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2010 - L'ann¿e du premier contact de Peter Hyams avec Bob Balaban 1984

2010 - L'ann¿e du premier contact de Peter Hyams avec Bob Balaban 1984

XRD1699971

2010 - L'annee du premier contact (L'odyssee continue) de Peter Hyams avec Roy Scheider, Bob Balaban, John Lithgow, 1984

2010 - L'annee du premier contact (L'odyssee continue) de Peter Hyams avec Roy Scheider, Bob Balaban, John Lithgow, 1984

XRD1728614

2010 - L'annee du premier contact (L'odyssee continue) de Peter Hyams avec Roy Scheider 1984

2010 - L'annee du premier contact (L'odyssee continue) de Peter Hyams avec Roy Scheider 1984

XRD1728238

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

PIX4639316

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space

PIX4639328

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

PIX4639389

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Here it lifts a weight of 10 kg. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space. Robonaut2 surpasses previous dexterous humanoid robots in strength, yet it is safe enough to work side-by-side with humans. It is able to lift, not just hold, this 20-pound weight (about four times heavier than what other dexterous robots can handle) both near and away from its body

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Here it lifts a weight of 10 kg. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space. Robonaut2 surpasses previous dexterous humanoid robots in strength, yet it is safe enough to work side-by-side with humans. It is able to lift, not just hold, this 20-pound weight (about four times heavier than what other dexterous robots can handle) both near and away from its body

PIX4639332

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

Robonaut2, the Next Generation Dexterous Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut2 - or R2 for short - is the next generation dexterous robot, developed through a Space Act Agreement by NASA and General Motors. It is faster, more dexterous and more technologically advanced than its predecessors and able to use its hands to do work beyond the scope of previously introduced humanoid robots. Robonauts are designed to use the same tools as humans, which allows them to work safely side-by-side humans on Earth and in space

PIX4639339

Barree spiral galaxy NGC 151 in the Whale - Barred Spiral galaxy NGC 151 in Cetus - Barree spiral galaxy about 160 million years ago - light

Barree spiral galaxy NGC 151 in the Whale - Barred Spiral galaxy NGC 151 in Cetus - Barree spiral galaxy about 160 million years ago - light

Adam Block

PIX4608640

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

PIX4570260

Barree spiral galaxy NGC 7479 in Pegase - Barred spiral galaxy NGC 7479 in Pegasus - Its distance is estimated to be about 105 million light years away

Barree spiral galaxy NGC 7479 in Pegase - Barred spiral galaxy NGC 7479 in Pegasus - Its distance is estimated to be about 105 million light years away

Adam Block

PIX4613178

Robonaut2, the Next Generation Dexterous Robot - Photographer - Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut 2, a dexterous, humanoid astronaut helper, will fly to the International Space Station aboard space shuttle Discovery on the STS-133 mission. Although it will initially only participate in operational tests, upgrades could eventually allow the robot to realize its true purpose - helping spacewalking astronauts with tasks outside the space station

Robonaut2, the Next Generation Dexterous Robot - Photographer - Robonaut 2, designed by Nasa and General Motors, is a humanoid robot designed to assist humans on Earth and in space. Robonaut 2, a dexterous, humanoid astronaut helper, will fly to the International Space Station aboard space shuttle Discovery on the STS-133 mission. Although it will initially only participate in operational tests, upgrades could eventually allow the robot to realize its true purpose - helping spacewalking astronauts with tasks outside the space station

PIX4639348

Super Pit, Gold Mine, Australia (photo)

Super Pit, Gold Mine, Australia (photo)

PIX5973630

Graomys lockwoodi

Graomys lockwoodi

NHM1459405

Phyllotis chacoensis

Phyllotis chacoensis

NHM1459404

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

PIX4604554

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

PIX4604559

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

PIX4604577

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

PIX4604549

Phyllotis cachinus

Phyllotis cachinus

NHM1459406

Graomys edithae

Graomys edithae

NHM1459407

Galaxies NGC 3430 and NGC 3424 in the Little Lion - Galaxies NGC 3430 and NGC 3424 in Leo Minor - Galaxy NGC 3430 (bottom) and NGC 3424 (middle). Image obtained with a telescope 61 cm in diameter. Galaxy NGC 3430 (bottom), and NGC 3424 (middle)

Galaxies NGC 3430 and NGC 3424 in the Little Lion - Galaxies NGC 3430 and NGC 3424 in Leo Minor - Galaxy NGC 3430 (bottom) and NGC 3424 (middle). Image obtained with a telescope 61 cm in diameter. Galaxy NGC 3430 (bottom), and NGC 3424 (middle)

Adam Block

PIX4610706

Image is a nadir camera view of the area around Kruger National Park in northeastern South Africa. Aug. 18, 2010. Satellite image.

