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Images of 'NASA' found, 1,650

 
The International Space Station 02/2001 - The International Space Station (ISS) 02/2001 - The Space Station over Chile. ISS STS - 98. 16/02/2001. The International Space Station is backdropped over clouds, water and land in South America. South central Chile shows up at bottom of the frame. Just below the Destiny laboratory, the Chacao Channel separates the large island of Chiloe from the mainland and connects the Gulf of Coronados on the Pacific side with the Gulf of Ancud southwest of the city of Puerto Montt. The crews of the Space Shuttle Atlantis and the International Space Station parted company at 8:06 a.m. (CST), February 16, as astronaut Mark L. Polansky, pilot, flew the shuttle halfway around the station and its new Destiny laboratory before moving off. Feb 16 2001

PIX4600213

The International Space Station 02/2001 - The International Space Station (ISS) 02/2001 - The Space Station over Chile. ISS STS - 98. 16/02/2001. The International Space Station is backdropped over clouds, water and land in South America. South central Chile shows up at bottom of the frame. Just below the Destiny laboratory, the Chacao Channel separates the large island of Chiloe from the mainland and connects the Gulf of Coronados on the Pacific side with the Gulf of Ancud southwest of the city of Puerto Montt. The crews of the Space Shuttle Atlantis and the International Space Station parted company at 8:06 a.m. (CST), February 16, as astronaut Mark L. Polansky, pilot, flew the shuttle halfway around the station and its new Destiny laboratory before moving off. Feb 16 2001

PIX4600213

 
The International Space Station 02/2001 - The International Space Station (ISS) 02/2001 - The Space Station seen from the Atlantis Shuttle. ISS STS - 98. 16/02/2001. The International Space Station (ISS) is backdropped against the blackness of space in this medium - distance, 70 mm frame, as photographed from the departing Space Shuttle Atlantis. The newly installed Destiny laboratory is in the left foreground. The crews of the Space Shuttle Atlantis and the International Space Station parted company at 8:06 a.m. (CST), February 16, as astronaut Mark L. Polansky, pilot, flew the shuttle halfway around the station and its new Destiny laboratory before moving off. Feb 16 2001

PIX4600219

The International Space Station 02/2001 - The International Space Station (ISS) 02/2001 - The Space Station seen from the Atlantis Shuttle. ISS STS - 98. 16/02/2001. The International Space Station (ISS) is backdropped against the blackness of space in this medium - distance, 70 mm frame, as photographed from the departing Space Shuttle Atlantis. The newly installed Destiny laboratory is in the left foreground. The crews of the Space Shuttle Atlantis and the International Space Station parted company at 8:06 a.m. (CST), February 16, as astronaut Mark L. Polansky, pilot, flew the shuttle halfway around the station and its new Destiny laboratory before moving off. Feb 16 2001

PIX4600219

 
Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was

PIX4623390

Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was

PIX4623390

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

PIX4640020

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

PIX4640020

 
Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

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Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

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Mir Station 03/1996 - Mir Space Station 03/1996 - Mir Space Station seen above New Zealand from the Atlantis Shuttle before its mooring. 23/03/1996. Backdropped against the waters of Cook Strait near New Zealand's South Island, Russia's Mir Space Station is seen from the aft flight deck window of the Space Shuttle Atlantis. The two spacecraft were in the process of making their third docking in Earth - orbit. With the subsequent delivery of astronaut Shannon W. Lucid to the Mir, the Mir - 21 crew grew to three, as the mission specialist quickly becomes a cosmonaut guest researcher. She will spend approximately 140 days on Mir before returning to Earth. Tue 23 1996

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Mir Station 03/1996 - Mir Space Station 03/1996 - Mir Space Station seen above New Zealand from the Atlantis Shuttle before its mooring. 23/03/1996. Backdropped against the waters of Cook Strait near New Zealand's South Island, Russia's Mir Space Station is seen from the aft flight deck window of the Space Shuttle Atlantis. The two spacecraft were in the process of making their third docking in Earth - orbit. With the subsequent delivery of astronaut Shannon W. Lucid to the Mir, the Mir - 21 crew grew to three, as the mission specialist quickly becomes a cosmonaut guest researcher. She will spend approximately 140 days on Mir before returning to Earth. Tue 23 1996

