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Mercury - Atlas 9: Astronaut Gordon Cooper before the start - Pilot and spacecraft - Astronaut L. Gordon Cooper, wearing his Mercury pressure suit, looks over the spacecraft which he named “” Faith 7”” at the top of the Pad 14 gantry at Cape Canaveral. Cooper is prime pilot for the MA - 9 mission - 196
Mercury - Atlas 9: Astronaut Gordon Cooper before the start - Pilot and spacecraft - Astronaut L. Gordon Cooper, wearing his Mercury pressure suit, looks over the spacecraft which he named “” Faith 7”” at the top of the Pad 14 gantry at Cape Canaveral. Cooper is prime pilot for the MA - 9 mission - 196

PIX4641897: Mercury - Atlas 9: Astronaut Gordon Cooper before the start - Pilot and spacecraft - Astronaut L. Gordon Cooper, wearing his Mercury pressure suit, looks over the spacecraft which he named “” Faith 7”” at the top of the Pad 14 gantry at Cape Canaveral. Cooper is prime pilot for the MA - 9 mission - 196 / Bridgeman Images

ID: PIX4641897

Mercury - Atlas 9: Astronaut Gordon Cooper before the start - Pilot and spacecraft - Astronaut L. Gordon Cooper, wearing his Mercury pressure suit, looks over the spacecraft which he named “” Faith 7”” at the top of the Pad 14 gantry at Cape Canaveral. Cooper is prime pilot for the MA - 9 mission - 196

Mercury - Atlas 9: No shooting the day before the decollage - View of the top of the Mercury - Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral, Florida. May 14 1963
Mercury - Atlas 9: No shooting the day before the decollage - View of the top of the Mercury - Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral, Florida. May 14 1963

PIX4641905: Mercury - Atlas 9: No shooting the day before the decollage - View of the top of the Mercury - Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral, Florida. May 14 1963 / Bridgeman Images

ID: PIX4641905

Mercury - Atlas 9: No shooting the day before the decollage - View of the top of the Mercury - Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral, Florida. May 14 1963

Mercury - Atlas 9: Return of Gordon Cooper - Astronaut Cooper, Gordon leaves Faith 7 Spacecraft After Recovery. MA - 9 was Launched on May 15,1963 One/onehalf Days Orbit Fligh
Mercury - Atlas 9: Return of Gordon Cooper - Astronaut Cooper, Gordon leaves Faith 7 Spacecraft After Recovery. MA - 9 was Launched on May 15,1963 One/onehalf Days Orbit Fligh

PIX4641939: Mercury - Atlas 9: Return of Gordon Cooper - Astronaut Cooper, Gordon leaves Faith 7 Spacecraft After Recovery. MA - 9 was Launched on May 15,1963 One/onehalf Days Orbit Fligh / Bridgeman Images

ID: PIX4641939

Mercury - Atlas 9: Return of Gordon Cooper - Astronaut Cooper, Gordon leaves Faith 7 Spacecraft After Recovery. MA - 9 was Launched on May 15,1963 One/onehalf Days Orbit Fligh

S.Lucid in Mir 09/1996 - S.Lucid in Mir station 09/1996 - Shannon Lucid observes cereal plants in Mir station. 23/09/1996. Astronaut Shannon W. Lucid, former cosmonaut guest researcher, checks on wheat plants aboard Russia's Mir Space Station, during Flight Day 8. Lucid, along with the rest of the STS - 79 crew except for John E. Blaha, current cosmonaut guest researcher, is leaving Mir today. 23 September 199
S.Lucid in Mir 09/1996 - S.Lucid in Mir station 09/1996 - Shannon Lucid observes cereal plants in Mir station. 23/09/1996. Astronaut Shannon W. Lucid, former cosmonaut guest researcher, checks on wheat plants aboard Russia's Mir Space Station, during Flight Day 8. Lucid, along with the rest of the STS - 79 crew except for John E. Blaha, current cosmonaut guest researcher, is leaving Mir today. 23 September 199

PIX4642198: S.Lucid in Mir 09/1996 - S.Lucid in Mir station 09/1996 - Shannon Lucid observes cereal plants in Mir station. 23/09/1996. Astronaut Shannon W. Lucid, former cosmonaut guest researcher, checks on wheat plants aboard Russia's Mir Space Station, during Flight Day 8. Lucid, along with the rest of the STS - 79 crew except for John E. Blaha, current cosmonaut guest researcher, is leaving Mir today. 23 September 199 / Bridgeman Images

