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Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

PIX4644143

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

PIX4644760

Satellite Integral - Illustration - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) observing a black hole. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

Satellite Integral - Illustration - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) observing a black hole. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

D. Ducros

PIX4646229

Satellite ERS-1 - Artist's view of the European satellite ERS-1 (European Remote Sensing - 1) in orbit around the Earth. Launched in July 1991, this radar satellite observes the Earth. ERS - 1 artist composition over the coast of the Netherlands. ERS-1 (European Remote Sensing Satellite) was put into orbit by Ariane in July 1991. Since then, day and night and even through the densest clouds, it has been using its three intsruments to survey the structure of the planets surface, taking radar images that reveal the smallest details and monitor changes

Satellite ERS-1 - Artist's view of the European satellite ERS-1 (European Remote Sensing - 1) in orbit around the Earth. Launched in July 1991, this radar satellite observes the Earth. ERS - 1 artist composition over the coast of the Netherlands. ERS-1 (European Remote Sensing Satellite) was put into orbit by Ariane in July 1991. Since then, day and night and even through the densest clouds, it has been using its three intsruments to survey the structure of the planets surface, taking radar images that reveal the smallest details and monitor changes

PIX4644282

Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

PIX4644635

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

Artist view of the European satellite GOCE in orbit around the Earth - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Artist view of the European satellite GOCE in orbit around the Earth - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

P. Carril

PIX4644095

Artist view of the European satellite GOCE in orbit around the Earth. - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Artist view of the European satellite GOCE in orbit around the Earth. - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

P. Carril

PIX4644100

Artist view of the European satellite GOCE in orbit around the Earth. - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Artist view of the European satellite GOCE in orbit around the Earth. - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

P. Carril

PIX4644106

Microsatellite TARANIS - Jet Bleu, Elf and Sprites - Microsatellite TARANIS - Blue jet, Elves and Sprites - Artist's view of the French satellite TARANIS observing a blue jet, elves (halos) and sprites (or red sylphs). TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching blue jet, elves and sprites. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

Microsatellite TARANIS - Jet Bleu, Elf and Sprites - Microsatellite TARANIS - Blue jet, Elves and Sprites - Artist's view of the French satellite TARANIS observing a blue jet, elves (halos) and sprites (or red sylphs). TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching blue jet, elves and sprites. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

D. Ducros

PIX4644258

Satellite Jason - 2 - Illustration - Artist's view of the satellite Jason - 2 in orbit around the Earth. This satellite launched on 20 June 2008 is dedicated to the study of the oceans. Artist's concept of the satellite Jason - 2. This satellite dedicated to studying the ocean was launched on June 20 2008

Satellite Jason - 2 - Illustration - Artist's view of the satellite Jason - 2 in orbit around the Earth. This satellite launched on 20 June 2008 is dedicated to the study of the oceans. Artist's concept of the satellite Jason - 2. This satellite dedicated to studying the ocean was launched on June 20 2008

D. Ducros

PIX4644458

Satellite Herschel - Illustration - Ariane 5 stage with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying 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 is in 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory

Satellite Herschel - Illustration - Ariane 5 stage with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying 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 is in 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory

D. Ducros

PIX4646153

Satellite Signe - 3 - Artist's view - Satellite Signe - 3. Artwork - Artist's view of the satellite Signe - 3 (Solar Interplanetary Gamma Ray Neutron Experiment) in orbit around the Earth. Lance on June 17, 1977, he studied the sources of gamma radiation from the sky. Satellite Signe - 3 (Solar Interplanetary Gamma Ray Neutron Experiment) seen above the Earth. This english satellite was launched on June 17 1977 and studied gamma rays

Satellite Signe - 3 - Artist's view - Satellite Signe - 3. Artwork - Artist's view of the satellite Signe - 3 (Solar Interplanetary Gamma Ray Neutron Experiment) in orbit around the Earth. Lance on June 17, 1977, he studied the sources of gamma radiation from the sky. Satellite Signe - 3 (Solar Interplanetary Gamma Ray Neutron Experiment) seen above the Earth. This english satellite was launched on June 17 1977 and studied gamma rays

