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William Fitzwilliam, 1st Earl of Southampton (1490-1542). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
William Fitzwilliam, 1st Earl of Southampton (1490-1542). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645739: William Fitzwilliam, 1st Earl of Southampton (1490-1542). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645739

William Fitzwilliam, 1st Earl of Southampton (1490-1542). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

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

Sir Thomas More, Lord Chancellor to King Henry VIII, English lawyer, author, statesman (1478-1535). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
Sir Thomas More, Lord Chancellor to King Henry VIII, English lawyer, author, statesman (1478-1535). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645783: Sir Thomas More, Lord Chancellor to King Henry VIII, English lawyer, author, statesman (1478-1535). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645783

Sir Thomas More, Lord Chancellor to King Henry VIII, English lawyer, author, statesman (1478-1535). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

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

PIX4645789: James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared - Primary Mirror Segment Cryogenic Testing - Six of the 18 James Webb Space Telescope mirror segments are being prepped to move into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test location / Bridgeman Images

ID: PIX4645789

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

Thomas Vaux, 2nd Baron Vaux of Harrowden (1509-1556), English poet and nobleman. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
Thomas Vaux, 2nd Baron Vaux of Harrowden (1509-1556), English poet and nobleman. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645805: Thomas Vaux, 2nd Baron Vaux of Harrowden (1509-1556), English poet and nobleman. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645805

Thomas Vaux, 2nd Baron Vaux of Harrowden (1509-1556), English poet and nobleman. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) - Artist view: The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2018. 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 - The shaded side of the James Webb Space Telescope (JWST) as it may appear later this decade when it is observing from the Earth-Sun L2 point about 930 thousand miles from the Earth. Part of the Milky Way can be seen reflected in the 21-foot diameter mirror assembly. This assembly is composed of 18 hexagonal segments of gold-coated beryllium which combines to create a near-infrared light-collecting area of about 80 square feet (the Hubble Space Telescope has a collecting area of 48 square feet) - The JWST's sensitive optical elements are shaded from the perpetual sunlight via a “” parasol” consisting of multiple spaced layers of polyimide film. These layers act as a passive cooling barrier between the 185* F sunward side and the -388* F shaded side hosting the optics and sensors
James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) - Artist view: The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2018. 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 - The shaded side of the James Webb Space Telescope (JWST) as it may appear later this decade when it is observing from the Earth-Sun L2 point about 930 thousand miles from the Earth. Part of the Milky Way can be seen reflected in the 21-foot diameter mirror assembly. This assembly is composed of 18 hexagonal segments of gold-coated beryllium which combines to create a near-infrared light-collecting area of about 80 square feet (the Hubble Space Telescope has a collecting area of 48 square feet) - The JWST's sensitive optical elements are shaded from the perpetual sunlight via a “” parasol” consisting of multiple spaced layers of polyimide film. These layers act as a passive cooling barrier between the 185* F sunward side and the -388* F shaded side hosting the optics and sensors

PIX4645827: James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) - Artist view: The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2018. 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 - The shaded side of the James Webb Space Telescope (JWST) as it may appear later this decade when it is observing from the Earth-Sun L2 point about 930 thousand miles from the Earth. Part of the Milky Way can be seen reflected in the 21-foot diameter mirror assembly. This assembly is composed of 18 hexagonal segments of gold-coated beryllium which combines to create a near-infrared light-collecting area of about 80 square feet (the Hubble Space Telescope has a collecting area of 48 square feet) - The JWST's sensitive optical elements are shaded from the perpetual sunlight via a “” parasol” consisting of multiple spaced layers of polyimide film. These layers act as a passive cooling barrier between the 185* F sunward side and the -388* F shaded side hosting the optics and sensors / Bridgeman Images

ID: PIX4645827

James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) - Artist view: The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2018. 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 - The shaded side of the James Webb Space Telescope (JWST) as it may appear later this decade when it is observing from the Earth-Sun L2 point about 930 thousand miles from the Earth. Part of the Milky Way can be seen reflected in the 21-foot diameter mirror assembly. This assembly is composed of 18 hexagonal segments of gold-coated beryllium which combines to create a near-infrared light-collecting area of about 80 square fe