ID: PIX4642198

S.Lucid in Mir 09/1996 - S.Lucid in Mir station 09/1996 - Shannon Lucid observes cereal plants in Mir station. 23/09/1996. Astronaut Shannon W. Lucid, former cosmonaut guest researcher, checks on wheat plants aboard Russia's Mir Space Station, during Flight Day 8. Lucid, along with the rest of the STS - 79 crew except for John E. Blaha, current cosmonaut guest researcher, is leaving Mir today. 23 September 199

Crews in Mir 06/98 - Crews Mir - 25 and STS - 91 in Mir, de g. a d.: Valery Ryumin, Wendy Lawrence, Charles Precourt, Andrew Thomas, Talgat Musabayev, Janet Kavandi, Dominic Gorie, Nikolai Budarin and Franklin Chang - Diaz. 12/06/1998
Crews in Mir 06/98 - Crews Mir - 25 and STS - 91 in Mir, de g. a d.: Valery Ryumin, Wendy Lawrence, Charles Precourt, Andrew Thomas, Talgat Musabayev, Janet Kavandi, Dominic Gorie, Nikolai Budarin and Franklin Chang - Diaz. 12/06/1998

PIX4642401: Crews in Mir 06/98 - Crews Mir - 25 and STS - 91 in Mir, de g. a d.: Valery Ryumin, Wendy Lawrence, Charles Precourt, Andrew Thomas, Talgat Musabayev, Janet Kavandi, Dominic Gorie, Nikolai Budarin and Franklin Chang - Diaz. 12/06/1998 / Bridgeman Images

ID: PIX4642401

Crews in Mir 06/98 - Crews Mir - 25 and STS - 91 in Mir, de g. a d.: Valery Ryumin, Wendy Lawrence, Charles Precourt, Andrew Thomas, Talgat Musabayev, Janet Kavandi, Dominic Gorie, Nikolai Budarin and Franklin Chang - Diaz. 12/06/1998

Deploiement du satellite LDEF - Deploiement du satellite LDEF (Long Duration Exposure Facility) seen from the Shuttle Challenger on April 7, 1984. This satellite remained in space for more than five years then was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space.
Deploiement du satellite LDEF - Deploiement du satellite LDEF (Long Duration Exposure Facility) seen from the Shuttle Challenger on April 7, 1984. This satellite remained in space for more than five years then was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space.

PIX4642482: Deploiement du satellite LDEF - Deploiement du satellite LDEF (Long Duration Exposure Facility) seen from the Shuttle Challenger on April 7, 1984. This satellite remained in space for more than five years then was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space. / Bridgeman Images

ID: PIX4642482

Deploiement du satellite LDEF - Deploiement du satellite LDEF (Long Duration Exposure Facility) seen from the Shuttle Challenger on April 7, 1984. This satellite remained in space for more than five years then was brought back to Earth to analyse the 57 experiments on board, intended to better understand the consequences of a long stay in space.

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 (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 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 (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

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 (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 / Bridgeman Images

ID: 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 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 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 (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

PIX4645755: 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 (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 / Bridgeman Images

ID: PIX4645755

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

Darwin Space Telescope - Illustration - Space Telescope Project consists of four telescopes measuring 3m in diameter observing infrared and operating interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth
Darwin Space Telescope - Illustration - Space Telescope Project consists of four telescopes measuring 3m in diameter observing infrared and operating interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth

PIX4645846: Darwin Space Telescope - Illustration - Space Telescope Project consists of four telescopes measuring 3m in diameter observing infrared and operating interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth / Bridgeman Images

ID: PIX4645846

Darwin Space Telescope - Illustration - Space Telescope Project consists of four telescopes measuring 3m in diameter observing infrared and operating interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth

Polar orbit of the Jason satellite - 1 - Polar orbit of Jason - 1 - Description of the polar orbit on which the Jason satellite is located - 1. Artwork showing the polar orbit where the satellite Jason - 1 is
Polar orbit of the Jason satellite - 1 - Polar orbit of Jason - 1 - Description of the polar orbit on which the Jason satellite is located - 1. Artwork showing the polar orbit where the satellite Jason - 1 is

