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Milky way all around the horizon - Panorama of 360 degrees. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. 360 degrees panorama. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up in the sky. The Large (LMC) and Small (SMC) Magellanic clouds are visible to the left, Orion constellation with Barnard loop to the right, California Nebula and 'tiny' Andromeda galaxy to the right while the Milky Way is visible all aro

Milky way all around the horizon - Panorama of 360 degrees. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. 360 degrees panorama. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up in the sky. The Large (LMC) and Small (SMC) Magellanic clouds are visible to the left, Orion constellation with Barnard loop to the right, California Nebula and 'tiny' Andromeda galaxy to the right while the Milky Way is visible all aro

Stephane Guisard

PIX4636028

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

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

P. Dumas

PIX4646076

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

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

P. Dumas

PIX4646082

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

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

PIX4644343

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

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

PIX4644364

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

PIX4610976

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained by Siding Spring's 3.9m telescope. NGC 1365, the largest spiral in the southern constellation of Fornax, is located at a distance of about 60 million light years. This beautiful galaxy is about as massive as the Milky Way, itself a substantial galaxy. Not much is known about how galaxies take on their beautiful forms, but a good deal is known about their internal organisation. The obvious 'bar' has the nucleus of the galaxy at its hub and is surrounded by masses of cooler stars that appear yellow on colour photographs. The bar itself is also yellowish, and has distinct dust lanes but it terminates abruptly in slender, curved arms that are lit by blue stars and the pink star - forming regions from which they spring

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained by Siding Spring's 3.9m telescope. NGC 1365, the largest spiral in the southern constellation of Fornax, is located at a distance of about 60 million light years. This beautiful galaxy is about as massive as the Milky Way, itself a substantial galaxy. Not much is known about how galaxies take on their beautiful forms, but a good deal is known about their internal organisation. The obvious 'bar' has the nucleus of the galaxy at its hub and is surrounded by masses of cooler stars that appear yellow on colour photographs. The bar itself is also yellowish, and has distinct dust lanes but it terminates abruptly in slender, curved arms that are lit by blue stars and the pink star - forming regions from which they spring

PIX4609870

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about

PIX4610090

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting gala

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting gala

PIX4611054

The Formation of the Earth and the Moon - Young Earth and Moon - The young Earth draped with thick clouds is illuminated by lightning and the reddish glow of volcanoes. Still surrounded by the remains of the primitive nebula, it will wait another 500 million years to cool sufisciously, form a solid crust and develop a primitive atmosphere. Top right is the Moon, still covered in molten lava. A young Earth is shrouded in turbulent, roiling clouds, while under the shadow of its night side can be seen flashes of lightning and the ruddy glow of volcanoes and lava fields illuminating the clouds from beneath. The space around the Earth is highlighted by remnants of the nebula from which the Solar System was born. On the upper right is the Earth's Moon whose lava - filled scars from massive impacts are still cooling. 500 million years after its molten birth the Earth's surface would have cooled enough for a solid crust to form, and gases delivered by comets and emissions from within would hav

The Formation of the Earth and the Moon - Young Earth and Moon - The young Earth draped with thick clouds is illuminated by lightning and the reddish glow of volcanoes. Still surrounded by the remains of the primitive nebula, it will wait another 500 million years to cool sufisciously, form a solid crust and develop a primitive atmosphere. Top right is the Moon, still covered in molten lava. A young Earth is shrouded in turbulent, roiling clouds, while under the shadow of its night side can be seen flashes of lightning and the ruddy glow of volcanoes and lava fields illuminating the clouds from beneath. The space around the Earth is highlighted by remnants of the nebula from which the Solar System was born. On the upper right is the Earth's Moon whose lava - filled scars from massive impacts are still cooling. 500 million years after its molten birth the Earth's surface would have cooled enough for a solid crust to form, and gases delivered by comets and emissions from within would hav

Walter B Myers

PIX4633451

S star Monocerotis and nebula - Fox Fur nebula in Monoceros - The region to the right of the bright star S Monocerotis is called Fox Fur nebula. This region where gas mixes with interstellar dust is located above the Cone nebula, about 2600 light years from Earth. Image obtained with a 50 cm telescope, composite of several images. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

S star Monocerotis and nebula - Fox Fur nebula in Monoceros - The region to the right of the bright star S Monocerotis is called Fox Fur nebula. This region where gas mixes with interstellar dust is located above the Cone nebula, about 2600 light years from Earth. Image obtained with a 50 cm telescope, composite of several images. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

R. Jay GaBany

PIX4618712

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

R. Gendler

PIX4619498

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

PIX4619538

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

R. Jay GaBany

PIX4619560

Release of Mr Lee 09/1994 - Astronaut M.Lee during EVA. Sep 16 1994 - Extra vehicle release by Mark Lee testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Mark C. Lee, STS - 64 mission specialist, tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The forward cargo bay is reflected in Lee's helmet visor in the 35 mm frame, exposed through the space shuttle Discovery's aft flight deck windows. Part of the hardware for the LIDAR - in - Space Technology Experiment (LITE) is in center foreground. Astronauts Lee and Carl J. Meade, mission specialist, took turns using the SAFER hardware during their shared Extrahicular Activity (EVA) on Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a p

Release of Mr Lee 09/1994 - Astronaut M.Lee during EVA. Sep 16 1994 - Extra vehicle release by Mark Lee testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Mark C. Lee, STS - 64 mission specialist, tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The forward cargo bay is reflected in Lee's helmet visor in the 35 mm frame, exposed through the space shuttle Discovery's aft flight deck windows. Part of the hardware for the LIDAR - in - Space Technology Experiment (LITE) is in center foreground. Astronauts Lee and Carl J. Meade, mission specialist, took turns using the SAFER hardware during their shared Extrahicular Activity (EVA) on Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a p

PIX4647074

Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

PIX4647118

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

PIX4568835

May 05, 1953 - FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Ranby, Lines., have just returned with these photographs taken by an air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which is within the Arctic circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H. D. Archer, D.F.C., and Flight Lieutenant R. W. Firmin, the aircraft each carried two staff navigators and five students, with other air and ground crew. BRITISH OFFICIAL PHOTO SHOWS: On returning from the North Pole, the two Hastings were inspected and serviced, and special engine covers were used.

