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2.4 m mirror inspects prior to installation on satellite - Inspection of the 94 inch primary mirror for Nasa's Hubble Space Telescope at Perkin-Elmers Optical facilities in Wilton, CT.: Mirror du telescope Hubble - The mirror of the Hubble space telescope

2.4 m mirror inspects prior to installation on satellite - Inspection of the 94 inch primary mirror for Nasa's Hubble Space Telescope at Perkin-Elmers Optical facilities in Wilton, CT.: Mirror du telescope Hubble - The mirror of the Hubble space telescope

PIX4644813

UARS Satellite - View of the UARS satellite during its deployment into space by space shuttle Discovery. UARS (Upper Atmosphere Research Satellite) is an Earth observation satellite from NASA developed to study the Earth's atmosphere in particular the ozone layer. The satellite, weighing 5.9 tons and 11 meters long, was launched in 1991 by the United States space shuttle during the STS-48 mission. It was placed in low orbit at an altitude of 700 km and was deactivated in December 2005. This STS - 48 onboard photo is of the Upper Atmosphere Research Satellite (UARS) in the grasp of the RMS (Remote Manipulator System) during deployment, September 1991. UARS gathers data related to the chemistry, dynamics, and energy of the ozone layer. UARS data is used to study energy input, stratospheric photo chemistry, and upper atmospheric circulation. Data from UARS enables scientists to study ozone depletion in the upper atmosphere

UARS Satellite - View of the UARS satellite during its deployment into space by space shuttle Discovery. UARS (Upper Atmosphere Research Satellite) is an Earth observation satellite from NASA developed to study the Earth's atmosphere in particular the ozone layer. The satellite, weighing 5.9 tons and 11 meters long, was launched in 1991 by the United States space shuttle during the STS-48 mission. It was placed in low orbit at an altitude of 700 km and was deactivated in December 2005. This STS - 48 onboard photo is of the Upper Atmosphere Research Satellite (UARS) in the grasp of the RMS (Remote Manipulator System) during deployment, September 1991. UARS gathers data related to the chemistry, dynamics, and energy of the ozone layer. UARS data is used to study energy input, stratospheric photo chemistry, and upper atmospheric circulation. Data from UARS enables scientists to study ozone depletion in the upper atmosphere

PIX4643847

James Webb Space Telescope (JWST) - JWST in clean room: View of the James Webb Space Telescope (JWST) at Nasa's Goddard Space Center on May 4, 2016. The JWST will replace the Hubble Space Telescope in 2018. A rare view of the James Webb Space Telescope face-on, from the NASA Goddard cleanroom observation window

James Webb Space Telescope (JWST) - JWST in clean room: View of the James Webb Space Telescope (JWST) at Nasa's Goddard Space Center on May 4, 2016. The JWST will replace the Hubble Space Telescope in 2018. A rare view of the James Webb Space Telescope face-on, from the NASA Goddard cleanroom observation window

PIX4645823

The SOHO satellite (photo)

The SOHO satellite (photo)

PIX5973655

The Earth and the Moon seen from space as it could appear from a satellite place at 35,000 km altitude. Composite image based on GOES (Geostationary Operational Environmental Satellite) data for clouds and Terra satellite for surface - This true-color image shows North and South America as they would appear from space 35,000 km (22,000 miles) above the Earth. The image is a combination of data from two satellites. The Moderate Resolution Imaging Spectroradiometer (MODIS) instrument aboard Nasa's Terra satellite collected the land surface data over 16 days, while Noaa's Geostationary Operational Environmental Satellite (GOES) produced a snapshot of the Earth's clouds: Earth seen by satellite - Earth seen by satellite

The Earth and the Moon seen from space as it could appear from a satellite place at 35,000 km altitude. Composite image based on GOES (Geostationary Operational Environmental Satellite) data for clouds and Terra satellite for surface - This true-color image shows North and South America as they would appear from space 35,000 km (22,000 miles) above the Earth. The image is a combination of data from two satellites. The Moderate Resolution Imaging Spectroradiometer (MODIS) instrument aboard Nasa's Terra satellite collected the land surface data over 16 days, while Noaa's Geostationary Operational Environmental Satellite (GOES) produced a snapshot of the Earth's clouds: Earth seen by satellite - Earth seen by satellite

PIX4669179

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

PIX4645435

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

PIX4645293

Satellite orbits METOP - SG - MetOp Second Generation satellites orbits - Artist view of METOP satellites - SG in orbit around the Earth. European MetOp second generation satellites will form a family of three pairs of meteorological satellites by 2020. Building on the current series of MetOp weather satellites, the family of MetOp - Second Generation missions will comprise three pairs of satellites to secure essential information for weather forecasting through the decades beyond 2020

Satellite orbits METOP - SG - MetOp Second Generation satellites orbits - Artist view of METOP satellites - SG in orbit around the Earth. European MetOp second generation satellites will form a family of three pairs of meteorological satellites by 2020. Building on the current series of MetOp weather satellites, the family of MetOp - Second Generation missions will comprise three pairs of satellites to secure essential information for weather forecasting through the decades beyond 2020

P. Carril

PIX4644818

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

PIX4645745

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

PIX4645755

James Webb Space Telescope (JWST) - JWST in clean room: View of the James Webb Space Telescope (JWST) at Nasa's Goddard Space Center on May 4, 2016. The JWST will replace the Hubble Space Telescope in 2018. A composite of nine wide-angle images showign the NASA Goddard clean room on May 4, 2016, when the uncovered flight primary mirror of the James Webb Space Telescope was tilted into a vertical position.

