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Constellation of Lupus and Norma - Constellation of Lupus and Norma - Also visible are the constellations of the Compas, the Southern Cross, and much of the Centaur. At the top of the picture, the bright spot is the planet Jupiter. Lupus, (the Wolf), was regarded by the Greeks and Romans as an unspecified wild animal, which the Centaur is carrying as a sacrifice the gods. The identification of Lupus as a wolf seems to have been made in relatively recent times. Both Lupus and Norma are in the rich starfields of the southern Milky Way, easily seen between Antares and alpha and beta Centaurii. The brightest object in this image is Jupiter, on the ecliptic at the top of the frame. Norma, (originally Norma and Regula, the builder's level and set square) is an insignificant scattering of stars compared to Lupus and Centaurus. Like the adjacent Circinus (the Drawing Compasses), it was invented by Nicolas de Lacaille, who charted the southern sky from South Africa in 1751 - 2 and felt obliged

Constellation of Lupus and Norma - Constellation of Lupus and Norma - Also visible are the constellations of the Compas, the Southern Cross, and much of the Centaur. At the top of the picture, the bright spot is the planet Jupiter. Lupus, (the Wolf), was regarded by the Greeks and Romans as an unspecified wild animal, which the Centaur is carrying as a sacrifice the gods. The identification of Lupus as a wolf seems to have been made in relatively recent times. Both Lupus and Norma are in the rich starfields of the southern Milky Way, easily seen between Antares and alpha and beta Centaurii. The brightest object in this image is Jupiter, on the ecliptic at the top of the frame. Norma, (originally Norma and Regula, the builder's level and set square) is an insignificant scattering of stars compared to Lupus and Centaurus. Like the adjacent Circinus (the Drawing Compasses), it was invented by Nicolas de Lacaille, who charted the southern sky from South Africa in 1751 - 2 and felt obliged

PIX4592189

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

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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

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Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai Volcano is an active volcano located in Tanzania in the Great Rift Valley. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Image obtained from the EO-1 satellite on 12 September 2009. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite. The lava of Ol Doinyo Lengai is extremely cool (500 - 600* C, compared to 1,160* C for typical basaltic lava) and relatively fluid. Ol Doinyo Lengai alternates between eruptions of liquid lava that form lava lakes and fountains (called effusive eruptions) and explosive eruptions that build large cinder and ash cones. The new cone and crater are clearly visible in the center of the image acquired by satellite EO-1 on September 12, 2009. The dark spot in the crater may be fresh lava erupted from a new volcanic vent. Gray ash covers the volcano and much of the surrounding landscape

Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai Volcano is an active volcano located in Tanzania in the Great Rift Valley. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Image obtained from the EO-1 satellite on 12 September 2009. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite. The lava of Ol Doinyo Lengai is extremely cool (500 - 600* C, compared to 1,160* C for typical basaltic lava) and relatively fluid. Ol Doinyo Lengai alternates between eruptions of liquid lava that form lava lakes and fountains (called effusive eruptions) and explosive eruptions that build large cinder and ash cones. The new cone and crater are clearly visible in the center of the image acquired by satellite EO-1 on September 12, 2009. The dark spot in the crater may be fresh lava erupted from a new volcanic vent. Gray ash covers the volcano and much of the surrounding landscape

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Sandy Cay - Bahamas - Seabed currents and sandbanks on Sandy Cay and Long Island, Bahamas. Image obtained on 27 November 2010 from the International Space Station (ISS). This astronaut photograph, taken from the International space station on November 27, 2010, provides a view of tidal flats and channels near Sandy Cay, on the western side of Long Island and along the eastern margin of the Great Bahama Bank (North is top). The continuously exposed parts of the island are brown, a result of soil formation and vegetation growth. To the north of Sandy Cay, an off - white tidal flat composed of carbonate sediments is visible; light blue - green regions indicate shallow water on the tidal flat. The tidal flow of seawater is concentrated through gaps in the land surface, leading to the formation of relatively deep channels that cut into the sediments. The channels and areas to the south of the island have a vivid blue color that indicates deeper water

Sandy Cay - Bahamas - Seabed currents and sandbanks on Sandy Cay and Long Island, Bahamas. Image obtained on 27 November 2010 from the International Space Station (ISS). This astronaut photograph, taken from the International space station on November 27, 2010, provides a view of tidal flats and channels near Sandy Cay, on the western side of Long Island and along the eastern margin of the Great Bahama Bank (North is top). The continuously exposed parts of the island are brown, a result of soil formation and vegetation growth. To the north of Sandy Cay, an off - white tidal flat composed of carbonate sediments is visible; light blue - green regions indicate shallow water on the tidal flat. The tidal flow of seawater is concentrated through gaps in the land surface, leading to the formation of relatively deep channels that cut into the sediments. The channels and areas to the south of the island have a vivid blue color that indicates deeper water