May 05, 1953 - FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Ranby, Lines., have just returned with these photographs taken by an air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which is within the Arctic circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H. D. Archer, D.F.C., and Flight Lieutenant R. W. Firmin, the aircraft each carried two staff navigators and five students, with other air and ground crew. BRITISH OFFICIAL PHOTO SHOWS: On returning from the North Pole, the two Hastings were inspected and serviced, and special engine covers were used.

ZUM4841627

Feb. 04, 1954 -” Actress of Year” - And” Showman of Year” Honour At Variety Club Luncheon. Miss Dorothy Tutin, whose performance in Graham Greene's” The Living Room” made her the talk of the entertainment world, and Mr. Jack Hylton, the impresario, were honoured by the Variety Club as the” Actress of the Year” and the” Showman of the Year” respectively at a special testimonial luncheon held at the Savoy Hotel today. Miss Tutin was presented by Dame Sybil Thorndike with a scroll on which are recorded extracts from reviews on her performance in “The Living Room” by London critics. Each extract credits the newspaper in which it appeared and is signed by its author-critic. The choice of Miss Tutin is that of the London critics themselves, as is that Mr. Jack Hylton, to whom an inscribed scroll was presented by Sir Malcolm Sargent. Keystone Photo Shows: - Miss Dorothy Tutin and Mr. Jack Hylton, photographed at the luncheon today

Feb. 04, 1954 -” Actress of Year” - And” Showman of Year” Honour At Variety Club Luncheon. Miss Dorothy Tutin, whose performance in Graham Greene's” The Living Room” made her the talk of the entertainment world, and Mr. Jack Hylton, the impresario, were honoured by the Variety Club as the” Actress of the Year” and the” Showman of the Year” respectively at a special testimonial luncheon held at the Savoy Hotel today. Miss Tutin was presented by Dame Sybil Thorndike with a scroll on which are recorded extracts from reviews on her performance in “The Living Room” by London critics. Each extract credits the newspaper in which it appeared and is signed by its author-critic. The choice of Miss Tutin is that of the London critics themselves, as is that Mr. Jack Hylton, to whom an inscribed scroll was presented by Sir Malcolm Sargent. Keystone Photo Shows: - Miss Dorothy Tutin and Mr. Jack Hylton, photographed at the luncheon today

ZUM4914706

Dec. 12, 1953 - Medieval Painting discoveredin tower of London. Scene inside the Byward Tower: During repairs to structure of the Byward Tower, Tower of London, it was found that the main beam carrying the second floor above the gateway has painted decoration, mostly in gold.There are the leopards of England, many times repeated in gold, with red tongues, fleur de lis and small birds all over the beam. Further searching resulted in the discovery of portions of a very fine mural painting of the first half of the 14th. century. The painting suggests the scene of Christ in Majesty with an abbreviated version of the last judgement - part of which may have been removed when a fireplace was inserted in the wall in the 16th century. It includes figures of the Blessed Virgin and of St. Michael the Archangell

Dec. 12, 1953 - Medieval Painting discoveredin tower of London. Scene inside the Byward Tower: During repairs to structure of the Byward Tower, Tower of London, it was found that the main beam carrying the second floor above the gateway has painted decoration, mostly in gold.There are the leopards of England, many times repeated in gold, with red tongues, fleur de lis and small birds all over the beam. Further searching resulted in the discovery of portions of a very fine mural painting of the first half of the 14th. century. The painting suggests the scene of Christ in Majesty with an abbreviated version of the last judgement - part of which may have been removed when a fireplace was inserted in the wall in the 16th century. It includes figures of the Blessed Virgin and of St. Michael the Archangell

ZUM4898032

Apr. 04, 1954 Captain Nikdai Khoklov appeared at a crowded Press conference in Bonn called by the U.S. High Commissioner, Mr. James b. Conant.

Apr. 04, 1954 Captain Nikdai Khoklov appeared at a crowded Press conference in Bonn called by the U.S. High Commissioner, Mr. James b. Conant.

ZUM4926272

Sep. 09, 1953 - One Hundred pounds Burial Fee In Village Churchyard Charges Against Country Vicar: Investigation officers of the Inland Revuneu are making inquiries about the ~ 100 burial fees said to be vharged at the ancient Saxon churchyard of St. Mary Simpting, near Worthing, Sussex. TheVicar of the Parish Rev. N.E.C. Hemsworth is said to have been charging fees up to ~ 100 to buy nonparishioners. The investigations into the high price burials were startrd by Miss Ursual Winer Wintle of Manor0Road, Worthing, two years ago when she informed the local Inland Revenue authorities. Mr. Joseph Goild-the gravedigger at the churchyard said that local feelings had been aroused by the high charges the Vicar said” Of Courre I charge ~ 100 to bury non Parishioners-i charge what I like and it is no body's business. The Bishop of Chichester-the Right Rev. George Bell-said her was” Very surprised

Sep. 09, 1953 - One Hundred pounds Burial Fee In Village Churchyard Charges Against Country Vicar: Investigation officers of the Inland Revuneu are making inquiries about the ~ 100 burial fees said to be vharged at the ancient Saxon churchyard of St. Mary Simpting, near Worthing, Sussex. TheVicar of the Parish Rev. N.E.C. Hemsworth is said to have been charging fees up to ~ 100 to buy nonparishioners. The investigations into the high price burials were startrd by Miss Ursual Winer Wintle of Manor0Road, Worthing, two years ago when she informed the local Inland Revenue authorities. Mr. Joseph Goild-the gravedigger at the churchyard said that local feelings had been aroused by the high charges the Vicar said” Of Courre I charge ~ 100 to bury non Parishioners-i charge what I like and it is no body's business. The Bishop of Chichester-the Right Rev. George Bell-said her was” Very surprised

ZUM4880271

Triumphs of the Mother of God or Panos de Oro, c.1500-02 (tapestry)