PIX4644407: Polar orbit of the Jason satellite - 1 - Polar orbit of Jason - 1 - Description of the polar orbit on which the Jason satellite is located - 1. Artwork showing the polar orbit where the satellite Jason - 1 is / Bridgeman Images

ID: PIX4644407

Polar orbit of the Jason satellite - 1 - Polar orbit of Jason - 1 - Description of the polar orbit on which the Jason satellite is located - 1. Artwork showing the polar orbit where the satellite Jason - 1 is

TIROS satellite - 1 - under test - View of TIROS satellite - 1 (Television Infrared Observation Satellite) being tested at the Goddard Space Flight Center of Nasa. TIROS-1 was the first operational meteorological satellite; it was successfully launched on 1 April 1960
TIROS satellite - 1 - under test - View of TIROS satellite - 1 (Television Infrared Observation Satellite) being tested at the Goddard Space Flight Center of Nasa. TIROS-1 was the first operational meteorological satellite; it was successfully launched on 1 April 1960

PIX4644527: TIROS satellite - 1 - under test - View of TIROS satellite - 1 (Television Infrared Observation Satellite) being tested at the Goddard Space Flight Center of Nasa. TIROS-1 was the first operational meteorological satellite; it was successfully launched on 1 April 1960 / Bridgeman Images

ID: PIX4644527

TIROS satellite - 1 - under test - View of TIROS satellite - 1 (Television Infrared Observation Satellite) being tested at the Goddard Space Flight Center of Nasa. TIROS-1 was the first operational meteorological satellite; it was successfully launched on 1 April 1960

Satellite Meteosat in test in Cannes - A first generation Meteosat weather satellite undergoes final checks - View of a first generation Meteosat satellite in an Aerospatiale building in Cannes. A first generation Meteosat weather satellite undergoes final checks at Aerospace's satellite plant in Cannes, on the English Riviera
Satellite Meteosat in test in Cannes - A first generation Meteosat weather satellite undergoes final checks - View of a first generation Meteosat satellite in an Aerospatiale building in Cannes. A first generation Meteosat weather satellite undergoes final checks at Aerospace's satellite plant in Cannes, on the English Riviera

PIX4644547: Satellite Meteosat in test in Cannes - A first generation Meteosat weather satellite undergoes final checks - View of a first generation Meteosat satellite in an Aerospatiale building in Cannes. A first generation Meteosat weather satellite undergoes final checks at Aerospace's satellite plant in Cannes, on the English Riviera / Bridgeman Images

ID: PIX4644547

Satellite Meteosat in test in Cannes - A first generation Meteosat weather satellite undergoes final checks - View of a first generation Meteosat satellite in an Aerospatiale building in Cannes. A first generation Meteosat weather satellite undergoes final checks at Aerospace's satellite plant in Cannes, on the English Riviera

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 accurate short and medium - range forecasts
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 accurate short and medium - range forecasts

PIX4644648: 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 accurate short and medium - range forecasts / Bridgeman Images

ID: PIX4644648

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

Risorgimento: “” The Italian patriot Giuseppe Garibaldi passes the Volturno River”” Scene of the Battle of Volturno during the expedition of the Thousand (or Red Shirts) in October 1860. Painting by Francesco Mancini (1830-1905) Naples, Museo Nazionale di San Martino
Risorgimento: “” The Italian patriot Giuseppe Garibaldi passes the Volturno River”” Scene of the Battle of Volturno during the expedition of the Thousand (or Red Shirts) in October 1860. Painting by Francesco Mancini (1830-1905) Naples, Museo Nazionale di San Martino

LRI4644017: Risorgimento: “” The Italian patriot Giuseppe Garibaldi passes the Volturno River”” Scene of the Battle of Volturno during the expedition of the Thousand (or Red Shirts) in October 1860. Painting by Francesco Mancini (1830-1905) Naples, Museo Nazionale di San Martino, Mancini, Francesco (1694-1758) / Bridgeman Images