King Francis II of France as dauphin, King consort of Scotland, 1544-1560. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
King Francis II of France as dauphin, King consort of Scotland, 1544-1560. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645829: King Francis II of France as dauphin, King consort of Scotland, 1544-1560. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645829

King Francis II of France as dauphin, King consort of Scotland, 1544-1560. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

Mary, Queen of Scots, or Mary Stuart (1542-1567). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
Mary, Queen of Scots, or Mary Stuart (1542-1567). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645845: Mary, Queen of Scots, or Mary Stuart (1542-1567). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645845

Mary, Queen of Scots, or Mary Stuart (1542-1567). Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

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

John More, son of Sir Thomas More and his first wife Jane. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
John More, son of Sir Thomas More and his first wife Jane. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645854: John More, son of Sir Thomas More and his first wife Jane. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645854

John More, son of Sir Thomas More and his first wife Jane. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

Monsieur de Saincte Corneille, French man at the court of King Henry VIII. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
Monsieur de Saincte Corneille, French man at the court of King Henry VIII. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645899: Monsieur de Saincte Corneille, French man at the court of King Henry VIII. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645899

Monsieur de Saincte Corneille, French man at the court of King Henry VIII. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

Elizabeth Jenkes, Lady Rich, wife to Sir Richard Rich, 1st Baron Rich (1496-1567), Lord Chancellor during the reign of King Edward VI. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.
Elizabeth Jenkes, Lady Rich, wife to Sir Richard Rich, 1st Baron Rich (1496-1567), Lord Chancellor during the reign of King Edward VI. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

FLO4645922: Elizabeth Jenkes, Lady Rich, wife to Sir Richard Rich, 1st Baron Rich (1496-1567), Lord Chancellor during the reign of King Edward VI. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884. / Bridgeman Images

ID: FLO4645922

Elizabeth Jenkes, Lady Rich, wife to Sir Richard Rich, 1st Baron Rich (1496-1567), Lord Chancellor during the reign of King Edward VI. Handcoloured copperplate engraving by Francis Bartolozzi after Hans Holbein from Facsimiles of Original Drawings by Hans Holbein, Hamilton, Adams, London, 1884.

Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration)
Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration)

PIX4645934: Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration) / Bridgeman Images

ID: PIX4645934

Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration)

Station Mir: release of J.Linenger 04/1997 - J.Linenger EVA - Mir station 04/1997 - Space release of astronaut Jerry Linenger on 29 April 1997. In the background of the solar panels and the Kvant module of the Mir space station. This photograph, taken by Mir 23 commander Vasili V. Tsibliyev shows NASA/Mir 23's Jerry M. Linenger, guest researcher during a five - hour spacewalk performed by the two outside the Russian Mir Space Station. Linenger blue stripes is backdropped by Kvant module and Cooperative Solar Array CSA while standing on the Docking Module not in fram
Station Mir: release of J.Linenger 04/1997 - J.Linenger EVA - Mir station 04/1997 - Space release of astronaut Jerry Linenger on 29 April 1997. In the background of the solar panels and the Kvant module of the Mir space station. This photograph, taken by Mir 23 commander Vasili V. Tsibliyev shows NASA/Mir 23's Jerry M. Linenger, guest researcher during a five - hour spacewalk performed by the two outside the Russian Mir Space Station. Linenger blue stripes is backdropped by Kvant module and Cooperative Solar Array CSA while standing on the Docking Module not in fram

PIX4642287: Station Mir: release of J.Linenger 04/1997 - J.Linenger EVA - Mir station 04/1997 - Space release of astronaut Jerry Linenger on 29 April 1997. In the background of the solar panels and the Kvant module of the Mir space station. This photograph, taken by Mir 23 commander Vasili V. Tsibliyev shows NASA/Mir 23's Jerry M. Linenger, guest researcher during a five - hour spacewalk performed by the two outside the Russian Mir Space Station. Linenger blue stripes is backdropped by Kvant module and Cooperative Solar Array CSA while standing on the Docking Module not in fram / Bridgeman Images

