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Images of 'NASA' found, 1,645

 
Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

PIX4597805

Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

PIX4597805

 
Apollo 17: Harrison Schmitt on the Moon - Apollo 17: Harrison Schmitt - H. Schmitt near the lunar jeep at Station 6. 13/12/1972. Astronaut Harrison H. Schmitt, lunar module pilot, works near the Lunar Roving Vehicle (LRV) during the third Apollo 17 extravehicular activity (EVA - 3) at the Taurus - Littrow site on the lunar surface. The front part of the LRV is out of frame at left, but the seats and several geological tools can be seen. The photo was taken by astronaut Eugene A. Cernan, mission commander

PIX4597983

Apollo 17: Harrison Schmitt on the Moon - Apollo 17: Harrison Schmitt - H. Schmitt near the lunar jeep at Station 6. 13/12/1972. Astronaut Harrison H. Schmitt, lunar module pilot, works near the Lunar Roving Vehicle (LRV) during the third Apollo 17 extravehicular activity (EVA - 3) at the Taurus - Littrow site on the lunar surface. The front part of the LRV is out of frame at left, but the seats and several geological tools can be seen. The photo was taken by astronaut Eugene A. Cernan, mission commander

PIX4597983

 
Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt collecting samples. 11/12/1972. Scientist - astronaut Harrison H. Schmitt, lunar module pilot, collects lunar rake samples at Station 1 during the first Apollo 17 Extrahicular Activity (EVA - 1) at the Taurus - Littrow landing site. This picture was taken by astronaut Eugene Cernan, commander. The lunar rake, an Apollo lunar geology hand tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 centimeter) to one inch (2.5 centimeter). 11 December 1972

PIX4598046

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt collecting samples. 11/12/1972. Scientist - astronaut Harrison H. Schmitt, lunar module pilot, collects lunar rake samples at Station 1 during the first Apollo 17 Extrahicular Activity (EVA - 1) at the Taurus - Littrow landing site. This picture was taken by astronaut Eugene Cernan, commander. The lunar rake, an Apollo lunar geology hand tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 centimeter) to one inch (2.5 centimeter). 11 December 1972

PIX4598046

 
Apollo 17: main site - Apollo 17 lunar landing site - View of the main site of Taurus - Littrow with the LEM. One of the last photos taken during the Apollo mission 17. 11/12/1972. The Lunar Module (LM) is in the background of this view of the Taurus - Littrow landing site. This was one of the last photographs taken on the lunar surface. The Apollo 17 crewmembers were astronauts Eugene A. Cernan, commander; Ronald E. Evans, command and service module pilot; and Harrison H. Schmitt, lunar module pilot. 11 Dec 1972

PIX4598259

Apollo 17: main site - Apollo 17 lunar landing site - View of the main site of Taurus - Littrow with the LEM. One of the last photos taken during the Apollo mission 17. 11/12/1972. The Lunar Module (LM) is in the background of this view of the Taurus - Littrow landing site. This was one of the last photographs taken on the lunar surface. The Apollo 17 crewmembers were astronauts Eugene A. Cernan, commander; Ronald E. Evans, command and service module pilot; and Harrison H. Schmitt, lunar module pilot. 11 Dec 1972

PIX4598259

 
Apollo 17: release of R. Evans - Apollo 17: Ronald E. Evans EVA - Extravehicular release of Ronald Evans to recover cameras and cameras. 17/12/1972. Astronaut Ronald E. Evans is photographed performing extravehicular activity during the Apollo 17 spacecraft's trans - earth coast. During his EVA, Evans, command module pilot, retrieved film cassettes from the lunar sounder, mapping camera and panoramic camera. The cylindrical object at Evans' left side is the mapping camera cassette. The total time for the trans - earth EVA was one hour, seven minutes, 18 seconds, starting at ground elapsed time of 257:25 (2:28 p.m.) and ending at G.E.T. of 258:42 (3:35 p.m.) on Sunday, December 17, 1972