Triumphs of the Mother of God or Panos de Oro, c.1500-02 (tapestry)

Coecke van Aelst, Pieter (1502-50) (attr. to)

CUL4908591

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. The greenish middle portion is evidence of excited oxygen atoms, while the outer red is predominantly light from nitrogen and hydrogen. The smallest of the radial blobs inside the red shell are about 150 astronomical units across (150 times the Earth - Sun distance) and they give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. The greenish middle portion is evidence of excited oxygen atoms, while the outer red is predominantly light from nitrogen and hydrogen. The smallest of the radial blobs inside the red shell are about 150 astronomical units across (150 times the Earth - Sun distance) and they give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars

PIX4623642

Decollage de la shuttle Discovery 05/2008 - Launch of space shuttle Discovery 05/2008 - Decollage de la shuttle Discovery on 31 May 2008. Mission STS-124. The Space Shuttle Discovery and its seven - member STS - 124 crew head towards Earth - orbit and a scheduled link - up with the International Space Station (ISS). Liftoff from Kennedy Space Center's launch pad 39A occurred on May 31, 2008 at 5:02 p.m. (EDT). The STS - 124 mission is the 26th in the assembly of the International Space Station. It is the second of three flights launching components to complete Jaxa's Kibo laboratory. During the mission, the shuttle crew will install Kibo's large Japanese Pressurized Module and its remote manipulator system. Onboard are astronauts Mark Kelly, commander; Ken Ham, pilot; Karen Nyberg, Mike Fossum, Ron Garan, Greg Chamitoff and Japan Aerospace Exploration Agency (JAXA) astronaut Akihiko Hoshide, all mission specialists. Chamitoff will join Expedition 17 in progress to serve as a flight eng

Decollage de la shuttle Discovery 05/2008 - Launch of space shuttle Discovery 05/2008 - Decollage de la shuttle Discovery on 31 May 2008. Mission STS-124. The Space Shuttle Discovery and its seven - member STS - 124 crew head towards Earth - orbit and a scheduled link - up with the International Space Station (ISS). Liftoff from Kennedy Space Center's launch pad 39A occurred on May 31, 2008 at 5:02 p.m. (EDT). The STS - 124 mission is the 26th in the assembly of the International Space Station. It is the second of three flights launching components to complete Jaxa's Kibo laboratory. During the mission, the shuttle crew will install Kibo's large Japanese Pressurized Module and its remote manipulator system. Onboard are astronauts Mark Kelly, commander; Ken Ham, pilot; Karen Nyberg, Mike Fossum, Ron Garan, Greg Chamitoff and Japan Aerospace Exploration Agency (JAXA) astronaut Akihiko Hoshide, all mission specialists. Chamitoff will join Expedition 17 in progress to serve as a flight eng

PIX4649025

Decolation of the space shuttle Atlantis. 05/2009 - STS - 125 lift - off - Decolation of the space shuttle Atlantis with the crew of the mission STS-125. This 11-day mission aims to maintain the Hubble space telescope. May 11, 2009. Space shuttle Atlantis roars into the cloudy sky above Launch Pad 39A at Nasa's Kennedy Space Center in Florida on the STS - 125 mission. Blue cones of light, mach diamonds, can be seen beneath the engine nozzles. The mach diamonds are a formation of shock waves in the exhaust plume of an aerospace propulsion system. Atlantis will meet with Nasa's Hubble Space Telescope. Liftoff was on time at 2:01 p.m. EDT. Atlantis' 11 - day flight will include five spacewalks to refurbish and upgrade the telescope with state - of - the - art science instruments that will expand Hubble's capabilities and extend its operational lifespan through at least 2014. The payload includes a Wide Field Camera 3, fine guidance sensor and the Cosmic Origins Spectrograph. May 11 2009

Decolation of the space shuttle Atlantis. 05/2009 - STS - 125 lift - off - Decolation of the space shuttle Atlantis with the crew of the mission STS-125. This 11-day mission aims to maintain the Hubble space telescope. May 11, 2009. Space shuttle Atlantis roars into the cloudy sky above Launch Pad 39A at Nasa's Kennedy Space Center in Florida on the STS - 125 mission. Blue cones of light, mach diamonds, can be seen beneath the engine nozzles. The mach diamonds are a formation of shock waves in the exhaust plume of an aerospace propulsion system. Atlantis will meet with Nasa's Hubble Space Telescope. Liftoff was on time at 2:01 p.m. EDT. Atlantis' 11 - day flight will include five spacewalks to refurbish and upgrade the telescope with state - of - the - art science instruments that will expand Hubble's capabilities and extend its operational lifespan through at least 2014. The payload includes a Wide Field Camera 3, fine guidance sensor and the Cosmic Origins Spectrograph. May 11 2009

PIX4649122

Decolation of the space shuttle Endeavour - 07/2009 - Space Shuttle Endeavour lift - off - Decolation of the space shuttle Endeavour with the crew of the mission STS - 127 on 15 July 2009. The purpose of this mission is to complete the assembly of the Kibo Laboratory of the International Space Station (ISS). Space Shuttle Endeavour and its seven - member STS - 127 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was on time at 6:03 p.m. (EDT) on July 15, 2009 from launch pad 39A at Nasa's Kennedy Space Center. Onboard are astronauts Mark Polansky, commander; Doug Hurley, pilot; Christopher Cassidy, Tom Marshburn, Dave Wolf, Tim Kopra and Canadian Space Agency's Julie Payette, all mission specialists. Kopra will join Expedition 20 in progress to serve as a flight engineer aboard the ISS. Endeavour will deliver the Japanese Experiment Model's Exposed Facility and the Experiment Logistics Module - Exposed Section in the final of three flights dedi