Image is a nadir camera view of the area around Kruger National Park in northeastern South Africa. Aug. 18, 2010. Satellite image.

UIG866670

Usher Hall

Usher Hall

Graham Salter

SLR3823829

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. This range of performance covers th

PIX4604568

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

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

PIX4616427

Barree spiral galaxy NGC 7741 in Pegase - Barred Spiral galaxy NGC 7741 in Pegasus - NGC 7741 is a barree spiral galaxy located about 30 million years ago - light in the constellation Pegase. Galaxy NGC 7741 is a barred spiral galaxy of type SB (s) cd, meaning that it has a central bar - like concentration, evident here, and a small number of fairly open large - scale spiral arms. NGC 7741 is quite nearby, and is receding from us at only 1.7 million miles per hour. (Distance: 30 million ly

Barree spiral galaxy NGC 7741 in Pegase - Barred Spiral galaxy NGC 7741 in Pegasus - NGC 7741 is a barree spiral galaxy located about 30 million years ago - light in the constellation Pegase. Galaxy NGC 7741 is a barred spiral galaxy of type SB (s) cd, meaning that it has a central bar - like concentration, evident here, and a small number of fairly open large - scale spiral arms. NGC 7741 is quite nearby, and is receding from us at only 1.7 million miles per hour. (Distance: 30 million ly

Adam Block

PIX4613213

Galaxy NGC 4536 in the Virgin - Galaxy NGC 4536 in Virgo - Spiral galaxy in the Virgin. Spiral galaxy in Virgo

Galaxy NGC 4536 in the Virgin - Galaxy NGC 4536 in Virgo - Spiral galaxy in the Virgin. Spiral galaxy in Virgo

Adam Block

PIX4611506

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

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

S. Corvaja

PIX4640078

Mountain view, 2010

premium — Mountain view, 2010

Mountain view, 2010

Ong, Diana (b.1940)

SSI2252864

Usher Hall

Usher Hall

Graham Salter

SLR3823825

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

UIG866613

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

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

PIX4640069

PING, 2010

premium — PING, 2010

Ong, Diana (b.1940)

SSI2252872

Spiral galaxy NGC 1961 in Giraffe - NGC 1961 spiral galaxy in Camelopardalis - Spiral galaxy NGC 1961 (Arp 184) in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1961 (Arp 184) is a problematic galaxy. Its highly disturbed and asymmetric spiral arms would normally indicate an interaction or merger with another galaxy. However, no culprit is found to be the source of NGC 1961's angst. Given the apparent size and brightness of this galaxy - it must be one of the largest galaxies in our “” local”” universe. The shape of the galaxy may be due to its interaction with the gas in the cluster. Most of this galaxy is still producing young and massive stars that live short lives and die violent deaths as supernovae

Spiral galaxy NGC 1961 in Giraffe - NGC 1961 spiral galaxy in Camelopardalis - Spiral galaxy NGC 1961 (Arp 184) in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1961 (Arp 184) is a problematic galaxy. Its highly disturbed and asymmetric spiral arms would normally indicate an interaction or merger with another galaxy. However, no culprit is found to be the source of NGC 1961's angst. Given the apparent size and brightness of this galaxy - it must be one of the largest galaxies in our “” local”” universe. The shape of the galaxy may be due to its interaction with the gas in the cluster. Most of this galaxy is still producing young and massive stars that live short lives and die violent deaths as supernovae

Adam Block

PIX4609981

Spiral galaxy NGC 5850 in Virgo - Spiral galaxy NGC 5850 in Virgo - Barree spiral galaxy NGC 5850 with right, elliptical galaxy NGC 5846. Barred spiral galaxy NGC 5850 with at right the elliptical galaxy NGC 5846

