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Metro station les Abbesses, Place des Abbesses, Paris 75018. Architect Hector Guimard (1867-1942).
Metro station les Abbesses, Place des Abbesses, Paris 75018. Architect Hector Guimard (1867-1942).

TEC4645331: Metro station les Abbesses, Place des Abbesses, Paris 75018. Architect Hector Guimard (1867-1942). / Bridgeman Images

ID: TEC4645331

Metro station les Abbesses, Place des Abbesses, Paris 75018. Architect Hector Guimard (1867-1942).

Le cabaret du Moulin Rouge, 82 boulevard de Clichy Paris 75018. This cabaret founded by Charles Zidler and Joseph Oller opened its doors on the occasion of the World Exposition in 1889.
Le cabaret du Moulin Rouge, 82 boulevard de Clichy Paris 75018. This cabaret founded by Charles Zidler and Joseph Oller opened its doors on the occasion of the World Exposition in 1889.

TEC4645450: Le cabaret du Moulin Rouge, 82 boulevard de Clichy Paris 75018. This cabaret founded by Charles Zidler and Joseph Oller opened its doors on the occasion of the World Exposition in 1889. / Bridgeman Images

ID: TEC4645450

Le cabaret du Moulin Rouge, 82 boulevard de Clichy Paris 75018. This cabaret founded by Charles Zidler and Joseph Oller opened its doors on the occasion of the World Exposition in 1889.

Boulevard Barbes in Paris 75018.
Boulevard Barbes in Paris 75018.

TEC4645545: Boulevard Barbes in Paris 75018. / Bridgeman Images

ID: TEC4645545

Boulevard Barbes in Paris 75018.

Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - 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
Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - 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

PIX4645627: Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - 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 / Bridgeman Images

ID: PIX4645627

Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - 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

Stormy night - Lightnin
Stormy night - Lightnin

PIX4670848: Stormy night - Lightnin / Bridgeman Images

ID: PIX4670848

Stormy night - Lightnin

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter
Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

PIX4671029: Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter / Bridgeman Images

ID: PIX4671029

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter

Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This darker band is called the Alexander's dark band. Notice too that the blue tints are missing in the rainbow, because the sun is setting, so is orange, which means that its blue tints are absent
Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This darker band is called the Alexander's dark band. Notice too that the blue tints are missing in the rainbow, because the sun is setting, so is orange, which means that its blue tints are absent

PIX4671117: Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This darker band is called the Alexander's dark band. Notice too that the blue tints are missing in the rainbow, because the sun is setting, so is orange, which means that its blue tints are absent / Bridgeman Images

ID: PIX4671117

Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This da

Rainbow at sunrise - Rainbow at sunrise - Arc - en - ciel observes 17 December 2005. At sunrise, the glowing light of the Sun caused an almost complete absence of blue and green colors in the rainbow. December 17, 2005. Rainbow seen at sunrise. Blue and green colors are almost invisible, because of this bright reddish sunshine
Rainbow at sunrise - Rainbow at sunrise - Arc - en - ciel observes 17 December 2005. At sunrise, the glowing light of the Sun caused an almost complete absence of blue and green colors in the rainbow. December 17, 2005. Rainbow seen at sunrise. Blue and green colors are almost invisible, because of this bright reddish sunshine

PIX4671138: Rainbow at sunrise - Rainbow at sunrise - Arc - en - ciel observes 17 December 2005. At sunrise, the glowing light of the Sun caused an almost complete absence of blue and green colors in the rainbow. December 17, 2005. Rainbow seen at sunrise. Blue and green colors are almost invisible, because of this bright reddish sunshine / Bridgeman Images

ID: PIX4671138

Rainbow at sunrise - Rainbow at sunrise - Arc - en - ciel observes 17 December 2005. At sunrise, the glowing light of the Sun caused an almost complete absence of blue and green colors in the rainbow. December 17, 2005. Rainbow seen at sunrise. Blue and green colors are almost invisible, because of this bright reddish sunshine

Rainbow in Lapland - Rainbow in Lapland - Rainbow in Lapland. Muonio, Mount Pallas (Finland), July 2003. Rainbow above Lapland landscape. Pallas fells, Finland. July 2003
Rainbow in Lapland - Rainbow in Lapland - Rainbow in Lapland. Muonio, Mount Pallas (Finland), July 2003. Rainbow above Lapland landscape. Pallas fells, Finland. July 2003

PIX4671151: Rainbow in Lapland - Rainbow in Lapland - Rainbow in Lapland. Muonio, Mount Pallas (Finland), July 2003. Rainbow above Lapland landscape. Pallas fells, Finland. July 2003 / Bridgeman Images

