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{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"Martian Surface","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":232,"search_results_page_number":1}

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Images of 'Martian Surface' found, 232

The Colonization of Mars-Illustration - Mars Colony - Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars
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
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
Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet
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
March: gullies in the crater Gale (photo)
Exploration of Mars-Illustration - Mars rover rendezvous - The exploration of Mars by men will require vehicles that can take a crew long distances and will have to provide them with all the necessary protection against this hostile environment. A pair of manned Mars rovers rendezvous on the martian surface. Humans may one day explore the martian surface with the help of pressurized rovers that would provide a shirt sleeve environment while protecting them from the deadly extremes of the martian environment. In this image each rover provides transportation and life support for two crew members. By traveling in pairs each rover can provide backup for the other, and if necessary a single rover could serve as refuge and transportation for all four explorers
August 24, 2016: Artist's view of the surface of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the star Proxima. Proxima b is a little more massive than the Earth, orbit in habitable area where the temperature would allow the presence of liquid water on its surface - This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface
Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of Planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the image. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface
August 24, 2016: Artist's view of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible between the planet and the star Proxima. Proxima b is a little more massive than Earth, orbit in habitable area or temperature would allow the presence of liquid water on its surface - This artist's impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface
Martian Base - Illustration
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
Martian surface of fine grained material
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 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.
Martian Landscape: March -Illustration - Martian surface Artwork
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Late winter in the southern hemisphere of Mars showing frost covered sand dunes, 2016
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
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 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 buttes in the distance contain sulfate minerals, perhaps indicating a change in the availability of water when they formed. Some of the layering patterns on higher levels of Mount Sharp in the background are tilted at different angles than others, evidence of complicated relationships still to be deciphered. The scene spans from southeastward at left to southwestward at right. The component images were taken on April 10 and 11, 2015, the 952nd and 953rd Martian days (or sols) since the rover's landing on Mars on Aug. 6, 2012, UTC (Aug. 5, PDT). Images in the central part of the panorama are from Mastcam's right - eye camera, which is equipped with a 100 - millimeter - focal - length telephoto lens. Images used in outer portions, including the most remote portions of the mountain in the scene, were taken with Mastcam's left - eye camera, using a wider - angle, 34 - millimeter lens
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
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
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 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
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 - 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
Snow on Mars - Illustration - Snow at the martian pole: Snow Tempete at the martian pole
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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
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
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 communications
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 degrees east longitude on Mars. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The images were taken throughout the period from the 13th Martian day, or sol, after landing to the 47th sol (June 5 through July 12, 2008)
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 degrees north latitude, 234.25 degrees east longitude on Mars. This view in approximately true color includes more than 100 different Stereo Surface Imager pointings, with images taken through three different filters at each pointing. The images were taken throughout the period from the 13th Martian day, or sol, after landing to the 47th sol (June 5 through July 12, 2008)
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 Abee EH4 enstatite chondrite
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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 smoothness to the curve. This pan captures the polar nature of the Phoenix mission in its similarity to time lapse pictures taken above the Arctic Circle on Earth
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 (about 100 feet by 100 feet). The landing site is at 68.22 degrees north latitude, 234.25 degrees east longitude on Mars. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. This view includes more than 100 different Stereo Surface Imager pointings, with images taken through three different filters at each pointing. The images were taken throughout the period from the 13th Martian day, or sol, after landing to the 47th sol (June 5 through July 12, 2008). The land's Robotic Arm is cut off in this mosaic view because component images were taken when the arm was out of the frame
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 the image. The spacecraft's meteorology mast, topped by the telltale wind gauge, extends into the sky portion of the panorama. 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 cylindrical projection
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
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, 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 spacecraft's meteorology mast, topped by the telltale wind gauge, extends into the sky portion of the panorama. 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 polar projection
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
Parnallee LL3.6 ordinary chondrite
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Mars: Valles Marineris - Illustration - Artist's view of the Martian canyon filled with haze. Artwork showing the great martian canyon filled with fog
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
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 a dozen images taken by the robot on October 6, 2015. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the “” Big Sky”” site, where its drill collected the mission's fifth taste of Mount Sharp. The scene combines dozens of images taken during the 1,126th Martian day, or sol, of Curiosity's work on Mars (Oct. 6, 2015, PDT), by the Mars Hand Lens Imager (MAHLI) camera at the end of the rover's robotic arm. The rock drilled at this site is sandstone in the Stimson geological unit inside Gale Crater. The view is centered toward the west-northwest. It does not include the rover's robotic arm, though the shadow of the arm is visible on the ground. 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. This portrait of the rover was designed to show the Chemistry and Camera (ChemCam) instrument atop the rover appearing level. This causes the horizon to appear to tilt toward the left, but in reality it is fairly flat. For scale, the rod's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide. The drilled hole in the rock, appearing grey near the lower left corner of the image, is 0.63 inch (1.6 centimeters) in diameter
United States, 1990s: View of stars
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The Canyon Diablo meteorite
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The Valles Marineris Canyon, 2005
Life on an exoplanet: View of an alien life artist on the surface of an exoplanet. Extraterrestrial life on an exoplanet
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 on Mars. This high-energy radiation can pass right through the skin, damaging cells or DNA along the way that can mean an increased risk for cancer later in life or, at its worst, acute radiation sickness
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a class F star. Extraterrestrial life on an exoplanet orbiting a F-type star
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a K-type star
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a star of type M1. Extraterrestrial life on an exoplanet orbiting a M1 star
Man, lines of the Nazca people, c.200BC-AD600 (photo)
Viking 1 On Mars
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting an M5 star. Extraterrestrial life on an exoplanet orbiting a M5 star
Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of the surface of the planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface
Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of the surface of the planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a M3 star. Extraterrestrial life on an exoplanet orbiting a M3 flaring star
Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a G-type star. Extraterrestrial life on an exoplanet orbiting a G-type star