D. Ducros

PIX4646264

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

PIX4644128

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

PIX4644136

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Satellite GOCE - Artist view - GOCE satellite - Artist view - Artist view of the European satellite GOCE in orbit around the Earth. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE in Earth orbit. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

PIX4644152

Satellite Sentinel-2 - Artist's view: Artist's view of the European Sentinel-2 satellite orbiting the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel-2A was launched on 23 June 2015 and Sentinel-2B will be launched in 2016 - Sentinel-2 carries a high-resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land-cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information on pollution in lakes

Satellite Sentinel-2 - Artist's view: Artist's view of the European Sentinel-2 satellite orbiting the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel-2A was launched on 23 June 2015 and Sentinel-2B will be launched in 2016 - Sentinel-2 carries a high-resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land-cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information on pollution in lakes

PIX4644364

Satellite MSG - 1 - Meteosat 8 - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more accurate short and medium - range forecasts

Satellite MSG - 1 - Meteosat 8 - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more accurate short and medium - range forecasts

D. Ducros

PIX4644628

Meteorology satellites MTG - MTG satellites. Artwork - Artist's view of the European satellite project MTG (Meteosat Third Generation). The MTG system will consist of twin satellites - an imager (MTG-I) and a sounder (MTG-S). This development programme will run from 2009 to 2020. Artist view of european meteorological satellites MTG (Meteosat Third Generation). MTG will be three - axis stabilized and based on a twin - satellite concept. Under this concept, there will be two types of satellites, one for imaging (MTG - I) and one for sounding (MTG - S). The development programme will last from 2009 until 2020

Meteorology satellites MTG - MTG satellites. Artwork - Artist's view of the European satellite project MTG (Meteosat Third Generation). The MTG system will consist of twin satellites - an imager (MTG-I) and a sounder (MTG-S). This development programme will run from 2009 to 2020. Artist view of european meteorological satellites MTG (Meteosat Third Generation). MTG will be three - axis stabilized and based on a twin - satellite concept. Under this concept, there will be two types of satellites, one for imaging (MTG - I) and one for sounding (MTG - S). The development programme will last from 2009 until 2020

P. Carril

PIX4644683

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

PIX4644746

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

Iris: system for air traffic management - Iris: satellite communications for air traffic management - Artist's view of the European telecommunication system Iris for air traffic management. Iris, element 10 of the ARTES programme, aims to develop a new Air - Ground Communication system for Air Traffic Management. By 2020 it will contribute to the modernisation of air traffic management by providing digital datalinks to cockpit crews in continental and oceanic airspace

Iris: system for air traffic management - Iris: satellite communications for air traffic management - Artist's view of the European telecommunication system Iris for air traffic management. Iris, element 10 of the ARTES programme, aims to develop a new Air - Ground Communication system for Air Traffic Management. By 2020 it will contribute to the modernisation of air traffic management by providing digital datalinks to cockpit crews in continental and oceanic airspace

P. Carril

PIX4642990

Artist view of the European satellite GOCE put into orbit by a Rockot rocket - GOCE satellite - Artist view - Artist view of the European satellite GOCE put into orbit by a Rockot rocket. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE launched by a Rockot launcher. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

Artist view of the European satellite GOCE put into orbit by a Rockot rocket - GOCE satellite - Artist view - Artist view of the European satellite GOCE put into orbit by a Rockot rocket. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) is expected to be launched in 2009. Artist view of the European satellite GOCE launched by a Rockot launcher. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and is scheduled in 2009