ID: LRI4644017

Risorgimento: “” The Italian patriot Giuseppe Garibaldi passes the Volturno River”” Scene of the Battle of Volturno during the expedition of the Thousand (or Red Shirts) in October 1860. Painting by Francesco Mancini (1830-1905) Naples, Museo Nazionale di San Martino

Mancini, Francesco (1694-1758)

Last session of the Senate of the Republic of Venice at the time of its entry into the Kingdom of Italy in 1866 (painting)
Last session of the Senate of the Republic of Venice at the time of its entry into the Kingdom of Italy in 1866 (painting)

LRI4644029: Last session of the Senate of the Republic of Venice at the time of its entry into the Kingdom of Italy in 1866 (painting), Jacovacci, Francesco (1838-1908) / Bridgeman Images

ID: LRI4644029

Last session of the Senate of the Republic of Venice at the time of its entry into the Kingdom of Italy in 1866 (painting)

Jacovacci, Francesco (1838-1908)

Old Neapolitan metiers: a pizza seller - 19th century watercolour - Naples Museo Nazionale di San Martino
Old Neapolitan metiers: a pizza seller - 19th century watercolour - Naples Museo Nazionale di San Martino

LRI4644219: Old Neapolitan metiers: a pizza seller - 19th century watercolour - Naples Museo Nazionale di San Martino, Italian School, (19th century) / Bridgeman Images

ID: LRI4644219

Old Neapolitan metiers: a pizza seller - 19th century watercolour - Naples Museo Nazionale di San Martino

Italian School, (19th century)

Neapolitan metiers: the seller of cherries from Marasca - (Old trade: the marasca cherries seller) Watercolour of the 19th century - Naples Museo Nazionale di San Martino
Neapolitan metiers: the seller of cherries from Marasca - (Old trade: the marasca cherries seller) Watercolour of the 19th century - Naples Museo Nazionale di San Martino

LRI4644256: Neapolitan metiers: the seller of cherries from Marasca - (Old trade: the marasca cherries seller) Watercolour of the 19th century - Naples Museo Nazionale di San Martino, Italian School, (19th century) / Bridgeman Images

ID: LRI4644256

Neapolitan metiers: the seller of cherries from Marasca - (Old trade: the marasca cherries seller) Watercolour of the 19th century - Naples Museo Nazionale di San Martino

Italian School, (19th century)

Petity Metier Neapolitan: a travelling seller of tablecloth and linen - (Old trade: tablecloth and linen seller) Painting by Pelliccia 19th century Museo Nazionale di San Martino Naples
Petity Metier Neapolitan: a travelling seller of tablecloth and linen - (Old trade: tablecloth and linen seller) Painting by Pelliccia 19th century Museo Nazionale di San Martino Naples

LRI4644319: Petity Metier Neapolitan: a travelling seller of tablecloth and linen - (Old trade: tablecloth and linen seller) Painting by Pelliccia 19th century Museo Nazionale di San Martino Naples, Pelliccia, (19th century) / Bridgeman Images

ID: LRI4644319

Petity Metier Neapolitan: a travelling seller of tablecloth and linen - (Old trade: tablecloth and linen seller) Painting by Pelliccia 19th century Museo Nazionale di San Martino Naples

Pelliccia, (19th century)

Spitzer space telescope - Artist's view - Artwork of Spitzer in its heliocentric orbit - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground
Spitzer space telescope - Artist's view - Artwork of Spitzer in its heliocentric orbit - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

PIX4645613: Spitzer space telescope - Artist's view - Artwork of Spitzer in its heliocentric orbit - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground / Bridgeman Images

ID: PIX4645613

Spitzer space telescope - Artist's view - Artwork of Spitzer in its heliocentric orbit - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

The Kepler Spacecraft: The Kepler satellite observes exoplanets in transit. Kepler is a satellite 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
The Kepler Spacecraft: The Kepler satellite observes exoplanets in transit. Kepler is a satellite 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

PIX4645639: The Kepler Spacecraft: The Kepler satellite observes exoplanets in transit. Kepler is a satellite 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 / Bridgeman Images

ID: PIX4645639

The Kepler Spacecraft: The Kepler satellite observes exoplanets in transit. Kepler is a satellite 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

La feast de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un salesman de cheeses et musicians (Cheese merchant and musicians) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino
La feast de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un salesman de cheeses et musicians (Cheese merchant and musicians) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino