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Southern Aurora observed from space station - Aurora Australis seen from space - Southern Aurora observed from the International Space Station (ISS) on 29 May 2010. Aurora australis seen from the International Space Station (ISS) on May 29, 2010. The ISS was located over the Southern Indian Ocean at an altitude of 350 km, with the astronaut observer most likely looking towards Antarctica (not visible) and the South Pole. The aurora has a sinuous ribbon shape that separates into discrete spots near the lower right corner of the image. While the dominant coloration of the aurora is green, there are faint suggestions of red photon emission as well (light fuscia tones at image center left). Dense cloud cover is dimly visible below the aurora. The curvature of the Earth's horizon, or limb, is clearly visible as is the faint blue line of the upper atmosphere directly above at image top center. Several stars appear as bright pinpoints against the blackness of space at image top right

Southern Aurora observed from space station - Aurora Australis seen from space - Southern Aurora observed from the International Space Station (ISS) on 29 May 2010. Aurora australis seen from the International Space Station (ISS) on May 29, 2010. The ISS was located over the Southern Indian Ocean at an altitude of 350 km, with the astronaut observer most likely looking towards Antarctica (not visible) and the South Pole. The aurora has a sinuous ribbon shape that separates into discrete spots near the lower right corner of the image. While the dominant coloration of the aurora is green, there are faint suggestions of red photon emission as well (light fuscia tones at image center left). Dense cloud cover is dimly visible below the aurora. The curvature of the Earth's horizon, or limb, is clearly visible as is the faint blue line of the upper atmosphere directly above at image top center. Several stars appear as bright pinpoints against the blackness of space at image top right

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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

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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

PIX4603155

Infrared view of the Andromeda galaxy - Composite of three different wavelengths 24 microns (blue), 70 microns (green), and 160 microns (red). Using these three bands, we can know the temperature differences of the dust: the warmest are the brightest at 24 microns and the coldest shine at 160 microns. The blue/white areas contain the hottest dust. View obtained by Spitzer space telescope on 25 August 2004. The multi - wavelength view of Andromeda combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star - forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions. The data were taken on August 25, 2004

Infrared view of the Andromeda galaxy - Composite of three different wavelengths 24 microns (blue), 70 microns (green), and 160 microns (red). Using these three bands, we can know the temperature differences of the dust: the warmest are the brightest at 24 microns and the coldest shine at 160 microns. The blue/white areas contain the hottest dust. View obtained by Spitzer space telescope on 25 August 2004. The multi - wavelength view of Andromeda combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star - forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions. The data were taken on August 25, 2004

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Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring

Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring

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Nebula IC 1318 in the Swan - IC 1318 the Butterfly nebula in Cygnus - IC 1318 is a very extended 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. This is a large area of emission nebulosity around Sadr, Gamma Cygnii, the brightest star in this photo and the heart of Cygnus. Stretching more than 2 x 3 degrees here, the nebulosity actually extends far out of the photo. 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

Nebula IC 1318 in the Swan - IC 1318 the Butterfly nebula in Cygnus - IC 1318 is a very extended 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. This is a large area of emission nebulosity around Sadr, Gamma Cygnii, the brightest star in this photo and the heart of Cygnus. Stretching more than 2 x 3 degrees here, the nebulosity actually extends far out of the photo. 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

Jerry Lodriguss

PIX4622154

Neptune - Voyager 2 - Image of the Great Dark Spot on Neptune obtained by the Voyager 2 probe on August 23, 1989. The Great Dark Spot is the size of the Earth and winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Date: 08/23/89 Range: 2.8 million km. (1.7 million miles) Smallest Resolvable Feature: 50 km or 31 miles This Voyager 2 image shows the last face on view of the Great Dark Spot that Voyager 2 will take with the narrow angle camera. It was made 45 hours before the closest approach to Neptune. the image shows feathery white clouds that overlie the boundary of the dark and light blue regions. the pinwheel (spiral) structure of both the dark boundary and the white cirrus suggest a storm system rotating counterclockwise. Periodic, small - scale patterns in the white clouds, possibly waves, are short - lived and do not persist from one Neptunian rotation to the next. This color composite was made from the clear and green

Neptune - Voyager 2 - Image of the Great Dark Spot on Neptune obtained by the Voyager 2 probe on August 23, 1989. The Great Dark Spot is the size of the Earth and winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Date: 08/23/89 Range: 2.8 million km. (1.7 million miles) Smallest Resolvable Feature: 50 km or 31 miles This Voyager 2 image shows the last face on view of the Great Dark Spot that Voyager 2 will take with the narrow angle camera. It was made 45 hours before the closest approach to Neptune. the image shows feathery white clouds that overlie the boundary of the dark and light blue regions. the pinwheel (spiral) structure of both the dark boundary and the white cirrus suggest a storm system rotating counterclockwise. Periodic, small - scale patterns in the white clouds, possibly waves, are short - lived and do not persist from one Neptunian rotation to the next. This color composite was made from the clear and green

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The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

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Apr 04, 1954 - Love Philtre kills two girls: Scotland Yard were sure last night that a love philtre drug killed the beauty queen and her girl fellow worker, who fell ill at a London office. Detectives are also sure that neither girl knew she had taken the drug. The girls, Miss June Malins, aged 19, of Wightman-road, Harringay, London, and Cliftonville; and Miss Betty Grant, 27, of Chobham - gardens, Wimbledon, worked in the office of manufacturing chemist. Police concentrated their inquiries on the theory that someone put the drug in food or drink taken by the girls. It is thought unlikely that the person intended to kill. The drug may have been given as a form of joke. But a strong dose is fatal. The girls' office manager, Mr. Arthur Ford, of Bath road, Hounslow, is in hospital with physical Excellence Girl of Margate” competition