P. Carril

PIX4644127

MSG-2 satellite (Meteosat 9) - View of the European satellite MSG-2 (Meteosat Second Generation) or Meteosat 9 in a clean room at the Guyanese Space Centre on 13 December 2005. Launch on 21 December 2005, it is a geostationary satellite dedicated to meteorology. MSG-2, the second model of the Meteosat Second Generation satellite series, is mated on top of its Ariane 5 launcher in the Final Assembly Building (BAF) of the Ariane Maunch Complex n* 3 (ELA-3) at the Guiana Space Centre, Europe's space port in Kourou, French Guiana, on December 13, 2005. The 2 - ton MSG - 2 was successfully lofted onto a geostationary transfer orbit by an Ariane 5GS (V169), on December 21, together with India's Insat 4A satellite communication

MSG-2 satellite (Meteosat 9) - View of the European satellite MSG-2 (Meteosat Second Generation) or Meteosat 9 in a clean room at the Guyanese Space Centre on 13 December 2005. Launch on 21 December 2005, it is a geostationary satellite dedicated to meteorology. MSG-2, the second model of the Meteosat Second Generation satellite series, is mated on top of its Ariane 5 launcher in the Final Assembly Building (BAF) of the Ariane Maunch Complex n* 3 (ELA-3) at the Guiana Space Centre, Europe's space port in Kourou, French Guiana, on December 13, 2005. The 2 - ton MSG - 2 was successfully lofted onto a geostationary transfer orbit by an Ariane 5GS (V169), on December 21, together with India's Insat 4A satellite communication

PIX4644590

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: 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

PIX4645443

The London Flower Mission, Clerkenwell Close, London - Making artificial flowers (engraving)

The London Flower Mission, Clerkenwell Close, London - Making artificial flowers (engraving)

Barnes, Robert (1840-95)

LLJ607839

Illustration for The Essays of Elia by Charles Lamb (litho)

Illustration for The Essays of Elia by Charles Lamb (litho)

Jones, A. Garth (1872-1955)

LLM3642146

An artificial eye from a Inca Mummy

An artificial eye from a Inca Mummy

UIG2910715

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 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

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

Artist view of the European satellite GOCE put into orbit by a Rockot rocket - GOCE satellite - Artist view - Artist view of the European satellite GOCE put into orbit by a Rockot rocket. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) was launched on 17 March 2009. Artist view of the European satellite GOCE launched by a Rockot launcher. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and was launched on March 17, 2009

Artist view of the European satellite GOCE put into orbit by a Rockot rocket - GOCE satellite - Artist view - Artist view of the European satellite GOCE put into orbit by a Rockot rocket. GoCE (Gravity - Field and Steady - State Ocean Circulation Explorer) was launched on 17 March 2009. Artist view of the European satellite GOCE launched by a Rockot launcher. GOCE (Gravity - Field and Steady - State Ocean Circulation Explorer) aims to measure the Earth's gravitational field and was launched on March 17, 2009

P. Carril

PIX4644117

Satellite Sentinel - 1 - Illustration - Artist's view of the European satellite Sentinel - 1 in orbit around the Earth. This satellite has a five-metre resolution radar, is the first of a series of satellites forming the Earth monitoring network of the Copernicus programme (formerly GMES), and together they will study the changes in the Earth's environment. The Sentinel-1 mission consists of two satellites in polar orbit. Sentinel - 1 carries an advanced synthetic aperture radar that works in several specialised modes to provide detailed imagery for Europe's Copernicus programme. These data will be used for applications such as monitoring the oceans, including shipping lanes, sea ice and oil spills. It also provides data to map changing land cover, ground deformation, ice shelves and glaciers, and can be used to help emergency response when disasters such as floods strike and to support humanitarian relief efforts at times of crisis. The SENTINEL - 1 mission comprises a constellation o