LRI4643643: La feast de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un salesman de cheeses et musicians (Cheese merchant and musicians) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino, Gigante, Gaetano (1770-1840) / Bridgeman Images

ID: LRI4643643

La feast de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un salesman de cheeses et musicians (Cheese merchant and musicians) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino

Gigante, Gaetano (1770-1840)

La fete de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un vendeur de chestnuts (Chesnut seller) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino
La fete de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un vendeur de chestnuts (Chesnut seller) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino

LRI4643672: La fete de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un vendeur de chestnuts (Chesnut seller) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino, Gigante, Gaetano (1770-1840) / Bridgeman Images

ID: LRI4643672

La fete de la Madonna dell'Arco a Naples (Feast of the Madonna of the Arch) Detail d'un vendeur de chestnuts (Chesnut seller) - Painting by Gaetano Gigante (1770-1840) 1825 Naples, Museo Nazionale di San Martino

Gigante, Gaetano (1770-1840)

A Shipowner and a Lady detail of a genre painting, 18th (painting)
A Shipowner and a Lady detail of a genre painting, 18th (painting)

LRI4643752: A Shipowner and a Lady detail of a genre painting, 18th (painting), Fabris, Pietro (fl.1768-78) / Bridgeman Images

ID: LRI4643752

A Shipowner and a Lady detail of a genre painting, 18th (painting)

Fabris, Pietro (fl.1768-78)

People from Gallipoli, Apulia, Italy (People from Gallipoli) Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) Naples, Museo Nazionale di San Martino
People from Gallipoli, Apulia, Italy (People from Gallipoli) Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) Naples, Museo Nazionale di San Martino

LRI4643797: People from Gallipoli, Apulia, Italy (People from Gallipoli) Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) Naples, Museo Nazionale di San Martino, Hackert, Jacob-Philippe (1737-1807) / Bridgeman Images

ID: LRI4643797

People from Gallipoli, Apulia, Italy (People from Gallipoli) Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) Naples, Museo Nazionale di San Martino

Hackert, Jacob-Philippe (1737-1807)

View of Messina harbour, workers(Painting, 1791)
View of Messina harbour, workers(Painting, 1791)

LRI4643842: View of Messina harbour, workers(Painting, 1791), Hackert, Jacob-Philippe (1737-1807) / Bridgeman Images

ID: LRI4643842

View of Messina harbour, workers(Painting, 1791)

Hackert, Jacob-Philippe (1737-1807)

Groups of people on the dock of the port of Gaeta (Gaete) (People on the docks of Gaeta harbour) Detail - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807), 18th century - Museo Nazionale di San Martino Naples
Groups of people on the dock of the port of Gaeta (Gaete) (People on the docks of Gaeta harbour) Detail - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807), 18th century - Museo Nazionale di San Martino Naples

LRI4643858: Groups of people on the dock of the port of Gaeta (Gaete) (People on the docks of Gaeta harbour) Detail - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807), 18th century - Museo Nazionale di San Martino Naples, Hackert, Jacob-Philippe (1737-1807) / Bridgeman Images

ID: LRI4643858

Groups of people on the dock of the port of Gaeta (Gaete) (People on the docks of Gaeta harbour) Detail - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807), 18th century - Museo Nazionale di San Martino Naples

Hackert, Jacob-Philippe (1737-1807)

View of the military fortifications of the port of Reggio Calabria (View of Reggio Calabria military fortifications) Detail of a guard and canons (cannons and guard) - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) 18th century - Museo Nazionale di San Martino Naples
View of the military fortifications of the port of Reggio Calabria (View of Reggio Calabria military fortifications) Detail of a guard and canons (cannons and guard) - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) 18th century - Museo Nazionale di San Martino Naples

LRI4643861: View of the military fortifications of the port of Reggio Calabria (View of Reggio Calabria military fortifications) Detail of a guard and canons (cannons and guard) - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) 18th century - Museo Nazionale di San Martino Naples, Hackert, Jacob-Philippe (1737-1807) / Bridgeman Images

ID: LRI4643861

View of the military fortifications of the port of Reggio Calabria (View of Reggio Calabria military fortifications) Detail of a guard and canons (cannons and guard) - Painting by Jacob Philipp Hackert dit Hackert d'Italie (1737-1807) 18th century - Museo Nazionale di San Martino Naples