James Webb Space Telescope (JWST) - JWST in clean room: View of the James Webb Space Telescope (JWST) at Nasa's Goddard Space Center on May 4, 2016. The JWST will replace the Hubble Space Telescope in 2018. A composite of nine wide-angle images showign the NASA Goddard clean room on May 4, 2016, when the uncovered flight primary mirror of the James Webb Space Telescope was tilted into a vertical position.

PIX4645824

Military communication satellite Syracuse 3A - Syracuse 3A military communication satellite - View of the French military satellite Syracuse 3A in clean room at the Guyanese Space Centre on 4 September 2005. France's Syracuse 3A military communication satellite is mated on top of its payload adapter in the S5 payload processing facility of the Guiana Space Centre (CSG), Europe's space port, on September 4, 2005, in preparation for its launch atop an Ariane 5GS on October 13

Military communication satellite Syracuse 3A - Syracuse 3A military communication satellite - View of the French military satellite Syracuse 3A in clean room at the Guyanese Space Centre on 4 September 2005. France's Syracuse 3A military communication satellite is mated on top of its payload adapter in the S5 payload processing facility of the Guiana Space Centre (CSG), Europe's space port, on September 4, 2005, in preparation for its launch atop an Ariane 5GS on October 13

PIX4642782

James Webb Space Telescope (JWST) - JWST in clean room: Curvature measurements of the JWST Space Telescope (James Webb Space Telescope) at Nasa's Goddard Space Center. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Engineers and technicians working on the James Webb Space Telescope successfully completed the first important optical measurement of Webb's fully assembled primary mirror, called a Center of Curvature test. Taking a “” before””” optical measurement of the telescope's deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way out into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb's primary mirror, which could degrade or, in the worst case, ruin it

James Webb Space Telescope (JWST) - JWST in clean room: Curvature measurements of the JWST Space Telescope (James Webb Space Telescope) at Nasa's Goddard Space Center. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Engineers and technicians working on the James Webb Space Telescope successfully completed the first important optical measurement of Webb's fully assembled primary mirror, called a Center of Curvature test. Taking a “” before””” optical measurement of the telescope's deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way out into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb's primary mirror, which could degrade or, in the worst case, ruin it

PIX4645835

Military satellite DSP - Military satellite DSP tilted to predeployment position - Deploiement d'un satellite militaire DSP (Defense Support Program) on board the space shuttle Atlantis on 1 December 1991. These American spy satellites detect missile and spacecraft launches and nuclear explosions thanks to their infrared sensor that detects heat emissions. Defense Support Program (DSP)/Inertial Upper Stage (IUS) spacecraft, with forward airborne support equipment payload retention latch actuator released (foreground), is raised to a 29 degree predeployment position by the ASE aft frame tilt actuator (AFTA) table in the payload bay of Atlantis, Orbiter Vehicle 104. DSP components include Infrared sensor (top), AR I, SHF Antenna, EHF Antenna, Link 2 High - Gain Antenna, star sensor, and stowed solar paddles (box - like structure around the base). The Earth's limb and the blackness of space create the backdrop for this deployment scene. DSP satellites detect missile or spacecraft launches

Military satellite DSP - Military satellite DSP tilted to predeployment position - Deploiement d'un satellite militaire DSP (Defense Support Program) on board the space shuttle Atlantis on 1 December 1991. These American spy satellites detect missile and spacecraft launches and nuclear explosions thanks to their infrared sensor that detects heat emissions. Defense Support Program (DSP)/Inertial Upper Stage (IUS) spacecraft, with forward airborne support equipment payload retention latch actuator released (foreground), is raised to a 29 degree predeployment position by the ASE aft frame tilt actuator (AFTA) table in the payload bay of Atlantis, Orbiter Vehicle 104. DSP components include Infrared sensor (top), AR I, SHF Antenna, EHF Antenna, Link 2 High - Gain Antenna, star sensor, and stowed solar paddles (box - like structure around the base). The Earth's limb and the blackness of space create the backdrop for this deployment scene. DSP satellites detect missile or spacecraft launches

PIX4642655

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Primary Mirror Segment Cryogenic Testing - Six of the 18 James Webb Space Telescope mirror segments are being prepped to move into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cry

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Primary Mirror Segment Cryogenic Testing - Six of the 18 James Webb Space Telescope mirror segments are being prepped to move into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cry

PIX4645789

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

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Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope in the cargo bay of the shuttle Atlantis after it was captured for its fourth maintenance mission on 13 May 2009. The Hubble Space Telescope stands tall in the cargo bay of the Space Shuttle Atlantis following its capture and lock - down in Earth orbit. 13 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope in the cargo bay of the shuttle Atlantis after it was captured for its fourth maintenance mission on 13 May 2009. The Hubble Space Telescope stands tall in the cargo bay of the Space Shuttle Atlantis following its capture and lock - down in Earth orbit. 13 May 2009