Satellite Sentinel - 1 - Illustration - Artist's view of the European satellite Sentinel - 1 in orbit around the Earth. This satellite has a five-metre resolution radar, is the first of a series of satellites forming the Earth monitoring network of the Copernicus programme (formerly GMES), and together they will study the changes in the Earth's environment. The Sentinel-1 mission consists of two satellites in polar orbit. Sentinel - 1 carries an advanced synthetic aperture radar that works in several specialised modes to provide detailed imagery for Europe's Copernicus programme. These data will be used for applications such as monitoring the oceans, including shipping lanes, sea ice and oil spills. It also provides data to map changing land cover, ground deformation, ice shelves and glaciers, and can be used to help emergency response when disasters such as floods strike and to support humanitarian relief efforts at times of crisis. The SENTINEL - 1 mission comprises a constellation o

PIX4644310

Satellite Jason - 1 - Illustration - Artist's view of the satellite Jason - 1 in orbit around the Earth. This satellite launched on 7 December 2001 is dedicated to the study of oceans. Artist's concept of the satellite Jason - 1. This satellite dedicated to studying the ocean was launched on December 7, 2001

Satellite Jason - 1 - Illustration - Artist's view of the satellite Jason - 1 in orbit around the Earth. This satellite launched on 7 December 2001 is dedicated to the study of oceans. Artist's concept of the satellite Jason - 1. This satellite dedicated to studying the ocean was launched on December 7, 2001

D. Ducros

PIX4644478

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying 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 is in 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observato

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying 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 is in 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observato

D. Ducros

PIX4646169

Satellite MSG - 1 - Meteosat 8 - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation, MSG) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Artist's view of Meteosat Second Generation (MSG). Satellite observations from space contribute to better weather forecasts as only satellites can observe weather patterns on a global scale, including the Atlantic Ocean over which most of Europe's weather originates

Satellite MSG - 1 - Meteosat 8 - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation, MSG) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Artist's view of Meteosat Second Generation (MSG). Satellite observations from space contribute to better weather forecasts as only satellites can observe weather patterns on a global scale, including the Atlantic Ocean over which most of Europe's weather originates

D. Ducros

PIX4644645

Satellite MSG - 1 - Meteosat 8 - Anaglyph - Satellite MSG - 1 - Meteosat 8 - Anaglyph - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more acc

Satellite MSG - 1 - Meteosat 8 - Anaglyph - Satellite MSG - 1 - Meteosat 8 - Anaglyph - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more acc

D. Ducros

PIX4644648

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 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

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

Spot satellites - Artist's view of Earth observation satellites Spot. Artwork showing the earth observation satellite SPOT family

Spot satellites - Artist's view of Earth observation satellites Spot. Artwork showing the earth observation satellite SPOT family

D. Ducros

PIX4643995

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) - 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

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

Dr. Michael DeBakey examining his artificial heart implant patient, Marcel De Rudder, Houston, 4/23/1966

Dr. Michael DeBakey examining his artificial heart implant patient, Marcel De Rudder, Houston, 4/23/1966

EVB2952572

Imitation emerald

Imitation emerald

NHM1453586

Dr Michael DeBakey showing artificial heart at a news briefing in Houston, 1/5/1971

Dr Michael DeBakey showing artificial heart at a news briefing in Houston, 1/5/1971

EVB2952571

The entrance to Coade and Sealy's (engraving)

The entrance to Coade and Sealy's (engraving)

Rawle, Samuel (1771-1860)

LLJ605064

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observa

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. 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. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observa

D. Ducros

PIX4646125

Artificial Flower Making (chromolitho)

Artificial Flower Making (chromolitho)

European School, (19th century)

LLR735565

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

PIX4645452

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

PIX4645465

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - 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: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - 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

PIX4645502

The Use of Ultra-Violet Rays, cover illustration from 'Le Petit Inventeur', 1929 (colour litho)

The Use of Ultra-Violet Rays, cover illustration from 'Le Petit Inventeur', 1929 (colour litho)

French School, (20th century)

CHT234590

Sinking Blocks of artificial Stone at Cherbourg (engraving)

Sinking Blocks of artificial Stone at Cherbourg (engraving)