Decolation of the space shuttle Endeavour - 07/2009 - Space Shuttle Endeavour lift - off - Decolation of the space shuttle Endeavour with the crew of the mission STS - 127 on 15 July 2009. The purpose of this mission is to complete the assembly of the Kibo Laboratory of the International Space Station (ISS). Space Shuttle Endeavour and its seven - member STS - 127 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was on time at 6:03 p.m. (EDT) on July 15, 2009 from launch pad 39A at Nasa's Kennedy Space Center. Onboard are astronauts Mark Polansky, commander; Doug Hurley, pilot; Christopher Cassidy, Tom Marshburn, Dave Wolf, Tim Kopra and Canadian Space Agency's Julie Payette, all mission specialists. Kopra will join Expedition 20 in progress to serve as a flight engineer aboard the ISS. Endeavour will deliver the Japanese Experiment Model's Exposed Facility and the Experiment Logistics Module - Exposed Section in the final of three flights dedi

PIX4649179

Discovery Shuttle Landing 03/2011 - Landing of Space Shuttle Discovery in March 2011 - Discovery Shuttle Landing at Kennedy Space Center March 9, 2011. Last mission of Shuttle Discovery. Space shuttle Discovery's drag chute deployys on Runway 15 at the Shuttle Landing Facility at Nasa's Kennedy Space Center in Florida. Discovery's final return from space completed the 13 - day, 5.3 - million - mile STS - 133 mission. Main gear touchdown was on March 9 2011 at 11:57:17 a.m., followed by nose gear touchdown at 11:57:28, and wheelstop at 11:58:14 a.m. On board are Commander Steve Lindsey, Pilot Eric Boe, and Mission Specialists Nicole Stott, Michael Barratt, Alvin Drew and Steve Bowen. Discovery and its six - member crew delivered the Permanent Multipurpose Module, packed with supplies and critical spare parts, as well as Robonaut 2, the dexterous humanoid astronaut helper, to the orbiting outpost. STS - 133 was Discovery's 39th and final mission. This was the 133rd Space Shuttle Program

Discovery Shuttle Landing 03/2011 - Landing of Space Shuttle Discovery in March 2011 - Discovery Shuttle Landing at Kennedy Space Center March 9, 2011. Last mission of Shuttle Discovery. Space shuttle Discovery's drag chute deployys on Runway 15 at the Shuttle Landing Facility at Nasa's Kennedy Space Center in Florida. Discovery's final return from space completed the 13 - day, 5.3 - million - mile STS - 133 mission. Main gear touchdown was on March 9 2011 at 11:57:17 a.m., followed by nose gear touchdown at 11:57:28, and wheelstop at 11:58:14 a.m. On board are Commander Steve Lindsey, Pilot Eric Boe, and Mission Specialists Nicole Stott, Michael Barratt, Alvin Drew and Steve Bowen. Discovery and its six - member crew delivered the Permanent Multipurpose Module, packed with supplies and critical spare parts, as well as Robonaut 2, the dexterous humanoid astronaut helper, to the orbiting outpost. STS - 133 was Discovery's 39th and final mission. This was the 133rd Space Shuttle Program

PIX4649595

Saturn by Voyager 2 - Rings in fake colors - Composition differences within Saturn's rings. Voyager 2 - Image in false colors made by the Voyager 2 probe on August 17, 1981 at a distance of 8.9 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The different colors correspond to differences in the chemical composition of the particles that make up the rings. Possible variations in chemical composition from one part of Saturn's ring system to another are visible in this Voyager 2 picture as subtle color variations that can be recorded with special computer - processing techniques. This highly enhanced color view was assembled from clear, orange and ultraviolet frames obtained Aug. 17 from a distance of 8.9 million kilometers (5.5 million miles). In addition to the previously known blue color of the C - ring and the Cassini Division, the picture shows additional color

Saturn by Voyager 2 - Rings in fake colors - Composition differences within Saturn's rings. Voyager 2 - Image in false colors made by the Voyager 2 probe on August 17, 1981 at a distance of 8.9 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The different colors correspond to differences in the chemical composition of the particles that make up the rings. Possible variations in chemical composition from one part of Saturn's ring system to another are visible in this Voyager 2 picture as subtle color variations that can be recorded with special computer - processing techniques. This highly enhanced color view was assembled from clear, orange and ultraviolet frames obtained Aug. 17 from a distance of 8.9 million kilometers (5.5 million miles). In addition to the previously known blue color of the C - ring and the Cassini Division, the picture shows additional color

PIX4624957

Jet stream over Canada - Jet stream over Canada - Jet stream over Cape Breton Island, Canada, seen by Space Shuttle Discovery in May 1991. The Northern Hemisphere Jet Stream can be seen crossing Cape Breton Island in the Maritime Provinces of Eastern Canada. The Jet Stream is a narrow zone of high - speed winds typically found at altitudes of 4 to 8 miles (8 - 12 km) above the earth. They result from temperature contrasts between polar and tropical regions. The strongest Jet Stream winds are found in the winter when the contrast between polar and tropical regions is the greatest. Wind speeds can reach 90 to over 180 miles per hour (145 to over 290 km/h) from west to east. During the winter months over the United States and southern Canada, the path taken by the Jet Stream can have a large influence on the weather conditions of this region. Image taken from the space shuttle Discovery in May 1991

Jet stream over Canada - Jet stream over Canada - Jet stream over Cape Breton Island, Canada, seen by Space Shuttle Discovery in May 1991. The Northern Hemisphere Jet Stream can be seen crossing Cape Breton Island in the Maritime Provinces of Eastern Canada. The Jet Stream is a narrow zone of high - speed winds typically found at altitudes of 4 to 8 miles (8 - 12 km) above the earth. They result from temperature contrasts between polar and tropical regions. The strongest Jet Stream winds are found in the winter when the contrast between polar and tropical regions is the greatest. Wind speeds can reach 90 to over 180 miles per hour (145 to over 290 km/h) from west to east. During the winter months over the United States and southern Canada, the path taken by the Jet Stream can have a large influence on the weather conditions of this region. Image taken from the space shuttle Discovery in May 1991