ID: PIX4671151

Rainbow in Lapland - Rainbow in Lapland - Rainbow in Lapland. Muonio, Mount Pallas (Finland), July 2003. Rainbow above Lapland landscape. Pallas fells, Finland. July 2003

Rainbow - Rainbow - Double Rainbow - Victoria Falls. Double rainbow over Victoria falls
Rainbow - Rainbow - Double Rainbow - Victoria Falls. Double rainbow over Victoria falls

PIX4671196: Rainbow - Rainbow - Double Rainbow - Victoria Falls. Double rainbow over Victoria falls / Bridgeman Images

ID: PIX4671196

Rainbow - Rainbow - Double Rainbow - Victoria Falls. Double rainbow over Victoria falls

Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals
Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals

PIX4671365: Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals / Bridgeman Images

ID: PIX4671365

Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals

Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia
Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia

PIX4671636: Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia / Bridgeman Images

ID: PIX4671636

Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia

The metro station Barbes Rochechouart in Paris 75018.
The metro station Barbes Rochechouart in Paris 75018.

TEC4645640: The metro station Barbes Rochechouart in Paris 75018. / Bridgeman Images

ID: TEC4645640

The metro station Barbes Rochechouart in Paris 75018.

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 Space Telescope (JWST) is a large, infrared-optimized space telescope scheduled for launch in 2018. 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 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 Space Telescope (JWST) is a large, infrared-optimized space telescope scheduled for launch in 2018. 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

PIX4645800: 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 Space Telescope (JWST) is a large, infrared-optimized space telescope scheduled for launch in 2018. 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: PIX4645800

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 (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: 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 / Bridgeman Images

ID: PIX4645823

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

GAIA - Artist's view - GAIA - Artist's view - View of the European satellite GAIA to be launched in 2011. The goal of the Gaia mission is to make the largest possible census of the stars of our Galaxy and to create a 3D map of them with great precision. The satellite will determine the position, color and proper movement of a billion stars
GAIA - Artist's view - GAIA - Artist's view - View of the European satellite GAIA to be launched in 2011. The goal of the Gaia mission is to make the largest possible census of the stars of our Galaxy and to create a 3D map of them with great precision. The satellite will determine the position, color and proper movement of a billion stars

PIX4645970: GAIA - Artist's view - GAIA - Artist's view - View of the European satellite GAIA to be launched in 2011. The goal of the Gaia mission is to make the largest possible census of the stars of our Galaxy and to create a 3D map of them with great precision. The satellite will determine the position, color and proper movement of a billion stars / Bridgeman Images

ID: PIX4645970

GAIA - Artist's view - GAIA - Artist's view - View of the European satellite GAIA to be launched in 2011. The goal of the Gaia mission is to make the largest possible census of the stars of our Galaxy and to create a 3D map of them with great precision. The satellite will determine the position, color and proper movement of a billion stars

Euclid Satellite - Illustration - Euclid Satellite. Artwork: Artist's view of the European satellite Euclid. This satellite, which is planned to launch around 2020, will study dark energy. - Artist's impression of the Euclid spacecraft, a dark energy and dark matter mission planned for launch in 2020
Euclid Satellite - Illustration - Euclid Satellite. Artwork: Artist's view of the European satellite Euclid. This satellite, which is planned to launch around 2020, will study dark energy. - Artist's impression of the Euclid spacecraft, a dark energy and dark matter mission planned for launch in 2020

PIX4646049: Euclid Satellite - Illustration - Euclid Satellite. Artwork: Artist's view of the European satellite Euclid. This satellite, which is planned to launch around 2020, will study dark energy. - Artist's impression of the Euclid spacecraft, a dark energy and dark matter mission planned for launch in 2020 / Bridgeman Images

ID: PIX4646049

Euclid Satellite - Illustration - Euclid Satellite. Artwork: Artist's view of the European satellite Euclid. This satellite, which is planned to launch around 2020, will study dark energy. - Artist's impression of the Euclid spacecraft, a dark energy and dark matter mission planned for launch in 2020

Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, launched in 2009, studies the formation of galaxies, stars and planetary systems in the infrared. 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) studies 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 is bigger and better than any of its predecessors. Moreover, it observes at wavelengths never covered before. It is located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, launched in 2009, studies the formation of galaxies, stars and planetary systems in the infrared. 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) studies 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 is bigger and better than any of its predecessors. Moreover, it observes at wavelengths never covered before. It is located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium

PIX4646124: Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, launched in 2009, studies the formation of galaxies, stars and planetary systems in the infrared. 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) studies 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 is bigger and better than any of its predecessors. Moreover, it observes at wavelengths never covered before. It is located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium / Bridgeman Images

