dioxide ice has warmed and evaporated into the planet's atmosphere. Only water ice is left behind, which shows up as bright white areas in this picture. From these layers, large bursts of water vapour are occasionally released into the atmosphere. In winter, part of the atmosphere recondenses as frost and snow on the northern cap. These seasonal deposits can extend as far south as 45* N latitude and be up to

PIX4616313

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

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

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

PIX4643733

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