European School, (19th century)

LLM3624791

Satellite Sentinel - 1 - Illustration - Artist's view of the European satellite Sentinel - 1 in orbit around the Earth. This satellite has a five-metre resolution radar, is the first of a series of satellites forming the Earth monitoring network of the Copernicus programme (formerly GMES), and together they will study the changes in the Earth's environment. The Sentinel-1 mission consists of two satellites in polar orbit. Sentinel - 1a was launched on April 3, 2014. Sentinel - 1 carries an advanced synthetic aperture radar that works in several specialised modes to provide detailed imagery for Europe's Copernicus programme. These data will be used for applications such as monitoring the oceans, including shipping lanes, sea ice and oil spills. It also provides data to map changing land cover, ground deformation, ice shelves and glaciers, and can be used to help emergency response when disasters such as floods strike and to support humanitarian relief efforts at times of crisis. The SEN

Satellite Sentinel - 1 - Illustration - Artist's view of the European satellite Sentinel - 1 in orbit around the Earth. This satellite has a five-metre resolution radar, is the first of a series of satellites forming the Earth monitoring network of the Copernicus programme (formerly GMES), and together they will study the changes in the Earth's environment. The Sentinel-1 mission consists of two satellites in polar orbit. Sentinel - 1a was launched on April 3, 2014. Sentinel - 1 carries an advanced synthetic aperture radar that works in several specialised modes to provide detailed imagery for Europe's Copernicus programme. These data will be used for applications such as monitoring the oceans, including shipping lanes, sea ice and oil spills. It also provides data to map changing land cover, ground deformation, ice shelves and glaciers, and can be used to help emergency response when disasters such as floods strike and to support humanitarian relief efforts at times of crisis. The SEN

PIX4644317

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

PIX4645302

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

PIX4645459

James Webb Space Telescope (JWST) - JWST Set for Testing in Space Simulation Chamber: The James Webb Space Telescope (JWST) in front of the empty chamber door of Nasa's Johnson Space Center. He'll be locked up for a series of tests. 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. 25 May 2017. Nasa's James Webb Space Telescope sits in front of the door to Chamber A, a giant thermal vacuum chamber located at Nasa's Johnson Space Center. The telescope will soon be moved into the chamber, where it will spend a hot Houston summer undergoing tests at sub-freezing cryogenic temperatures. The telescope will operate at an extremely cold 39 K (-234* C or -389* F) in space, so NASA is simulating those conditions on the ground, ensuring the optics and instruments will perform perfectly after launch. May 25 2017.

James Webb Space Telescope (JWST) - JWST Set for Testing in Space Simulation Chamber: The James Webb Space Telescope (JWST) in front of the empty chamber door of Nasa's Johnson Space Center. He'll be locked up for a series of tests. 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. 25 May 2017. Nasa's James Webb Space Telescope sits in front of the door to Chamber A, a giant thermal vacuum chamber located at Nasa's Johnson Space Center. The telescope will soon be moved into the chamber, where it will spend a hot Houston summer undergoing tests at sub-freezing cryogenic temperatures. The telescope will operate at an extremely cold 39 K (-234* C or -389* F) in space, so NASA is simulating those conditions on the ground, ensuring the optics and instruments will perform perfectly after launch. May 25 2017.

PIX4607506

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Examination of two mirrors of the James Webb Space Telescope (JWST) 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 - Inside Nasa's Goddard Space Flight Center's giant clean room in Greenbelt, Md., JWST Optical Engineer Larkin Carey from Ball Aerospace, examines two test mirror segments recently placed on a black composite structure. This black composite structure is called the James Webb Space Telescope's “” Pathfinder”” and acts as a spine supporting the telescope's primary mirror segments. The Pathfinder is a non-flight prototype - The mirrors were placed on Pathfinder using a robotic arm move that involved highly trained engineers and technicians from Exelis, Northrop Grumman and NASA - The James Webb Space Telescope is the successor to NASA's Hubble Space Telescope. It will be the most pow