Hackert, Jacob-Philippe (1737-1807)

Allegory of the government of the city of Siena surrounded by citizens who are symbolically linked to it by a rope, 1385 (painting on wood)
Allegory of the government of the city of Siena surrounded by citizens who are symbolically linked to it by a rope, 1385 (painting on wood)

LRI4643310: Allegory of the government of the city of Siena surrounded by citizens who are symbolically linked to it by a rope, 1385 (painting on wood), Italian School, (14th century) / Bridgeman Images

ID: LRI4643310

Allegory of the government of the city of Siena surrounded by citizens who are symbolically linked to it by a rope, 1385 (painting on wood)

Italian School, (14th century)

Battle between Sienese and Florentines at Poggio Imperiale on 8/10/1479. Detail. Fresco by G. di Cristoforo and F. D'Andrea, 1480. Palazzo Pubblico, Siena
Battle between Sienese and Florentines at Poggio Imperiale on 8/10/1479. Detail. Fresco by G. di Cristoforo and F. D'Andrea, 1480. Palazzo Pubblico, Siena

LRI4643345: Battle between Sienese and Florentines at Poggio Imperiale on 8/10/1479. Detail. Fresco by G. di Cristoforo and F. D'Andrea, 1480. Palazzo Pubblico, Siena, Cristofano Ghini, Giovanni di & d’Andrea, Francesco (15th century) / Bridgeman Images

ID: LRI4643345

Battle between Sienese and Florentines at Poggio Imperiale on 8/10/1479. Detail. Fresco by G. di Cristoforo and F. D'Andrea, 1480. Palazzo Pubblico, Siena

Cristofano Ghini, Giovanni di & d’Andrea, Francesco (15th century)

Fete at Palazzo Barberini in honor of Christine de Suede (Cristina di Svezia), on 28/02/1656 Detail. Painting by Filippo Lauri (1623-1694) and Filippo Gagliardi (died 1659). 17th century Rome, Museum of Rome
Fete at Palazzo Barberini in honor of Christine de Suede (Cristina di Svezia), on 28/02/1656 Detail. Painting by Filippo Lauri (1623-1694) and Filippo Gagliardi (died 1659). 17th century Rome, Museum of Rome

LRI4643398: Fete at Palazzo Barberini in honor of Christine de Suede (Cristina di Svezia), on 28/02/1656 Detail. Painting by Filippo Lauri (1623-1694) and Filippo Gagliardi (died 1659). 17th century Rome, Museum of Rome, Lauri, Filippo (1623-94) / Bridgeman Images

ID: LRI4643398

Fete at Palazzo Barberini in honor of Christine de Suede (Cristina di Svezia), on 28/02/1656 Detail. Painting by Filippo Lauri (1623-1694) and Filippo Gagliardi (died 1659). 17th century Rome, Museum of Rome

Lauri, Filippo (1623-94)

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

PIX4644813: 2.4 m mirror inspects prior to installation on satellite - Inspection of the 94 inch primary mirror for Nasa's Hubble Space Telescope at Perkin-Elmers Optical facilities in Wilton, CT.: Mirror du telescope Hubble - The mirror of the Hubble space telescope / Bridgeman Images

ID: PIX4644813

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

Hubble Satellite Deployment 25 - 04 - 1990 - The Hubble Space Telescope deployment April 25 1990 - Seen from the window of the Shuttle Discovery. Grappled by the remote manipulator system end effector of Discovery, the Hubble Space Telescope is held in appendage deploy position. The starboard solar array wing and the two high gain antennae are fully extended. An STS - 31 crewmember took this view through aft flight deck window. The HST is backdropped against the Earth's limb
Hubble Satellite Deployment 25 - 04 - 1990 - The Hubble Space Telescope deployment April 25 1990 - Seen from the window of the Shuttle Discovery. Grappled by the remote manipulator system end effector of Discovery, the Hubble Space Telescope is held in appendage deploy position. The starboard solar array wing and the two high gain antennae are fully extended. An STS - 31 crewmember took this view through aft flight deck window. The HST is backdropped against the Earth's limb