PIX4645315

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from Shuttle Atlantis before it was captured for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope as the two spacecraft approached each other in Earth orbit prior to the capture of the giant observatory. 13 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from Shuttle Atlantis before it was captured for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope as the two spacecraft approached each other in Earth orbit prior to the capture of the giant observatory. 13 May 2009

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James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

PIX4645744

Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite launched in March 2009, designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope launched in march 2009 and designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun

Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite launched in March 2009, designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope launched in march 2009 and designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun

PIX4645650

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will resist the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Ball Aerospace lead optical test engineer Dave Chaney inspects six primary mirror segments, critical elements of Nasa's James Webb Space Telescope, prior to cryogenic testing in the X-ray & Cryogenic Facility at Nasa's Marshall Space Flight Center in Huntsville, Ala. The James Webb Space Telescope will be launched in 2018 to study the formation of the first stars and galaxies and shed new light on the evolution of the universe

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will resist the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Ball Aerospace lead optical test engineer Dave Chaney inspects six primary mirror segments, critical elements of Nasa's James Webb Space Telescope, prior to cryogenic testing in the X-ray & Cryogenic Facility at Nasa's Marshall Space Flight Center in Huntsville, Ala. The James Webb Space Telescope will be launched in 2018 to study the formation of the first stars and galaxies and shed new light on the evolution of the universe

PIX4645803

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will resist the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Space Telescope's primary mirror segments are prepared to begin final cryogenic testing at Nasa's Marshall Space Flight Center in Huntsville, Ala. This represents the first six of 18 segments that will form Nasa's James Webb Space Telescope's primary mirror for space observations. Engineers began final round-the-clock cryogenic testing to confirm that the mirrors will respond as expected to the extreme temperatures of space prior to integration into the telescope's permanent housing structure

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will resist the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Space Telescope's primary mirror segments are prepared to begin final cryogenic testing at Nasa's Marshall Space Flight Center in Huntsville, Ala. This represents the first six of 18 segments that will form Nasa's James Webb Space Telescope's primary mirror for space observations. Engineers began final round-the-clock cryogenic testing to confirm that the mirrors will respond as expected to the extreme temperatures of space prior to integration into the telescope's permanent housing structure

PIX4645785

Satellite photo of Malosmadulu atolls (Maldives) - Malosmadulu atolls (Maldives) seen from space - Satellite photo of Malosmadulu atolls in Maldives obtained by Terra satellite on 22 December 2002. North and South Malosmadulu Atoll are in the Maldives, an island republic in the northern Indian Ocean, southwest of India. The Maldives are made up of a chain of 1,192 small coral islands, which are grouped into clusters of atolls. Arguably the lowest - lying country in the world, the average elevation is just 1 meter above sea level. The natural - color ASTER image of the Malosmadulu Atoll was acquired on December 22, 2002, and is centered near 5.3 degrees North latitude, 73.9 degrees West longitude

Satellite photo of Malosmadulu atolls (Maldives) - Malosmadulu atolls (Maldives) seen from space - Satellite photo of Malosmadulu atolls in Maldives obtained by Terra satellite on 22 December 2002. North and South Malosmadulu Atoll are in the Maldives, an island republic in the northern Indian Ocean, southwest of India. The Maldives are made up of a chain of 1,192 small coral islands, which are grouped into clusters of atolls. Arguably the lowest - lying country in the world, the average elevation is just 1 meter above sea level. The natural - color ASTER image of the Malosmadulu Atoll was acquired on December 22, 2002, and is centered near 5.3 degrees North latitude, 73.9 degrees West longitude

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ENVISAT building at ESRIN - Envisat building, ESRIN, Italy - An engineer works on the data transmitted by the ENVISAT satellite; outside the antenna receiving the information sent by the satellite. ENVISAT Building, ESRIN (European Space Research Institute), Italy. The validation and calibration desk, in the Envisat building at ESA's European Space Research Institute (ESRIN), in Frascati, Italy. Here, scientists and technicians work together to ensure that the instruments onboard the Envisat Earth observation satellite perform correctly

ENVISAT building at ESRIN - Envisat building, ESRIN, Italy - An engineer works on the data transmitted by the ENVISAT satellite; outside the antenna receiving the information sent by the satellite. ENVISAT Building, ESRIN (European Space Research Institute), Italy. The validation and calibration desk, in the Envisat building at ESA's European Space Research Institute (ESRIN), in Frascati, Italy. Here, scientists and technicians work together to ensure that the instruments onboard the Envisat Earth observation satellite perform correctly

A. Gonin

PIX4598582

TDRS-E communication satellite - View of the TDRS-E (Tracking and Data Relay Satellite - E) satellite en route to its orbit after its deployment from the Atlantis space shuttle in August 1991. This satellite belongs to a network of American communications satellites. Tracking and Data Relay Satellite E (TDRS-E) and the attached Inertial Upper Stage booster after deployment from Atlantis, STS-43