Apr 04, 1954 - Love Philtre kills two girls: Scotland Yard were sure last night that a love philtre drug killed the beauty queen and her girl fellow worker, who fell ill at a London office. Detectives are also sure that neither girl knew she had taken the drug. The girls, Miss June Malins, aged 19, of Wightman-road, Harringay, London, and Cliftonville; and Miss Betty Grant, 27, of Chobham - gardens, Wimbledon, worked in the office of manufacturing chemist. Police concentrated their inquiries on the theory that someone put the drug in food or drink taken by the girls. It is thought unlikely that the person intended to kill. The drug may have been given as a form of joke. But a strong dose is fatal. The girls' office manager, Mr. Arthur Ford, of Bath road, Hounslow, is in hospital with physical Excellence Girl of Margate” competition

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Apr. 04, 1954 - Africa starts a new town and port: The Gold Coast, African colony which is moving rapidly toward self-government with British cooperation, has begun the most ambitious construction project in its history the building of a completely new town of 80,000 people and a harbor. The town, to be called Tema, will be divided into seven self-contained communities, each with its own schools, market, churches and recreational facilities

Apr. 04, 1954 - Africa starts a new town and port: The Gold Coast, African colony which is moving rapidly toward self-government with British cooperation, has begun the most ambitious construction project in its history the building of a completely new town of 80,000 people and a harbor. The town, to be called Tema, will be divided into seven self-contained communities, each with its own schools, market, churches and recreational facilities

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May 05, 1953 - Belgian Ambassador-Presents Letters And Scrapbook To Children Of Flood Damaged Schools: The newly arrived Belgian Ambassador to London H.E. Baron du Parc this morning presented letters written by children of Belgian Schools, to child representatives of 59 flood damaged schools on the East Coast, expressing sympathy at the flood damage and suffering. At the same time a handsome” Scrapbook of Belgium” -prepared by pupils of the Ecole Primaire, Lagere School, Belgium was presented to two representatives of the long Road School, Canvey Island-commanded to be the hardest hit school of the floods. The presentations took place at the Belgian Embassy

May 05, 1953 - Belgian Ambassador-Presents Letters And Scrapbook To Children Of Flood Damaged Schools: The newly arrived Belgian Ambassador to London H.E. Baron du Parc this morning presented letters written by children of Belgian Schools, to child representatives of 59 flood damaged schools on the East Coast, expressing sympathy at the flood damage and suffering. At the same time a handsome” Scrapbook of Belgium” -prepared by pupils of the Ecole Primaire, Lagere School, Belgium was presented to two representatives of the long Road School, Canvey Island-commanded to be the hardest hit school of the floods. The presentations took place at the Belgian Embassy

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Field of distant galaxies - Hubble eXtreme Deep Field (XDF) - Distant galaxies - Hubble eXtreme Deep Field (XDF) - Image of distant galaxies obtained in infrared by the Hubble space telescope in the constellation of the Furnace. The farthest galaxies visible in this image are 13.2 billion light years away. Called the Extreme Deep Field, or XDF, the photo was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The XDF is a small fraction of the angular diameter of the full Moon. The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time. The new full - color XDF image reaches much fainter galaxies, and i

Field of distant galaxies - Hubble eXtreme Deep Field (XDF) - Distant galaxies - Hubble eXtreme Deep Field (XDF) - Image of distant galaxies obtained in infrared by the Hubble space telescope in the constellation of the Furnace. The farthest galaxies visible in this image are 13.2 billion light years away. Called the Extreme Deep Field, or XDF, the photo was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The XDF is a small fraction of the angular diameter of the full Moon. The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time. The new full - color XDF image reaches much fainter galaxies, and i

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The Hanger and Nebula SH2 - 83 - Coathanger and nebula SH2 - 83 in Vulpecula - The Hanger cluster or Brocchi cluster (left) is not a true cluster of stars but an asterism located in the constellation of Little Fox. Towards the center of the image, a small nebula emitted, Sh2 - 83. Little Fox Constellation. Brocchi's Cluster (also known as the Coathanger or Collinder 399) is an asterism located in the constellation Vulpecula. It was first described by the Persian astronomer Al Sufi in his Book of Fixed Stars in 964 and was independently rediscovered by Giovanni Hodierna in the seventeenth century. In the 1920s, D. F. Brocchi, an amateur astronomer and chart maker for the American Association of Variable Star Observers, created a map of this object for use in calibrating photometers. The asterism is made up of ten stars ranging from fifth to seventh magnitude which form the conspicuous Coathanger, a straight line of six stars with a “” hook””” of four stars on the south side. An addition