ID: PIX4642287

Station Mir: release of J.Linenger 04/1997 - J.Linenger EVA - Mir station 04/1997 - Space release of astronaut Jerry Linenger on 29 April 1997. In the background of the solar panels and the Kvant module of the Mir space station. This photograph, taken by Mir 23 commander Vasili V. Tsibliyev shows NASA/Mir 23's Jerry M. Linenger, guest researcher during a five - hour spacewalk performed by the two outside the Russian Mir Space Station. Linenger blue stripes is backdropped by Kvant module and Cooperative Solar Array CSA while standing on the Docking Module not in fram

Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997
Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997

PIX4642319: Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997 / Bridgeman Images

ID: PIX4642319

Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module is visible. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997

Station Mir - Damage panel.12/1997 - Mir station with damaged solar panel - View of the solar panel Damage of the Spektr module. The damaged Spektr module on the Mir Space Station. The Earth limb is visible in the background
Station Mir - Damage panel.12/1997 - Mir station with damaged solar panel - View of the solar panel Damage of the Spektr module. The damaged Spektr module on the Mir Space Station. The Earth limb is visible in the background

PIX4642322: Station Mir - Damage panel.12/1997 - Mir station with damaged solar panel - View of the solar panel Damage of the Spektr module. The damaged Spektr module on the Mir Space Station. The Earth limb is visible in the background / Bridgeman Images

ID: PIX4642322

Station Mir - Damage panel.12/1997 - Mir station with damaged solar panel - View of the solar panel Damage of the Spektr module. The damaged Spektr module on the Mir Space Station. The Earth limb is visible in the background

Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997
Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997

PIX4642335: Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997 / Bridgeman Images

ID: PIX4642335

Station Mir - Panel damage.10/1997 - Mir station with damaged solar panel. 10/1997 - The Mir space station seen from the shuttle Atlantis. A solar panel damage to the Spektr module (2nd to left from the top) is visible. 01/10/1997. Russia's Mir Space Station backdropped against a cloud - covered Earth photographed during a fly - around by the Space Shuttle Atlantis following the conclusion of joint docking activities between the Mir - 24 and STS - 86 crews. One of the solar array panels on the Spektr Module shows damage incurred during the impact of a Russian unmanned Progress re - supply ship with collided with the space station on June 25, 1997. Oct 01 1997

Wild or Wild Lettuce - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Lactuca vitosa - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Wild or Wild Lettuce - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Lactuca vitosa - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642366: Wild or Wild Lettuce - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Lactuca vitosa - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642366

Wild or Wild Lettuce - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Lactuca vitosa - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Dairy maraicher - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sonchus oleraceus - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Dairy maraicher - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sonchus oleraceus - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642371: Dairy maraicher - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sonchus oleraceus - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642371

Dairy maraicher - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sonchus oleraceus - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

The Mir space station seen from the shuttle Discovery. 12/06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. 12/06/1998. Overall view of Mir over the Earth horizon
The Mir space station seen from the shuttle Discovery. 12/06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. 12/06/1998. Overall view of Mir over the Earth horizon

PIX4642375: The Mir space station seen from the shuttle Discovery. 12/06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. 12/06/1998. Overall view of Mir over the Earth horizon / Bridgeman Images

ID: PIX4642375

The Mir space station seen from the shuttle Discovery. 12/06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. 12/06/1998. Overall view of Mir over the Earth horizon

Red Mahogany - Lithograph by F. Guimpel, extracted from botanical medicine by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Resin-bearing red mahogany, Eucalyptus resinifera - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Red Mahogany - Lithograph by F. Guimpel, extracted from botanical medicine by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Resin-bearing red mahogany, Eucalyptus resinifera - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642395: Red Mahogany - Lithograph by F. Guimpel, extracted from botanical medicine by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Resin-bearing red mahogany, Eucalyptus resinifera - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642395

Red Mahogany - Lithograph by F. Guimpel, extracted from botanical medicine by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Resin-bearing red mahogany, Eucalyptus resinifera - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

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

Copaiba or copahu - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera guyanensis - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Copaiba or copahu - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera guyanensis - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642421: Copaiba or copahu - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera guyanensis - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642421