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Skylab Station - 06/1973 - Skylab Station seen from Skylab Module - 2 before returning to Earth. An overhead view of the Skylab 1 space station cluster in Earth orbit photographed from the Skylab 2 Command/Service Module during the final “” fly around”” inspection by the CSM. The space station is sharply contrasted against a black sky background. Note the deployed parasol solar shield which shades the Orbital Workshop where the micrometeoroid shield is missing. The one remaining OWS solar array system wing has been fully deployed successfully. The OWS solar panel on the opposite side is missing completely. 22 June 197

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Skylab Station - 06/1973 - Skylab Station seen from Skylab Module - 2 before returning to Earth. An overhead view of the Skylab 1 space station cluster in Earth orbit photographed from the Skylab 2 Command/Service Module during the final “” fly around”” inspection by the CSM. The space station is sharply contrasted against a black sky background. Note the deployed parasol solar shield which shades the Orbital Workshop where the micrometeoroid shield is missing. The one remaining OWS solar array system wing has been fully deployed successfully. The OWS solar panel on the opposite side is missing completely. 22 June 197

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Skylab station 07/1973 - Skylab station seen from Skylab module - 3 just before mooring. 28/07/1973. The Skylab space station photographed from the Skylab 3 Command/Service Module during station keeping maneuvers prior to docking. Aboard the command module were astronauts Alan Bean, Owen Garriott and Jack Lousma, who remained with the Skylab space station in Earth's orbit for 59 days. Note the one solar array system wing on the Orbital Workshop (OWS) which was successfully deployed during extravehicular activity (EVA) on the first manned Skylab flight. The parasol solar shield which was deployed by the Skylab 2 crew can be seen through the support struts of the Apollo Telescope Mount. Jul 28 1973

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Skylab station 07/1973 - Skylab station seen from Skylab module - 3 just before mooring. 28/07/1973. The Skylab space station photographed from the Skylab 3 Command/Service Module during station keeping maneuvers prior to docking. Aboard the command module were astronauts Alan Bean, Owen Garriott and Jack Lousma, who remained with the Skylab space station in Earth's orbit for 59 days. Note the one solar array system wing on the Orbital Workshop (OWS) which was successfully deployed during extravehicular activity (EVA) on the first manned Skylab flight. The parasol solar shield which was deployed by the Skylab 2 crew can be seen through the support struts of the Apollo Telescope Mount. Jul 28 1973

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B.Mac Candless Extra Vehicle Release STS - 41 - B - 02/1984 - Astronaut Bruce McCandless II EVA 02/1984 - Astronaut Bruce McCandless II, works in the cargo bay of the Shuttle Challenger. 11/02/1984. Astronaut Bruce McCandless, II, is using a special tool to conduct an experiment. His feet are anchored in the mobile foot restraints, which are connected to the remote manipulator system (RMS). The Shuttle pallet satellite (SPAS-01A) serves as a test subject for McCandless's experiment. Feb 11 1984

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B.Mac Candless Extra Vehicle Release STS - 41 - B - 02/1984 - Astronaut Bruce McCandless II EVA 02/1984 - Astronaut Bruce McCandless II, works in the cargo bay of the Shuttle Challenger. 11/02/1984. Astronaut Bruce McCandless, II, is using a special tool to conduct an experiment. His feet are anchored in the mobile foot restraints, which are connected to the remote manipulator system (RMS). The Shuttle pallet satellite (SPAS-01A) serves as a test subject for McCandless's experiment. Feb 11 1984

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Extra Release - Vehicle B.Mac Candless STS - 41 - B - 02/1984 - B.Mac Candless space walk. 02/1984 - Astronaut Bruce McCandless, II uses his hands to control his movements in space while using the MMU (Manned Maneuvering Unit), a standalone space chair allowing him to move away from the Challenger Space Shuttle by several meters without being connected. 11 - 02 - 1984. Astronaut Bruce McCandless, II, mission specialist, uses his hands to control his movement in space while using the nitrogen propelled manned maneuvering unit (MMU). He is participating in a extravehicular activity (EVA), a few meters away from the cabin of the shuttle Challenger. He is floating without tethers attaching him to the shuttle. Feb 11 1984