PIX4644838: Hubble Satellite Deployment 25 - 04 - 1990 - The Hubble Space Telescope deployment April 25 1990 - Seen from the window of the Shuttle Discovery. Grappled by the remote manipulator system end effector of Discovery, the Hubble Space Telescope is held in appendage deploy position. The starboard solar array wing and the two high gain antennae are fully extended. An STS - 31 crewmember took this view through aft flight deck window. The HST is backdropped against the Earth's limb / Bridgeman Images

ID: PIX4644838

Hubble Satellite Deployment 25 - 04 - 1990 - The Hubble Space Telescope deployment April 25 1990 - Seen from the window of the Shuttle Discovery. Grappled by the remote manipulator system end effector of Discovery, the Hubble Space Telescope is held in appendage deploy position. The starboard solar array wing and the two high gain antennae are fully extended. An STS - 31 crewmember took this view through aft flight deck window. The HST is backdropped against the Earth's limb

Hubble Space Telescope: 2nd Maintenance Mission 02 - 1997 - View of astronauts Steven Smith (centre) and Mark Lee (right, arm) during the fifth and last extravehicular exit of this maintenance mission
Hubble Space Telescope: 2nd Maintenance Mission 02 - 1997 - View of astronauts Steven Smith (centre) and Mark Lee (right, arm) during the fifth and last extravehicular exit of this maintenance mission

PIX4644976: Hubble Space Telescope: 2nd Maintenance Mission 02 - 1997 - View of astronauts Steven Smith (centre) and Mark Lee (right, arm) during the fifth and last extravehicular exit of this maintenance mission / Bridgeman Images

ID: PIX4644976

Hubble Space Telescope: 2nd Maintenance Mission 02 - 1997 - View of astronauts Steven Smith (centre) and Mark Lee (right, arm) during the fifth and last extravehicular exit of this maintenance mission

Hubble Space Telescope: 2nd maintenance mission 02 - 1997 - Redeployment of the telescope after its second maintenance mission
Hubble Space Telescope: 2nd maintenance mission 02 - 1997 - Redeployment of the telescope after its second maintenance mission

PIX4644985: Hubble Space Telescope: 2nd maintenance mission 02 - 1997 - Redeployment of the telescope after its second maintenance mission / Bridgeman Images

ID: PIX4644985

Hubble Space Telescope: 2nd maintenance mission 02 - 1997 - Redeployment of the telescope after its second maintenance mission

Hubble Space Telescope: 3rd maintenance mission 12 - 1999 - View of astronauts Michael Foale (left) and Claude Nicollier (on arm) during the second extravehicular exit of this maintenance mission, 23 - 12 - 1999
Hubble Space Telescope: 3rd maintenance mission 12 - 1999 - View of astronauts Michael Foale (left) and Claude Nicollier (on arm) during the second extravehicular exit of this maintenance mission, 23 - 12 - 1999

PIX4645060: Hubble Space Telescope: 3rd maintenance mission 12 - 1999 - View of astronauts Michael Foale (left) and Claude Nicollier (on arm) during the second extravehicular exit of this maintenance mission, 23 - 12 - 1999 / Bridgeman Images

ID: PIX4645060

Hubble Space Telescope: 3rd maintenance mission 12 - 1999 - View of astronauts Michael Foale (left) and Claude Nicollier (on arm) during the second extravehicular exit of this maintenance mission, 23 - 12 - 1999

Galileo satellites - Illustration - Artist's view of the European satellite network Galileo consists of 30 satellites at about 24,000 km of altitude (27 operationals, 3 reserve). This satellite positioning system is expected to be operational in 2011
Galileo satellites - Illustration - Artist's view of the European satellite network Galileo consists of 30 satellites at about 24,000 km of altitude (27 operationals, 3 reserve). This satellite positioning system is expected to be operational in 2011

PIX4643031: Galileo satellites - Illustration - Artist's view of the European satellite network Galileo consists of 30 satellites at about 24,000 km of altitude (27 operationals, 3 reserve). This satellite positioning system is expected to be operational in 2011 / Bridgeman Images

ID: PIX4643031

Galileo satellites - Illustration - Artist's view of the European satellite network Galileo consists of 30 satellites at about 24,000 km of altitude (27 operationals, 3 reserve). This satellite positioning system is expected to be operational in 2011


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