ID: PIX4646124

Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, launched in 2009, studies the formation of galaxies, stars and planetary systems in the infrared. 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) studies 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 is bigger and better than any of its predecessors. Moreover, it observes at wavelengths never covered b

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

PIX4646287: 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 / Bridgeman Images

ID: PIX4646287

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

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

PIX4646322: 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 / Bridgeman Images

ID: PIX4646322

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

Clouds at sunset - Clouds in sunse
Clouds at sunset - Clouds in sunse

PIX4671882: Clouds at sunset - Clouds in sunse / Bridgeman Images

ID: PIX4671882

Clouds at sunset - Clouds in sunse

Landscape at Sunrise - Coloured clouds at sunrise - Sunrise taken in January 2010 in the Gers. Sunrise in winter. January 2010, Gers, France
Landscape at Sunrise - Coloured clouds at sunrise - Sunrise taken in January 2010 in the Gers. Sunrise in winter. January 2010, Gers, France

PIX4671917: Landscape at Sunrise - Coloured clouds at sunrise - Sunrise taken in January 2010 in the Gers. Sunrise in winter. January 2010, Gers, France / Bridgeman Images

ID: PIX4671917

Landscape at Sunrise - Coloured clouds at sunrise - Sunrise taken in January 2010 in the Gers. Sunrise in winter. January 2010, Gers, France

Trees and Sunset - Gum trees agains the evening sky
Trees and Sunset - Gum trees agains the evening sky

PIX4671931: Trees and Sunset - Gum trees agains the evening sky / Bridgeman Images

ID: PIX4671931

Trees and Sunset - Gum trees agains the evening sky

Light pollution - Light pollution - Photographic installation on the star sky of Arizona. On the horizon, the light pollution of Prescott (green halo) and Phoenix, which is 120 km away.
Light pollution - Light pollution - Photographic installation on the star sky of Arizona. On the horizon, the light pollution of Prescott (green halo) and Phoenix, which is 120 km away.

PIX4672231: Light pollution - Light pollution - Photographic installation on the star sky of Arizona. On the horizon, the light pollution of Prescott (green halo) and Phoenix, which is 120 km away. / Bridgeman Images

ID: PIX4672231

Light pollution - Light pollution - Photographic installation on the star sky of Arizona. On the horizon, the light pollution of Prescott (green halo) and Phoenix, which is 120 km away.

Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)
Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)

LRI4672548: Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo) / Bridgeman Images

ID: LRI4672548

Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)

Grand Canyon, Arizona, seen by shuttle - 1985 - Grand Canyon, Arizona, USA, observed by shuttle STS-61-B in November 1985
Grand Canyon, Arizona, seen by shuttle - 1985 - Grand Canyon, Arizona, USA, observed by shuttle STS-61-B in November 1985

PIX4672561: Grand Canyon, Arizona, seen by shuttle - 1985 - Grand Canyon, Arizona, USA, observed by shuttle STS-61-B in November 1985 / Bridgeman Images

ID: PIX4672561

Grand Canyon, Arizona, seen by shuttle - 1985 - Grand Canyon, Arizona, USA, observed by shuttle STS-61-B in November 1985

