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Earth by Artist - Earth by Artist - Earth by Artist

Earth by Artist - Earth by Artist - Earth by Artist

L. Bret

PIX4633200

Map of the southern polar cap of Mars - Map of the southern pole of Mars showing different ice thickness in the basement. Reaching a thickness of 3.7 km, the volume of water ice contained in the basement of the southern Martian pole would reach 1.6 million km3, enough to cover the entire planet under an ocean 11 m deep! This map is based on data obtained by the Marsis radar on the European Mars Express probe.

Map of the southern polar cap of Mars - Map of the southern pole of Mars showing different ice thickness in the basement. Reaching a thickness of 3.7 km, the volume of water ice contained in the basement of the southern Martian pole would reach 1.6 million km3, enough to cover the entire planet under an ocean 11 m deep! This map is based on data obtained by the Marsis radar on the European Mars Express probe.

PIX4616235

Mars - Phobos satellite - Martian moon Phobos - View of the Phobos satellite over the Mars blade obtained by the Mars Express probe on 10 January 2007. An image of Phobos by the High - Resolution Stereo Camera on board Mars Express on 10 January 2007. The larger and inner of the two martian moons is seen here floating just above the martian limb. The image has been enhanced slightly to bring out the detail on the moon

Mars - Phobos satellite - Martian moon Phobos - View of the Phobos satellite over the Mars blade obtained by the Mars Express probe on 10 January 2007. An image of Phobos by the High - Resolution Stereo Camera on board Mars Express on 10 January 2007. The larger and inner of the two martian moons is seen here floating just above the martian limb. The image has been enhanced slightly to bring out the detail on the moon

PIX4616255

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs to the north (top) and to the east (right) s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs on the northern (top) and eastern (right) sides of the image rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amp

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs to the north (top) and to the east (right) s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs on the northern (top) and eastern (right) sides of the image rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amp

PIX4616330

March - Illustration - Mars - Artist's view

March - Illustration - Mars - Artist's view

S. Numazawa

PIX4616729

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

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

PIX4616846

Phobos - Illustration - Phobos - Illustratio

Phobos - Illustration - Phobos - Illustratio

S. Numazawa

PIX4617062

Mars seen by the Hubble Space Telescope - 1997 - Image obtained on March 10, 1997 just before the opposition of Mars when the planet was only 100 million km away from Earth. The image shows the region of Syrtis Major and the north pole

Mars seen by the Hubble Space Telescope - 1997 - Image obtained on March 10, 1997 just before the opposition of Mars when the planet was only 100 million km away from Earth. The image shows the region of Syrtis Major and the north pole

PIX4614946

Mars seen by the Hubble Space Telescope - 2001 - Images obtained by the Hubble Space Telescope on 26 June 2001 (left) during the opposition of Mars when the planet was only 68 million km away from Earth and on 4 September 2001 (right). In June, dust storms were already visible, on the lower right, under Syris Major and north of Mars. On September 4, the whole planet is covered by a gigantic tempete

Mars seen by the Hubble Space Telescope - 2001 - Images obtained by the Hubble Space Telescope on 26 June 2001 (left) during the opposition of Mars when the planet was only 68 million km away from Earth and on 4 September 2001 (right). In June, dust storms were already visible, on the lower right, under Syris Major and north of Mars. On September 4, the whole planet is covered by a gigantic tempete

PIX4614959

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

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

PIX4614968

March - March by Viking probes. Mosaic of about 1000 images. Resolution: 1km/pixe

March - March by Viking probes. Mosaic of about 1000 images. Resolution: 1km/pixe

PIX4615093

Mars - Hellas Basin - Mosaic of images obtained by the Viking probe 1. To the north, the large clear circular region is Arabia. Below, the white spot represents the Hellas Basin, an impact crater of 2000 km in diameter and 6 km deep covered with carbon dioxide gele

Mars - Hellas Basin - Mosaic of images obtained by the Viking probe 1. To the north, the large clear circular region is Arabia. Below, the white spot represents the Hellas Basin, an impact crater of 2000 km in diameter and 6 km deep covered with carbon dioxide gele

PIX4615133

Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons

Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons

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March: 1st photo of the surface - 1st photo of the surface of Mars obtained by the Viking 1 probe on 20 July 1976