The Hanger and Nebula SH2 - 83 - Coathanger and nebula SH2 - 83 in Vulpecula - The Hanger cluster or Brocchi cluster (left) is not a true cluster of stars but an asterism located in the constellation of Little Fox. Towards the center of the image, a small nebula emitted, Sh2 - 83. Little Fox Constellation. Brocchi's Cluster (also known as the Coathanger or Collinder 399) is an asterism located in the constellation Vulpecula. It was first described by the Persian astronomer Al Sufi in his Book of Fixed Stars in 964 and was independently rediscovered by Giovanni Hodierna in the seventeenth century. In the 1920s, D. F. Brocchi, an amateur astronomer and chart maker for the American Association of Variable Star Observers, created a map of this object for use in calibrating photometers. The asterism is made up of ten stars ranging from fifth to seventh magnitude which form the conspicuous Coathanger, a straight line of six stars with a “” hook””” of four stars on the south side. An addition

Tom Davis

PIX4620989

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

PIX4625336

Illustration of Titanic at Night. 'A Last Vision of the Titanic by Night - An Impression at Cherbourg'. The illustration shows the Titanic during her one and only visit to the French port of Cherbourg on the evening of Wednesday, April 10, 1912, having sailed from Southampton. Her hundreds of portholes are described as producing a kind of shimmering glow upon the darkness of the surrounding water. The ship,built by Harland & Wolff in Belfast Ireland during 1910 - 1911, sank on April 16th 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) ©UIG/Leemage

Illustration of Titanic at Night. 'A Last Vision of the Titanic by Night - An Impression at Cherbourg'. The illustration shows the Titanic during her one and only visit to the French port of Cherbourg on the evening of Wednesday, April 10, 1912, having sailed from Southampton. Her hundreds of portholes are described as producing a kind of shimmering glow upon the darkness of the surrounding water. The ship,built by Harland & Wolff in Belfast Ireland during 1910 - 1911, sank on April 16th 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) ©UIG/Leemage

UIG5447066

Purgatorius and Bistahieversor - The Bistahieversor is a carnivorous dinosaur living in New Mexico at the end of the cretace 75 million years ago. It was about 9 metres long and weighed at least one ton. In the foreground, a Purgatorius tries to hide himself. A rat-sized Purgatorius hides among the undergrowth of a cretaceous forest while a 30 foot long, 2,000 pound tyrannosaur boreages for its next meal in what is today the western United States. Bistahieversor is a genus of tyrannosauroid dinosaur named after Bisti/De-Na-Zin Wilderness where it was found. Purgatorius is the genus for several species of small omnivorous mammals that are believed to be the among the earliest ancestors of modern-day chimps, rhesus monkeys, and humans. The extinction of the larger and more powerful dinosaurs may have been what led to world's domination by mammals today. While there is no direct evidence that Purgatorius and Bistahieversor ever shared the same wilderness, this image is yet illustrative of

Purgatorius and Bistahieversor - The Bistahieversor is a carnivorous dinosaur living in New Mexico at the end of the cretace 75 million years ago. It was about 9 metres long and weighed at least one ton. In the foreground, a Purgatorius tries to hide himself. A rat-sized Purgatorius hides among the undergrowth of a cretaceous forest while a 30 foot long, 2,000 pound tyrannosaur boreages for its next meal in what is today the western United States. Bistahieversor is a genus of tyrannosauroid dinosaur named after Bisti/De-Na-Zin Wilderness where it was found. Purgatorius is the genus for several species of small omnivorous mammals that are believed to be the among the earliest ancestors of modern-day chimps, rhesus monkeys, and humans. The extinction of the larger and more powerful dinosaurs may have been what led to world's domination by mammals today. While there is no direct evidence that Purgatorius and Bistahieversor ever shared the same wilderness, this image is yet illustrative of

Walter B Myers

PIX4663694

Algerian Sahara seen by satellite - Algerian Sahara seen from space: Part of the Sahara desert, in southeast Algeria. The Japanese satellite ALOS (Advanced Land Observation Satellite) took this image on 28 January 2011. This satellite image was captured over southeastern Algeria in the heart of the Sahara desert. In this image, a large area of rock appearing purple stretches across the right side of the image, with fluvial erosion patterns testament to an earlier time when the area received more rainfall. Today, this area sees an average of about 10 mm of rainfall per year. Windshaped sand dunes are visible on the left. The area at the bottom appears to be flat, with tiny specks of vegetation. Just south of this image lies the Tassili n 'Ajjer National Park and UNESCO World Heritage Site, renowned for its 10 000 year-old cave art. The drawings and engravings depict culture and the environment from a time when climatic conditions were more favourable to human occupation. Japan's ALOS sa

Algerian Sahara seen by satellite - Algerian Sahara seen from space: Part of the Sahara desert, in southeast Algeria. The Japanese satellite ALOS (Advanced Land Observation Satellite) took this image on 28 January 2011. This satellite image was captured over southeastern Algeria in the heart of the Sahara desert. In this image, a large area of rock appearing purple stretches across the right side of the image, with fluvial erosion patterns testament to an earlier time when the area received more rainfall. Today, this area sees an average of about 10 mm of rainfall per year. Windshaped sand dunes are visible on the left. The area at the bottom appears to be flat, with tiny specks of vegetation. Just south of this image lies the Tassili n 'Ajjer National Park and UNESCO World Heritage Site, renowned for its 10 000 year-old cave art. The drawings and engravings depict culture and the environment from a time when climatic conditions were more favourable to human occupation. Japan's ALOS sa