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Extra Release - Vehicle B.Mac Candless STS - 41 - B - 02/1984 - B.Mac Candless space walk. 02/1984 - Astronaut Bruce McCandless, II uses his hands to control his movements in space while using the MMU (Manned Maneuvering Unit), a standalone space chair allowing him to move away from the Challenger Space Shuttle by several meters without being connected. 11 - 02 - 1984. Astronaut Bruce McCandless, II, mission specialist, uses his hands to control his movement in space while using the nitrogen propelled manned maneuvering unit (MMU). He is participating in a extravehicular activity (EVA), a few meters away from the cabin of the shuttle Challenger. He is floating without tethers attaching him to the shuttle. Feb 11 1984

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Extra-vehicle exit J. Ross STS61B 12/1985 - Extra-vehicle exit J. Ross STS61B 12/1985 - Extra-vehicle exit of astronaut Jerry L. Ross, fixed on the arm of the shuttle. He approaches ACCESS (Assembly Concept for Construction of Eable Space Structures) an experiment to test the assembly of structures in space. 01/12/1985. Astronaut Jerry L. Ross, anchored to the foot restraint on the remote manipulator system (RMS), approaches the tower - like Assembly Concept for Construction of Ecrectable Space Structures (ACCESS) device. Dec 01 1985

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Extra-vehicle exit J. Ross STS61B 12/1985 - Extra-vehicle exit J. Ross STS61B 12/1985 - Extra-vehicle exit of astronaut Jerry L. Ross, fixed on the arm of the shuttle. He approaches ACCESS (Assembly Concept for Construction of Eable Space Structures) an experiment to test the assembly of structures in space. 01/12/1985. Astronaut Jerry L. Ross, anchored to the foot restraint on the remote manipulator system (RMS), approaches the tower - like Assembly Concept for Construction of Ecrectable Space Structures (ACCESS) device. Dec 01 1985

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Mount Everest - Nepal - seen by Apollo 7 - Mount Everest - Nepal - seen by Apollo 7 - Part of the Himalayan chain with Mount Everest (below, in the center), the K - 2, as well as a dozen peaks over 8000m are visible in this photo obtained by the crew of Apollo 7 in October 1968. At the bottom of the picture, on the right, Mount Kanchenjunga, culminating at 8586m, marks the border between India and Nepal. At the top right, the lakes of the Tibetan plateau. The Mount Everest (29,028 ft) is at lower center and the K - 2 (28,250 ft) on the central horizon photographed from the Apollo 7 spacecraft. In the lower right, Mount Kanchenjunga rises 28,208 ft. to separate Nepal from India. In the upper right the lake - studded highlands of Tibet are visible. Nepal, October 1968

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Mount Everest - Nepal - seen by Apollo 7 - Mount Everest - Nepal - seen by Apollo 7 - Part of the Himalayan chain with Mount Everest (below, in the center), the K - 2, as well as a dozen peaks over 8000m are visible in this photo obtained by the crew of Apollo 7 in October 1968. At the bottom of the picture, on the right, Mount Kanchenjunga, culminating at 8586m, marks the border between India and Nepal. At the top right, the lakes of the Tibetan plateau. The Mount Everest (29,028 ft) is at lower center and the K - 2 (28,250 ft) on the central horizon photographed from the Apollo 7 spacecraft. In the lower right, Mount Kanchenjunga rises 28,208 ft. to separate Nepal from India. In the upper right the lake - studded highlands of Tibet are visible. Nepal, October 1968

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Tibet Plateau seen by Space Shuttle - The Tibetan plateau from space - South-eastern part of the Tibet Plateau, seen from Space Shuttle Columbia on October 20, 1993. Lower left is Lake Namco, the highest dirty lake in the world. The southeast portion of the high Tibetan Plateau, called the Northern Plain by the Chinese, is seen in this southwest - looking, high - oblique photograph taken by astronauts in the space shuttle Columbia in october 1993. Many great rivers originate in the Tibetan Plateau - - Indus, Brahmaputra, Sutlej, Salween, Mekong, Yangtze, and Yellow. The plateau has no river system; however, it has numerous brackish lakes, some of which are visible in this photograph. Saline Namco Lake (southeast corner of photograph), the largest lake in Tibet, covers 950 square miles (2461 square kilometers) and sits at an altitude of 15 180 feet (4630 meters)