March: 1st photo of the surface - 1st photo of the surface of Mars obtained by the Viking 1 probe on 20 July 1976

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March - Dust Tempete. - Dust Tempete and North Martian pole seen by the Mars Global Surveyor probe in May 2002

March - Dust Tempete. - Dust Tempete and North Martian pole seen by the Mars Global Surveyor probe in May 2002

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Detail of the southern polar cap of Mars. - The region photographed here by the Mars Global Surveyor probe on 23 February 2000 measures 2.9 km by 4.8 km The southern polar cap seen here in the middle of the southern summer is mostly composed of carbon dioxide gele. It extends for about 400 km

Detail of the southern polar cap of Mars. - The region photographed here by the Mars Global Surveyor probe on 23 February 2000 measures 2.9 km by 4.8 km The southern polar cap seen here in the middle of the southern summer is mostly composed of carbon dioxide gele. It extends for about 400 km

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Mars Pathfinder Probe - Rover Sojourner before deployment - Mars Pathfinder landed on Mars in the Ares Vallis region, July 4, 1997

Mars Pathfinder Probe - Rover Sojourner before deployment - Mars Pathfinder landed on Mars in the Ares Vallis region, July 4, 1997

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Mars Pathfinder Probe - Rover Sojourner - Mosaic of images showing the Mars Pathfinder probe in the foreground, the Sojourner rover and in the distance, Twin Peaks. Mars Pathfinder landed on Mars in the Ares Vallis region on July 4, 1997

Mars Pathfinder Probe - Rover Sojourner - Mosaic of images showing the Mars Pathfinder probe in the foreground, the Sojourner rover and in the distance, Twin Peaks. Mars Pathfinder landed on Mars in the Ares Vallis region on July 4, 1997

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Mars seen by the Rosetta probe on 24/02/2007 - Image obtained by the Rosetta probe on 24 February 2007, at a distance of 240,000 km from Mars. The image shows the region of Elysium and the southern pole of the planet

Mars seen by the Rosetta probe on 24/02/2007 - Image obtained by the Rosetta probe on 24 February 2007, at a distance of 240,000 km from Mars. The image shows the region of Elysium and the southern pole of the planet

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Twin Peaks hills seen by the Mars Pathfinder probe. - Mosaic images showing the Twin Peaks hills. These hills are about 30 - 35 m high; these two peaks are approximately 860m and 1 km from the Mars Pathfinder probe. Mars Pathfinder landed on Mars in the Ares Vallis region on July 4, 1997

Twin Peaks hills seen by the Mars Pathfinder probe. - Mosaic images showing the Twin Peaks hills. These hills are about 30 - 35 m high; these two peaks are approximately 860m and 1 km from the Mars Pathfinder probe. Mars Pathfinder landed on Mars in the Ares Vallis region on July 4, 1997

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Mars: Hills east of the Spirit landing site. - Detail of the 360 degres panorama obtained by Spirit at its landing site. This row of hills is located 2 - 3 km from the probe. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

Mars: Hills east of the Spirit landing site. - Detail of the 360 degres panorama obtained by Spirit at its landing site. This row of hills is located 2 - 3 km from the probe. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

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March: Surface seen by Spirit. - Detail of the panorama obtained by Spirit between 3 and 5 March 2004 when the rover was halfway between its landing site and the Bonnevile crater. In the distance the Columbia Hills. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

March: Surface seen by Spirit. - Detail of the panorama obtained by Spirit between 3 and 5 March 2004 when the rover was halfway between its landing site and the Bonnevile crater. In the distance the Columbia Hills. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

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March: traces left by the Spirit rover. - Panorama obtained by Spirit on 21, 25 and 26 May 2004. The rover was about 600m from the Columbia Hills and had crossed 3/4 of the distance between the Bonneville crater and the hills. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

March: traces left by the Spirit rover. - Panorama obtained by Spirit on 21, 25 and 26 May 2004. The rover was about 600m from the Columbia Hills and had crossed 3/4 of the distance between the Bonneville crater and the hills. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

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March - Spirit - Panorama McMurdo - Detail - 10 - 2006 - March: McMurdo panorama - Spirit - Detail 10 - 2006 - Detail of the panorama “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. “McMurdo” panorama detail. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “Winter Haven”” is presented in approximately true color

