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Military News Reports - Military occupation, Helmand Province 2010

Military News Reports - Military occupation, Helmand Province 2010

BOF6288485

Dresden, historical, new market, Frauenkirche Ruin, Reconstruction, historical Coin from the Years 1726 Publication …, 1993 (photo)

Dresden, historical, new market, Frauenkirche Ruin, Reconstruction, historical Coin from the Years 1726 Publication …, 1993 (photo)

Sächsische Zeitung

IMO8755573

May Day Celebrations - East Bloc Countries

May Day Celebrations - East Bloc Countries

BOF8832795

William Widdrington, 4th Baron Widdrington of Blankney (1678-1743)

William Widdrington, 4th Baron Widdrington of Blankney (1678-1743)

English School, (18th century)

USB1160555

Cassini - Huygens en route to Titan - The Cassini - Huygens probe above Titan's atmosphere - Artist's view of the Cassini probe before the separation of the European Huygens module on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe before separation to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Equipped with a variety of scientific sensors, the Huygens probe will spend 2 - 2.5 hours descending through Titan's dense, murky atmosphere of nitrogen and carbon - based molecules, beaming its findings to the distant Cassini orbiter overhead. The probe could continue to relay information for up to 30 minutes after it lands on Titan's frigid surface, after which the orbiter passes beneath the horizon as seen

Cassini - Huygens en route to Titan - The Cassini - Huygens probe above Titan's atmosphere - Artist's view of the Cassini probe before the separation of the European Huygens module on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe before separation to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Equipped with a variety of scientific sensors, the Huygens probe will spend 2 - 2.5 hours descending through Titan's dense, murky atmosphere of nitrogen and carbon - based molecules, beaming its findings to the distant Cassini orbiter overhead. The probe could continue to relay information for up to 30 minutes after it lands on Titan's frigid surface, after which the orbiter passes beneath the horizon as seen

D. Ducros

PIX4606041

The Chapel of Queen Mersyankh III (photo)

The Chapel of Queen Mersyankh III (photo)

Sandro Vannini

SVA833907

The photographers art, 1880 (b/w photo)

The photographers art, 1880 (b/w photo)

Burke, John (fl.1878-79)

NAM5924215

The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speedin

The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speedin

PIX4620190

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

PIX4625583

Nebula IC 1396 in Cephee infrared view - 18/12/2003 The large composite image on the left is a product of combining data from the observator's multiband imaging photometer and the infrared array camera. The thermal emission at 24 microns measured by the photometer (red) is combined with near - infrared emission from the camera at 3.6/4.5 microns (blue) and from 5.8/8.0 microns (green). The colors of the diffuse emission and filaments vary, and are a combination of molecular hydrogen (which tends to be green) and polycyclic aromatic hydrocarbon (brown) emissions. Nasa's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light - years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive

Nebula IC 1396 in Cephee infrared view - 18/12/2003 The large composite image on the left is a product of combining data from the observator's multiband imaging photometer and the infrared array camera. The thermal emission at 24 microns measured by the photometer (red) is combined with near - infrared emission from the camera at 3.6/4.5 microns (blue) and from 5.8/8.0 microns (green). The colors of the diffuse emission and filaments vary, and are a combination of molecular hydrogen (which tends to be green) and polycyclic aromatic hydrocarbon (brown) emissions. Nasa's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light - years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive

PIX4622272

Mrs Paine and the Misses Paine, 1765 (oil on canvas)

Mrs Paine and the Misses Paine, 1765 (oil on canvas)

Reynolds, Joshua (1723-92)

WGL1764517

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

PIX4611595

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. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

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. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

PIX4619490

The photographers art, Afghanistan, 1880 (b/w photo)

The photographers art, Afghanistan, 1880 (b/w photo)

Burke, John (fl.1878-79)