PIX4630452

Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Walter B Myers

PIX4626138

Center of the Trifid Nebula (M20) - Center of the Trifid Nebula - The Trifid Nebula (M20) is located between 5000 and 10,000 years - light of the Earth in the constellation of Sagittarius. This image obtained by the Hubble space telescope shows the center of this nebula. A group of bright stars is visible in the center of the image near the dark bands of interstellar dust. These stars are young, blue, massive and extremely hot stars; they are O-type stars and the radiation they emit influence the evolution and structure of the nebula. Trifid Nebula, also known as Messier 20 and NGC 6514, lies within our own Milky Way Galaxy between 5000 and 10 000 light - years from Earth, in the constellation Sagittarius. This image from the Hubble Space Telescope offers a close - up view of the center of the Trifid Nebula, near the intersection of the dust bands, where a group of recently formed, massive, bright stars is easily visible. These stars, which astronomers classify as belonging to the hott

Center of the Trifid Nebula (M20) - Center of the Trifid Nebula - The Trifid Nebula (M20) is located between 5000 and 10,000 years - light of the Earth in the constellation of Sagittarius. This image obtained by the Hubble space telescope shows the center of this nebula. A group of bright stars is visible in the center of the image near the dark bands of interstellar dust. These stars are young, blue, massive and extremely hot stars; they are O-type stars and the radiation they emit influence the evolution and structure of the nebula. Trifid Nebula, also known as Messier 20 and NGC 6514, lies within our own Milky Way Galaxy between 5000 and 10 000 light - years from Earth, in the constellation Sagittarius. This image from the Hubble Space Telescope offers a close - up view of the center of the Trifid Nebula, near the intersection of the dust bands, where a group of recently formed, massive, bright stars is easily visible. These stars, which astronomers classify as belonging to the hott

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Black Holes in 3C75 - Black Holes in 3C75 - Composite X-ray image (blue) and radio (pink) of the active galaxy 3C 75. At the center of this very hot gas mass, two supermassive black holes separated by 25,000 years - light form a binary system of black holes (the two bright points). This composite X - ray/radio image of Abell 400 shows radio jets (pink), immersed in a vast cloud of multimillion degree X - ray emitting gas (blue) that pervades the cluster. The jets emanate from the vicinity of two supermassive black holes (bright spots in the image) in the galaxy. Chandra and radio data confirm that the unusual structure is due to the merger of two large galaxies, whose supermassive black holes are bound together by their mutual gravity. The swept - back appearance of the radio jets is produced by the rapid motion of the galaxy through the hot gas of the cluster, in much the same way that a motorcyclist's scarf is swept back while speeding down the road

Black Holes in 3C75 - Black Holes in 3C75 - Composite X-ray image (blue) and radio (pink) of the active galaxy 3C 75. At the center of this very hot gas mass, two supermassive black holes separated by 25,000 years - light form a binary system of black holes (the two bright points). This composite X - ray/radio image of Abell 400 shows radio jets (pink), immersed in a vast cloud of multimillion degree X - ray emitting gas (blue) that pervades the cluster. The jets emanate from the vicinity of two supermassive black holes (bright spots in the image) in the galaxy. Chandra and radio data confirm that the unusual structure is due to the merger of two large galaxies, whose supermassive black holes are bound together by their mutual gravity. The swept - back appearance of the radio jets is produced by the rapid motion of the galaxy through the hot gas of the cluster, in much the same way that a motorcyclist's scarf is swept back while speeding down the road

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Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It rises more than 9 km above the Martian surface and its caldera extends for 110 km. Image obtained by the Mars Global Surveyor probe. Arsia Mons is one of the largest volcanoes known. This shield volcano is part of an aligned trio known as the Tharsis Montes (the others are Pavonis Mons and Ascraeus Mons). Arsia Mons is rivaled only by Olympus Mons in terms of its volume. The summit of Arsia Mons is more than 9 kilometers (5.6 miles) higher than the surrounding plains. The crater (or caldera) at the volcano summit is approximately 110 km (68 mi) across. This view of Arsia Mons was taken by the red and blue wide angle cameras of the Mars Global Surveyor Mars Orbiter Camera (MOC) system. Bright water ice clouds (the whitish/bluish wisps) hang above the volcano, a common sight every martian afternoon in this region. Arsia Mons is located at 120* west longitude and 9* south latitude. Illumination

Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It rises more than 9 km above the Martian surface and its caldera extends for 110 km. Image obtained by the Mars Global Surveyor probe. Arsia Mons is one of the largest volcanoes known. This shield volcano is part of an aligned trio known as the Tharsis Montes (the others are Pavonis Mons and Ascraeus Mons). Arsia Mons is rivaled only by Olympus Mons in terms of its volume. The summit of Arsia Mons is more than 9 kilometers (5.6 miles) higher than the surrounding plains. The crater (or caldera) at the volcano summit is approximately 110 km (68 mi) across. This view of Arsia Mons was taken by the red and blue wide angle cameras of the Mars Global Surveyor Mars Orbiter Camera (MOC) system. Bright water ice clouds (the whitish/bluish wisps) hang above the volcano, a common sight every martian afternoon in this region. Arsia Mons is located at 120* west longitude and 9* south latitude. Illumination