March - Spirit - Panorama McMurdo - Detail - 10 - 2006 - March: McMurdo panorama - Spirit - Detail 10 - 2006 - Detail of the panorama “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. “McMurdo” panorama detail. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “Winter Haven”” is presented in approximately true color

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March - Spirit - Panorama McMurdo - Detail - 10 - 2006 - March: McMurdo panorama - Spirit - Detail - 10 - 2006 - Detail of the panorama “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. “McMurdo” panorama detail. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “Winter Haven”” is presented in approximately true color

March - Spirit - Panorama McMurdo - Detail - 10 - 2006 - March: McMurdo panorama - Spirit - Detail - 10 - 2006 - Detail of the panorama “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. “McMurdo” panorama detail. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “Winter Haven”” is presented in approximately true color

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March - Opportunity - Landing site - Challenger memorial station photography by the rover Opportunity around February 20, 2004. The probe landed in a 20-metre-wide impact crater named Eagle. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

March - Opportunity - Landing site - Challenger memorial station photography by the rover Opportunity around February 20, 2004. The probe landed in a 20-metre-wide impact crater named Eagle. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

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March - Opportunity - Landing site - Panorama of 180 degrees obtained by Opportunity from its landing site. 558 images obtained at the end of March 2004 were assembled. The probe landed in a 20-metre-wide impact crater named Eagle. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

March - Opportunity - Landing site - Panorama of 180 degrees obtained by Opportunity from its landing site. 558 images obtained at the end of March 2004 were assembled. The probe landed in a 20-metre-wide impact crater named Eagle. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

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Mars - Opportunity - Shield Wreck - View of impact crater with a diameter of approx. 3 meters due to the fall of the probe thermal shield. On the left, the rest of the thermal shield (1.3m high by 2.5m in diameter) that protected the rentree of the probe in the atmosphere of Mars. Mosaic of images obtained on 28 December 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

Mars - Opportunity - Shield Wreck - View of impact crater with a diameter of approx. 3 meters due to the fall of the probe thermal shield. On the left, the rest of the thermal shield (1.3m high by 2.5m in diameter) that protected the rentree of the probe in the atmosphere of Mars. Mosaic of images obtained on 28 December 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region, January 25, 2004

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March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

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March: Albor Tholus volcano summit seen in perspective. - This volcano in the region of Elysium has a diameter of 160 km and stands at 4500m. Its caldera seen here measures 30 km in diameter and a depth of 3000m. Image obtained by the Mars Express probe on January 19, 2004

March: Albor Tholus volcano summit seen in perspective. - This volcano in the region of Elysium has a diameter of 160 km and stands at 4500m. Its caldera seen here measures 30 km in diameter and a depth of 3000m. Image obtained by the Mars Express probe on January 19, 2004

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March: Ice in an impact crater - View of an unnamed impact crater located in Vastitas Borealis, a region near the north pole of Mars.. This crater measures 35 km in diameter and is 2000m deep. In the centre, an accumulation of water ice; ice is also visible on the walls of the crater. Image obtained by the Mars Express probe on February 2, 2005

March: Ice in an impact crater - View of an unnamed impact crater located in Vastitas Borealis, a region near the north pole of Mars.. This crater measures 35 km in diameter and is 2000m deep. In the centre, an accumulation of water ice; ice is also visible on the walls of the crater. Image obtained by the Mars Express probe on February 2, 2005

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March: Impact crater and dunes - View of a 12 km by 7 km dune field at the bottom of an impact crater located in Argyre Planitia. The sand is dark and probably of basaltic origin. This crater is 45 km in diameter and is 2000m deep. Image obtained by the Mars Express probe on May 22, 2004

March: Impact crater and dunes - View of a 12 km by 7 km dune field at the bottom of an impact crater located in Argyre Planitia. The sand is dark and probably of basaltic origin. This crater is 45 km in diameter and is 2000m deep. Image obtained by the Mars Express probe on May 22, 2004

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Mars - Phobos satellite - Martian moon Phobos - View of the Phobos satellite above the Mars blade obtained by the Mars Express probe on 22 January 2007. An image of Phobos by the High - Resolution Stereo Camera on board Mars Express on 22 January 2007. The larger and inner of the two martian moons is seen here floating just above the martian limb. The image has been enhanced slightly to bring out the detail on the moon