NAM5924214

Normandy Invasion, 1944

Normandy Invasion, 1944

IMW7393546

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

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

PIX4624957

Cuban Missile Crisis 1962

Cuban Missile Crisis 1962

BOF6283648

Evolution of The Oil Industry, 1960s 3 of 3

Evolution of The Oil Industry, 1960s 3 of 3

BOF6285564

Dresden, historical, new market, Frauenkirche Ruin, Reconstruction, historical …, 1993 (photo)

Dresden, historical, new market, Frauenkirche Ruin, Reconstruction, historical …, 1993 (photo)

Sächsische Zeitung

IMO8755572

Sep. 09, 1954 - Demonstration Of British Military Vehicles: Many Hundreds of visitors from this country and overseas, attended a special and unique demonstration of British military at the Fighting Vehicles Research and Development Establishment (F.V.R.D.E.) at Chertsey, Surrey, today. Stages primarily to promote sales in this special of our exports trade, the display included short of 100 different trade, the display included little short of 100 different vehicles giving an inmates compasset of usage, Lad and personnel carrying motor vehicles 5 cwt. to 230 tons carrying capacity, workshop lorries, mobile cranes, tankers and tailers up to 60 tons for tank transportation, and even armoured cars are among the exhibits part in seen either in the display centre, or taking [art in specatcular demonstrations of their qualities on test circuits. The event has been organised jointly by the Miistry of Supply, to who specifiction the vehicles are built, and by the society of Motor Manufacturers

Sep. 09, 1954 - Demonstration Of British Military Vehicles: Many Hundreds of visitors from this country and overseas, attended a special and unique demonstration of British military at the Fighting Vehicles Research and Development Establishment (F.V.R.D.E.) at Chertsey, Surrey, today. Stages primarily to promote sales in this special of our exports trade, the display included short of 100 different trade, the display included little short of 100 different vehicles giving an inmates compasset of usage, Lad and personnel carrying motor vehicles 5 cwt. to 230 tons carrying capacity, workshop lorries, mobile cranes, tankers and tailers up to 60 tons for tank transportation, and even armoured cars are among the exhibits part in seen either in the display centre, or taking [art in specatcular demonstrations of their qualities on test circuits. The event has been organised jointly by the Miistry of Supply, to who specifiction the vehicles are built, and by the society of Motor Manufacturers

ZUM4941609

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036713

The passenger liner 'Great Britain' (1843) at Brandon Warf, Bristol, 1844 (salted paper print, paper)

The passenger liner 'Great Britain' (1843) at Brandon Warf, Bristol, 1844 (salted paper print, paper)

Talbot, William Henry Fox (1800-77)

MMM7342531

Cathedral Interior (oil on canvas)

Cathedral Interior (oil on canvas)

Streeton, Ernest Arthur (1867-1943)

MEM1268336

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. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

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. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

PIX4619447

(Recto) The 'Sans Pareil' in Besika Bay, 3 October 1853 and the French steamer 'Mogador' towing the French 'Valmy' into the Dardanelles, 29 October 1853; (Verso) broadside studies of the French 'Jupiter', 'Jena' and 'Ville de Paris' drying sails, 1853 (graphite)

(Recto) The 'Sans Pareil' in Besika Bay, 3 October 1853 and the French steamer 'Mogador' towing the French 'Valmy' into the Dardanelles, 29 October 1853; (Verso) broadside studies of the French 'Jupiter', 'Jena' and 'Ville de Paris' drying sails, 1853 (graphite)

Mends, George Pechell (1815-71)

MMM7342259

Men in a boat near two Dutch ships, 1652 (oil on panel)

Men in a boat near two Dutch ships, 1652 (oil on panel)

Sillemans, Experiens (fl.c.1650)

MMM7340545

Saxony, historical, hotel, restaurants, restaurants, cafes, Beer gardens Dresden, Folk House Laubegast, closed, exterior …, 1985 (photo)

Saxony, historical, hotel, restaurants, restaurants, cafes, Beer gardens Dresden, Folk House Laubegast, closed, exterior …, 1985 (photo)