TDRS-E communication satellite - View of the TDRS-E (Tracking and Data Relay Satellite - E) satellite en route to its orbit after its deployment from the Atlantis space shuttle in August 1991. This satellite belongs to a network of American communications satellites. Tracking and Data Relay Satellite E (TDRS-E) and the attached Inertial Upper Stage booster after deployment from Atlantis, STS-43

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Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

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Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

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Mosaic of satellite data taken from a NASA sensor called the Moderate Resolution Imaging Spectroradiometer (MODIS) that flies board NASA's Terra satellite.: Earth seen by satellite

Mosaic of satellite data taken from a NASA sensor called the Moderate Resolution Imaging Spectroradiometer (MODIS) that flies board NASA's Terra satellite.: Earth seen by satellite

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The Mission STEREO - STEREO Artist View - STEREO (Solar Terrestrial Relationships Observatory) is a space mission of NASA to study Sun - Earth relations. STEREO consists of two twin satellites, one precedent the Earth in its revolution around the Sun and the other following it. The mission entered the operational phase in December 2006. Its nominal term of 2 years has been extended. STEREO (Solar Terrestrial Relationships Observatory) is the third mission in NASA's Solar Terrestrial Probes program (STP). The mission, launched in October 2006, has provided a unique and revolutionary view of the Sun - Earth System. The two almost identical observatories - one ahead of Earth in its orbit, the other trailing behind - have traced the flow of energy and matter from the Sun to Earth. STEREO has revealed the 3D structure of coronal mass ejections; violent eruptions of matter from the sun that can disrupt satellites and power grids, and help us understand why they happen. STEREO is a key additi

The Mission STEREO - STEREO Artist View - STEREO (Solar Terrestrial Relationships Observatory) is a space mission of NASA to study Sun - Earth relations. STEREO consists of two twin satellites, one precedent the Earth in its revolution around the Sun and the other following it. The mission entered the operational phase in December 2006. Its nominal term of 2 years has been extended. STEREO (Solar Terrestrial Relationships Observatory) is the third mission in NASA's Solar Terrestrial Probes program (STP). The mission, launched in October 2006, has provided a unique and revolutionary view of the Sun - Earth System. The two almost identical observatories - one ahead of Earth in its orbit, the other trailing behind - have traced the flow of energy and matter from the Sun to Earth. STEREO has revealed the 3D structure of coronal mass ejections; violent eruptions of matter from the sun that can disrupt satellites and power grids, and help us understand why they happen. STEREO is a key additi

PIX4646347

Iceland seen from satellite Aqua 28/01/2004 - Iceland seen by satellite - Iceland totally covered with snow and ice seen on 28 January 2004. Iceland is shown here covered in a white blanket of ice and snow. This true - color image was acquired on January 28, 2004, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Aqua satellite

Iceland seen from satellite Aqua 28/01/2004 - Iceland seen by satellite - Iceland totally covered with snow and ice seen on 28 January 2004. Iceland is shown here covered in a white blanket of ice and snow. This true - color image was acquired on January 28, 2004, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Aqua satellite

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Tongatapu satellite view - Tongatapu seen from space: Tongatapu Island (Kingdom of Tonga) observed by Sentinel-2A satellite on 23 May 2016 - The island of Tongatapu and the nearby smaller islands - all part of the Kingdom of Tonga archipelago in the southern Pacific Ocean - are pictured in this Sentinel-2A image from 23 May 2016 - Tonga's population is spread across 36 of Tonga's 169 islands, but about 70% live on this main island. The capital, Nuku alofa, sits on the island's north coast and along the Fanga'uta Lagoon. The lagoon's mangroves provide an important breeding ground for fish and birds

Tongatapu satellite view - Tongatapu seen from space: Tongatapu Island (Kingdom of Tonga) observed by Sentinel-2A satellite on 23 May 2016 - The island of Tongatapu and the nearby smaller islands - all part of the Kingdom of Tonga archipelago in the southern Pacific Ocean - are pictured in this Sentinel-2A image from 23 May 2016 - Tonga's population is spread across 36 of Tonga's 169 islands, but about 70% live on this main island. The capital, Nuku alofa, sits on the island's north coast and along the Fanga'uta Lagoon. The lagoon's mangroves provide an important breeding ground for fish and birds

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Najd Plateau - Saudi Arabia - Najd plateau - Saudi Arabia - Image obtained by Envisat satellite centree on the Najd region of Saudi Arabia. The circular shapes visible at the top and left center of the image are irrigated fields. This Envisat image is centred over the plateau region of Najd located in Saudi Arabia, bounded on the west by the Al Hijaz mountains and on all other sides by desert sands. A curious feature about this image are the irrigated fields shown as grey and black circular patterns at the top and centre left of the image. Image taken on July 13 2003

Najd Plateau - Saudi Arabia - Najd plateau - Saudi Arabia - Image obtained by Envisat satellite centree on the Najd region of Saudi Arabia. The circular shapes visible at the top and left center of the image are irrigated fields. This Envisat image is centred over the plateau region of Najd located in Saudi Arabia, bounded on the west by the Al Hijaz mountains and on all other sides by desert sands. A curious feature about this image are the irrigated fields shown as grey and black circular patterns at the top and centre left of the image. Image taken on July 13 2003