Mars - Phobos satellite - Martian moon Phobos - View of the Phobos satellite above the Mars blade obtained by the Mars Express probe on 22 January 2007. An image of Phobos by the High - Resolution Stereo Camera on board Mars Express on 22 January 2007. The larger and inner of the two martian moons is seen here floating just above the martian limb. The image has been enhanced slightly to bring out the detail on the moon

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The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. Backdropped by the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. Backdropped by the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

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International Space Station: the European Columbus module - The International Space Station: the Columbus laboratory - Detail of the International Space Station with its new element, the European Columbus Laboratory (right) connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

International Space Station: the European Columbus module - The International Space Station: the Columbus laboratory - Detail of the International Space Station with its new element, the European Columbus Laboratory (right) connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

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The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

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Life aboard the International Space Station - Astronauts in the International Space Station - Astronaut Robert L. Behnken manipulates the articulated arm of the International Space Station from the Destiny module, observed by astronaut Leopold Eyharts. 15 March 2008. (15 March 2008) - - - NASA Astronaut Robert L. Behnken (right), STS - 123 mission specialist, works the controls of the space station's robotic Canadarm2 in the Destiny laboratory of the International Space Station while Space Shuttle Endeavour is docked with the station. European Space Agency (ESA) astronaut Leopold Eyharts, mission specialist, looks on

Life aboard the International Space Station - Astronauts in the International Space Station - Astronaut Robert L. Behnken manipulates the articulated arm of the International Space Station from the Destiny module, observed by astronaut Leopold Eyharts. 15 March 2008. (15 March 2008) - - - NASA Astronaut Robert L. Behnken (right), STS - 123 mission specialist, works the controls of the space station's robotic Canadarm2 in the Destiny laboratory of the International Space Station while Space Shuttle Endeavour is docked with the station. European Space Agency (ESA) astronaut Leopold Eyharts, mission specialist, looks on

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The International Space Station (ISS) 03/2008 - The International Space Station 03/2008 - View of the International Space Station after the start of the shuttle Endeavour on March 24, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station appears small from the point of view of the Space Shuttle Endeavour as the two spacecraft carry out their relative separation. Endeavour's vertical stabilizer is seen in this image photographed by a STS - 123 crewmember onboard the shuttle. Earlier the STS - 123 and Expedition 16 crews concluded 12 days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 7:25 p.m. (CDT) on March 24, 2008

The International Space Station (ISS) 03/2008 - The International Space Station 03/2008 - View of the International Space Station after the start of the shuttle Endeavour on March 24, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station appears small from the point of view of the Space Shuttle Endeavour as the two spacecraft carry out their relative separation. Endeavour's vertical stabilizer is seen in this image photographed by a STS - 123 crewmember onboard the shuttle. Earlier the STS - 123 and Expedition 16 crews concluded 12 days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 7:25 p.m. (CDT) on March 24, 2008

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Centaur Omega globular cluster - NGC 5139, Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the ACS camera of the Hubble space telescope and observations made by the southern Gemini telescope seem to indicate the presence of a black hole in the center of the cluster. NGC 5139 is the largest and most spectacular globular cluster in the entire night sky, and the largest in our galaxy. At 36 arc minutes, Omega Centauri is larger than the full moon in apparent size. It is located about 17,000 light years away from our Sun and at 4th magnitude, is easily visible without a telescope as a “” star”” in the constellation of Centaurus. It contains about 2 million stars, almost twice as many as M13. This composite image obtained with the Advanced Camera for Surveys onboard

Centaur Omega globular cluster - NGC 5139, Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the ACS camera of the Hubble space telescope and observations made by the southern Gemini telescope seem to indicate the presence of a black hole in the center of the cluster. NGC 5139 is the largest and most spectacular globular cluster in the entire night sky, and the largest in our galaxy. At 36 arc minutes, Omega Centauri is larger than the full moon in apparent size. It is located about 17,000 light years away from our Sun and at 4th magnitude, is easily visible without a telescope as a “” star”” in the constellation of Centaurus. It contains about 2 million stars, almost twice as many as M13. This composite image obtained with the Advanced Camera for Surveys onboard

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Jupiter and Io seen by the New Horizons probe

Jupiter and Io seen by the New Horizons probe

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Surface of Europe, one of Jupiter's satellites. Illustration - Europa surface. Illustration - Artist's view of the ice surface of the Europe satellite. In the sky, satellite Io and Jupiter. Artwork showing the icy surface of Europa, a jovian moon. In the sky, the satellite Io and Jupiter