Sächsische Zeitung

IMO8758243

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

PIX4615848

The Doge's Palace and Riva degli Schiavoni, Venice

The Doge's Palace and Riva degli Schiavoni, Venice

Canaletto, (Giovanni Antonio Canal) (1697-1768)

USB1158562

Globular cluster NGC 1806 in Dorado - Globular cluster NGC 1806 in Dorado - Image of the globular cluster NGC 1806 located in the southern constellation of Dorado. NGC 1806 belongs to the galaxy of the Great Magellan Cloud, a galaxy adjacent to our lactee path. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has turned its sharp eye towards a tight collection of stars, first seen 174 years ago. The result is a sparkling image of NGC 1806, tens of thousands of stars gravitationally bound into a rich cluster. Commonly called globular clusters, most of these objects are very old, having formed in the distant past when the Universe was only a fraction of its current age. NGC 1806 lies within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. It can be observed within the constellation of Dorado (the dolphin - fish), an area of the sky best seen from the Earth's southern hemisphere. NGC 1806 was discovered in 1836 by the British astr

Globular cluster NGC 1806 in Dorado - Globular cluster NGC 1806 in Dorado - Image of the globular cluster NGC 1806 located in the southern constellation of Dorado. NGC 1806 belongs to the galaxy of the Great Magellan Cloud, a galaxy adjacent to our lactee path. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has turned its sharp eye towards a tight collection of stars, first seen 174 years ago. The result is a sparkling image of NGC 1806, tens of thousands of stars gravitationally bound into a rich cluster. Commonly called globular clusters, most of these objects are very old, having formed in the distant past when the Universe was only a fraction of its current age. NGC 1806 lies within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. It can be observed within the constellation of Dorado (the dolphin - fish), an area of the sky best seen from the Earth's southern hemisphere. NGC 1806 was discovered in 1836 by the British astr

PIX4564335

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory

PIX4615845

Saturn and Mimas seen by the Cassini probe 18/01/2005 - Saturn and Mimas seen by Cassini spacecraft Jan. 18 2005 - The Mimas satellite photographed in front of Saturn by the Cassini probe on 18 January 2005 at a distance of 1.4 million km from the planet. The shadow of Saturn's rings is projected on the planet. Mimas drifts along in its orbit against the azure backdrop of Saturn's northern latitudes in this true color view. The long, dark lines on the atmosphere are shadows cast by the planet's rings. Saturn's northern hemisphere is presently relatively cloud - free, and rays of sunlight take a long path through the atmosphere. This results in sunlight being scattered at shorter (bluer) wavelengths, thus giving the northernmost latitudes their bluish appearance at visible wavelengths. At the bottom, craters on icy Mimas (398 kilometers, or 247 miles across) give the moon a dimpled appearance. Images taken using infrared (930 nanometers), green (568 nanometers) and ultraviolet (338 nano

Saturn and Mimas seen by the Cassini probe 18/01/2005 - Saturn and Mimas seen by Cassini spacecraft Jan. 18 2005 - The Mimas satellite photographed in front of Saturn by the Cassini probe on 18 January 2005 at a distance of 1.4 million km from the planet. The shadow of Saturn's rings is projected on the planet. Mimas drifts along in its orbit against the azure backdrop of Saturn's northern latitudes in this true color view. The long, dark lines on the atmosphere are shadows cast by the planet's rings. Saturn's northern hemisphere is presently relatively cloud - free, and rays of sunlight take a long path through the atmosphere. This results in sunlight being scattered at shorter (bluer) wavelengths, thus giving the northernmost latitudes their bluish appearance at visible wavelengths. At the bottom, craters on icy Mimas (398 kilometers, or 247 miles across) give the moon a dimpled appearance. Images taken using infrared (930 nanometers), green (568 nanometers) and ultraviolet (338 nano

PIX4625133

Soap Box Derby 1974

Soap Box Derby 1974

LTT7260018

Bloomdale China Clay and Stone Works, St. Stephen-in-Brannel, Cornwall, UK (b/w photo)