Exit extra - vehicular 04/1983 - Astronauts extravehicular activity. 04/1983 - Exit extra - vehicle for astronauts Story Musgrave (left) and Don Peterson on April 7, 1983. Astronauts Story Musgrave, left, and Don Peterson float in the cargo bay of the Earth - orbiting space shuttle Challenger during their April 7, 1983, spacewalk on the STS - 6 mission. Their” floating” is restricted via tethers to safety slide wires. Thanks to the tether and slide wire combination, Peterson is able to translate, or move, along the port side hand rails. First called STA-099, Challenger was built to serve as a test vehicle for the Space Shuttle program. Challenger, the second orbiter to join Nasa's Space Shuttle fleet, arrived at Kennedy Space Center in Florida in July 1982. Challenger launched on her maiden voyage, STS - 6, on April 4, 1983 and saw the first spacewalk of the shuttle program, as well as the deployment of the first satellite - - the Tracking and Data Relay System. The orbiter launched the first American woman, Sally Ride, into space on mission STS - 7 and was the first to carry two U.S. female astronauts on mission STS - 41 - G. The first orbiter to launch and land at night on mission STS - 8, Challenger also made the first Space Shuttle landing at Kennedy Space Center, concluding mission STS 41 - B. Spacelabs 2 and 3 flew aboard the ship on missions STS 51 - F and STS 51 - B, as did the first German - dedicated Spacelab on STS 61 - A. A host of scientific experiments and satellite deployments were performed during Challenger's missions. Challenger's service to America's space program ended in tragedy on Jan. 28, 1986. Just 73 seconds into mission STS - 51L, a booster failure caused an explosion that resulted in the loss of seven astronauts, as well as the vehicle
Exit extra - vehicular 04/1983 - Astronauts extravehicular activity. 04/1983 - Exit extra - vehicle for astronauts Story Musgrave (left) and Don Peterson on April 7, 1983. Astronauts Story Musgrave, left, and Don Peterson float in the cargo bay of the Earth - orbiting space shuttle Challenger during their April 7, 1983, spacewalk on the STS - 6 mission. Their” floating” is restricted via tethers to safety slide wires. Thanks to the tether and slide wire combination, Peterson is able to translate, or move, along the port side hand rails. First called STA-099, Challenger was built to serve as a test vehicle for the Space Shuttle program. Challenger, the second orbiter to join Nasa's Space Shuttle fleet, arrived at Kennedy Space Center in Florida in July 1982. Challenger launched on her maiden voyage, STS - 6, on April 4, 1983 and saw the first spacewalk of the shuttle program, as well as the deployment of the first satellite - - the Tracking and Data Relay System. The orbiter launched the first American woman, Sally Ride, into space on mission STS - 7 and was the first to carry two U.S. female astronauts on mission STS - 41 - G. The first orbiter to launch and land at night on mission STS - 8, Challenger also made the first Space Shuttle landing at Kennedy Space Center, concluding mission STS 41 - B. Spacelabs 2 and 3 flew aboard the ship on missions STS 51 - F and STS 51 - B, as did the first German - dedicated Spacelab on STS 61 - A. A host of scientific experiments and satellite deployments were performed during Challenger's missions. Challenger's service to America's space program ended in tragedy on Jan. 28, 1986. Just 73 seconds into mission STS - 51L, a booster failure caused an explosion that resulted in the loss of seven astronauts, as well as the vehicle

PIX4646670: Exit extra - vehicular 04/1983 - Astronauts extravehicular activity. 04/1983 - Exit extra - vehicle for astronauts Story Musgrave (left) and Don Peterson on April 7, 1983. Astronauts Story Musgrave, left, and Don Peterson float in the cargo bay of the Earth - orbiting space shuttle Challenger during their April 7, 1983, spacewalk on the STS - 6 mission. Their” floating” is restricted via tethers to safety slide wires. Thanks to the tether and slide wire combination, Peterson is able to translate, or move, along the port side hand rails. First called STA-099, Challenger was built to serve as a test vehicle for the Space Shuttle program. Challenger, the second orbiter to join Nasa's Space Shuttle fleet, arrived at Kennedy Space Center in Florida in July 1982. Challenger launched on her maiden voyage, STS - 6, on April 4, 1983 and saw the first spacewalk of the shuttle program, as well as the deployment of the first satellite - - the Tracking and Data Relay System. The orbiter launched the first American woman, Sally Ride, into space on mission STS - 7 and was the first to carry two U.S. female astronauts on mission STS - 41 - G. The first orbiter to launch and land at night on mission STS - 8, Challenger also made the first Space Shuttle landing at Kennedy Space Center, concluding mission STS 41 - B. Spacelabs 2 and 3 flew aboard the ship on missions STS 51 - F and STS 51 - B, as did the first German - dedicated Spacelab on STS 61 - A. A host of scientific experiments and satellite deployments were performed during Challenger's missions. Challenger's service to America's space program ended in tragedy on Jan. 28, 1986. Just 73 seconds into mission STS - 51L, a booster failure caused an explosion that resulted in the loss of seven astronauts, as well as the vehicle / Bridgeman Images

ID: PIX4646670

Exit extra - vehicular 04/1983 - Astronauts extravehicular activity. 04/1983 - Exit extra - vehicle for astronauts Story Musgrave (left) and Don Peterson on April 7, 1983. Astronauts Story Musgrave, left, and Don Peterson float in the cargo bay of the Earth - orbiting space shuttle Challenger during their April 7, 1983, spacewalk on the STS - 6 mission. Their” floating” is restricted via tethers to safety slide wires. Thanks to the tether and slide wire combination, Peterson is able to translate, or move, along the port side hand rails. First called STA-099, Challenger was built to serve as a test vehicle for the Space Shuttle program. Challenger, the second orbiter to join Nasa's Space Shuttle fleet, arrived at Kennedy Space Center in Florida in July 1982. Challenger launched on her maiden voyage, STS - 6, on April 4, 1983 and saw the first spacewalk of the shuttle program, as well as the deployment of the first satellite - - the Tracking and Data Relay System. The orbiter launched th