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Volcano Fogo - Cape Verde - Volcano Fogo - Cape Verde islands - Fogo Island with its highest volcano 2800 meters south of the Cape Verde archipelago. Image obtained from the EO-1 satellite on 10 June 2009. Fogo is one of the Cape Verde Islands located roughly 640 kilometers off the westernmost tip of Africa, Fogo received its name from English colonists around 1500 AD. The Advanced Land Imager on Nasa's EO - 1 satellite captured this detailed image of the volcano on June 10, 2009. The volcano's most distinctive feature, its nine - kilometer wide caldera, Cha Caldera, is shown in this image. The eastern half of the crater wall is gone, erased in a massive collapse deep in its ancient history. In the center of the crater, a steep cone named Pico rises about 100 meters above the crater rim (more than a kilometer from the crater floor). The young peak reaches 2,829 meters (9,281 feet) above sea level, making it the island's highest point. The crater is inhabited. A straight road cuts betwe

Volcano Fogo - Cape Verde - Volcano Fogo - Cape Verde islands - Fogo Island with its highest volcano 2800 meters south of the Cape Verde archipelago. Image obtained from the EO-1 satellite on 10 June 2009. Fogo is one of the Cape Verde Islands located roughly 640 kilometers off the westernmost tip of Africa, Fogo received its name from English colonists around 1500 AD. The Advanced Land Imager on Nasa's EO - 1 satellite captured this detailed image of the volcano on June 10, 2009. The volcano's most distinctive feature, its nine - kilometer wide caldera, Cha Caldera, is shown in this image. The eastern half of the crater wall is gone, erased in a massive collapse deep in its ancient history. In the center of the crater, a steep cone named Pico rises about 100 meters above the crater rim (more than a kilometer from the crater floor). The young peak reaches 2,829 meters (9,281 feet) above sea level, making it the island's highest point. The crater is inhabited. A straight road cuts betwe

PIX4658526

Le Piton de la Fournaise, Ile de la Reunion - Piton de la Fournaise, Reunion island - Le Piton de la Fournaise seen by satellite EO - 1 on 16 January 2009. This shield volcano is one of the most active volcanoes in the world. Considered one of the world's most active volcanoes, Piton de la Fournaise occupies the east - southeastern end of Reunion Island in the western Indian Ocean. It is a shield volcano with a low, broad shape that resemble an ancient warrior shield. The volcano sports an 8 - kilometer - (5 - mile -) wide crater that slopes eastward to the coast. Within that crater sits a lava shield, Dolomieu, and most of Piton de la Fournaise's historic eruptions have occurred from the summit or flanks of Dolomieu. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Piton de la Fournaise on January 16, 2009. Dolomieu is the circular feature at the center of the large crater. Lava flows from earlier eruptions have left their marks around Dolo

Le Piton de la Fournaise, Ile de la Reunion - Piton de la Fournaise, Reunion island - Le Piton de la Fournaise seen by satellite EO - 1 on 16 January 2009. This shield volcano is one of the most active volcanoes in the world. Considered one of the world's most active volcanoes, Piton de la Fournaise occupies the east - southeastern end of Reunion Island in the western Indian Ocean. It is a shield volcano with a low, broad shape that resemble an ancient warrior shield. The volcano sports an 8 - kilometer - (5 - mile -) wide crater that slopes eastward to the coast. Within that crater sits a lava shield, Dolomieu, and most of Piton de la Fournaise's historic eruptions have occurred from the summit or flanks of Dolomieu. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Piton de la Fournaise on January 16, 2009. Dolomieu is the circular feature at the center of the large crater. Lava flows from earlier eruptions have left their marks around Dolo

PIX4659236

MTG Meteorology Satellite - MTG Satellite. Artwork - Artist's view of the European satellite project MTG (Meteosat Third Generation). This development programme will run from 2009 to 2020. Artist view of european meteorological satellite MTG (Meteosat Third Generation). The development programme will last from 2009 until 2020

MTG Meteorology Satellite - MTG Satellite. Artwork - Artist's view of the European satellite project MTG (Meteosat Third Generation). This development programme will run from 2009 to 2020. Artist view of european meteorological satellite MTG (Meteosat Third Generation). The development programme will last from 2009 until 2020

P. Carril

PIX4644662

Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai Volcano is an active volcano located in Tanzania in the Great Rift Valley. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Image obtained from the EO-1 satellite on 12 September 2009. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite. The lava of Ol Doinyo Lengai is extremely cool (500 - 600* C, compared to 1,160* C for typical basaltic lava) and relatively fluid. Ol Doinyo Lengai alternates between eruptions of liquid lava that form lava lakes and fountains (called effusive eruptions) and explosive eruptions that build large cinder and ash cones. The new cone and crater are clearly visible in the center of the image acquired by satellite EO-1 on September 12, 2009. The dark spot in the crater may be fresh lava erupted from a new volcanic vent. Gray ash covers the volcano and much of the surrounding landscape

Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai Volcano is an active volcano located in Tanzania in the Great Rift Valley. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Image obtained from the EO-1 satellite on 12 September 2009. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite. The lava of Ol Doinyo Lengai is extremely cool (500 - 600* C, compared to 1,160* C for typical basaltic lava) and relatively fluid. Ol Doinyo Lengai alternates between eruptions of liquid lava that form lava lakes and fountains (called effusive eruptions) and explosive eruptions that build large cinder and ash cones. The new cone and crater are clearly visible in the center of the image acquired by satellite EO-1 on September 12, 2009. The dark spot in the crater may be fresh lava erupted from a new volcanic vent. Gray ash covers the volcano and much of the surrounding landscape

PIX4659350

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - The space telescope seen from the shuttle Atlantis during its capture for its fourth maintenance mission, May 13, 2009. An STS - 125 crewmember onboard the Space Shuttle Atlantis snapped a still photo of the Hubble Space Telescope following grapple of the giant observatory by the shuttle's Canadian - built remote manipulator system. 13 May 2009

PIX4645290

Spartan 201 satellite - Spartan 201 satellite seen over the Earth from space shuttle Discovery in September 1994. Astronauts onboard the space shuttle Discovery used a 70 mm camera to capture this photograph of the retrieval operations with the Shuttle Pointed Autonomous Research Tool for Astronomy 201 (SPARTAN 201). A gibbous moon can be seen in the background. 9 - 20 Sep 1994

Spartan 201 satellite - Spartan 201 satellite seen over the Earth from space shuttle Discovery in September 1994. Astronauts onboard the space shuttle Discovery used a 70 mm camera to capture this photograph of the retrieval operations with the Shuttle Pointed Autonomous Research Tool for Astronomy 201 (SPARTAN 201). A gibbous moon can be seen in the background. 9 - 20 Sep 1994

PIX4646354

Maldives - Haa Alifu Atoll (detail) - Maldives - Haa Alif Atoll - Detail - Satellite photo obtained by Kompsat-2 satellite on January 9, 2011. Top right: Filladhoo, top left: Vashafaru, bottom center: Baarah, left: Maafahi, Muraidhoo and Alidhoo. This image from the Kompsat-2 satellite, acquired on 9 January 2011, shows islands of the Haa Alif Atoll in northern Maldives

Maldives - Haa Alifu Atoll (detail) - Maldives - Haa Alif Atoll - Detail - Satellite photo obtained by Kompsat-2 satellite on January 9, 2011. Top right: Filladhoo, top left: Vashafaru, bottom center: Baarah, left: Maafahi, Muraidhoo and Alidhoo. This image from the Kompsat-2 satellite, acquired on 9 January 2011, shows islands of the Haa Alif Atoll in northern Maldives

PIX4661095

Test in anechoid chamber - Test in Anechoid Chamber - Test of the SAPHIR instrument in the anechoid chamber of CNES in Toulouse in May 2009. SAPHIR will be embarked on board the Franco-Indian satellite Megha-Tropiques to measure water vapour on Earth.

Test in anechoid chamber - Test in Anechoid Chamber - Test of the SAPHIR instrument in the anechoid chamber of CNES in Toulouse in May 2009. SAPHIR will be embarked on board the Franco-Indian satellite Megha-Tropiques to measure water vapour on Earth.

H. Piraud

PIX4644404

Jupiter from his satellite Io - Illustration - Jupiter from Io - Illustration - Io is the closest galileen satellite to Jupiter. Io is Jupiter's innermost large satellite and is about the same size and density as Earth's moon. At 260,000 miles from Jupiter, Io is about the same distance as the Moon is from the Earth

Jupiter from his satellite Io - Illustration - Jupiter from Io - Illustration - Io is the closest galileen satellite to Jupiter. Io is Jupiter's innermost large satellite and is about the same size and density as Earth's moon. At 260,000 miles from Jupiter, Io is about the same distance as the Moon is from the Earth

Walter B Myers

PIX4575280

Satellite Picard - Artist's view of the Picard satellite in orbit around the Earth. This microsatellite should study the Sun and the links between the solar cycle and the Earth's climate. Satellite Picard seen above the Earth. This english microsatellite will study the Sun and the relations between the sun and the Earth's climate

Satellite Picard - Artist's view of the Picard satellite in orbit around the Earth. This microsatellite should study the Sun and the links between the solar cycle and the Earth's climate. Satellite Picard seen above the Earth. This english microsatellite will study the Sun and the relations between the sun and the Earth's climate

D. Ducros

PIX4646322

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - This image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits: Night land. Europe and Africa - Earth by night. Europe and Africa

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - This image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits: Night land. Europe and Africa - Earth by night. Europe and Africa

PIX4669260

Africa seen from space - Africa seen from space - Southern Africa seen from space. Composite satellite photos and computer illustration. Artwork composed from satellite photographs and computer generated images

Africa seen from space - Africa seen from space - Southern Africa seen from space. Composite satellite photos and computer illustration. Artwork composed from satellite photographs and computer generated images

