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Images of 'NASA' found, 1,645

 
Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground sta

PIX4611992

Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground sta

PIX4611992

 
Northwest Iceland seen by Landsat 7 satellite on 6 June 2000

PIX4666192

Northwest Iceland seen by Landsat 7 satellite on 6 June 2000

PIX4666192

 
Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

 
Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

PIX4623677

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

PIX4623677

 
Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

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Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

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Andromede Galaxy (M31) view in ultraviolet - The Andromeda galaxy seen in UV - This ultraviolet image is a mosaic of 10 images obtained by the GALEX satellite in September and October 2003. Regions of blue stars, young, warm and massive stars are clearly visible in the arms, where the stars are formed; in the center near the core, colder, orange-white, much older stars. The stars visible in the foreground belong to our Lactee Way. The GALEX observation of the large galaxy in Andromeda, Messier 31, was performed during September and October 2003. The image is a mosaic of 10 separate GALEX images combining the Far UV (colored blue) and Near UV detector (colored red) images together to make a color image of the sky almost six full moons across. The Andromeda galaxy is the most massive in the local group of galaxies, which includes our Milky Way, and is the nearest large galaxy to our own. The GALEX image shows blue regions of young, hot, high mass stars tracing out the spiral arms where s

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Andromede Galaxy (M31) view in ultraviolet - The Andromeda galaxy seen in UV - This ultraviolet image is a mosaic of 10 images obtained by the GALEX satellite in September and October 2003. Regions of blue stars, young, warm and massive stars are clearly visible in the arms, where the stars are formed; in the center near the core, colder, orange-white, much older stars. The stars visible in the foreground belong to our Lactee Way. The GALEX observation of the large galaxy in Andromeda, Messier 31, was performed during September and October 2003. The image is a mosaic of 10 separate GALEX images combining the Far UV (colored blue) and Near UV detector (colored red) images together to make a color image of the sky almost six full moons across. The Andromeda galaxy is the most massive in the local group of galaxies, which includes our Milky Way, and is the nearest large galaxy to our own. The GALEX image shows blue regions of young, hot, high mass stars tracing out the spiral arms where s

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Remnants of the supernova Cassiopee A en X by Chandra - Object Description: Cas A is the remnant of a star that exploded about 300 years ago. The X - ray image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees. Scale: Image is 6 arcmin on a side. Cassiopeia A: The 320 year old remnant of a massive star that exploded. Located in the constellation Cassiopeia, it is 10 light years across and 10,000 light years from Earth

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Remnants of the supernova Cassiopee A en X by Chandra - Object Description: Cas A is the remnant of a star that exploded about 300 years ago. The X - ray image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees. Scale: Image is 6 arcmin on a side. Cassiopeia A: The 320 year old remnant of a massive star that exploded. Located in the constellation Cassiopeia, it is 10 light years across and 10,000 light years from Earth

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Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

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Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

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Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

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Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

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Core of the Tempel 1 comet seen by the Deep impact probe - Comet Tempel 1 nucleus seen by Deep impact spacecraft - Composite image of different cliches. The core is 5 km by 7 km. This composite image was built up from scaling all images to 5 meters/pixel, and aligning images to fixed points. Each image at closer range, replaced equivalent locations observed at a greater distance. The impact site has the highest resolution because images were acquired until about 4 sec from impact or a few meters from the surface

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Core of the Tempel 1 comet seen by the Deep impact probe - Comet Tempel 1 nucleus seen by Deep impact spacecraft - Composite image of different cliches. The core is 5 km by 7 km. This composite image was built up from scaling all images to 5 meters/pixel, and aligning images to fixed points. Each image at closer range, replaced equivalent locations observed at a greater distance. The impact site has the highest resolution because images were acquired until about 4 sec from impact or a few meters from the surface

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La comete ISON pres du Soleil - 11/2013 - Comet ISON with Sun - 11/2013 - Comet ISON seen before and after its passage near the Sun. Composite of 60 images obtained by the Soho space telescope on 28 and 29 November 2013. This view captures the transformation of Comet ISON as it rounded the sun. It combines 60 SOHO C2 frames in which ISON appears (Nov. 28, 1248 UT, to Nov. 29, 0316 UT) with stars, noise and particle tracks removed, plus an SDO AIA 171 image of the sun taken just before the spacecraft attempted to image the comet near perihelion

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La comete ISON pres du Soleil - 11/2013 - Comet ISON with Sun - 11/2013 - Comet ISON seen before and after its passage near the Sun. Composite of 60 images obtained by the Soho space telescope on 28 and 29 November 2013. This view captures the transformation of Comet ISON as it rounded the sun. It combines 60 SOHO C2 frames in which ISON appears (Nov. 28, 1248 UT, to Nov. 29, 0316 UT) with stars, noise and particle tracks removed, plus an SDO AIA 171 image of the sun taken just before the spacecraft attempted to image the comet near perihelion

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Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

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Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

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Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

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Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

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Japan seen by shuttle 04/94 - Japan seen by shuttle STS - 59 on 14/04/1994

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Japan seen by shuttle 04/94 - Japan seen by shuttle STS - 59 on 14/04/1994