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Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. 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 galaxies

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. 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 galaxies

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Supernova type 1a 1994D in galaxy NGC 4526 - Supernova 1994D in galaxy NGC 4526 - Supernova 1994D, visible as the bright spot on the lower left, occurred in the outskirts of disk galaxy NGC4526. Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae. In fact, the light emitted during the weeksafter its explosion caused it to be given the familiar designation of a Type Ia supernova. If all Type 1a supernovae have the same intrinsic brightness, then the dimmer a supernova appears, the farther away it must be. By calibrating a precise brightness - distance relation, astronomers are able to estimate not only the expansion rate of the universe (parameterized by the Hubble Constant), but also the geometry of the universe we live in (parameterized by Omega and Lambda). The large number and great distances to supernovae measured in 1998 have been interpreted as indicating that we live in a previously unexpected universe

Supernova type 1a 1994D in galaxy NGC 4526 - Supernova 1994D in galaxy NGC 4526 - Supernova 1994D, visible as the bright spot on the lower left, occurred in the outskirts of disk galaxy NGC4526. Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae. In fact, the light emitted during the weeksafter its explosion caused it to be given the familiar designation of a Type Ia supernova. If all Type 1a supernovae have the same intrinsic brightness, then the dimmer a supernova appears, the farther away it must be. By calibrating a precise brightness - distance relation, astronomers are able to estimate not only the expansion rate of the universe (parameterized by the Hubble Constant), but also the geometry of the universe we live in (parameterized by Omega and Lambda). The large number and great distances to supernovae measured in 1998 have been interpreted as indicating that we live in a previously unexpected universe

PIX4582396

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

PIX4603105

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

PIX4603114

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

PIX4603120

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

R. Gendler

PIX4619230

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

PIX4646089

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - At the bottom left, the large cart, asterism of the Great Bear; at the top right, the small cart, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - At the bottom left, the large cart, asterism of the Great Bear; at the top right, the small cart, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Jerry Lodriguss

PIX4591316

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

PIX4564844

Globular cluster Terzan 5 in Sagittarius - Globular cluster Terzan 5 in Sagittarius - The globular cluster Terzan 5 is located in the constellation Sagittarius. Its stars are not all at the same time and show great age differences between 6 and 12 billion years. Image obtained by the Hubble Space Telescope (HST). Deep within the Milky Way lies the ancient globular cluster Terzan 5. This NASA/ESA Hubble Space Telescope image shows the cluster in wonderful detail, but it is the chaotic motions of its stars that make it particularly interesting to astronomers. Terzan 5 has an exceptionally dense core. As a result, it is thought to have one of the highest stellar collision rates for a globular cluster. And packed in at such close quarters, many stars are pushed so close together that they form tight binary systems. Interestingly, studies of individual stars within the cluster reveal that they can be split into two age groups: 6 and 12 billion years old. Some astronomers have hypothesised t

Globular cluster Terzan 5 in Sagittarius - Globular cluster Terzan 5 in Sagittarius - The globular cluster Terzan 5 is located in the constellation Sagittarius. Its stars are not all at the same time and show great age differences between 6 and 12 billion years. Image obtained by the Hubble Space Telescope (HST). Deep within the Milky Way lies the ancient globular cluster Terzan 5. This NASA/ESA Hubble Space Telescope image shows the cluster in wonderful detail, but it is the chaotic motions of its stars that make it particularly interesting to astronomers. Terzan 5 has an exceptionally dense core. As a result, it is thought to have one of the highest stellar collision rates for a globular cluster. And packed in at such close quarters, many stars are pushed so close together that they form tight binary systems. Interestingly, studies of individual stars within the cluster reveal that they can be split into two age groups: 6 and 12 billion years old. Some astronomers have hypothesised t

PIX4565214

Aug. 08, 1954 - Demonstration of the U.S. Army's new 75 MM Skysweeper anti - aircraft gun: The United States Army's new 75 mm Skysweeper, a large caliber automatic anti-aircraft artillery weapon, was fired at radio controlled and towed targets before high ranking British Army officials and members of the press, at Weybourns, Norfolk, today. The new gun which can find and track approaching aircraft as far away as 15 miles, is capable of firing on and defeating air targets as far away as four miles. The weapon, equipped with radar, computer, and gun all on one carriage, operates day on night regardless of weather conditions, even when aircraft are invisible in a blanketing fog

Aug. 08, 1954 - Demonstration of the U.S. Army's new 75 MM Skysweeper anti - aircraft gun: The United States Army's new 75 mm Skysweeper, a large caliber automatic anti-aircraft artillery weapon, was fired at radio controlled and towed targets before high ranking British Army officials and members of the press, at Weybourns, Norfolk, today. The new gun which can find and track approaching aircraft as far away as 15 miles, is capable of firing on and defeating air targets as far away as four miles. The weapon, equipped with radar, computer, and gun all on one carriage, operates day on night regardless of weather conditions, even when aircraft are invisible in a blanketing fog