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Examination of two mirrors of the James Webb Space Telescope (JWST) 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 - Inside Nasa's Goddard Space Flight Center's giant clean room in Greenbelt, Md., JWST Optical Engineer Larkin Carey from Ball Aerospace, examines two test mirror segments recently placed on a black composite structure. This black composite structure is called the James Webb Space Telescope's “” Pathfinder”” and acts as a spine supporting the telescope's primary mirror segments. The Pathfinder is a non-flight prototype - The mirrors were placed on Pathfinder using a robotic arm move that involved highly trained engineers and technicians from Exelis, Northrop Grumman and NASA - The James Webb Space Telescope is the successor to NASA's Hubble Space Telescope. It will be the most pow

PIX4645828

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

PIX4646327

Ice Mountains, the artificial sledge runs which were constructed during the winter for public amusement in Russian cities such as St Petersburg and Moscow. Woodcut, 1833.

Ice Mountains, the artificial sledge runs which were constructed during the winter for public amusement in Russian cities such as St Petersburg and Moscow. Woodcut, 1833.

UIG530596

Douglasss Artificial Leg

Douglasss Artificial Leg

UIG2902336

Launch of the space telescope XMM - Newton - Artist's view - Launch of XMM - Newton space telescope - The space telescope XMM - Newton is a European satellite that observes the Universe in X-ray; it was launched and put into orbit in December 1999 by an Ariane 5 rocket. XMM - Newton is an european X - Ray observatory launched in december 1999 by an Ariane 5 rocket

Launch of the space telescope XMM - Newton - Artist's view - Launch of XMM - Newton space telescope - The space telescope XMM - Newton is a European satellite that observes the Universe in X-ray; it was launched and put into orbit in December 1999 by an Ariane 5 rocket. XMM - Newton is an european X - Ray observatory launched in december 1999 by an Ariane 5 rocket

D. Ducros

PIX4645580

Shuttle Discovery in orbit and satellite 06/1999 - Shuttle Discovery with a satellite 06/1999 - STARSHINE (Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment) leaves Shuttle Discovery. The Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment (STARSHINE) satellite leaves the cargo bay of Discovery near the completion of the STS-96. Jun 05 1999

Shuttle Discovery in orbit and satellite 06/1999 - Shuttle Discovery with a satellite 06/1999 - STARSHINE (Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment) leaves Shuttle Discovery. The Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment (STARSHINE) satellite leaves the cargo bay of Discovery near the completion of the STS-96. Jun 05 1999

PIX4647712

Satellite INTEGRAL - Artist's view - Satellite INTEGRAL. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) in orbit around the Earth. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

Satellite INTEGRAL - Artist's view - Satellite INTEGRAL. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) in orbit around the Earth. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

D. Ducros

PIX4646238

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

Microsatellite TARANIS et Elfe - Artist view - Microsatellite TARANIS and elve - Artist view - Artist view of the french satellite TARANIS observing an elf (luminous disc in the ionosphere). TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching an elve. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

Microsatellite TARANIS et Elfe - Artist view - Microsatellite TARANIS and elve - Artist view - Artist view of the french satellite TARANIS observing an elf (luminous disc in the ionosphere). TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching an elve. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

D. Ducros

PIX4644340

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

PIX4645724

The points of Lagrange and the satellite SOHO - Lagrangian points with Soho spacecraft - Schema showing the different points of Lagrange and the position of the satellite SOHO (Solar and Heliospheric Observatory), place near the point of Lagrange L1. Launched in December 1995, this satellite observes the Sun. Artwork showing the different Lagrange points with the Soho spacecraft located around the L1 point

The points of Lagrange and the satellite SOHO - Lagrangian points with Soho spacecraft - Schema showing the different points of Lagrange and the position of the satellite SOHO (Solar and Heliospheric Observatory), place near the point of Lagrange L1. Launched in December 1995, this satellite observes the Sun. Artwork showing the different Lagrange points with the Soho spacecraft located around the L1 point