Spiral galaxy NGC 5850 in Virgo - Spiral galaxy NGC 5850 in Virgo - Barree spiral galaxy NGC 5850 with right, elliptical galaxy NGC 5846. Barred spiral galaxy NGC 5850 with at right the elliptical galaxy NGC 5846

Adam Block

PIX4612792

Galaxy NGC 5701 in the Virgin - Galaxy NGC 5701 in Virgo - Spiral galaxy barree in the Virgin. Barred spiral galaxy in Virgo

Galaxy NGC 5701 in the Virgin - Galaxy NGC 5701 in Virgo - Spiral galaxy barree in the Virgin. Barred spiral galaxy in Virgo

Adam Block

PIX4612768

The lunar orbit - Artist's view - The lunar orbit - Artwork - Inclination of the lunar orbit in relation to the ecliptic. The orbit of the Moon is inclined about 5* from the plane of the Earth's orbit (ecliptic). The lunar orbit around the Earth

The lunar orbit - Artist's view - The lunar orbit - Artwork - Inclination of the lunar orbit in relation to the ecliptic. The orbit of the Moon is inclined about 5* from the plane of the Earth's orbit (ecliptic). The lunar orbit around the Earth

Sebastien Beaucourt

PIX4575998

The Paris Observatory - Coupole Arago - Paris observatory - The Arago dome which houses the large astronomical bezel. Aragon's dome, house of the great refractor

The Paris Observatory - Coupole Arago - Paris observatory - The Arago dome which houses the large astronomical bezel. Aragon's dome, house of the great refractor

Sebastien Beaucourt

PIX4655519

ISS: Tranquility and Cupola - Tranquility and Cupola modules on ISS - The Tranquility module overcomes Cupola, the new observation module of the International Space Station (ISS). 17 February 2010. February 17, 2010

ISS: Tranquility and Cupola - Tranquility and Cupola modules on ISS - The Tranquility module overcomes Cupola, the new observation module of the International Space Station (ISS). 17 February 2010. February 17, 2010

PIX4602747

Barree spiral galaxy NGC 1530 in Giraffe - NGC 1530 spiral galaxy in Camelopardalis - Barree spiral galaxy NGC 1530 in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1530 is a large barred spiral galaxy

Barree spiral galaxy NGC 1530 in Giraffe - NGC 1530 spiral galaxy in Camelopardalis - Barree spiral galaxy NGC 1530 in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1530 is a large barred spiral galaxy

Adam Block

PIX4609892

Galaxy NGC 7217 in Pegase - Galaxy NGC 7217 in Pegasus - The galaxy NGC 7217 is about 40 million years away - light from Earth. Galaxy NGC 7217 located around 40 million light years away in Pegasus

Galaxy NGC 7217 in Pegase - Galaxy NGC 7217 in Pegasus - The galaxy NGC 7217 is about 40 million years away - light from Earth. Galaxy NGC 7217 located around 40 million light years away in Pegasus

Adam Block

PIX4613122

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

Sebastien Beaucourt

PIX4671044

Straight from the Heart, 2010

premium — Straight from the Heart, 2010

Straight from the Heart, 2010

Ong, Diana (b.1940)

SSI2252873

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Image of the core of the Hartley 2 comet seen on November 4, 2010 by the probe Epoxi (Deep Impact) at a distance of 700 km. The core is 2 km long. The image, one of the closest taken of comet Hartley 2 by NASA'S EPOXI mission, shows many features across the comet's surface. There are two obvious regions of jet activity associated with rough terrain. The smooth surface in the middle is lower than the rest of the comet and may accumulate fine - grain dust. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Image of the core of the Hartley 2 comet seen on November 4, 2010 by the probe Epoxi (Deep Impact) at a distance of 700 km. The core is 2 km long. The image, one of the closest taken of comet Hartley 2 by NASA'S EPOXI mission, shows many features across the comet's surface. There are two obvious regions of jet activity associated with rough terrain. The smooth surface in the middle is lower than the rest of the comet and may accumulate fine - grain dust. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

PIX4570280

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained with a telescope 61 cm diameter

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained with a telescope 61 cm diameter

Adam Block

PIX4610143

Granny Smith Gold Mine, Australia, 2010 (photo)

Granny Smith Gold Mine, Australia, 2010 (photo)

PIX6039514

Sunrise Dam Gold Mine, Australia (photo)

Sunrise Dam Gold Mine, Australia (photo)

PIX5973631

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

PIX4624317

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

UIG866630

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

Dramatic changes have been observed at the Eyjafjallajökull volcano in Iceland. On May 2, 2010, lava flow had been previously reported. Satellite image.