Surface of Europe, one of Jupiter's satellites. Illustration - Europa surface. Illustration - Artist's view of the ice surface of the Europe satellite. In the sky, satellite Io and Jupiter. Artwork showing the icy surface of Europa, a jovian moon. In the sky, the satellite Io and Jupiter

P. Carril

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Expedition to Europe, one of Jupiter's satellites. Illustration - Europa mission. Illustration - View of astronaut artist evoluting on the icy surface of the Europe satellite. In the sky, satellite Io and Jupiter. Artwork showing a manned mission on the icy surface of Europa, a jovian moon. In the sky, the satellite Io and Jupiter

Expedition to Europe, one of Jupiter's satellites. Illustration - Europa mission. Illustration - View of astronaut artist evoluting on the icy surface of the Europe satellite. In the sky, satellite Io and Jupiter. Artwork showing a manned mission on the icy surface of Europa, a jovian moon. In the sky, the satellite Io and Jupiter

P. Carril

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Jupiter seen by the Hubble Space Telescope - 02 - 2007 - Visible view of Jupiter obtained on 17 February 2007 by the Hubble Space Telescope

Jupiter seen by the Hubble Space Telescope - 02 - 2007 - Visible view of Jupiter obtained on 17 February 2007 by the Hubble Space Telescope

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Jupiter and satellites seen from Mars by the MRO probe - View of Jupiter and its Galilean satellites obtained on 11 January 2007 by the Mars Reconnaissance Orbiter probe (MRO) from the Mars orbit

Jupiter and satellites seen from Mars by the MRO probe - View of Jupiter and its Galilean satellites obtained on 11 January 2007 by the Mars Reconnaissance Orbiter probe (MRO) from the Mars orbit

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Jupiter and Galilean satellites - Photomontage - Voyager 1 - Mounting representing the Jupiter planet accompanied by its four main satellites, Io, Europe, Callisto, Ganymede

Jupiter and Galilean satellites - Photomontage - Voyager 1 - Mounting representing the Jupiter planet accompanied by its four main satellites, Io, Europe, Callisto, Ganymede

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Io seen by the probe Voyager 1 - Region of the south pole - At the bottom of the image Haemus Mons, not far from the southern pole of Io, is one of the largest mountains in the solar system. It extends 200 km in diameter and is more than 10 000m; it is completely covered with sulfur frost. Mosaic of images obtained by the Voyager 1 probe

Io seen by the probe Voyager 1 - Region of the south pole - At the bottom of the image Haemus Mons, not far from the southern pole of Io, is one of the largest mountains in the solar system. It extends 200 km in diameter and is more than 10 000m; it is completely covered with sulfur frost. Mosaic of images obtained by the Voyager 1 probe

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Large red spot of Jupiter seen by Voyager 2 - 03 - 07 - 1979 - Large red spot of Jupiter seen by Voyager 2 - 03 - 07 - 1979 - The red spot of Jupiter seen by the Voyager 2 probe on July 3, 1979 has a distance of 6 million km from the planet. The Jupiter Red Spot is a gigantic tempete measuring nearly 25,000 km in diameter, about twice the diameter of the Earth.

Large red spot of Jupiter seen by Voyager 2 - 03 - 07 - 1979 - Large red spot of Jupiter seen by Voyager 2 - 03 - 07 - 1979 - The red spot of Jupiter seen by the Voyager 2 probe on July 3, 1979 has a distance of 6 million km from the planet. The Jupiter Red Spot is a gigantic tempete measuring nearly 25,000 km in diameter, about twice the diameter of the Earth.