P. Carril

PIX4658332

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

PIX4646048

Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Obser

Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Obser

P. Dumas

PIX4646076

Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Obser

Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Obser

P. Dumas

PIX4646082

Jupiter and Ganymede seen by Voyager 1. 02/1979 - Jupiter and Ganymede as seen by Voyager 1. 02/1979 - Jupiter and his satellite Ganymede (bottom left) seen by the Voyager 1 probe on February 24, 1979 40 million km from the planet. Jupiter and its satellite Ganymede (bottom left) are visible in this photo taken on February 24 1979 by Voyager 1. The space probe was 40 million kilometers from the planet at the time

Jupiter and Ganymede seen by Voyager 1. 02/1979 - Jupiter and Ganymede as seen by Voyager 1. 02/1979 - Jupiter and his satellite Ganymede (bottom left) seen by the Voyager 1 probe on February 24, 1979 40 million km from the planet. Jupiter and its satellite Ganymede (bottom left) are visible in this photo taken on February 24 1979 by Voyager 1. The space probe was 40 million kilometers from the planet at the time

PIX4574604

Volcanic eruption on Io, one of Jupiter's satellites.: Volcanic eruption on Io -Illustration - Volcanic eruption on Io. Artwork

Volcanic eruption on Io, one of Jupiter's satellites.: Volcanic eruption on Io -Illustration - Volcanic eruption on Io. Artwork

PIX4614055

Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun

Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun

PIX4645644

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Team with a 6.5 m mirror, he will observe the universe mainly in infrared - Six of the 18 James Webb Space Telescope mirror segments are being moved into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Team with a 6.5 m mirror, he will observe the universe mainly in infrared - Six of the 18 James Webb Space Telescope mirror segments are being moved into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb

PIX4645800

James Webb Space Telescope (JWST) - Thermal Shield - JWST sunshield: Thermal Shield Deployment to Northrop Grumann, California, July 2014. The JWST will replace the Hubble Space Telescope in 2018. The Sunshield on Nasa's James Webb Space Telescope is the largest part of the observatory - five layers of thin membrane that must unfurl reliably in space to precise tolerances. Last week, for the first time, engineers stacked and unfurled a full-sized test unit of the Sunshield and it worked perfectly. The Sunshield is about the length of a tennis court, and will be folded up like an umbrella around the Webb telescope's mirrors and instruments during launch. Once it reaches its orbit, the Webb telescope will receive a command from Earth to unfold, and separate the Sunshield's five layers into their precisely stacked arrangement with its kite-like shape

James Webb Space Telescope (JWST) - Thermal Shield - JWST sunshield: Thermal Shield Deployment to Northrop Grumann, California, July 2014. The JWST will replace the Hubble Space Telescope in 2018. The Sunshield on Nasa's James Webb Space Telescope is the largest part of the observatory - five layers of thin membrane that must unfurl reliably in space to precise tolerances. Last week, for the first time, engineers stacked and unfurled a full-sized test unit of the Sunshield and it worked perfectly. The Sunshield is about the length of a tennis court, and will be folded up like an umbrella around the Webb telescope's mirrors and instruments during launch. Once it reaches its orbit, the Webb telescope will receive a command from Earth to unfold, and separate the Sunshield's five layers into their precisely stacked arrangement with its kite-like shape

PIX4645844

Io and its shadow (photo)

Io and its shadow (photo)

Sebastian Voltmer

PIX6333925

Lake Chad seen by satellite in 2007 - Lake Chad as seen by satellite in 2007 - Lake Chad seen by Envisat satellite on 19 December 2007. This Envisat image highlights Lake Chad, a freshwater lake located in central Africa at the junction of Chad, Cameroon, Nigeria and Niger. Lake Chad, once Africa's third largest inland water body, is located in West Africa's Sahel region - a transition zone between the Sahara Desert to the north and savannas and woodlands to the south. Because the lake is shallow, between 1 m in the northwest and 7 m in the south, it has always undergone seasonal fluctuations. However, it has shrunk dramatically over the last four decades due to a decrease in rainfall and an increase in the amount of water used for irrigation projects. Lake Chad's surface area was 25 000 sq km in the early 1960s, compared with 1350 sq km in 2001. Lake Chad is fed primarily by the Chari and Logone Rivers, which are both located in the southwest and flow northward into the lake, which do

Lake Chad seen by satellite in 2007 - Lake Chad as seen by satellite in 2007 - Lake Chad seen by Envisat satellite on 19 December 2007. This Envisat image highlights Lake Chad, a freshwater lake located in central Africa at the junction of Chad, Cameroon, Nigeria and Niger. Lake Chad, once Africa's third largest inland water body, is located in West Africa's Sahel region - a transition zone between the Sahara Desert to the north and savannas and woodlands to the south. Because the lake is shallow, between 1 m in the northwest and 7 m in the south, it has always undergone seasonal fluctuations. However, it has shrunk dramatically over the last four decades due to a decrease in rainfall and an increase in the amount of water used for irrigation projects. Lake Chad's surface area was 25 000 sq km in the early 1960s, compared with 1350 sq km in 2001. Lake Chad is fed primarily by the Chari and Logone Rivers, which are both located in the southwest and flow northward into the lake, which do