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Mount Everest seen from space - Mount Everest seen from space - Part of the Himalayan chain with Mount Everest (in the center), on the border between China and Nepal, observed by the shuttle Endeavour in February 2000. Mt. Everest (29,028 ft/8848 m; center of photo), also called Qomolangma Feng, is just north of the border between Nepal and China. The Himalayas and the Tibetan Plateau are products of the collision of the Indian and Eurasian tectonic plates. With the continuing northward march of India, the crust of the Earth has become thicker and the Tibetan Plateau has been uplifted to an average elevation of about 15,000 feet. Image taken by astronauts in the space shuttle Endeavour in february 2000

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Mount Everest seen from space - Mount Everest seen from space - Part of the Himalayan chain with Mount Everest (in the center), on the border between China and Nepal, observed by the shuttle Endeavour in February 2000. Mt. Everest (29,028 ft/8848 m; center of photo), also called Qomolangma Feng, is just north of the border between Nepal and China. The Himalayas and the Tibetan Plateau are products of the collision of the Indian and Eurasian tectonic plates. With the continuing northward march of India, the crust of the Earth has become thicker and the Tibetan Plateau has been uplifted to an average elevation of about 15,000 feet. Image taken by astronauts in the space shuttle Endeavour in february 2000

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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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J. Voss release 09/1995 - Astronaut James S. Voss extravehicular activity - James Voss extra - vehicle exit, connects to the fixed foot at the end of Endeavour's arm (Canadarm). Part of the shuttle is visible in reflection on Voss's helmet. 16/09/1995. Astronaut James S. Voss, payload commander, is pictured during the September 16, 1995, Extravehicular Activity (EVA) which was conducted in and around Space Shuttle Endeavour's cargo bay. Voss, whose visor reflects Endeavour's forward section, was standing on a mobile foot restraint attached to the arm of the Remote Manipulator System (RMS). As evidenced by the thin white cable, Voss was tethered to the end of the RMS as well. Evaluations for Space Station - era tools and various elements of the space suits were performed by Voss and his space walking crewmate, astronaut Michael L. Gernhardt, mission specialist. Sep 16 1995

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J. Voss release 09/1995 - Astronaut James S. Voss extravehicular activity - James Voss extra - vehicle exit, connects to the fixed foot at the end of Endeavour's arm (Canadarm). Part of the shuttle is visible in reflection on Voss's helmet. 16/09/1995. Astronaut James S. Voss, payload commander, is pictured during the September 16, 1995, Extravehicular Activity (EVA) which was conducted in and around Space Shuttle Endeavour's cargo bay. Voss, whose visor reflects Endeavour's forward section, was standing on a mobile foot restraint attached to the arm of the Remote Manipulator System (RMS). As evidenced by the thin white cable, Voss was tethered to the end of the RMS as well. Evaluations for Space Station - era tools and various elements of the space suits were performed by Voss and his space walking crewmate, astronaut Michael L. Gernhardt, mission specialist. Sep 16 1995

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Mir station 09/95 - Mir space station stowed with Atlantis shuttle. 22/09/1995

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Mir station 09/95 - Mir space station stowed with Atlantis shuttle. 22/09/1995

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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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Deploiement du satellite LDEF - Deployment of the LDEF satellite - Deployment of the Long Duration Exposure Facility (LDEF) satellite seen from the Challenger Shuttle over Florida on 7 April 1984. This satellite remained in space for more than five years and was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space. This single scene, taken during the Long Duration Exposure Facility (LDEF) satellite deploy, captures the entire Florida Peninsula (27.0N, 85.0W) in a single view. The multi - paneled LDEF satellite, suspended by the RMS, is undergoing final checkout procedures immediately prior to release. As a long term materials testing facility, the LDEF contained material samples in the many surface panels to determine the effects of long term exposure to space. multi - paneled LDEF satellite was deployed 27.0N, 85.0W)

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Deploiement du satellite LDEF - Deployment of the LDEF satellite - Deployment of the Long Duration Exposure Facility (LDEF) satellite seen from the Challenger Shuttle over Florida on 7 April 1984. This satellite remained in space for more than five years and was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space. This single scene, taken during the Long Duration Exposure Facility (LDEF) satellite deploy, captures the entire Florida Peninsula (27.0N, 85.0W) in a single view. The multi - paneled LDEF satellite, suspended by the RMS, is undergoing final checkout procedures immediately prior to release. As a long term materials testing facility, the LDEF contained material samples in the many surface panels to determine the effects of long term exposure to space. multi - paneled LDEF satellite was deployed 27.0N, 85.0W)

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Skylab station 07/1973 - Skylab station seen from Skylab module - 3 just before mooring. 28/07/1973. A close - up view of the Skylab space station cluster photographed against a black sky background from the Skylab 3 command module during the “” fly around”” inspection prior to docking. Note the one solar array system wing on the Orbital Workshop (OWS) which was successfully deployed during EVA on the first manned Skylab mission. The primary docking part at the forward end of the Multiple Docking Adapter (MDA) is visible below the Apollo Telescope Mount (ATM)

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Skylab station 07/1973 - Skylab station seen from Skylab module - 3 just before mooring. 28/07/1973. A close - up view of the Skylab space station cluster photographed against a black sky background from the Skylab 3 command module during the “” fly around”” inspection prior to docking. Note the one solar array system wing on the Orbital Workshop (OWS) which was successfully deployed during EVA on the first manned Skylab mission. The primary docking part at the forward end of the Multiple Docking Adapter (MDA) is visible below the Apollo Telescope Mount (ATM)

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Egypt shuttle view 2000 - Egypt view by shuttle STS - 106 in 2000

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Egypt shuttle view 2000 - Egypt view by shuttle STS - 106 in 2000

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