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Planisphere de Io - False colors - Planisphere of 11,420 km wide made from images obtained by the Galileo probe between July and September 1996 has distances between 485,000 and 2,243,000 kilometres from the satellite. The overlaid grid corresponds to longitude and latitude intervals of 30 degrees

Planisphere de Io - False colors - Planisphere of 11,420 km wide made from images obtained by the Galileo probe between July and September 1996 has distances between 485,000 and 2,243,000 kilometres from the satellite. The overlaid grid corresponds to longitude and latitude intervals of 30 degrees

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Jupiter and Io by Cassini probe - Hemisphere south of Jupiter seen by the Cassini probe on 12 December 2000 at a distance of 19.5 million km. In front of the planet, one of Jupiter's satellites, Io and its shadow projected on the planet

Jupiter and Io by Cassini probe - Hemisphere south of Jupiter seen by the Cassini probe on 12 December 2000 at a distance of 19.5 million km. In front of the planet, one of Jupiter's satellites, Io and its shadow projected on the planet

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Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

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Astronauts in Destiny STS - 105 08/01 - James S. Voss (a d.) and Scott J. Horowitz, weightlessly in the airlock leading to the Unity module. ISS STS - 105. 17/08/2001

Astronauts in Destiny STS - 105 08/01 - James S. Voss (a d.) and Scott J. Horowitz, weightlessly in the airlock leading to the Unity module. ISS STS - 105. 17/08/2001

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Crew STS - 105 in Destiny 08/01 - Photo of crew STS - 105 in Destiny module. Clockwise, bottom left: Scott Horowitz, Frederick (Rick) Sturckow, Patrick Forrester and Daniel Barry. ISS STS - 105. 17/08/2001

Crew STS - 105 in Destiny 08/01 - Photo of crew STS - 105 in Destiny module. Clockwise, bottom left: Scott Horowitz, Frederick (Rick) Sturckow, Patrick Forrester and Daniel Barry. ISS STS - 105. 17/08/2001

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Meals in Zvezda 08/01 - Meals in Zvezda. Around the table, clockwise, from the bottom: Scott Horowitz, Daniel Barry, Frederick (Rick) Sturckow, Vladimir Dezhurov, Susan J. Helms, Patrick Forrester and Yury Usachev. At the bottom of g. a. d.: Mikhail Tyurin, Frank Culbertson, and James Voss. ISS STS - 105. 15/08/2001

Meals in Zvezda 08/01 - Meals in Zvezda. Around the table, clockwise, from the bottom: Scott Horowitz, Daniel Barry, Frederick (Rick) Sturckow, Vladimir Dezhurov, Susan J. Helms, Patrick Forrester and Yury Usachev. At the bottom of g. a. d.: Mikhail Tyurin, Frank Culbertson, and James Voss. ISS STS - 105. 15/08/2001

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Russian Mooring Module Pirs 09/01 - Russian Mooring Module Pirs seen from the International Space Station on 16/09/2001

Russian Mooring Module Pirs 09/01 - Russian Mooring Module Pirs seen from the International Space Station on 16/09/2001

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ISS 12/01 - The international space station after stowage seen from the shuttle Endeavour. ISS STS-108. Dec 2001

ISS 12/01 - The international space station after stowage seen from the shuttle Endeavour. ISS STS-108. Dec 2001

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ISS 12/01 - ISS 12/01 - The international space station after stowage from the shuttle Endeavour. ISS STS - 108. 15 Dec 2001

ISS 12/01 - ISS 12/01 - The international space station after stowage from the shuttle Endeavour. ISS STS - 108. 15 Dec 2001

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ITS S0 Segment 04/02 - The ITS S0 (S - Zero) central segment extracted from the cargo compartment of the shuttle Atlantis. ISS STS - 110. 11/O4/2002

ITS S0 Segment 04/02 - The ITS S0 (S - Zero) central segment extracted from the cargo compartment of the shuttle Atlantis. ISS STS - 110. 11/O4/2002

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ITS S0 Centre Segment 04/02 - ITS S0 (S - Zero) Central Segment extracted from the cargo compartment of Shuttle Atlantis. ISS STS - 110. 11/O4/2002

ITS S0 Centre Segment 04/02 - ITS S0 (S - Zero) Central Segment extracted from the cargo compartment of Shuttle Atlantis. ISS STS - 110. 11/O4/2002

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Release of L. Morin 04/02 - Lee M.E. Morin carries one of the elements of the ITS S0 segment. ISS STS - 110. 13/04/2002

Release of L. Morin 04/02 - Lee M.E. Morin carries one of the elements of the ITS S0 segment. ISS STS - 110. 13/04/2002

PIX4600752

ISS 04/02 - The international space station after stowage from the shuttle Atlantis. ISS STS - 110. 17/04/2002

ISS 04/02 - The international space station after stowage from the shuttle Atlantis. ISS STS - 110. 17/04/2002

PIX4600761

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