PIX4598344

Apollo 17: release of R. Evans - Apollo 17: Ronald E. Evans EVA - Extravehicular release of Ronald Evans to recover cameras and cameras. 17/12/1972. Astronaut Ronald E. Evans is photographed performing extravehicular activity during the Apollo 17 spacecraft's trans - earth coast. During his EVA, Evans, command module pilot, retrieved film cassettes from the lunar sounder, mapping camera and panoramic camera. The cylindrical object at Evans' left side is the mapping camera cassette. The total time for the trans - earth EVA was one hour, seven minutes, 18 seconds, starting at ground elapsed time of 257:25 (2:28 p.m.) and ending at G.E.T. of 258:42 (3:35 p.m.) on Sunday, December 17, 1972

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Gemini 4: release of Ed.White - Gemini 4: Ed White EVA - First release of an American into space made by Edward White on June 3, 1965. On June 3, 1965 Edward H. White II became the first American to step outside his spacecraft and let go, effectively setting himself adrift in the zero gravity of space. For 23 minutes White floated and maneuvered himself around the Gemini spacecraft while logging 6500 miles during his orbital walk. White was attached to the spacecraft by a 25 foot umbilical line and a 23 - ft. tether line, both wrapped in gold tape to form one cord. In his right hand White carries a Hand Held Self Maneuvering Unit (HHSMU) which is used to move about the weightless environment of space. The visor of his helmet is gold plated to protect him from the unfiltered rays of the sun

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Gemini 4: release of Ed.White - Gemini 4: Ed White EVA - First release of an American into space made by Edward White on June 3, 1965. On June 3, 1965 Edward H. White II became the first American to step outside his spacecraft and let go, effectively setting himself adrift in the zero gravity of space. For 23 minutes White floated and maneuvered himself around the Gemini spacecraft while logging 6500 miles during his orbital walk. White was attached to the spacecraft by a 25 foot umbilical line and a 23 - ft. tether line, both wrapped in gold tape to form one cord. In his right hand White carries a Hand Held Self Maneuvering Unit (HHSMU) which is used to move about the weightless environment of space. The visor of his helmet is gold plated to protect him from the unfiltered rays of the sun

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The International Space Station seen in December 2000 - The International Space Station seen in December 2000 - The International Space Station (ISS) seen from the shuttle Endeavour before its return to Earth. 09/12/2000. Picture of the International Space Station (ISS) following undocking at 1:13 p.m. (CST), December 9, 2000. This image, represents the first imagery of the entire station with its new solar array panels deployed. Before separation, the shuttle and space station had been docked to one another for 6 days, 23 hours and 13 minutes. Endeavour moved downward from the space station, then began a tail - first circle at a distance of about 500 feet. Dec 09 2000

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The International Space Station seen in December 2000 - The International Space Station seen in December 2000 - The International Space Station (ISS) seen from the shuttle Endeavour before its return to Earth. 09/12/2000. Picture of the International Space Station (ISS) following undocking at 1:13 p.m. (CST), December 9, 2000. This image, represents the first imagery of the entire station with its new solar array panels deployed. Before separation, the shuttle and space station had been docked to one another for 6 days, 23 hours and 13 minutes. Endeavour moved downward from the space station, then began a tail - first circle at a distance of about 500 feet. Dec 09 2000

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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

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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

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SolarMax Satellite Repair Mission 04/1984 - Solar Maximum Mission repair 04/1984 - View of astronaut George D.Nelson approaching the Solar Max (Solar Maximum Mission or SMM) satellite on April 8, 1984. View of the damaged Solar Maximum Mission Satellite from the 41 - C space shuttle orbiter Challenger. The satellite's solar panels are fully extended. Astronaut George D. Nelson, using the manned maneuvering unit (MMU), approaches the satellite to attempt to “” lock - on”” to it