Decollage Challenger STS - 7 06/1983 - Space shuttle Challenger launch on June 18 1983. - Launch of the Shuttle Challenger STS - 7 with Robert Crippen, Frederick Hauck, John Fabian, Sally Ride and Norman Thagard. 18/06/1983
Decollage Challenger STS - 7 06/1983 - Space shuttle Challenger launch on June 18 1983. - Launch of the Shuttle Challenger STS - 7 with Robert Crippen, Frederick Hauck, John Fabian, Sally Ride and Norman Thagard. 18/06/1983

PIX4646676: Decollage Challenger STS - 7 06/1983 - Space shuttle Challenger launch on June 18 1983. - Launch of the Shuttle Challenger STS - 7 with Robert Crippen, Frederick Hauck, John Fabian, Sally Ride and Norman Thagard. 18/06/1983 / Bridgeman Images

ID: PIX4646676

Decollage Challenger STS - 7 06/1983 - Space shuttle Challenger launch on June 18 1983. - Launch of the Shuttle Challenger STS - 7 with Robert Crippen, Frederick Hauck, John Fabian, Sally Ride and Norman Thagard. 18/06/1983

Shuttle Challenger - STS - 7 06/1983 - Space shuttle Challenger in space taken by the SPAS satellite - Shuttle Challenger STS - 7 in orbit from SPAS 01A (Shuttle Pallet Satellite). 27/06/1983. Challenger in space, seen beyond the Earth's horizon, taken by the SPAS satellite. Its cargo bay is open, revealing its contents. Visible in the cargo bay are the protective cradles for the Palapa - B and Telesat F. communications satellites, the pallet for the NASA Office of Space and Terrestrial Applications (OSTA - 2), the remote manipulator system (RMS) arm in the shape of the numeral seven and the KU - band antenna. A number of getaway special (GAS) canisters are also visible along the port side
Shuttle Challenger - STS - 7 06/1983 - Space shuttle Challenger in space taken by the SPAS satellite - Shuttle Challenger STS - 7 in orbit from SPAS 01A (Shuttle Pallet Satellite). 27/06/1983. Challenger in space, seen beyond the Earth's horizon, taken by the SPAS satellite. Its cargo bay is open, revealing its contents. Visible in the cargo bay are the protective cradles for the Palapa - B and Telesat F. communications satellites, the pallet for the NASA Office of Space and Terrestrial Applications (OSTA - 2), the remote manipulator system (RMS) arm in the shape of the numeral seven and the KU - band antenna. A number of getaway special (GAS) canisters are also visible along the port side

PIX4646707: Shuttle Challenger - STS - 7 06/1983 - Space shuttle Challenger in space taken by the SPAS satellite - Shuttle Challenger STS - 7 in orbit from SPAS 01A (Shuttle Pallet Satellite). 27/06/1983. Challenger in space, seen beyond the Earth's horizon, taken by the SPAS satellite. Its cargo bay is open, revealing its contents. Visible in the cargo bay are the protective cradles for the Palapa - B and Telesat F. communications satellites, the pallet for the NASA Office of Space and Terrestrial Applications (OSTA - 2), the remote manipulator system (RMS) arm in the shape of the numeral seven and the KU - band antenna. A number of getaway special (GAS) canisters are also visible along the port side / Bridgeman Images

ID: PIX4646707

Shuttle Challenger - STS - 7 06/1983 - Space shuttle Challenger in space taken by the SPAS satellite - Shuttle Challenger STS - 7 in orbit from SPAS 01A (Shuttle Pallet Satellite). 27/06/1983. Challenger in space, seen beyond the Earth's horizon, taken by the SPAS satellite. Its cargo bay is open, revealing its contents. Visible in the cargo bay are the protective cradles for the Palapa - B and Telesat F. communications satellites, the pallet for the NASA Office of Space and Terrestrial Applications (OSTA - 2), the remote manipulator system (RMS) arm in the shape of the numeral seven and the KU - band antenna. A number of getaway special (GAS) canisters are also visible along the port side

Lighting on Challenger STS - 8 08/1983 - Lightning strikes Space Shuttle Challenger - Lightning on the firing pitch before launching the Challenger STS shuttle - 8. 08/1983. Lightning strikes Space Shuttle Launch Complex 39A in the hours preceding the launch of Challenger on mission STS-8. Aug 1983
Lighting on Challenger STS - 8 08/1983 - Lightning strikes Space Shuttle Challenger - Lightning on the firing pitch before launching the Challenger STS shuttle - 8. 08/1983. Lightning strikes Space Shuttle Launch Complex 39A in the hours preceding the launch of Challenger on mission STS-8. Aug 1983

PIX4646720: Lighting on Challenger STS - 8 08/1983 - Lightning strikes Space Shuttle Challenger - Lightning on the firing pitch before launching the Challenger STS shuttle - 8. 08/1983. Lightning strikes Space Shuttle Launch Complex 39A in the hours preceding the launch of Challenger on mission STS-8. Aug 1983 / Bridgeman Images