PIX4659459

Satellite METOP - A - Artist's view of the European satellite METOP - A in orbit around the Earth. Launch on October 19, 2006, it is the first European meteorological satellite in polar orbit; it includes twelve meteorological instruments. MetOp is a series of three meteorological operational polar orbiting satellites, the first of which, MetOp-1 is the prototype. The instruments on MetOp will produce high - resolution images, vertical temperature and humidity profiles, and temperatures of the land and ocean surface on a global basis. Also on board the satellites will be instruments for monitoring ozone and wind flow over the oceans. The first launch was on October 19 2006

Satellite METOP - A - Artist's view of the European satellite METOP - A in orbit around the Earth. Launch on October 19, 2006, it is the first European meteorological satellite in polar orbit; it includes twelve meteorological instruments. MetOp is a series of three meteorological operational polar orbiting satellites, the first of which, MetOp-1 is the prototype. The instruments on MetOp will produce high - resolution images, vertical temperature and humidity profiles, and temperatures of the land and ocean surface on a global basis. Also on board the satellites will be instruments for monitoring ozone and wind flow over the oceans. The first launch was on October 19 2006

D. Ducros

PIX4644893

CRYOSAT-2 satellite - The European Cryosat-2 satellite is being tested at the Space Test Centre at IABG (Industrieanlagen - Betriebsgesellschaft mbH) in Ottobrunn, Germany, in September 2009. This satellite is intended to study polar ice. CryoSat - 2 undergoing testing at the Space Test Centre at IABG (Industrieanlagen - Betriebsgesellschaft mbH) in Ottobrunn, Germany in September 2009. CryoSat will be the third of ESA's Earth Explorer satellites in orbit. The 700 kg CryoSat spacecraft whose name comes from the Greek kryos meaning cold or ice carries the first all - weather microwave radar altimeter. The instrument has been optimised for determining changes in the thickness of both floating sea ice, which can be up to several meters, and polar land ice sheets, which in Antarctica can be close to 5 km thick. The mission will deliver data on the rate of change of the ice thickness accurate to within one centimetre

CRYOSAT-2 satellite - The European Cryosat-2 satellite is being tested at the Space Test Centre at IABG (Industrieanlagen - Betriebsgesellschaft mbH) in Ottobrunn, Germany, in September 2009. This satellite is intended to study polar ice. CryoSat - 2 undergoing testing at the Space Test Centre at IABG (Industrieanlagen - Betriebsgesellschaft mbH) in Ottobrunn, Germany in September 2009. CryoSat will be the third of ESA's Earth Explorer satellites in orbit. The 700 kg CryoSat spacecraft whose name comes from the Greek kryos meaning cold or ice carries the first all - weather microwave radar altimeter. The instrument has been optimised for determining changes in the thickness of both floating sea ice, which can be up to several meters, and polar land ice sheets, which in Antarctica can be close to 5 km thick. The mission will deliver data on the rate of change of the ice thickness accurate to within one centimetre

S. Corvaja

PIX4644073

La France vue la nuit - 2012 - France by night - 2012 - View of France at night composed of images taken by the Suomi NPP satellite in April and October 2012. This image of France at night is a composite assembled from data acquired by the Suomi NPP satellite in April and October 2012

La France vue la nuit - 2012 - France by night - 2012 - View of France at night composed of images taken by the Suomi NPP satellite in April and October 2012. This image of France at night is a composite assembled from data acquired by the Suomi NPP satellite in April and October 2012

PIX4665202

Tempete of 24 January 2009 over France seen by satellite - Storm above France seen by satellite. 24/01/2009 - The Tempete of 24 January 2009 seen by Envisat satellite at 10:12 am. Severe storm above France on January 24 2009 seen by the satellite Envisat at 10:12mn

Tempete of 24 January 2009 over France seen by satellite - Storm above France seen by satellite. 24/01/2009 - The Tempete of 24 January 2009 seen by Envisat satellite at 10:12 am. Severe storm above France on January 24 2009 seen by the satellite Envisat at 10:12mn

PIX4674286

Cyclone Yasi over Australia - February 2011 - Cyclone Yasi above Australia - Cyclone Yasi over Queensland seen by MTSAT satellite - 2 February 2011. Cyclone Yasi made landfall in Queensland, Australia in the early morning hours of February 3, 2011 as a Category 5 storm. This image of Cyclone Yasi uses MTSAT - 2 visible imagery from February 2, 2011 in late afternoon in Australia

Cyclone Yasi over Australia - February 2011 - Cyclone Yasi above Australia - Cyclone Yasi over Queensland seen by MTSAT satellite - 2 February 2011. Cyclone Yasi made landfall in Queensland, Australia in the early morning hours of February 3, 2011 as a Category 5 storm. This image of Cyclone Yasi uses MTSAT - 2 visible imagery from February 2, 2011 in late afternoon in Australia

PIX4674306

Earth by satellite - Earth seen by satellite

Earth by satellite - Earth seen by satellite

PIX4669205

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