UIG866624

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

PIX4565068

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

Exoplanete HD 156668 b: HD 156668 b is an exoplanet orbiting the star HD 156668 has 78.5 light years of Earth, in the constellation of Hercules. With 4.15 times the mass of the Earth, it is, on the date of its discovery in 2010, the second smallest super-earth after Gliese 581 e. HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses

Exoplanete HD 156668 b: HD 156668 b is an exoplanet orbiting the star HD 156668 has 78.5 light years of Earth, in the constellation of Hercules. With 4.15 times the mass of the Earth, it is, on the date of its discovery in 2010, the second smallest super-earth after Gliese 581 e. HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses

Miller, Ron (b.1947)

PIX4608494

Spiral Galaxy M61 in Virgo - Spiral galaxy M61 in Virgo - The spiral galaxy M61 (NGC 4303) is located about 60 million years away - light from Earth. It is one of the largest galaxies in the Virgin's cluster, measuring 100,000 years - light. The SabBC spiral galaxy M61 is one of the larger galaxies in the Virgo cluster, with a dimension some 100 000 light - years (6 arc minutes) across, comparable to the size of our own Galaxy

Spiral Galaxy M61 in Virgo - Spiral galaxy M61 in Virgo - The spiral galaxy M61 (NGC 4303) is located about 60 million years away - light from Earth. It is one of the largest galaxies in the Virgin's cluster, measuring 100,000 years - light. The SabBC spiral galaxy M61 is one of the larger galaxies in the Virgo cluster, with a dimension some 100 000 light - years (6 arc minutes) across, comparable to the size of our own Galaxy

R. Gendler

PIX4611251

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

Sebastien Beaucourt

PIX4671056

snow leopard, 2010,

premium — snow leopard, 2010,

snow leopard, 2010,

Ong, Diana (b.1940)

SSI2252847

Open cluster M6 in Scorpio - Open star cluster M6 in Scorpius - M6 (NGC 6405) is visible to the naked eye in the constellation Scorpio. Its stars are estimated to be between 50 and 100 million years old. The open cluster M6 (NGC 6405) is also called the Butterfly cluster. The open star cluster M6, (NGC 6405), is also known as the Butterfly Cluster. M6 is visible to the naked eye in the constellation Scorpius. M6 is variously estimated as between 50 and 100 million years old

Open cluster M6 in Scorpio - Open star cluster M6 in Scorpius - M6 (NGC 6405) is visible to the naked eye in the constellation Scorpio. Its stars are estimated to be between 50 and 100 million years old. The open cluster M6 (NGC 6405) is also called the Butterfly cluster. The open star cluster M6, (NGC 6405), is also known as the Butterfly Cluster. M6 is visible to the naked eye in the constellation Scorpius. M6 is variously estimated as between 50 and 100 million years old

Stephane Guisard

PIX4568321

Sculptor's Dwarf Galaxy - Sculptor dwarf galaxy - The Sculptor's dwarf galaxy belongs to the local group, just like our galaxy or the Andromede galaxy. The Sculptor dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2

Sculptor's Dwarf Galaxy - Sculptor dwarf galaxy - The Sculptor's dwarf galaxy belongs to the local group, just like our galaxy or the Andromede galaxy. The Sculptor dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2

PIX4613898

The dwarf galaxy of the furnace - Fornax dwarf galaxy - The dwarf galaxy of the furnace belongs to the local group, just like our galaxy or the galaxy of Andromede. The Fornax dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2

The dwarf galaxy of the furnace - Fornax dwarf galaxy - The dwarf galaxy of the furnace belongs to the local group, just like our galaxy or the galaxy of Andromede. The Fornax dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2

PIX4613904

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