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Tibet Plateau seen by Space Shuttle - The Tibetan plateau from space - South-eastern part of the Tibet Plateau, seen from Space Shuttle Columbia on October 20, 1993. Lower left is Lake Namco, the highest dirty lake in the world. The southeast portion of the high Tibetan Plateau, called the Northern Plain by the Chinese, is seen in this southwest - looking, high - oblique photograph taken by astronauts in the space shuttle Columbia in october 1993. Many great rivers originate in the Tibetan Plateau - - Indus, Brahmaputra, Sutlej, Salween, Mekong, Yangtze, and Yellow. The plateau has no river system; however, it has numerous brackish lakes, some of which are visible in this photograph. Saline Namco Lake (southeast corner of photograph), the largest lake in Tibet, covers 950 square miles (2461 square kilometers) and sits at an altitude of 15 180 feet (4630 meters)

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Lake Chad seen by shuttle 12/93 - Lake Chad seen by shuttle STS - 61 on 03/12/1993

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Lake Chad seen by shuttle 12/93 - Lake Chad seen by shuttle STS - 61 on 03/12/1993

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Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997

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Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997

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Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997

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Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997

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Intelsat satellite 6 - Intelsat VI satellite - Recoveration of the Intelsat VI satellite by shuttle Endeavour in May 1992. From left to right are astronauts Richard J. Hieb, Thomas D. Akers, and Pierre J. Thuot. Three STS - 49 crewmembers hold onto the 4.5 - ton Intelsat VI satellite in May 1992 after a six - handed “” capture””” was made minutes earlier. Left to right are astronauts Richard J. Hieb, Thomas D. Akers and Pierre J. Thuot. Thuot stands on the end of the Canadarm, which was instrumental as a mobile working platform in the capture

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Intelsat satellite 6 - Intelsat VI satellite - Recoveration of the Intelsat VI satellite by shuttle Endeavour in May 1992. From left to right are astronauts Richard J. Hieb, Thomas D. Akers, and Pierre J. Thuot. Three STS - 49 crewmembers hold onto the 4.5 - ton Intelsat VI satellite in May 1992 after a six - handed “” capture””” was made minutes earlier. Left to right are astronauts Richard J. Hieb, Thomas D. Akers and Pierre J. Thuot. Thuot stands on the end of the Canadarm, which was instrumental as a mobile working platform in the capture

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Hubble space telescope: 1st maintenance mission 12 - 1993 - Hubble space telescope: first repair mission 12 - 1993 - Astronauts Story Musgrave (right) and Jeffrey Hoffman, on the arm of the shuttle Endeavour, prepare the installation of the new planetary wide field camera (WFPC2); the old camera is visible at the bottom right of the image; third extravehicular exit. Anchored on the end of Endeavour's Remote Manipulator System (RMS) arm, Jeffrey Hoffman (foreground) prepares to install the new Wide Field/Planetary Camera (WFPC II) into the empty cavity (top left) on the Hubble Space Telescope (HST). WFPC I is seen temporarily stowed at bottom right. Story Musgrave works with a Portable Foot Restraint (PFR) at frame center, as his image is reflected in the shiny surface of the telescope. Hoffman and Musgrave shared chores on three of the five space walks during the STS - 61 mission

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Hubble space telescope: 1st maintenance mission 12 - 1993 - Hubble space telescope: first repair mission 12 - 1993 - Astronauts Story Musgrave (right) and Jeffrey Hoffman, on the arm of the shuttle Endeavour, prepare the installation of the new planetary wide field camera (WFPC2); the old camera is visible at the bottom right of the image; third extravehicular exit. Anchored on the end of Endeavour's Remote Manipulator System (RMS) arm, Jeffrey Hoffman (foreground) prepares to install the new Wide Field/Planetary Camera (WFPC II) into the empty cavity (top left) on the Hubble Space Telescope (HST). WFPC I is seen temporarily stowed at bottom right. Story Musgrave works with a Portable Foot Restraint (PFR) at frame center, as his image is reflected in the shiny surface of the telescope. Hoffman and Musgrave shared chores on three of the five space walks during the STS - 61 mission