PIX4674483

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

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

PIX4644423

Spiral Galaxy NGC 247 in the Whale - Spiral galaxy NGC 247 in Cetus - Dwarf spiral galaxy in the Whale, located about 11 million years ago - light from Earth. Image obtained with the 2.2 meter MPG/ESO telescope at the La Silla Observatory. The spiral galaxy NGC 247 is one of the closest spiral galaxies of the southern sky. In this view from the Wide Field Imager on the MPG/ESO 2.2 - metre telescope in Chile large numbers of the galaxy's component stars are clearly resolved and many glowing pink clouds of hydrogen, marking regions of active star formation, can be made out in the loose and ragged spiral arms. NGC 247 is part of the Sculptor Group. This is the nearest group of galaxies to our Local Group, which includes the Milky Way, but putting a precise value on such celestial distances is inherently difficult. Astronomers have reported that NGC 247 is more than a million light - years closer to the Milky Way than was previously thought, bringing its distance down to just over 11 milli

Spiral Galaxy NGC 247 in the Whale - Spiral galaxy NGC 247 in Cetus - Dwarf spiral galaxy in the Whale, located about 11 million years ago - light from Earth. Image obtained with the 2.2 meter MPG/ESO telescope at the La Silla Observatory. The spiral galaxy NGC 247 is one of the closest spiral galaxies of the southern sky. In this view from the Wide Field Imager on the MPG/ESO 2.2 - metre telescope in Chile large numbers of the galaxy's component stars are clearly resolved and many glowing pink clouds of hydrogen, marking regions of active star formation, can be made out in the loose and ragged spiral arms. NGC 247 is part of the Sculptor Group. This is the nearest group of galaxies to our Local Group, which includes the Milky Way, but putting a precise value on such celestial distances is inherently difficult. Astronomers have reported that NGC 247 is more than a million light - years closer to the Milky Way than was previously thought, bringing its distance down to just over 11 milli

PIX4609139

Galaxies M81 and M82 in the Great Bear - Galaxies M81 and M82 in Ursa major - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 12 million light years away from Earth. M81, seen here at left, is a grand design spiral galaxy that forms a physical pair with irregular galaxy M82. They are separated by 150,000 light years at a distance of 12 million light years. This galaxy group, consisting of M81, M82, NGC 3077 and NGC 2976, is the nearest galaxy group to our own local group of galaxies that contains the Milky Way, Magellanic Clouds, M33, and the M31 - M32 - M110 system. This galaxy group, consisting of M81, M82, NGC 3077 and NGC 2976, is the nearest galaxy group to our own local group of galaxies that contains the Milky Way, Magellanic Clouds, M33, and the M31 - M32 - M110 system

Galaxies M81 and M82 in the Great Bear - Galaxies M81 and M82 in Ursa major - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 12 million light years away from Earth. M81, seen here at left, is a grand design spiral galaxy that forms a physical pair with irregular galaxy M82. They are separated by 150,000 light years at a distance of 12 million light years. This galaxy group, consisting of M81, M82, NGC 3077 and NGC 2976, is the nearest galaxy group to our own local group of galaxies that contains the Milky Way, Magellanic Clouds, M33, and the M31 - M32 - M110 system. This galaxy group, consisting of M81, M82, NGC 3077 and NGC 2976, is the nearest galaxy group to our own local group of galaxies that contains the Milky Way, Magellanic Clouds, M33, and the M31 - M32 - M110 system

Jerry Lodriguss

PIX4610297

Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Fie

Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Fie

PIX4612005

Globular cluster NGC 6522 in Sagittarius - Globular cluster NGC 6522 in Sagittarius - This cluster of stars is located about 25,000 years - light from Earth towards the center of our galaxy

Globular cluster NGC 6522 in Sagittarius - Globular cluster NGC 6522 in Sagittarius - This cluster of stars is located about 25,000 years - light from Earth towards the center of our galaxy

PIX4564845

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564863

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

PIX4603085

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

PIX4603096

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

The International Space Station (ISS) and the Shuttle Endeavour 05/2011 - The Space Shuttle Endeavour docked to the International Space Station (ISS) 05/2011 - View of the Space Shuttle Endeavour moored at the International Space Station, from the Soyuz TMA spaceship - 20 on 23 May 2011. This series of images shows for the first time a shuttle moored to the space station from a Russian Soyuz spaceship. This image of the International Space Station and the docked Space Shuttle Endeavour, flying at an altitude of approximately 220 miles, was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA - 20 following its undocking on May 23, 2011 (USA time). The pictures are the first taken of a shuttle docked to the International Space Station from the perspective of a Russian Soyuz spacecraft. Onboard the Soyuz were Russian cosmonaut and Expedition 27 commander Dmitry Kondratyev; Nespoli, a European Space Agency astronaut; and NASA astronaut Cady Coleman. Coleman and Nespoli were

PIX4603143

Crews STS - 98 and Expedition1 in Destiny (ISS) 02/2001 - STS - 98 and expedition 1 crews in Destiny (ISS) 02/2001 - Crew group photo. Expedition 1 in first row (from left to right): Sergei Krikalev, William (Bill) Shepherd and Yuri Gidzenko; STS - 98 in second place (from left to right): Mark Polansky, Kenneth Cockrell, Marsha Ivins, Robert Curbeam and Thomas Jones. STS-98. 12/02/2001. The crews of the Space Shuttle Atlantis and International Space Station (ISS) interrupt work aboard the newly installed Destiny laboratory to pose for an in - flight joint group portrait. In front are (from the left) cosmonaut Sergei K. Krikalev, Expedition One flight engineer; astronaut William M. (Bill) Shepherd, Expedition One mission commander; and Yuri P. Gidzenko, Soyuz commander. The shuttle crew is made up of (from the left) astronauts Mark L. Polansky, pilot; Kenneth D. Cockrell, mission commander; and Marsha S. Ivins, Robert L. Curbeam and Thomas D. Jones, all mission specialists. Krikalev and