Bloomdale China Clay and Stone Works, St. Stephen-in-Brannel, Cornwall, UK (b/w photo)

EHT6948191

Base sur Mars - Illustration - Mars Ice Home concept - Artist's view of an inhabited base on Mars. Inflatable housing concept surrounded by a layer of ice. The “” Mars Ice Home”” is a large inflatable torus, a shape similar to an inner tube, that is surrounded by a shell of water ice. The Mars Ice Home design has several advantages that make it an appealing concept. It is lightweight and can be transported and deployed with simple robotics, then filled with water before the crew arrives. It incorporates materials extracted from Mars, and because water in the Ice Home could potentially be converted to rocket fuel for the Mars Ascent Vehicle, the structure itself doubles as a storage tank that can be refilled for the next crew. Another critical benefit is that water, a hydrogen-rich material, is an excellent shielding material for galactic cosmic rays - and many areas of Mars have abundant water ice just below the surface. Galactic cosmic rays are one of the biggest risks of long stays o

Base sur Mars - Illustration - Mars Ice Home concept - Artist's view of an inhabited base on Mars. Inflatable housing concept surrounded by a layer of ice. The “” Mars Ice Home”” is a large inflatable torus, a shape similar to an inner tube, that is surrounded by a shell of water ice. The Mars Ice Home design has several advantages that make it an appealing concept. It is lightweight and can be transported and deployed with simple robotics, then filled with water before the crew arrives. It incorporates materials extracted from Mars, and because water in the Ice Home could potentially be converted to rocket fuel for the Mars Ascent Vehicle, the structure itself doubles as a storage tank that can be refilled for the next crew. Another critical benefit is that water, a hydrogen-rich material, is an excellent shielding material for galactic cosmic rays - and many areas of Mars have abundant water ice just below the surface. Galactic cosmic rays are one of the biggest risks of long stays o

PIX4640020

Mr. William Armstrong's design for a chain bridge across the River Avon, from St. Vincents Rock to Leigh Down, 1830 (hand coloured litho on paper)

Mr. William Armstrong's design for a chain bridge across the River Avon, from St. Vincents Rock to Leigh Down, 1830 (hand coloured litho on paper)

West, William (1793-1860)

IGM7483092

Comic Song, Bradshaw's Guide, 1876 (lithograph on paper)

Comic Song, Bradshaw's Guide, 1876 (lithograph on paper)

Packer, Thomas (1824-1896)

IGM8836223

South African Propaganda Films of The Apartheid Era - Volume X

South African Propaganda Films of The Apartheid Era - Volume X

VLF6436742

WWII - North African Campaign 1942 : The image from the Nazi Propaganda! depicts camouflaged tents of the German Wehrmacht in Africa, published on 29 January 1942. Place unknown. The text on the back of the image reads: ""Tents in Africa. On the flat terrain of the desert, the soldiers can often only shield themselves from enemy view through special camouflaging. But also this camouflaging is at times linked to great difficulties because there are not many trees or bushes available. Here, the soldiers have brought brushwood to cover their tents on the open terrain so that they cannot be seen in the bird's eye perspective. - On the top: camouflage works on the tent, in which they live in. - Below: The camouflaged tent that can barely be recognized even at a small distance."" """"

WWII - North African Campaign 1942 : The image from the Nazi Propaganda! depicts camouflaged tents of the German Wehrmacht in Africa, published on 29 January 1942. Place unknown. The text on the back of the image reads: ""Tents in Africa. On the flat terrain of the desert, the soldiers can often only shield themselves from enemy view through special camouflaging. But also this camouflaging is at times linked to great difficulties because there are not many trees or bushes available. Here, the soldiers have brought brushwood to cover their tents on the open terrain so that they cannot be seen in the bird's eye perspective. - On the top: camouflage works on the tent, in which they live in. - Below: The camouflaged tent that can barely be recognized even at a small distance."" """"