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Hubble Space Telescope: 1st maintenance mission 12 - 1993 - Astronauts install COSTAR during EVA for HST repair - Astronaut Thomas Akers prepares the installation of COSTAR, an instrument intended to correct Hubble's myopia. Kathryn C. Thornton is on the arm of the shuttle Endeavour with the instrument. Fourth extravehicular exit. Astronaut Thomas D. Akers maneuvers inside the bay which will house the Corrective Optics Space Telescope Axial Replacement (COSTAR) while assisting astronaut Kathryn C. Thornton with the installation of the 640 - pound instrument. Thornton, anchored on the end of the Remote Manipulator System (RMS) arm, is partially visible as she prepares to install the COSTAR. Dec 1993

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Hubble Space Telescope: 1st maintenance mission 12 - 1993 - Astronauts install COSTAR during EVA for HST repair - Astronaut Thomas Akers prepares the installation of COSTAR, an instrument intended to correct Hubble's myopia. Kathryn C. Thornton is on the arm of the shuttle Endeavour with the instrument. Fourth extravehicular exit. Astronaut Thomas D. Akers maneuvers inside the bay which will house the Corrective Optics Space Telescope Axial Replacement (COSTAR) while assisting astronaut Kathryn C. Thornton with the installation of the 640 - pound instrument. Thornton, anchored on the end of the Remote Manipulator System (RMS) arm, is partially visible as she prepares to install the COSTAR. Dec 1993

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Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

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Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

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Extra - vehicle exit C.Meade - M.Lee STS - 64 1994 - Astronauts Carl Meade and Mark Lee EVA - Extra - vehicle exit by Carl Meade and Mark Lee (right at the end of the articule arm) who are testing a SAFER (Simplified Aid for EVA Rescue) rescue procedure. 16/09/1994. Astronauts Carl Meade and Mark Lee (red strip on suit) test the new Simplified Aid for EVA Rescue (SAFER) system. The pair was actually performing an in - space rehearsal or demonstration of a contingency rescue using the never - before flown hardware. Sep 16 1994

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Extra - vehicle exit C.Meade - M.Lee STS - 64 1994 - Astronauts Carl Meade and Mark Lee EVA - Extra - vehicle exit by Carl Meade and Mark Lee (right at the end of the articule arm) who are testing a SAFER (Simplified Aid for EVA Rescue) rescue procedure. 16/09/1994. Astronauts Carl Meade and Mark Lee (red strip on suit) test the new Simplified Aid for EVA Rescue (SAFER) system. The pair was actually performing an in - space rehearsal or demonstration of a contingency rescue using the never - before flown hardware. Sep 16 1994

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Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

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Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

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Crew STS - 91 in the shuttle Discovery 06/1998 - STS - 91 crew in Discovery. 06/1998 - Downstairs, Wendy Lawrence, then clockwise, Andrew Thomas, Charles Precourt, Valery Ryumin, Janet Kavandi, Dominic Gorie, and Franklin Chang - Diaz. 1998. The seven crew members of STS - 91 pose for their traditional in - flight crew portrait aboard the Space Shuttle Discovery. Wendy B. Lawrence, mission specialist, at bottom center, (counter - clockwise from Lawrence) Andrew Thomas, mission specialist; Charles Precourt, mission commander; Valery Ryumin, mission specialist representing the Russian Aviation and Space Agency; Janet Kavandi, mission specialist; Dominic Gorie, pilot and Franklin Chang - Diaz, payload commander

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Crew STS - 91 in the shuttle Discovery 06/1998 - STS - 91 crew in Discovery. 06/1998 - Downstairs, Wendy Lawrence, then clockwise, Andrew Thomas, Charles Precourt, Valery Ryumin, Janet Kavandi, Dominic Gorie, and Franklin Chang - Diaz. 1998. The seven crew members of STS - 91 pose for their traditional in - flight crew portrait aboard the Space Shuttle Discovery. Wendy B. Lawrence, mission specialist, at bottom center, (counter - clockwise from Lawrence) Andrew Thomas, mission specialist; Charles Precourt, mission commander; Valery Ryumin, mission specialist representing the Russian Aviation and Space Agency; Janet Kavandi, mission specialist; Dominic Gorie, pilot and Franklin Chang - Diaz, payload commander