ID: PIX4646720

Lighting on Challenger STS - 8 08/1983 - Lightning strikes Space Shuttle Challenger - Lightning on the firing pitch before launching the Challenger STS shuttle - 8. 08/1983. Lightning strikes Space Shuttle Launch Complex 39A in the hours preceding the launch of Challenger on mission STS-8. Aug 1983

Launch of the Space Shuttle Discovery STS - 26. 29/09/1988 - Launch of the Space Shuttle Discovery STS - 26 09/1988 - Launch of the Space Shuttle Discovery STS - 26 and its five man crew from Pad 39 - B. Sep 29 1988
Launch of the Space Shuttle Discovery STS - 26. 29/09/1988 - Launch of the Space Shuttle Discovery STS - 26 09/1988 - Launch of the Space Shuttle Discovery STS - 26 and its five man crew from Pad 39 - B. Sep 29 1988

PIX4646732: Launch of the Space Shuttle Discovery STS - 26. 29/09/1988 - Launch of the Space Shuttle Discovery STS - 26 09/1988 - Launch of the Space Shuttle Discovery STS - 26 and its five man crew from Pad 39 - B. Sep 29 1988 / Bridgeman Images

ID: PIX4646732

Launch of the Space Shuttle Discovery STS - 26. 29/09/1988 - Launch of the Space Shuttle Discovery STS - 26 09/1988 - Launch of the Space Shuttle Discovery STS - 26 and its five man crew from Pad 39 - B. Sep 29 1988

Discovery Shuttle Discovery 04/1990 - Launch of Shuttle Discovery STS - 31. Apr 24 1990 - Decolation of the shuttle Discovery (STS-31 mission) with Loren Shriver, Charles Bolden, Steven Hawley, Bruce McCandless and Kathryn Sullivan on board as well as the Hubble space telescope. 24/04/1990. The Space Shuttle Discovery soars into the morning skies above Florida, carying a crew of five and the Hubble Space Telescope. Launch of Space Shuttle Mission STS - 31from Pad 39B occurred at 8:33:51 a.m. EDT, April 24. Crew members are Commander Loren J. Shriver; Pilot Charles F. Bolden Jr.; and Mission Specialists Kathryn D. Sullivan, Steven A. Hawley, and Bruce McCandless II
Discovery Shuttle Discovery 04/1990 - Launch of Shuttle Discovery STS - 31. Apr 24 1990 - Decolation of the shuttle Discovery (STS-31 mission) with Loren Shriver, Charles Bolden, Steven Hawley, Bruce McCandless and Kathryn Sullivan on board as well as the Hubble space telescope. 24/04/1990. The Space Shuttle Discovery soars into the morning skies above Florida, carying a crew of five and the Hubble Space Telescope. Launch of Space Shuttle Mission STS - 31from Pad 39B occurred at 8:33:51 a.m. EDT, April 24. Crew members are Commander Loren J. Shriver; Pilot Charles F. Bolden Jr.; and Mission Specialists Kathryn D. Sullivan, Steven A. Hawley, and Bruce McCandless II

PIX4646822: Discovery Shuttle Discovery 04/1990 - Launch of Shuttle Discovery STS - 31. Apr 24 1990 - Decolation of the shuttle Discovery (STS-31 mission) with Loren Shriver, Charles Bolden, Steven Hawley, Bruce McCandless and Kathryn Sullivan on board as well as the Hubble space telescope. 24/04/1990. The Space Shuttle Discovery soars into the morning skies above Florida, carying a crew of five and the Hubble Space Telescope. Launch of Space Shuttle Mission STS - 31from Pad 39B occurred at 8:33:51 a.m. EDT, April 24. Crew members are Commander Loren J. Shriver; Pilot Charles F. Bolden Jr.; and Mission Specialists Kathryn D. Sullivan, Steven A. Hawley, and Bruce McCandless II / Bridgeman Images

ID: PIX4646822

Discovery Shuttle Discovery 04/1990 - Launch of Shuttle Discovery STS - 31. Apr 24 1990 - Decolation of the shuttle Discovery (STS-31 mission) with Loren Shriver, Charles Bolden, Steven Hawley, Bruce McCandless and Kathryn Sullivan on board as well as the Hubble space telescope. 24/04/1990. The Space Shuttle Discovery soars into the morning skies above Florida, carying a crew of five and the Hubble Space Telescope. Launch of Space Shuttle Mission STS - 31from Pad 39B occurred at 8:33:51 a.m. EDT, April 24. Crew members are Commander Loren J. Shriver; Pilot Charles F. Bolden Jr.; and Mission Specialists Kathryn D. Sullivan, Steven A. Hawley, and Bruce McCandless II