Copaiba or copahu - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera guyanensis - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Astragalus producer of adragante gum - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Tragacanth gum tree, Astragalus gummifer - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Astragalus producer of adragante gum - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Tragacanth gum tree, Astragalus gummifer - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642428: Astragalus producer of adragante gum - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Tragacanth gum tree, Astragalus gummifer - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642428

Astragalus producer of adragante gum - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Tragacanth gum tree, Astragalus gummifer - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Orcanette des dyers - Lithograph by F. Guimpel, extracted from botanique medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Alkanet or dyers' bugloss, Alkanna tinctoria - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Orcanette des dyers - Lithograph by F. Guimpel, extracted from botanique medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Alkanet or dyers' bugloss, Alkanna tinctoria - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642439: Orcanette des dyers - Lithograph by F. Guimpel, extracted from botanique medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Alkanet or dyers' bugloss, Alkanna tinctoria - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642439

Orcanette des dyers - Lithograph by F. Guimpel, extracted from botanique medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Alkanet or dyers' bugloss, Alkanna tinctoria - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Copaiba (variete) - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera jacquinii - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Copaiba (variete) - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera jacquinii - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642459: Copaiba (variete) - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera jacquinii - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642459

Copaiba (variete) - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera jacquinii - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station and the moon share a 70 mm frame exposed by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery as it passed over a line of heavy thunderstorms on Earth
Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station and the moon share a 70 mm frame exposed by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery as it passed over a line of heavy thunderstorms on Earth

PIX4642471: Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station and the moon share a 70 mm frame exposed by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery as it passed over a line of heavy thunderstorms on Earth / Bridgeman Images

ID: PIX4642471

Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station and the moon share a 70 mm frame exposed by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery as it passed over a line of heavy thunderstorms on Earth

Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station seen by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery
Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station seen by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery

PIX4642478: Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station seen by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery / Bridgeman Images

ID: PIX4642478

Mir station 06/1998 - Mir station seen in june 1998 - Mir space station seen from the shuttle Discovery. Russia's Mir space station seen by one of the STS - 91 crew members aboard the Earth - orbiting Space Shuttle Discovery

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.

Copayer (variete) or copaiba - Lithography by F. Guimpel, extracted from botany medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera oblongifolia - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Copayer (variete) or copaiba - Lithography by F. Guimpel, extracted from botany medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera oblongifolia - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642485: Copayer (variete) or copaiba - Lithography by F. Guimpel, extracted from botany medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera oblongifolia - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642485

Copayer (variete) or copaiba - Lithography by F. Guimpel, extracted from botany medicale by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Copal or copaiba tree, Copaifera oblongifolia - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

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.

PIX4642492: 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: PIX4642492

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.

Mimosa fragrant - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sweet thorn bush, Acacia karroo - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822
Mimosa fragrant - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sweet thorn bush, Acacia karroo - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

FLO4642656: Mimosa fragrant - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sweet thorn bush, Acacia karroo - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822 / Bridgeman Images

ID: FLO4642656

Mimosa fragrant - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Sweet thorn bush, Acacia karroo - Handcoloured copperplate by F. Guimpel from Dr. F. G. Hayne's Medical Botany, Berlin, 1822

Cloves or cloves - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Clove spice, Syzygium aromatium -
Cloves or cloves - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Clove spice, Syzygium aromatium -

FLO4642697: Cloves or cloves - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Clove spice, Syzygium aromatium - / Bridgeman Images

ID: FLO4642697

Cloves or cloves - Lithography by F. Guimpel, extracted from medical botany by Friedrich Gottlob Haynes (1763-1832), Berlin, 1822 - Clove spice, Syzygium aromatium -

A satellite is directed to a cemetery orbit - Reorbiting a spacecraft into a graveyard orbit - Artist's view of a satellite in geostationary orbit at the end of the mission directs to a cemetery orbit. In order to prevent possible collisions, the satellite must be placed 300 km above its initial orbit. In order to eliminate collision risk, GEO satellites should be moved out of the geostationary ring at the end of their mission. It is recommended that their orbit should be raised by about 300 km, which is considered a safe distance to avoid future interference with active GEO spacecraft
A satellite is directed to a cemetery orbit - Reorbiting a spacecraft into a graveyard orbit - Artist's view of a satellite in geostationary orbit at the end of the mission directs to a cemetery orbit. In order to prevent possible collisions, the satellite must be placed 300 km above its initial orbit. In order to eliminate collision risk, GEO satellites should be moved out of the geostationary ring at the end of their mission. It is recommended that their orbit should be raised by about 300 km, which is considered a safe distance to avoid future interference with active GEO spacecraft