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Pyrenees views by shuttle 2001 - STS108 - 10/12/2001 The high spine of the Pyrenees Mountains at the French and Spanish border is snow covered in this 70 mm frame, photographed from the Space Shuttle Endeavour. The highest point of the Pyrenees is 3404 meters, though outside the area pictured. Snow - free foothills of the Pyrenees in Aquitaine (France) appear at the bottom (north is to the bottom of the view). According to geologists studying the STS - 108 photo collection, the Pyrenees range began forming about 320 million years ago and was strongly uplifted again during early stages of Eurasian - African plate collision. Complex folded strata on the Spanish side (near Pamplona) appear as bends and waves in foothill rock across the top of the view. Tin, tungsten, talc, fluorite, barium and gold have been mined from the mountains, and petroleum is produced from the adjacent Aquitaine sedimentary basin

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Pyrenees views by shuttle 2001 - STS108 - 10/12/2001 The high spine of the Pyrenees Mountains at the French and Spanish border is snow covered in this 70 mm frame, photographed from the Space Shuttle Endeavour. The highest point of the Pyrenees is 3404 meters, though outside the area pictured. Snow - free foothills of the Pyrenees in Aquitaine (France) appear at the bottom (north is to the bottom of the view). According to geologists studying the STS - 108 photo collection, the Pyrenees range began forming about 320 million years ago and was strongly uplifted again during early stages of Eurasian - African plate collision. Complex folded strata on the Spanish side (near Pamplona) appear as bends and waves in foothill rock across the top of the view. Tin, tungsten, talc, fluorite, barium and gold have been mined from the mountains, and petroleum is produced from the adjacent Aquitaine sedimentary basin

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White dwarf and planet in the globular cluster M4 - Oldest known planet in globular cluster M4 - The globular cluster M4 is located about 7000 years from Earth and seems to be 13 billion years old. The Hubble a space telescope identifies a Jupiter-sized planet orbiting a white dwarf star (green circle on the image). It would be the oldest planet known to date. Image of a starfield in the globular cluster M4. The green circle at right shows the location of a white dwarf star where a Jupiter - sized planet is orbiting. The planet is 2.5 times the mass of Jupiter. It is the oldest known planet identified. M4 is located 7000 light - years away in the summer constellation Scorpius

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White dwarf and planet in the globular cluster M4 - Oldest known planet in globular cluster M4 - The globular cluster M4 is located about 7000 years from Earth and seems to be 13 billion years old. The Hubble a space telescope identifies a Jupiter-sized planet orbiting a white dwarf star (green circle on the image). It would be the oldest planet known to date. Image of a starfield in the globular cluster M4. The green circle at right shows the location of a white dwarf star where a Jupiter - sized planet is orbiting. The planet is 2.5 times the mass of Jupiter. It is the oldest known planet identified. M4 is located 7000 light - years away in the summer constellation Scorpius

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Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

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Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

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Interacting galaxies in the Austral Fish - Interacting galaxies in Piscis Austrinus - The galaxies NGC 7173 (middle left), NGC 7174 (middle right) and NGC 7176 (bottom right) photographed here by the Hubble Space Telescope (HST), belong to a cluster of galaxies called Hickson Compact Group 90 (HCG 90), located about 100 million years ago lights in the constellation of Southern Fish. NGC 7173 and NGC 7176 are two elliptical galaxies while NGC 7174 is a spiral galaxy deformed by the gravitational forces exerted by its neighbors. The three pictured galaxies - - NGC 7173 (middle left), NCG 7174 (middle right) and NGC 7176 (lower right) - - are part of the Hickson Compact Group 90, named after astronomer Paul Hickson, who first catalogued these small clusters of galaxies in the 1980s. NGC 7173 and NGC 7176 appear to be smooth, normal elliptical galaxies without much gas and dust. In stark contrast, NGC 7174 is a mangled spiral galaxy, barely clinging to independent existence as it is ripped