DPA5344398

Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. Colour - composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region. Several well known astronomical objects can be seen in this wide field image: to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. North is up and Eas

Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. Colour - composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region. Several well known astronomical objects can be seen in this wide field image: to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. North is up and Eas

PIX4619045

Napoleon surrendering to Captain Frederick Lewis Maitland on 15 July 1815, c.1815 (etching)

Napoleon surrendering to Captain Frederick Lewis Maitland on 15 July 1815, c.1815 (etching)

Baugean, Jean Jerome (1764-1819)

MMM7341964

Kopeka Bird Caves, Atiu Island, Cook Island, Polynesia, South Pacific Ocean (photo)

Kopeka Bird Caves, Atiu Island, Cook Island, Polynesia, South Pacific Ocean (photo)

Sergi Reboredo

SRB1202899

General view of wooden houses in remote ethnic Lao Lum village, Ban Naphia, the "War Spoon/Bracelet village" where, in cottage industries, war scrap (bomb and plane metal from Second Indochina War) is melted down and cast into spoons and bracelets, motto: "Make Bracelets not War" Phaxay District, Xieng Khouang Province, Laos, Southeast Asia MORE INFO: RISE (Rural Income through Sustainable Energy), a project supporting remote communities in gaining access to sustainable and locally produced clean energy and using local resources to generate income while safeguarding the environment, implemented by Helvetas Laos, a Swiss Association for International Cooperation & Development, see: www.helvetas-laos.org

General view of wooden houses in remote ethnic Lao Lum village, Ban Naphia, the "War Spoon/Bracelet village" where, in cottage industries, war scrap (bomb and plane metal from Second Indochina War) is melted down and cast into spoons and bracelets, motto: "Make Bracelets not War" Phaxay District, Xieng Khouang Province, Laos, Southeast Asia MORE INFO: RISE (Rural Income through Sustainable Energy), a project supporting remote communities in gaining access to sustainable and locally produced clean energy and using local resources to generate income while safeguarding the environment, implemented by Helvetas Laos, a Swiss Association for International Cooperation & Development, see: www.helvetas-laos.org

Chinch Gryniewicz

POV499106

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

PIX4568892

Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 is located in the constellation Taurus. Image obtained by the Hubble Space Telescope (HST). The little - known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. It appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye - catching shapes of the gas. However, the bright boomerang - shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp - edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 20

Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 is located in the constellation Taurus. Image obtained by the Hubble Space Telescope (HST). The little - known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. It appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye - catching shapes of the gas. However, the bright boomerang - shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp - edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 20

PIX4621402

Barree spiral galaxy NGC 6872 in interaction with IC 4970 in the Peacock - Barred spiral interacting galaxy NGC 6872 in Pavo - The barree spiral galaxy NGC 6872 and lenticular IC 4970 are located about 300 million years away - light from Earth. NGC 6872 extends over nearly 750,000 years - light. Image obtained by the ANTU telescope of the VLT on March 29, 1999. View of the spectacular barred spiral galaxy NGC 6872 obtained with FORS1 at ANTU telescope (VLT) in the morning of March 29, 1999. It is of type SBB and is accompanied by a smaller, interacting galaxy, IC 4970 of type S0 (just above the centre). The bright object to the lower right of the galaxies is a star in the Milky Way whose image has been strongly overexposed and exhibits multiple optical reflections in the telescope and instrument. There are also many other, fainter and more distant galaxies of many different forms in the field. The upper left spiral arm of NGC 6872 is significantly disturbed and is populated by a pletho