D. Ducros

PIX4646287

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

Satellite COROT - Artist's view of COROT - Artist's view of COROT - Artist's view of the satellite COROT in space. Launched at the end of December 2006, this satellite studies the physical phenomena occurring inside the stars. It is also used for the detection of extrasolar planets by observing the periodic micro-eclipses that these planets cause by passing in front of their mother star. Artist's view of COROT, the exoplanet hunter mission led by CNES, with ESA participation. Launched in December 2006, COROT is placed on a circular, polar orbit around Earth that allow for continuous observations of two large and opposite regions in the sky for more than 150 days each. Within each region there are many selected fields that will be monitored in turn. The reason for the oppositely sited regions is that, because of the Earth's movement around the Sun, the sun's rays start to interfere with the observations after 150 days. COROT then rotates by 180 degrees and start observing the other regi

Satellite COROT - Artist's view of COROT - Artist's view of COROT - Artist's view of the satellite COROT in space. Launched at the end of December 2006, this satellite studies the physical phenomena occurring inside the stars. It is also used for the detection of extrasolar planets by observing the periodic micro-eclipses that these planets cause by passing in front of their mother star. Artist's view of COROT, the exoplanet hunter mission led by CNES, with ESA participation. Launched in December 2006, COROT is placed on a circular, polar orbit around Earth that allow for continuous observations of two large and opposite regions in the sky for more than 150 days each. Within each region there are many selected fields that will be monitored in turn. The reason for the oppositely sited regions is that, because of the Earth's movement around the Sun, the sun's rays start to interfere with the observations after 150 days. COROT then rotates by 180 degrees and start observing the other regi

D. Ducros

PIX4645890

Artificial Lake for a Dinner Table (engraving)

Artificial Lake for a Dinner Table (engraving)

English School, (19th century)

LLM3628642

Manufacturing of artificial ice (chromolitho)

Manufacturing of artificial ice (chromolitho)

European School, (19th century)

LLM968619

Leg Replacement

Leg Replacement

UIG2902372

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

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

PIX4646332

Artificial bismuth crystals

Artificial bismuth crystals

NHM1460350

Launch of satellite METOP - A - Launch of satellite METOP - A - Artist's view of the European satellite METOP - A put into orbit by a Soyuz - Fregat rocket. Launched on October 19, 2006, it is the first European meteorological satellite in polar orbit; it includes twelve meteorological instruments. Launch of satellite METOP - A by a Soyuz rocket. MetOp is a series of three meteorological operational polar orbiting satellites, the first of which, MetOp - A 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

Launch of satellite METOP - A - Launch of satellite METOP - A - Artist's view of the European satellite METOP - A put into orbit by a Soyuz - Fregat rocket. Launched on October 19, 2006, it is the first European meteorological satellite in polar orbit; it includes twelve meteorological instruments. Launch of satellite METOP - A by a Soyuz rocket. MetOp is a series of three meteorological operational polar orbiting satellites, the first of which, MetOp - A 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

PIX4644759

Launch of the Helios 2A satellite - Satellite Helios 2A launch - Artist's view of the launch of the military satellite Helios 2A and the parasol and swarm microsatellites by an Ariane 5 G+rocket in December 2004. Artwork of the launch of the military satellite Helios 2A with the microsatellites Essaim and Parasol by an ariane 5 rocket in december 2004

Launch of the Helios 2A satellite - Satellite Helios 2A launch - Artist's view of the launch of the military satellite Helios 2A and the parasol and swarm microsatellites by an Ariane 5 G+rocket in December 2004. Artwork of the launch of the military satellite Helios 2A with the microsatellites Essaim and Parasol by an ariane 5 rocket in december 2004