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Interacting galaxies in the Austral Fish - Interacting galaxies in Piscis Austrinus - The galaxies NGC 7173 (middle left), NGC 7174 (middle right) and NGC 7176 (bottom right) photographed here by the Hubble Space Telescope (HST), belong to a cluster of galaxies called Hickson Compact Group 90 (HCG 90), located about 100 million years ago lights in the constellation of Southern Fish. NGC 7173 and NGC 7176 are two elliptical galaxies while NGC 7174 is a spiral galaxy deformed by the gravitational forces exerted by its neighbors. The three pictured galaxies - - NGC 7173 (middle left), NCG 7174 (middle right) and NGC 7176 (lower right) - - are part of the Hickson Compact Group 90, named after astronomer Paul Hickson, who first catalogued these small clusters of galaxies in the 1980s. NGC 7173 and NGC 7176 appear to be smooth, normal elliptical galaxies without much gas and dust. In stark contrast, NGC 7174 is a mangled spiral galaxy, barely clinging to independent existence as it is ripped

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Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon

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Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon

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Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

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Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

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Globular cluster M30 in Capricornus - Globular cluster M30 in Capricornus - The globular cluster M30 (NGC 7099) is located about 28,000 light years away from Earth. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. Messier 30 formed 13 billion years ago and was discovered in 1764 by Charles Messier. Located about 28 000 light - years away from Earth, this globular cluster - - a dense swarm of several hundred thousand stars - - is about 90 light - years across. Although globular clusters such as this one are mainly populated by old stars, the crowded field of stars leads to some old stars apparently reclaiming their youth in the form of blue stragglers. Researchers using data from Hubble's now - retired Wide Field Planetary Camera 2 (WFPC2) have identified two types of blue stragglers in Messier 30: those that form in near head - on collisions with one another and those that are in twin (or bi

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Globular cluster M30 in Capricornus - Globular cluster M30 in Capricornus - The globular cluster M30 (NGC 7099) is located about 28,000 light years away from Earth. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. Messier 30 formed 13 billion years ago and was discovered in 1764 by Charles Messier. Located about 28 000 light - years away from Earth, this globular cluster - - a dense swarm of several hundred thousand stars - - is about 90 light - years across. Although globular clusters such as this one are mainly populated by old stars, the crowded field of stars leads to some old stars apparently reclaiming their youth in the form of blue stragglers. Researchers using data from Hubble's now - retired Wide Field Planetary Camera 2 (WFPC2) have identified two types of blue stragglers in Messier 30: those that form in near head - on collisions with one another and those that are in twin (or bi

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Clusters of distant galaxies CL0024+1654 - Distant cluster of galaxies CL0024+1654 - False color image of cluster CL0024+1654 obtained with the 12k camera of CFHT (Canada France Hawaii Telescope) in Hawaii. This cluster is 4.5 billion light years away. This is a colour image of the galaxy cluster CL0024+1654 obtained with the CFHT12k camera at the Canada France Hawaii Telescope on Mauna Kea (Hawaii). Distance of 4.5 thousand million light - years (about one third of the look - back time to the Big Bang) from Earth. The cluster clearly appears as a concentration of yellow galaxies in the centre of this image although cluster galaxies actually extend at least to the edge of this image. This image measures 21 x 21 arc - minutes

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Clusters of distant galaxies CL0024+1654 - Distant cluster of galaxies CL0024+1654 - False color image of cluster CL0024+1654 obtained with the 12k camera of CFHT (Canada France Hawaii Telescope) in Hawaii. This cluster is 4.5 billion light years away. This is a colour image of the galaxy cluster CL0024+1654 obtained with the CFHT12k camera at the Canada France Hawaii Telescope on Mauna Kea (Hawaii). Distance of 4.5 thousand million light - years (about one third of the look - back time to the Big Bang) from Earth. The cluster clearly appears as a concentration of yellow galaxies in the centre of this image although cluster galaxies actually extend at least to the edge of this image. This image measures 21 x 21 arc - minutes

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Globular cluster M10 in Ophiuchus - Globular Cluster M10 - M10 (NGC 6254) is a globular cluster of magnitude 7 located about 15,000 years - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). M10, or NGC 6254, is a seventh magnitude globular cluster in the constellation Ophiuchus, close to M12. About 15000 light - years away and about 70 light - years across, M10 on the sky has about half the diameter of the full moon. This image is made up of observations made in visible and infrared light using Hubble's Advanced Camera for Surveys