ZUM4939813

May 05, 1953 - British Official Photograph (Air Ministry) Crown Copyright Reserved. FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Manby, 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 lies 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 H.W. Firmin, D.F.C., the aircraft carried two staff navigators and five students, with other air and ground crew. British Official Photo Shows: Pack ice and open water between Devon Island, in the North-West

May 05, 1953 - British Official Photograph (Air Ministry) Crown Copyright Reserved. FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Manby, 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 lies 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 H.W. Firmin, D.F.C., the aircraft carried two staff navigators and five students, with other air and ground crew. British Official Photo Shows: Pack ice and open water between Devon Island, in the North-West

ZUM4841681

May 05, 1953 - Thirty-one Sicilian bandits sentenced Giuliano gang's six hundred years.: After a trial lasting nearly four months, the Central Court of Palermo, Sicily, recently delivered its verdict, which took eight days to reach in the case of 45 men accused of serious crimes while members of the gang of Salvatore Giuliano, the bandit who, after terrorizing Sicily for six years, was shot dead by the police in 1950. Thirty-one of the accused bandits were found guilty of complicity in 11 murders, 15 attempted murders, 14 kidnapping and a number of other serious crimes. They received sentences of imprisonment two of them penal servitude for life - which totalled 600 years. The other 14 were ac ~ uitted, though nine of them still have to serve long sentences for previous crimes. Some of the guilty are still in hiding and were sentenced in their absence

May 05, 1953 - Thirty-one Sicilian bandits sentenced Giuliano gang's six hundred years.: After a trial lasting nearly four months, the Central Court of Palermo, Sicily, recently delivered its verdict, which took eight days to reach in the case of 45 men accused of serious crimes while members of the gang of Salvatore Giuliano, the bandit who, after terrorizing Sicily for six years, was shot dead by the police in 1950. Thirty-one of the accused bandits were found guilty of complicity in 11 murders, 15 attempted murders, 14 kidnapping and a number of other serious crimes. They received sentences of imprisonment two of them penal servitude for life - which totalled 600 years. The other 14 were ac ~ uitted, though nine of them still have to serve long sentences for previous crimes. Some of the guilty are still in hiding and were sentenced in their absence

ZUM4841425

Irishmen Avenge Irish Dead, Londonderry, Northern Ireland, 1975 (oil on board)

Irishmen Avenge Irish Dead, Londonderry, Northern Ireland, 1975 (oil on board)

Lillford, Ralph (b.1932)

NAM5920329

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

PIX4616545

Galaxy ESO 77 - 14 - Galaxy ESO 77 - 14 - The galaxy ESO 77 - 14 is about 550 million light years away from Earth in the southern constellation of the Indian. This system consists of two interacting galaxies. Image obtained by the Hubble Space Telescope on August 17, 2001. This image of ESO 77 - 14 is a stunning snapshot of a celestial dance performed by a pair of similar sized galaxies. Two clear signatures of the gravitational tug of war between the galaxies are the bridge of material that connects them and the disruption of their main bodies. The galaxy on the right has a long, bluish arm while its companion has a shorter, redder arm. This interacting pair is in the constellation of Indus, the Indian, some 550 million light - years away from Earth. The dust lanes between the two galaxy centers show the extent of the distortion to the originally flat disks that have been pulled into three - dimensional shapes. Image taken by the Hubble space telescope on august 17, 2001

Galaxy ESO 77 - 14 - Galaxy ESO 77 - 14 - The galaxy ESO 77 - 14 is about 550 million light years away from Earth in the southern constellation of the Indian. This system consists of two interacting galaxies. Image obtained by the Hubble Space Telescope on August 17, 2001. This image of ESO 77 - 14 is a stunning snapshot of a celestial dance performed by a pair of similar sized galaxies. Two clear signatures of the gravitational tug of war between the galaxies are the bridge of material that connects them and the disruption of their main bodies. The galaxy on the right has a long, bluish arm while its companion has a shorter, redder arm. This interacting pair is in the constellation of Indus, the Indian, some 550 million light - years away from Earth. The dust lanes between the two galaxy centers show the extent of the distortion to the originally flat disks that have been pulled into three - dimensional shapes. Image taken by the Hubble space telescope on august 17, 2001

PIX4613637

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

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,

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Apollo 15: J. Irwin on the Moon - Jim Irwin works at the LRV during Apollo 15 EVA - 1 - Irwin works near the Lunar Roving Vehicle. 31/07/1971. Astronaut James B. Irwin, lunar module pilot, works at the Lunar Roving Vehicle (LRV) during the first Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site (31 July 1971). The Lunar Module (LM) “” Falcon””” is on the left. The undeployed Laser Ranging Reflector (LR - 3) lies atop the LM's modular equipment stowage assembly (MESA). This view is looking slightly west of south. Hadley Delta and the Apennine Front are in the background to the left. St. George crater is approximately five kilometers (about three statute miles) in the distance behind Irwin's head. This photograph was taken by astronaut David R. Scott, commander. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar or