D. Ducros

PIX4644070

Microsatellite TARANIS et Jet Bleu - Vue d'artiste - Microsatellite TARANIS and Blue jet - Artist view - Vue d'artiste du satellite francais TARANIS observant un jet bleu. TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching a blue jet. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

Microsatellite TARANIS et Jet Bleu - Vue d'artiste - Microsatellite TARANIS and Blue jet - Artist view - Vue d'artiste du satellite francais TARANIS observant un jet bleu. TARANIS (for Tool for the Analysis of Radiation from LightNing and Sprites) will study in particular the light phenomena ephemeres (or TLE) that occur in the high atmosphere. Artist view of the CNES satellite TARANIS (for Tool for the Analysis of Radiation from Lightning and Sprites) watching a blue jet. This microsatellite will study the transient luminous events (TLE) which appear in the high atmosphere

D. Ducros

PIX4644308

Artemis communication satellite - Artemis satellite communication. Artwork - Artist's view of the European satellite Artemis (Advanced Relay and Technology Mission). Communication and relay satellite for other satellites, it was launched in July 2001. Built by ESA with an industrial team led by Italy's Alenia Spazio, Artemis carries three payloads plus a number of experiments developed to demonstrate new telecommunications technologies. The L - band Land Mobile (LLM) payload provides relay for two - way voice and data communications between fixed Earth stations and land mobiles - trucks, trains or cars - anywhere in Europe and North Africa. LLM is also broadcasting corrective GPS - like navigation signals for the European Global Navigation Overlay Service (EGNOS) programme, Europe's first satellite navigation system and a forerunner to the Galileo global navigation system. The other two primary payloads are designed to provide direct high data rate communications links between satellit

Artemis communication satellite - Artemis satellite communication. Artwork - Artist's view of the European satellite Artemis (Advanced Relay and Technology Mission). Communication and relay satellite for other satellites, it was launched in July 2001. Built by ESA with an industrial team led by Italy's Alenia Spazio, Artemis carries three payloads plus a number of experiments developed to demonstrate new telecommunications technologies. The L - band Land Mobile (LLM) payload provides relay for two - way voice and data communications between fixed Earth stations and land mobiles - trucks, trains or cars - anywhere in Europe and North Africa. LLM is also broadcasting corrective GPS - like navigation signals for the European Global Navigation Overlay Service (EGNOS) programme, Europe's first satellite navigation system and a forerunner to the Galileo global navigation system. The other two primary payloads are designed to provide direct high data rate communications links between satellit

J. Huart

PIX4642928

Natural and artificial teeth (engraving)

Natural and artificial teeth (engraving)

English School, (19th century)

LLM5223894

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

Royal Surrey Zoological Gardens (engraving)

Royal Surrey Zoological Gardens (engraving)

English School, (19th century)

LLJ610409

Edmond Carre's apparatus for the artificial production of ice

Edmond Carre's apparatus for the artificial production of ice

UIG3735903

Satellite Integral - Illustration - Satellite INTEGRAL in Proton fairing. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) during the opening of the cap of the Proton rocket. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

Satellite Integral - Illustration - Satellite INTEGRAL in Proton fairing. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) during the opening of the cap of the Proton rocket. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

D. Ducros

PIX4646258

Satellite Integral - Illustration - Satellite INTEGRAL in Proton fairing. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) during the opening of the cap of the Proton rocket. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

Satellite Integral - Illustration - Satellite INTEGRAL in Proton fairing. Artwork - Artist's view of the European satellite INTEGRAL (International Gamma - Ray Astrophysics Laboratory) during the opening of the cap of the Proton rocket. Integral (International Gamma - Ray Astrophysics Laboratory) is the first space observatory that can simultaneously observe objects in gamma rays, X - rays, and visible light. Its main targets are violent explosions known as gamma - ray bursts, powerful phenomena such as supernova explosions, and regions in the Universe thought to contain black holes. Launched on 17 October 2002 (Proton launcher from Baikonur, Kazakhstan)

D. Ducros

PIX4646283

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