Barree spiral galaxy NGC 6872 in interaction with IC 4970 in the Peacock - Barred spiral interacting galaxy NGC 6872 in Pavo - The barree spiral galaxy NGC 6872 and lenticular IC 4970 are located about 300 million years away - light from Earth. NGC 6872 extends over nearly 750,000 years - light. Image obtained by the ANTU telescope of the VLT on March 29, 1999. View of the spectacular barred spiral galaxy NGC 6872 obtained with FORS1 at ANTU telescope (VLT) in the morning of March 29, 1999. It is of type SBB and is accompanied by a smaller, interacting galaxy, IC 4970 of type S0 (just above the centre). The bright object to the lower right of the galaxies is a star in the Milky Way whose image has been strongly overexposed and exhibits multiple optical reflections in the telescope and instrument. There are also many other, fainter and more distant galaxies of many different forms in the field. The upper left spiral arm of NGC 6872 is significantly disturbed and is populated by a pletho

PIX4613035

Interior of a Kafir Fort, Upsai. September 1885. View of interior court. Unsharp. 'Central Court, Apsai'. 'The villages Shui, Apsai, and Shidgol resemble forts rather than villages. Their plan is an irregular four-sided figure, the houses being built contiguously round a central court, the only entrance to which is through a large door capable of being sngly closed and secured from the inside in the event of attack. The houses consist of a basement and one, or two, stories above; the outside walls presenting only flat faces of mud and stone, with framework and ties of timber, broken up in the upper rooms by numerous very small windows; inside, overlooking the courtyard, are picturesque wooden verandahs, the rooms opening on to them. The houses are two rooms deep; the rooms facing outwards are very dark, receiving their light only from the little loop-holes, mentioned above, or through the doorway communicating with the other room, which is lighted from the balcony...There is a good dea

Interior of a Kafir Fort, Upsai. September 1885. View of interior court. Unsharp. 'Central Court, Apsai'. 'The villages Shui, Apsai, and Shidgol resemble forts rather than villages. Their plan is an irregular four-sided figure, the houses being built contiguously round a central court, the only entrance to which is through a large door capable of being sngly closed and secured from the inside in the event of attack. The houses consist of a basement and one, or two, stories above; the outside walls presenting only flat faces of mud and stone, with framework and ties of timber, broken up in the upper rooms by numerous very small windows; inside, overlooking the courtyard, are picturesque wooden verandahs, the rooms opening on to them. The houses are two rooms deep; the rooms facing outwards are very dark, receiving their light only from the little loop-holes, mentioned above, or through the doorway communicating with the other room, which is lighted from the balcony...There is a good dea

BL3292911

German fleet manoeuvres on the high seas, c.1900 (oil on canvas)

German fleet manoeuvres on the high seas, c.1900 (oil on canvas)

Saltzmann, Carl (1847-1923)

MMM7337721

Rāvaṇa assigns the defence of Laṅkā's eastern gate to his general Prahasta; the southern gate to his brothers MahÄpÄrÅ›va and Mahodara; the western gate to his son Indrajit; and the northern gate, where he himself would also go, to the spies Åšuka and SÄraá¹‡a. The centre he leaves to VirūpÄká¹£a. Having thus directed Laṅkā's key defences, he retires to his chamber. Along with his allies, Rāma has now decided to climb the nearby Mount Suvela, from which there is a splendid view of the city of Laṅkā 'as if suspended in the sky'. All of Rāvaṇa's dispositions are soon known to VibhÄ«á¹£aá¹‡a through the birds he has sent out as spies.

Rāvaṇa assigns the defence of Laṅkā's eastern gate to his general Prahasta; the southern gate to his brothers MahÄpÄrÅ›va and Mahodara; the western gate to his son Indrajit; and the northern gate, where he himself would also go, to the spies Åšuka and SÄraá¹‡a. The centre he leaves to VirūpÄká¹£a. Having thus directed Laṅkā's key defences, he retires to his chamber. Along with his allies, Rāma has now decided to climb the nearby Mount Suvela, from which there is a splendid view of the city of Laṅkā 'as if suspended in the sky'. All of Rāvaṇa's dispositions are soon known to VibhÄ«á¹£aá¹‡a through the birds he has sent out as spies.