Crews STS - 98 and Expedition1 in Destiny (ISS) 02/2001 - STS - 98 and expedition 1 crews in Destiny (ISS) 02/2001 - Crew group photo. Expedition 1 in first row (from left to right): Sergei Krikalev, William (Bill) Shepherd and Yuri Gidzenko; STS - 98 in second place (from left to right): Mark Polansky, Kenneth Cockrell, Marsha Ivins, Robert Curbeam and Thomas Jones. STS-98. 12/02/2001. The crews of the Space Shuttle Atlantis and International Space Station (ISS) interrupt work aboard the newly installed Destiny laboratory to pose for an in - flight joint group portrait. In front are (from the left) cosmonaut Sergei K. Krikalev, Expedition One flight engineer; astronaut William M. (Bill) Shepherd, Expedition One mission commander; and Yuri P. Gidzenko, Soyuz commander. The shuttle crew is made up of (from the left) astronauts Mark L. Polansky, pilot; Kenneth D. Cockrell, mission commander; and Marsha S. Ivins, Robert L. Curbeam and Thomas D. Jones, all mission specialists. Krikalev and

PIX4600245

Remains of supernova des Voiles - detail - Pencil nebula - NGC 2736, the Pencil nebula in Vela - Detail of the rest of the supernova des Voiles: the nebula of the pencil (NGC 2736). The supernova exploded 12,000 years ago. The rest of the supernova is approximately 815 years away from Earth. Image obtained with Siding Spring's 3.9m telescope. This is an outlying wisp of the Vela supernova remnant (SNR), almost the only sign of the eastern part of this vast bubble of expanding shock wave from a stellar explosion 12,000 years ago. Although clearly detected with radio and X - ray telescopes, the Vela SNR is partially hidden to optical observers. Many fine, tangled filaments are seen in the western part of the nebula, but in the east, most of it is hidden in dust. This is one of the brighter eastern fragments, and its unusual linear appearance in the telescope was remarked on by Sir John Herschel who discovered to nebula in the 1840s. This spindly shape is the source of its popular name

Remains of supernova des Voiles - detail - Pencil nebula - NGC 2736, the Pencil nebula in Vela - Detail of the rest of the supernova des Voiles: the nebula of the pencil (NGC 2736). The supernova exploded 12,000 years ago. The rest of the supernova is approximately 815 years away from Earth. Image obtained with Siding Spring's 3.9m telescope. This is an outlying wisp of the Vela supernova remnant (SNR), almost the only sign of the eastern part of this vast bubble of expanding shock wave from a stellar explosion 12,000 years ago. Although clearly detected with radio and X - ray telescopes, the Vela SNR is partially hidden to optical observers. Many fine, tangled filaments are seen in the western part of the nebula, but in the east, most of it is hidden in dust. This is one of the brighter eastern fragments, and its unusual linear appearance in the telescope was remarked on by Sir John Herschel who discovered to nebula in the 1840s. This spindly shape is the source of its popular name

PIX4582828

Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

PIX4589225

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

PIX4593306

Eagle and Fleche Constellations - Aquila and Sagitta constellations - The brightest star of this constellation is Altair. It is one of the brightest stars in the night sky. It is the center of an almost perfect alignment of three stars and is located about 16 years - light from the Sun. Above the small constellation of the Fleche. Aquila (the Eagle) well represents a mythological bird that was the companion of Jupiter. It lies in the northern Milky Way and contans rich fields of stars particularly in the western half and into adjoining Scutum. The brightest star in the constellation is Altair (Arabic for flying eagle), which is at one corner of the Summer Triangle (Altair, Deneb and Vega). Sagitta (the Arrow) is the third smallest constellation in the sky, and although it contains no bright stars, was well known to the ancient Greeks. Its arrow seems directed through Vulpecula and Pegasus towards Andromeda, skirting Cygnus. These constellations are a little north of the celestial equat

Eagle and Fleche Constellations - Aquila and Sagitta constellations - The brightest star of this constellation is Altair. It is one of the brightest stars in the night sky. It is the center of an almost perfect alignment of three stars and is located about 16 years - light from the Sun. Above the small constellation of the Fleche. Aquila (the Eagle) well represents a mythological bird that was the companion of Jupiter. It lies in the northern Milky Way and contans rich fields of stars particularly in the western half and into adjoining Scutum. The brightest star in the constellation is Altair (Arabic for flying eagle), which is at one corner of the Summer Triangle (Altair, Deneb and Vega). Sagitta (the Arrow) is the third smallest constellation in the sky, and although it contains no bright stars, was well known to the ancient Greeks. Its arrow seems directed through Vulpecula and Pegasus towards Andromeda, skirting Cygnus. These constellations are a little north of the celestial equat

PIX4588824

Open cluster NGC 2244 in the nebula of the Rosette - The Rosette Nebula and NGC 2244 cluster - The Rosette nebula is a vast cloud of dust and gas situated about 5500 years away from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

Open cluster NGC 2244 in the nebula of the Rosette - The Rosette Nebula and NGC 2244 cluster - The Rosette nebula is a vast cloud of dust and gas situated about 5500 years away from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

PIX4618488

Apr. 04, 1953 - The scene of the crucifixion. The great climax of the passion play, floodlit. CHRISTM'S PASSION RE-ENACTED IN ITALY. Every Good Friday, thousands of visitors, many from overseas, flock to Grassina, near Florence, Italy, to see the re-enactment of Christ's journey to the Cross and the crucifixion. Some six hundred people take part in the ceremony. The procession is led by Roman Soldiers and includes the Virgin Mary, Mary Magdalen and Judas. Lastly comes Christ carrying the heavy cross. The man who plays the part of Christ has nothing to eat the day before the ceremony, he really suffers carrying the heavy cross which lends great drama and realism to the performance. When the procession reaches the top of Calvario Hill, the Music of Handel, Wagner, Verdi and Rossini is played, the three crosses are illuminated by floodlighting provided by the Italian Army Engineers and a dramatic climax is given by the outbreak of a terrible storm.