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SolarMax Satellite Repair Mission 04/1984 - Solar Maximum Mission repair 04/1984 - View of astronaut George D.Nelson approaching the Solar Max (Solar Maximum Mission or SMM) satellite on April 8, 1984. View of the damaged Solar Maximum Mission Satellite from the 41 - C space shuttle orbiter Challenger. The satellite's solar panels are fully extended. Astronaut George D. Nelson, using the manned maneuvering unit (MMU), approaches the satellite to attempt to “” lock - on”” to it

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Crew of the shuttle Enterprise - 1977 - Crew members of the shuttle orbiter Enterprise - Commander Fred Haise and pilot Gordon Fullerton, crew of the shuttle Enterprise used for the ALT Approach & Landing Test (ALT Approach & Landing Test) and initiated the development of the STS program. Its name is taken from “Star trek”, the popular TV series in the 1960s in the United States. 1977. The first crew members for the Space Shuttle Approach and Landing Tests (ALT). From l. to r.: Fred Haise, former Apollo 13 Lunar Module pilot and Gordon Fullerton, pilot. The Shuttle Orbiter Enterprise was named after the fictional Starship Enterprise from the popular 1960's television series, Star Trek. 1977

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Crew of the shuttle Enterprise - 1977 - Crew members of the shuttle orbiter Enterprise - Commander Fred Haise and pilot Gordon Fullerton, crew of the shuttle Enterprise used for the ALT Approach & Landing Test (ALT Approach & Landing Test) and initiated the development of the STS program. Its name is taken from “Star trek”, the popular TV series in the 1960s in the United States. 1977. The first crew members for the Space Shuttle Approach and Landing Tests (ALT). From l. to r.: Fred Haise, former Apollo 13 Lunar Module pilot and Gordon Fullerton, pilot. The Shuttle Orbiter Enterprise was named after the fictional Starship Enterprise from the popular 1960's television series, Star Trek. 1977

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Hubble Space Telescope Deployment 25 - 04 - 1990 - Hubble Space Telescope is released over Andes Mountains - The satellite, deployed by the shuttle Discovery floats over the Andes. The area visible in this image extends over 1000 km and covers parts of Peru, Bolivia, Chile and Argentina. The Hubble Space Telescope, with solar array wings and high gain antennae masts fully extended, is released by the remote manipulator system end effector. The STS - 31 crew aboard Discovery, set the HST into Earth orbit high above the Andes Mountains. Parts of Bolivia, Peru, Chile, and Argentina are visible. This picture covers a huge area of the western half of South America stretching from 14 degrees south latitude to 23 degrees, about 1,000 kilometers

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Hubble Space Telescope Deployment 25 - 04 - 1990 - Hubble Space Telescope is released over Andes Mountains - The satellite, deployed by the shuttle Discovery floats over the Andes. The area visible in this image extends over 1000 km and covers parts of Peru, Bolivia, Chile and Argentina. The Hubble Space Telescope, with solar array wings and high gain antennae masts fully extended, is released by the remote manipulator system end effector. The STS - 31 crew aboard Discovery, set the HST into Earth orbit high above the Andes Mountains. Parts of Bolivia, Peru, Chile, and Argentina are visible. This picture covers a huge area of the western half of South America stretching from 14 degrees south latitude to 23 degrees, about 1,000 kilometers

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View of debris in orbit around the Earth - Graphic computer of objects around the earth - View of debris in low orbit and geostationary orbit (35,785 km) around the Earth, from then a genere point above the north pole. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. This image is generated from a vantage point above the north pole, showing the concentrations of objects in Low Earth Orbit and in the geosynchronous region. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions

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View of debris in orbit around the Earth - Graphic computer of objects around the earth - View of debris in low orbit and geostationary orbit (35,785 km) around the Earth, from then a genere point above the north pole. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. This image is generated from a vantage point above the north pole, showing the concentrations of objects in Low Earth Orbit and in the geosynchronous region. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions

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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

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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

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Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

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Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