BL3283073

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

Nebula of the Lagoon (M8) in Sagittarius - M8, The Lagoon Nebula - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several giant O stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two supergiant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 giant B stars, 3 to 4 times more than the Orion nebula. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the distinctive dark lane that runs through the heart of the nebula, just to the west of open cluster NGC 6530. Bok globules, small dark knots which are condensing protostella

Nebula of the Lagoon (M8) in Sagittarius - M8, The Lagoon Nebula - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several giant O stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two supergiant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 giant B stars, 3 to 4 times more than the Orion nebula. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the distinctive dark lane that runs through the heart of the nebula, just to the west of open cluster NGC 6530. Bok globules, small dark knots which are condensing protostella

Jerry Lodriguss

PIX4619667

Development Of Transportation

Development Of Transportation

BOF6287337

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding ga

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding ga

PIX4609732

Cuban Crisis 1962

Cuban Crisis 1962

BOF877534

Spiral Galaxy NGC 4452 - Galaxy Spiral NGC 4452 - NGC 4452 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope has imaged a striking galaxy called NGC 4452, which appears to lie exactly edge - on as seen from Earth. The bright nucleus can be seen at the centre, along with the very thin disc that looks like a straight line from our unusual viewing position. To complete the picture, a hazy halo of stars on the periphery of the galaxy makes it seem to glow. NGC 4452 was first seen by William Herschel in 1784 with his 47 cm telescope in England. He described the object as a bright nebula, small and very much elongated. The new Hubble image shows just how elongated this unusual object really is. NGC 4452 is part of the Virgo Cluster, so - called because many

Spiral Galaxy NGC 4452 - Galaxy Spiral NGC 4452 - NGC 4452 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope has imaged a striking galaxy called NGC 4452, which appears to lie exactly edge - on as seen from Earth. The bright nucleus can be seen at the centre, along with the very thin disc that looks like a straight line from our unusual viewing position. To complete the picture, a hazy halo of stars on the periphery of the galaxy makes it seem to glow. NGC 4452 was first seen by William Herschel in 1784 with his 47 cm telescope in England. He described the object as a bright nebula, small and very much elongated. The new Hubble image shows just how elongated this unusual object really is. NGC 4452 is part of the Virgo Cluster, so - called because many

PIX4611380

Hornbill Festival of Nagaland-India. People from an ethnic community feasting on the annual Hornbill festival at the village of Kisama in Nagaland, India. The festival held through the 1st week of December, is a cultural extravaganza where the government, local communities and various NGOs get a chance to revive, protect and preserve the richness and uniqueness of the Naga cultural heritage. It is an opportunity for tourists from around the globe to get a wide view of this elusive land and its culture. During this period activities of all the Naga tribes (16 in number) are featured in the form of traditional dance, music, folk songs, and traditional sports. Tribal foods and drinks go around in plenty. Arts are also featured, with paintings, wood carvings and sculptures by modern Naga artists on display during this festival. Nagaland, India. December 3, 2008. (photo)

Hornbill Festival of Nagaland-India. People from an ethnic community feasting on the annual Hornbill festival at the village of Kisama in Nagaland, India. The festival held through the 1st week of December, is a cultural extravaganza where the government, local communities and various NGOs get a chance to revive, protect and preserve the richness and uniqueness of the Naga cultural heritage. It is an opportunity for tourists from around the globe to get a wide view of this elusive land and its culture. During this period activities of all the Naga tribes (16 in number) are featured in the form of traditional dance, music, folk songs, and traditional sports. Tribal foods and drinks go around in plenty. Arts are also featured, with paintings, wood carvings and sculptures by modern Naga artists on display during this festival. Nagaland, India. December 3, 2008. (photo)

UIG800591

Hubble deep field north - Hubble Deep Field North - North of the constellation of the Great Bear, the Hubble space telescope posed 75h to obtain this image of the distant universe. More than 1500 galaxies distant from 1 to 12 billion years - light are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. Representing a narrow “” keyhole”” view all the way to the visible horizon of the universe, the HDF image covers a speck of sky 1/30th the diameter of the full Moon. This is so narrow, just a few foreground stars in our Milky Way galaxy are visible and are vastly outnumbered by the menagerie of far more distant galaxies, some nearly as faint as 30th magnitude, or nearly four billion times fainter than the limits of human vision. Although the