Decollage Atlantis STS - 45 03/1992 - Launch of Space Shuttle Atlantis. Mar 24 1992 - Decolving the shuttle Atlantis STS - 45 with Charles Bolden, Brian Duffy, Kathryn Sullivan, David Leestma, Colin Foale, Byron Lichtenberg and Dirk Frimout on board. 24/03/1992
Decollage Atlantis STS - 45 03/1992 - Launch of Space Shuttle Atlantis. Mar 24 1992 - Decolving the shuttle Atlantis STS - 45 with Charles Bolden, Brian Duffy, Kathryn Sullivan, David Leestma, Colin Foale, Byron Lichtenberg and Dirk Frimout on board. 24/03/1992

PIX4646945: Decollage Atlantis STS - 45 03/1992 - Launch of Space Shuttle Atlantis. Mar 24 1992 - Decolving the shuttle Atlantis STS - 45 with Charles Bolden, Brian Duffy, Kathryn Sullivan, David Leestma, Colin Foale, Byron Lichtenberg and Dirk Frimout on board. 24/03/1992 / Bridgeman Images

ID: PIX4646945

Decollage Atlantis STS - 45 03/1992 - Launch of Space Shuttle Atlantis. Mar 24 1992 - Decolving the shuttle Atlantis STS - 45 with Charles Bolden, Brian Duffy, Kathryn Sullivan, David Leestma, Colin Foale, Byron Lichtenberg and Dirk Frimout on board. 24/03/1992

STS-47: Weightless crew in Spacelab - STS-47 crew portrait in zero gravity: The crew of the STS-47 mission poses weightlessly in the Spacelab aboard the shuttle Endeavour. From left to right, in the last row: Robert L. Gibson and Curtis L. Brown, in the middle: N. Jan Davis, Jerome Apt and Mae C. Jemison, in front: Mark C. Lee and Mamoru Mohri. It was during this mission that Mae C. Jemison was the first black woman in space and Mark C. Lee and Jan Davis were the first American married couple to fly into space. Portrait of the crew of STS-47 aboard Spacelab-Japan (SLJ). Pictured, left to right, back row are Commander Robert L. Gibson and Pilot Curtis L. Brown; middle row, Mission Specialist (MS) N. Jan Davis, MS Jerome Apt and MS Mae C. Jemison; front row, Payload Commander (PLC) Mark C. Lee and Payload Specialist (PS) Mamoru Mohri.
STS-47: Weightless crew in Spacelab - STS-47 crew portrait in zero gravity: The crew of the STS-47 mission poses weightlessly in the Spacelab aboard the shuttle Endeavour. From left to right, in the last row: Robert L. Gibson and Curtis L. Brown, in the middle: N. Jan Davis, Jerome Apt and Mae C. Jemison, in front: Mark C. Lee and Mamoru Mohri. It was during this mission that Mae C. Jemison was the first black woman in space and Mark C. Lee and Jan Davis were the first American married couple to fly into space. Portrait of the crew of STS-47 aboard Spacelab-Japan (SLJ). Pictured, left to right, back row are Commander Robert L. Gibson and Pilot Curtis L. Brown; middle row, Mission Specialist (MS) N. Jan Davis, MS Jerome Apt and MS Mae C. Jemison; front row, Payload Commander (PLC) Mark C. Lee and Payload Specialist (PS) Mamoru Mohri.

PIX4646964: STS-47: Weightless crew in Spacelab - STS-47 crew portrait in zero gravity: The crew of the STS-47 mission poses weightlessly in the Spacelab aboard the shuttle Endeavour. From left to right, in the last row: Robert L. Gibson and Curtis L. Brown, in the middle: N. Jan Davis, Jerome Apt and Mae C. Jemison, in front: Mark C. Lee and Mamoru Mohri. It was during this mission that Mae C. Jemison was the first black woman in space and Mark C. Lee and Jan Davis were the first American married couple to fly into space. Portrait of the crew of STS-47 aboard Spacelab-Japan (SLJ). Pictured, left to right, back row are Commander Robert L. Gibson and Pilot Curtis L. Brown; middle row, Mission Specialist (MS) N. Jan Davis, MS Jerome Apt and MS Mae C. Jemison; front row, Payload Commander (PLC) Mark C. Lee and Payload Specialist (PS) Mamoru Mohri. / Bridgeman Images