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Aegean Sea from the shuttle Atlantis - 09/2000 - Aegean Sea from the space shuttle Atlantis 09/2000 - The Aegean Sea, with Greece and Turkey, seen by the shuttle Atlantis on 09/09/2000. Crete (foreground), the Cyclades Islands, Greece and Turkey lie along the margin of the Eurasian and African tectonic plates; Africa is moving northward and being driven down beneath Eurasia. As a result volcanic islands, such as Santorini, develop and fault - bounded basin such, as the Gulf of Corinth, are formed. In addition, lavas and sediments that were originally deposited on the Mediterranean seafloor are uplifted and deformed

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Aegean Sea from the shuttle Atlantis - 09/2000 - Aegean Sea from the space shuttle Atlantis 09/2000 - The Aegean Sea, with Greece and Turkey, seen by the shuttle Atlantis on 09/09/2000. Crete (foreground), the Cyclades Islands, Greece and Turkey lie along the margin of the Eurasian and African tectonic plates; Africa is moving northward and being driven down beneath Eurasia. As a result volcanic islands, such as Santorini, develop and fault - bounded basin such, as the Gulf of Corinth, are formed. In addition, lavas and sediments that were originally deposited on the Mediterranean seafloor are uplifted and deformed

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PACA region seen by the satellite Landsat - Southern Coast of France - Part of the region Provence - Alpes - Cote d'Azur with to the north, Lake Sainte - Croix sur le Verdon, to the south, Toulon and the islands of Hyere. Lower left, Marseille. Image obtained by Landsat-7 satellite on 1 May 2003. France's famed Provence region meets the Mediterranean as a gentle curve intricately sculpted into sheltered bays and fringing peninsulas. The ancient port of Marseille nestles in the large bay at the lower left corner of the image Image taken on May 1st 2003 by satellite Landsat - 7

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PACA region seen by the satellite Landsat - Southern Coast of France - Part of the region Provence - Alpes - Cote d'Azur with to the north, Lake Sainte - Croix sur le Verdon, to the south, Toulon and the islands of Hyere. Lower left, Marseille. Image obtained by Landsat-7 satellite on 1 May 2003. France's famed Provence region meets the Mediterranean as a gentle curve intricately sculpted into sheltered bays and fringing peninsulas. The ancient port of Marseille nestles in the large bay at the lower left corner of the image Image taken on May 1st 2003 by satellite Landsat - 7

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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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Mir station 01/1997 - Mir station seen from the shuttle Atlantis before docking 01/1997 - Mir space station seen from the shuttle Atlantis approaching for mooring. 14/01/1997. In the upper center: a Progress ship, the Kvant module - and the central module; centre left: the Priroda module; centre right: the Spektr module; bottom left: the Kvant module - 2; centre low: a Soyuz ship; bottom right, the Kristall module and the mooring module. This is a view of the Russian Mir Space Station photographed by a crewmember of the fifth Shuttle/Mir docking mission, STS-81. The image shows: upper center - Progress supply vehicle, Kvant - 1 module, and Core module; center left - Priroda module; center right - Spektr module; bottom left - Kvant - 2 module; bottom center - Soyuz; and bottom right - Kristall module and Docking module. The Progress was an unmarned, automated version of the Soyuz crew transfer vehicle, designed to resupply the Mir. The Kvant - 1 provided research in the physics of galax

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Mir station 01/1997 - Mir station seen from the shuttle Atlantis before docking 01/1997 - Mir space station seen from the shuttle Atlantis approaching for mooring. 14/01/1997. In the upper center: a Progress ship, the Kvant module - and the central module; centre left: the Priroda module; centre right: the Spektr module; bottom left: the Kvant module - 2; centre low: a Soyuz ship; bottom right, the Kristall module and the mooring module. This is a view of the Russian Mir Space Station photographed by a crewmember of the fifth Shuttle/Mir docking mission, STS-81. The image shows: upper center - Progress supply vehicle, Kvant - 1 module, and Core module; center left - Priroda module; center right - Spektr module; bottom left - Kvant - 2 module; bottom center - Soyuz; and bottom right - Kristall module and Docking module. The Progress was an unmarned, automated version of the Soyuz crew transfer vehicle, designed to resupply the Mir. The Kvant - 1 provided research in the physics of galax

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