Hubble deep field north - Hubble Deep Field North - North of the constellation of the Great Bear, the Hubble space telescope posed 75h to obtain this image of the distant universe. More than 1500 galaxies distant from 1 to 12 billion years - light are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. Representing a narrow “” keyhole”” view all the way to the visible horizon of the universe, the HDF image covers a speck of sky 1/30th the diameter of the full Moon. This is so narrow, just a few foreground stars in our Milky Way galaxy are visible and are vastly outnumbered by the menagerie of far more distant galaxies, some nearly as faint as 30th magnitude, or nearly four billion times fainter than the limits of human vision. Although the

PIX4613757

Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101)

Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101)

D. De Martin

PIX4612725

March: impact crater Maunder - Mars: Maunder crater - Perspective view of an impact crater located between Argyre Planitia and Hellas Planitia. The Maunder crater is 90 km in diameter and 900 m deep. The dark areas at the bottom of the crater are dunes. Image obtained by the Mars Express probe in 2005. On 29 November and 14 December 2005 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 15 meters per pixel. The data were acquired in the region of Noachis Terra at approximately 50* southern latitude and 2* eastern longitude. The Maunder Crater, located halfway between Argyre Planitia and Hellas Planitia on the southern Highlands of Mars, has a diameter of 90 kilometers and a current depth of barely 900 meters. In the east, the crater floor is bounded by an approximately 700 meters deep trough. It may be associated with the landslide on the western edge of the crater. Some gullies formed on th

March: impact crater Maunder - Mars: Maunder crater - Perspective view of an impact crater located between Argyre Planitia and Hellas Planitia. The Maunder crater is 90 km in diameter and 900 m deep. The dark areas at the bottom of the crater are dunes. Image obtained by the Mars Express probe in 2005. On 29 November and 14 December 2005 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 15 meters per pixel. The data were acquired in the region of Noachis Terra at approximately 50* southern latitude and 2* eastern longitude. The Maunder Crater, located halfway between Argyre Planitia and Hellas Planitia on the southern Highlands of Mars, has a diameter of 90 kilometers and a current depth of barely 900 meters. In the east, the crater floor is bounded by an approximately 700 meters deep trough. It may be associated with the landslide on the western edge of the crater. Some gullies formed on th

PIX4615975

Hornbill Festival of Nagaland-India. People from the ethnic Angami community feasting on the annual Hornbill festival at the village of Kisama in Nagaland, India. The festival held through the 1st week of December, is a cultural extravaganza where the government, local communities and various NGOs get a chance to revive, protect and preserve the richness and uniqueness of the Naga cultural heritage. It is an opportunity for tourists from around the globe to get a wide view of this elusive land and its culture. During this period activities of all the Naga tribes (16 in number) are featured in the form of traditional dance, music, folk songs, and traditional sports. Tribal foods and drinks go around in plenty. Arts are also featured, with paintings, wood carvings and sculptures by modern Naga artists on display during this festival. Nagaland, India. December 3, 2008. (photo)

Hornbill Festival of Nagaland-India. People from the ethnic Angami community feasting on the annual Hornbill festival at the village of Kisama in Nagaland, India. The festival held through the 1st week of December, is a cultural extravaganza where the government, local communities and various NGOs get a chance to revive, protect and preserve the richness and uniqueness of the Naga cultural heritage. It is an opportunity for tourists from around the globe to get a wide view of this elusive land and its culture. During this period activities of all the Naga tribes (16 in number) are featured in the form of traditional dance, music, folk songs, and traditional sports. Tribal foods and drinks go around in plenty. Arts are also featured, with paintings, wood carvings and sculptures by modern Naga artists on display during this festival. Nagaland, India. December 3, 2008. (photo)

UIG800587

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