ID: PIX4646964

STS-47: Weightless crew in Spacelab - STS-47 crew portrait in zero gravity: The crew of the STS-47 mission poses weightlessly in the Spacelab aboard the shuttle Endeavour. From left to right, in the last row: Robert L. Gibson and Curtis L. Brown, in the middle: N. Jan Davis, Jerome Apt and Mae C. Jemison, in front: Mark C. Lee and Mamoru Mohri. It was during this mission that Mae C. Jemison was the first black woman in space and Mark C. Lee and Jan Davis were the first American married couple to fly into space. Portrait of the crew of STS-47 aboard Spacelab-Japan (SLJ). Pictured, left to right, back row are Commander Robert L. Gibson and Pilot Curtis L. Brown; middle row, Mission Specialist (MS) N. Jan Davis, MS Jerome Apt and MS Mae C. Jemison; front row, Payload Commander (PLC) Mark C. Lee and Payload Specialist (PS) Mamoru Mohri.

Marsha Ivins en weightlessness - Marsha Ivins in the space shuttle Columbia: Astronaut Marsha Ivins weightless in space shuttle Columbia. Together with astronaut Pierre Thuot, on the right, she performs a thermal analysis of the crew compartment. March 1994. STS-62 Mission Specialists Marsha Ivins and Pierre Thuot performing an infrared thermal survey of the Columbia orbiter crew compartment
Marsha Ivins en weightlessness - Marsha Ivins in the space shuttle Columbia: Astronaut Marsha Ivins weightless in space shuttle Columbia. Together with astronaut Pierre Thuot, on the right, she performs a thermal analysis of the crew compartment. March 1994. STS-62 Mission Specialists Marsha Ivins and Pierre Thuot performing an infrared thermal survey of the Columbia orbiter crew compartment

PIX4647073: Marsha Ivins en weightlessness - Marsha Ivins in the space shuttle Columbia: Astronaut Marsha Ivins weightless in space shuttle Columbia. Together with astronaut Pierre Thuot, on the right, she performs a thermal analysis of the crew compartment. March 1994. STS-62 Mission Specialists Marsha Ivins and Pierre Thuot performing an infrared thermal survey of the Columbia orbiter crew compartment / Bridgeman Images

ID: PIX4647073

Marsha Ivins en weightlessness - Marsha Ivins in the space shuttle Columbia: Astronaut Marsha Ivins weightless in space shuttle Columbia. Together with astronaut Pierre Thuot, on the right, she performs a thermal analysis of the crew compartment. March 1994. STS-62 Mission Specialists Marsha Ivins and Pierre Thuot performing an infrared thermal survey of the Columbia orbiter crew compartment

Decolving the shuttle Endeavour STS - 68 09/1994 - Launch of the space shuttle Endeavour - 09/1994 - Decolving the shuttle Endeavour STS - 68 with Michael Baker, Terrence Wilcutt, Thomas Jones, Peter Wisoff, Daniel Bursch and Steven Smith as well as the SRL-2 (Space Radar Laboratory). 30/09/1994. Launch of Space Shuttle Endeavour from Pad 39A. Aboard are a crew of six astronauts and the Space Radar Laboratory (SRL-2). Sep 30 1994
Decolving the shuttle Endeavour STS - 68 09/1994 - Launch of the space shuttle Endeavour - 09/1994 - Decolving the shuttle Endeavour STS - 68 with Michael Baker, Terrence Wilcutt, Thomas Jones, Peter Wisoff, Daniel Bursch and Steven Smith as well as the SRL-2 (Space Radar Laboratory). 30/09/1994. Launch of Space Shuttle Endeavour from Pad 39A. Aboard are a crew of six astronauts and the Space Radar Laboratory (SRL-2). Sep 30 1994

PIX4647124: Decolving the shuttle Endeavour STS - 68 09/1994 - Launch of the space shuttle Endeavour - 09/1994 - Decolving the shuttle Endeavour STS - 68 with Michael Baker, Terrence Wilcutt, Thomas Jones, Peter Wisoff, Daniel Bursch and Steven Smith as well as the SRL-2 (Space Radar Laboratory). 30/09/1994. Launch of Space Shuttle Endeavour from Pad 39A. Aboard are a crew of six astronauts and the Space Radar Laboratory (SRL-2). Sep 30 1994 / Bridgeman Images

ID: PIX4647124

Decolving the shuttle Endeavour STS - 68 09/1994 - Launch of the space shuttle Endeavour - 09/1994 - Decolving the shuttle Endeavour STS - 68 with Michael Baker, Terrence Wilcutt, Thomas Jones, Peter Wisoff, Daniel Bursch and Steven Smith as well as the SRL-2 (Space Radar Laboratory). 30/09/1994. Launch of Space Shuttle Endeavour from Pad 39A. Aboard are a crew of six astronauts and the Space Radar Laboratory (SRL-2). Sep 30 1994


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