PIX4642742: A satellite is directed to a cemetery orbit - Reorbiting a spacecraft into a graveyard orbit - Artist's view of a satellite in geostationary orbit at the end of the mission directs to a cemetery orbit. In order to prevent possible collisions, the satellite must be placed 300 km above its initial orbit. In order to eliminate collision risk, GEO satellites should be moved out of the geostationary ring at the end of their mission. It is recommended that their orbit should be raised by about 300 km, which is considered a safe distance to avoid future interference with active GEO spacecraft / Bridgeman Images

ID: PIX4642742

A satellite is directed to a cemetery orbit - Reorbiting a spacecraft into a graveyard orbit - Artist's view of a satellite in geostationary orbit at the end of the mission directs to a cemetery orbit. In order to prevent possible collisions, the satellite must be placed 300 km above its initial orbit. In order to eliminate collision risk, GEO satellites should be moved out of the geostationary ring at the end of their mission. It is recommended that their orbit should be raised by about 300 km, which is considered a safe distance to avoid future interference with active GEO spacecraft

Space Debris: Meteosat type satellite - Space debris: Meteosat satellite - Artist's view of a Meteosat satellite when it is put into orbit. As with many satellites, orbit operations cause new space debris (ejection of covers, bolts...); in view of the dangerous increase in space debris, it is imperative to design cleaner satellites today (here a cover remains attached to the satellite). A measure against space debris is minimizing the number of objects released during spacecraft operations. Typical “” mission - related objects”” (MRO) include adapters used between two satellites in a dual launch, telescope covers, bolts, cast off yo - yo spinners, etc. Spacecraft designers and operators must design missions so that objects stay attached to the spacecraft and do not become additional space debris
Space Debris: Meteosat type satellite - Space debris: Meteosat satellite - Artist's view of a Meteosat satellite when it is put into orbit. As with many satellites, orbit operations cause new space debris (ejection of covers, bolts...); in view of the dangerous increase in space debris, it is imperative to design cleaner satellites today (here a cover remains attached to the satellite). A measure against space debris is minimizing the number of objects released during spacecraft operations. Typical “” mission - related objects”” (MRO) include adapters used between two satellites in a dual launch, telescope covers, bolts, cast off yo - yo spinners, etc. Spacecraft designers and operators must design missions so that objects stay attached to the spacecraft and do not become additional space debris

PIX4642769: Space Debris: Meteosat type satellite - Space debris: Meteosat satellite - Artist's view of a Meteosat satellite when it is put into orbit. As with many satellites, orbit operations cause new space debris (ejection of covers, bolts...); in view of the dangerous increase in space debris, it is imperative to design cleaner satellites today (here a cover remains attached to the satellite). A measure against space debris is minimizing the number of objects released during spacecraft operations. Typical “” mission - related objects”” (MRO) include adapters used between two satellites in a dual launch, telescope covers, bolts, cast off yo - yo spinners, etc. Spacecraft designers and operators must design missions so that objects stay attached to the spacecraft and do not become additional space debris / Bridgeman Images

ID: PIX4642769

Space Debris: Meteosat type satellite - Space debris: Meteosat satellite - Artist's view of a Meteosat satellite when it is put into orbit. As with many satellites, orbit operations cause new space debris (ejection of covers, bolts...); in view of the dangerous increase in space debris, it is imperative to design cleaner satellites today (here a cover remains attached to the satellite). A measure against space debris is minimizing the number of objects released during spacecraft operations. Typical “” mission - related objects”” (MRO) include adapters used between two satellites in a dual launch, telescope covers, bolts, cast off yo - yo spinners, etc. Spacecraft designers and operators must design missions so that objects stay attached to the spacecraft and do not become additional space debris


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