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Globular cluster M10 in Ophiuchus - Globular Cluster M10 - M10 (NGC 6254) is a globular cluster of magnitude 7 located about 15,000 years - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). M10, or NGC 6254, is a seventh magnitude globular cluster in the constellation Ophiuchus, close to M12. About 15000 light - years away and about 70 light - years across, M10 on the sky has about half the diameter of the full moon. This image is made up of observations made in visible and infrared light using Hubble's Advanced Camera for Surveys

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Globular cluster NGC 6642 - Stars in globular cluster NGC 6642 in Sagittarius - Stars in globular cluster NGC 6642 in Sagittarius - Image of the center of the globular cluster NGC 6642 located in the constellation Sagittarius. The Hubble Space Telescope (HST) observed blue straggler. The core of NGC 6642, shown here in this Hubble Space Telescope image, is particularly dense, making this globular a difficult observational target for most telescopes. Using Hubble's ACS, astronomers have already made many interesting finds about NGC 6642. For example, many blue stragglers”” (stars which seemingly lag behind in their rate of aging) have been spotted in this globular, and it is known to be lacking in low - mass stars. This picture was created from visible and infrared images taken with the Wide Field Channel of the Advanced Camera for Surveys. The field of view is approximately 1.6 by 1.6 arcminutes.

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Globular cluster NGC 6642 - Stars in globular cluster NGC 6642 in Sagittarius - Stars in globular cluster NGC 6642 in Sagittarius - Image of the center of the globular cluster NGC 6642 located in the constellation Sagittarius. The Hubble Space Telescope (HST) observed blue straggler. The core of NGC 6642, shown here in this Hubble Space Telescope image, is particularly dense, making this globular a difficult observational target for most telescopes. Using Hubble's ACS, astronomers have already made many interesting finds about NGC 6642. For example, many blue stragglers”” (stars which seemingly lag behind in their rate of aging) have been spotted in this globular, and it is known to be lacking in low - mass stars. This picture was created from visible and infrared images taken with the Wide Field Channel of the Advanced Camera for Surveys. The field of view is approximately 1.6 by 1.6 arcminutes.

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Moon: part of the hidden face seen by Clementine - Part of the far side of the moon - Mosaic of images obtained by the Clementine probe in 1994. Part of the visible face appears to the right of the image with the Ocean of Tempetes. At the bottom of the picture the large concentric zone is the East Sea on the hidden face of the Moon. Mosaic image taken by Clementine spacecraft in 1994. The concentric, circular Orientale basin, 600 miles across, is bottom center; the near side is to the right, the far side to the left. At right is the large, dark Oceanus Procellarum

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Moon: part of the hidden face seen by Clementine - Part of the far side of the moon - Mosaic of images obtained by the Clementine probe in 1994. Part of the visible face appears to the right of the image with the Ocean of Tempetes. At the bottom of the picture the large concentric zone is the East Sea on the hidden face of the Moon. Mosaic image taken by Clementine spacecraft in 1994. The concentric, circular Orientale basin, 600 miles across, is bottom center; the near side is to the right, the far side to the left. At right is the large, dark Oceanus Procellarum

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Remnants of the supernova Cassiopee A in X-rays - Chandra 3 - color X - ray Image of Cassiopeia A This spectacular image of the supernova remnant Cassiopeia A is the most detailed image ever made of the remains of an exploded star. The one million second image shows a bright outer ring (green) ten light years in diameter that marks the location of a shock wave generated by the supernova explosion. A large jet - like structure that protrudes beyond the shock wave can be seen in the upper left. In this image, the colors represent different ranges of X - rays with red, green, and blue representing, low, medium, and higher X - ray energies

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Remnants of the supernova Cassiopee A in X-rays - Chandra 3 - color X - ray Image of Cassiopeia A This spectacular image of the supernova remnant Cassiopeia A is the most detailed image ever made of the remains of an exploded star. The one million second image shows a bright outer ring (green) ten light years in diameter that marks the location of a shock wave generated by the supernova explosion. A large jet - like structure that protrudes beyond the shock wave can be seen in the upper left. In this image, the colors represent different ranges of X - rays with red, green, and blue representing, low, medium, and higher X - ray energies

PIX4582936

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