Apollo 15: J. Irwin on the Moon - Jim Irwin works at the LRV during Apollo 15 EVA - 1 - Irwin works near the Lunar Roving Vehicle. 31/07/1971. Astronaut James B. Irwin, lunar module pilot, works at the Lunar Roving Vehicle (LRV) during the first Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site (31 July 1971). The Lunar Module (LM) “” Falcon””” is on the left. The undeployed Laser Ranging Reflector (LR - 3) lies atop the LM's modular equipment stowage assembly (MESA). This view is looking slightly west of south. Hadley Delta and the Apennine Front are in the background to the left. St. George crater is approximately five kilometers (about three statute miles) in the distance behind Irwin's head. This photograph was taken by astronaut David R. Scott, commander. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar or

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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

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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

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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

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Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 12 million light years away. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. NGC 253 is a spiral galaxy (about 12 million light years away), a member of a small group straggling across the southern constellation of Sculptor. It appears elongated because we see it almost edge - on. NGC 253 is a prototypical starburst galaxy.This galaxy is also one of the dustiest galaxies known and much of its internal detail is hidden by obscuring matter which can be seen as dark patches against the background stars. Despite the obscuration, two spiral arms and many bluish clusters of stars can be seen around the edge of the galaxy. NGC 253 is so close to us that some of the brightest stars are apparent as individuals within the spiral arms. Image taken with the ESO/Danish 1.5m telescope at La Si

Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 12 million light years away. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. NGC 253 is a spiral galaxy (about 12 million light years away), a member of a small group straggling across the southern constellation of Sculptor. It appears elongated because we see it almost edge - on. NGC 253 is a prototypical starburst galaxy.This galaxy is also one of the dustiest galaxies known and much of its internal detail is hidden by obscuring matter which can be seen as dark patches against the background stars. Despite the obscuration, two spiral arms and many bluish clusters of stars can be seen around the edge of the galaxy. NGC 253 is so close to us that some of the brightest stars are apparent as individuals within the spiral arms. Image taken with the ESO/Danish 1.5m telescope at La Si

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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

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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

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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

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Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters

Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters

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Most of the area of the southern Milky Way covered by this picture never sets for those of us who live at southern latitudes south on -30 degrees. The main constellations here are Centaurus, Crux and Carina, containing some of the most interesting, beautiful and bizzare astronomical objects, including the nearest stars. Alpha Centauri is at lower left and with its companion, beta points (more or less) to the Southern Cross, which in turn lies alongside the Coalsack, one of the nearest dust clouds. Further along the Milky Way is the astonishing Carina nebula, which is home to eta Carinae, probably the most massive star known, and a prime candidate for the next Galactic supernova. It is in Carina that the Sagittarius arm of our galaxy curves sharply away from us, so we see deep into a rich star-forming region.: The Lactee Way from Centaur to Carene - Souther Milky Way form Centaurus to Carina

Most of the area of the southern Milky Way covered by this picture never sets for those of us who live at southern latitudes south on -30 degrees. The main constellations here are Centaurus, Crux and Carina, containing some of the most interesting, beautiful and bizzare astronomical objects, including the nearest stars. Alpha Centauri is at lower left and with its companion, beta points (more or less) to the Southern Cross, which in turn lies alongside the Coalsack, one of the nearest dust clouds. Further along the Milky Way is the astonishing Carina nebula, which is home to eta Carinae, probably the most massive star known, and a prime candidate for the next Galactic supernova. It is in Carina that the Sagittarius arm of our galaxy curves sharply away from us, so we see deep into a rich star-forming region.: The Lactee Way from Centaur to Carene - Souther Milky Way form Centaurus to Carina

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Nebulae of the horse's head and M42 in Orion - Orion deepfield - Dark Nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Mosaic of images obtained during more than 20 hours of application, using an H - Alpha filter. This large complex of nebulosity is located about 1,500 light years away in Orion. The Orion complex is a gigantic stellar nursery where stars are forming out of the dust and gas in the region. Young energetic stars excite the gas in the region ionizing it and causing it to glow in the hydrogen - alpha and oxygen III emission lines. The brightest star in the photo at upper right at magnitude 1.8 is Alnilam, the middle star of the three distinctive stars in the belt of Orion. At the left is the Flame, NGC 2024, and below it is dark nebula B33, the Horsehead Nebula. Below is a patch of blue reflection nebulosity NGC 1973 - 4 - 5 and bottom is the beautiful Orion Nebula, M 42. Long - exposure image with an Hydrogen al

Nebulae of the horse's head and M42 in Orion - Orion deepfield - Dark Nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Mosaic of images obtained during more than 20 hours of application, using an H - Alpha filter. This large complex of nebulosity is located about 1,500 light years away in Orion. The Orion complex is a gigantic stellar nursery where stars are forming out of the dust and gas in the region. Young energetic stars excite the gas in the region ionizing it and causing it to glow in the hydrogen - alpha and oxygen III emission lines. The brightest star in the photo at upper right at magnitude 1.8 is Alnilam, the middle star of the three distinctive stars in the belt of Orion. At the left is the Flame, NGC 2024, and below it is dark nebula B33, the Horsehead Nebula. Below is a patch of blue reflection nebulosity NGC 1973 - 4 - 5 and bottom is the beautiful Orion Nebula, M 42. Long - exposure image with an Hydrogen al

R. Gendler

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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

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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

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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

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

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