Apr. 04, 1953 - The scene of the crucifixion. The great climax of the passion play, floodlit. CHRISTM'S PASSION RE-ENACTED IN ITALY. Every Good Friday, thousands of visitors, many from overseas, flock to Grassina, near Florence, Italy, to see the re-enactment of Christ's journey to the Cross and the crucifixion. Some six hundred people take part in the ceremony. The procession is led by Roman Soldiers and includes the Virgin Mary, Mary Magdalen and Judas. Lastly comes Christ carrying the heavy cross. The man who plays the part of Christ has nothing to eat the day before the ceremony, he really suffers carrying the heavy cross which lends great drama and realism to the performance. When the procession reaches the top of Calvario Hill, the Music of Handel, Wagner, Verdi and Rossini is played, the three crosses are illuminated by floodlighting provided by the Italian Army Engineers and a dramatic climax is given by the outbreak of a terrible storm.

ZUM4832621

Jun. 06, 1953 - Mrs. Maclean Vanishes, With The Children: Mrs. Melinda Maclean, wife of the missing British diplomat, Donald Maclean, and her children have “disappeared and are being looked for”, spokesman of the British Consulate General said in Geneva today., The Foreign Office have been told mrs.Maclean's dis appearance, the spokesman added information about the disappearance. Some week ago Mrs. Maclaen when to holiday to Majorca, in the Balearic Isles. She returned to Geneva to take her two eldest children to the International School there, But she found that the School terminal had been postponed for a week. Mrs. Maclean is then believed to have gone holiday for a few days in the Montreu area. The school term began on September 14. Neither of the Maclean children was there

Jun. 06, 1953 - Mrs. Maclean Vanishes, With The Children: Mrs. Melinda Maclean, wife of the missing British diplomat, Donald Maclean, and her children have “disappeared and are being looked for”, spokesman of the British Consulate General said in Geneva today., The Foreign Office have been told mrs.Maclean's dis appearance, the spokesman added information about the disappearance. Some week ago Mrs. Maclaen when to holiday to Majorca, in the Balearic Isles. She returned to Geneva to take her two eldest children to the International School there, But she found that the School terminal had been postponed for a week. Mrs. Maclean is then believed to have gone holiday for a few days in the Montreu area. The school term began on September 14. Neither of the Maclean children was there

ZUM4851068

Feb. 02, 1954 -” Actress of year” - and” Showman of year” honour at Variety Club Luncheon. Miss Dorthy Tutin, whose performance in Graham Greene's” The living Room” made her the talk of the entertainment world, and Mr. Jack Hylton, the impresaric, were honoured by the Variety Club as the” Actress of the Year” and the” Showman of the Year” redpectively at a special testimonial luncheon held at hte Savoy Hotel today. Miss Tutin was presented by Dame Sybil Thorndike with a scroll on which are recroduced extracts from reviews on her performance in” The Living Room'By London critics. Each extract credits the newspaper in which it appeared and is signed by its author-critic. The choies of Miss Tutin is that of the London Critics themselves, as is that of Mr. Jack Hylton, to whom an inscribrd scroll was presented by Sir Malcolm Sargent

Feb. 02, 1954 -” Actress of year” - and” Showman of year” honour at Variety Club Luncheon. Miss Dorthy Tutin, whose performance in Graham Greene's” The living Room” made her the talk of the entertainment world, and Mr. Jack Hylton, the impresaric, were honoured by the Variety Club as the” Actress of the Year” and the” Showman of the Year” redpectively at a special testimonial luncheon held at hte Savoy Hotel today. Miss Tutin was presented by Dame Sybil Thorndike with a scroll on which are recroduced extracts from reviews on her performance in” The Living Room'By London critics. Each extract credits the newspaper in which it appeared and is signed by its author-critic. The choies of Miss Tutin is that of the London Critics themselves, as is that of Mr. Jack Hylton, to whom an inscribrd scroll was presented by Sir Malcolm Sargent

ZUM4910481

Dec. 12, 1953 - Russian shoot Mother and son family travelling from East to West Berlin.: Russian troops on Sunday night killed Joachim Wozniak (16) and seriously wounded his mother in the thight they fired on the van in which the family was travelling from the Autobabn checkpoint at Babelsberg in teh East Zone to West Berlin Police post on the intersector frontier. West Berlin police, to whom the father run for assistance, were not permitted by the Russians to cross the frontier to give medical help. People's Police later allowed Wozniak to drive the vehicle back to their post at Babelzberg. No medical help was available there. After further delay he was allowed to drive the vehicle into West Berlin. By this time his son had died and his wife was seriously ill from loss of blood. The West Berlin murder squad are investigating the incident

Dec. 12, 1953 - Russian shoot Mother and son family travelling from East to West Berlin.: Russian troops on Sunday night killed Joachim Wozniak (16) and seriously wounded his mother in the thight they fired on the van in which the family was travelling from the Autobabn checkpoint at Babelsberg in teh East Zone to West Berlin Police post on the intersector frontier. West Berlin police, to whom the father run for assistance, were not permitted by the Russians to cross the frontier to give medical help. People's Police later allowed Wozniak to drive the vehicle back to their post at Babelzberg. No medical help was available there. After further delay he was allowed to drive the vehicle into West Berlin. By this time his son had died and his wife was seriously ill from loss of blood. The West Berlin murder squad are investigating the incident

ZUM4900296

Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to tran

Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to tran

Walter B Myers

PIX4640726

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Walter B Myers

PIX4629809

Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop is a very low emission nebula, very large, that surrounds the great Orion nebula. Here, the brightest part of the Loop, with lower left the cluster of stars NGC 2112, and to the right the nebula by refexion M78. Also visible is a dark nebula LDN 1622 at the top left of the image. Barnard's Loop is an extremely faint emission nebula which is part of an amazing, even larger complex of nebulosity in the constellation of Orion. This photo shows only the brightest central portion of the loop which runs diagonally across the frame here from lower left to upper right. NGC 2112, a ninth magnitude open cluster 11 arc minutes in diameter and containing about 50 stars, is seen at lower left - center, and reflection nebulae M78 and NGC 2071 are at lower right. An interesting dark nebula, LDN 1622, lies at the upper left of the image, surrounded by very faint emission nebulosity, with a hi

Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop is a very low emission nebula, very large, that surrounds the great Orion nebula. Here, the brightest part of the Loop, with lower left the cluster of stars NGC 2112, and to the right the nebula by refexion M78. Also visible is a dark nebula LDN 1622 at the top left of the image. Barnard's Loop is an extremely faint emission nebula which is part of an amazing, even larger complex of nebulosity in the constellation of Orion. This photo shows only the brightest central portion of the loop which runs diagonally across the frame here from lower left to upper right. NGC 2112, a ninth magnitude open cluster 11 arc minutes in diameter and containing about 50 stars, is seen at lower left - center, and reflection nebulae M78 and NGC 2071 are at lower right. An interesting dark nebula, LDN 1622, lies at the upper left of the image, surrounded by very faint emission nebulosity, with a hi

Jerry Lodriguss

PIX4618145

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Tom Davis

PIX4618385

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

PIX4618821

Nebula IC 1318 in the Swan - IC 1318 Butterfly nebula in Cygnus - IC 1318 is a very large emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. LDN 889 is a vast region of dark nebulae that separates the nebula on the left from Sadr. On the extreme right, another dark nebula, B343. Image obtained with H - alpha filter, 5 hours of cumulative poses. This is a large area of emission nebulosity around Sadr, Gamma Cygnii, the brightest star in this photo and the heart of Cygnus. Most of the nebulosity is fairly faint, but brighter patches can be seen in a modest instrument. The two sections of nebulosity to the left of Gamma are called the Butterfly Nebula and have the catalog designation of IC 1318. LDN 889 is the large area of dark nebulosity that separates the two halves of the Butterfly Nebula, and B 343 is the small but very dense dark nebula on the right side of the image. This is a hydrogen alpha color composite image

Nebula IC 1318 in the Swan - IC 1318 Butterfly nebula in Cygnus - IC 1318 is a very large emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. LDN 889 is a vast region of dark nebulae that separates the nebula on the left from Sadr. On the extreme right, another dark nebula, B343. Image obtained with H - alpha filter, 5 hours of cumulative poses. This is a large area of emission nebulosity around Sadr, Gamma Cygnii, the brightest star in this photo and the heart of Cygnus. Most of the nebulosity is fairly faint, but brighter patches can be seen in a modest instrument. The two sections of nebulosity to the left of Gamma are called the Butterfly Nebula and have the catalog designation of IC 1318. LDN 889 is the large area of dark nebulosity that separates the two halves of the Butterfly Nebula, and B 343 is the small but very dense dark nebula on the right side of the image. This is a hydrogen alpha color composite image

R. Gendler

PIX4622161

Decolation of the space shuttle Endeavour - 07/2009 - Space Shuttle Endeavour lift - off - Decolation of the space shuttle Endeavour with the crew of the mission STS - 127 on 15 July 2009. The purpose of this mission is to complete the assembly of the Kibo Laboratory of the International Space Station (ISS). Space Shuttle Endeavour and its seven - member STS - 127 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was on time at 6:03 p.m. (EDT) on July 15, 2009 from launch pad 39A at Nasa's Kennedy Space Center. Onboard are astronauts Mark Polansky, commander; Doug Hurley, pilot; Christopher Cassidy, Tom Marshburn, Dave Wolf, Tim Kopra and Canadian Space Agency's Julie Payette, all mission specialists. Kopra will join Expedition 20 in progress to serve as a flight engineer aboard the ISS. Endeavour will deliver the Japanese Experiment Model's Exposed Facility and the Experiment Logistics Module - Exposed Section in the final of three flights dedi

Decolation of the space shuttle Endeavour - 07/2009 - Space Shuttle Endeavour lift - off - Decolation of the space shuttle Endeavour with the crew of the mission STS - 127 on 15 July 2009. The purpose of this mission is to complete the assembly of the Kibo Laboratory of the International Space Station (ISS). Space Shuttle Endeavour and its seven - member STS - 127 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was on time at 6:03 p.m. (EDT) on July 15, 2009 from launch pad 39A at Nasa's Kennedy Space Center. Onboard are astronauts Mark Polansky, commander; Doug Hurley, pilot; Christopher Cassidy, Tom Marshburn, Dave Wolf, Tim Kopra and Canadian Space Agency's Julie Payette, all mission specialists. Kopra will join Expedition 20 in progress to serve as a flight engineer aboard the ISS. Endeavour will deliver the Japanese Experiment Model's Exposed Facility and the Experiment Logistics Module - Exposed Section in the final of three flights dedi

PIX4649180

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of 57 images taken by the robot on January 19, 2016. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at “” Namib Dune,””” where the rover's activities included scuffing into the dune with a wheel and scooping samples of sand for laboratory analysis. The scene combines 57 images taken on Jan. 19, 2016, during the 1,228th Martian day, or sol, of Curiosity's work on Mars. The camera used for this is the Mars Hand Lens Imager (MAHLI) at the end of the rover's robotic arm. The view does not include the rover's arm. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. For scale, the rover's wheels are 20 inches (50 centimeters) in diamet

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of 57 images taken by the robot on January 19, 2016. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at “” Namib Dune,””” where the rover's activities included scuffing into the dune with a wheel and scooping samples of sand for laboratory analysis. The scene combines 57 images taken on Jan. 19, 2016, during the 1,228th Martian day, or sol, of Curiosity's work on Mars. The camera used for this is the Mars Hand Lens Imager (MAHLI) at the end of the rover's robotic arm. The view does not include the rover's arm. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. For scale, the rover's wheels are 20 inches (50 centimeters) in diamet

PIX4643637

Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes

Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes

PIX4619692

Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

Release of Carl J. Meade 09/1994 - Astronaut Carl J. Meade during EVA. Sep 16 1994 - Extra vehicle release by Carl J. Meade testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Carl J. Meade tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The scene was captured with a 70 mm handheld Hasselblad camera with a 30 mm lens attached. The hardware supporting the LIDAR - in - Space Technology Experiment (LITE) is in the lower right. A TV camera on the Remote Manipulator System (RMS) arm records the Extravehicular Activity (EVA). Astronauts Meade and Mark C. Lee took turns using the SAFER hardware during their shared EVA of Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a production versi

PIX4647091

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564866

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