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Bilder zu 'Covering' gefunden, 3,267

 
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Saxony, historical, Trade, Retail trade, Care, Businesses, department stores, Shopping Dresden, Centrum Department …, 1985 (photo)

Sächsische Zeitung

IMO8757711

Saxony, historical, Trade, Retail trade, Care, Businesses, department stores, Shopping Dresden, Centrum Department …, 1985 (photo)

Sächsische Zeitung

IMO8757711

 
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Saxony, historical, Trade, Retail trade, Care, Businesses, department stores, Shopping Dresden, Centrum Department …, 1985 (photo)

Sächsische Zeitung

IMO8757704

Saxony, historical, Trade, Retail trade, Care, Businesses, department stores, Shopping Dresden, Centrum Department …, 1985 (photo)

Sächsische Zeitung

IMO8757704

 
Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

PIX4618453

Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

PIX4618453

 
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Evolution of The Oil Industry, 1960s 3 of 3

BOF6285564

Evolution of The Oil Industry, 1960s 3 of 3

BOF6285564

 
View of the winding road leading to the train des train the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584746

View of the winding road leading to the train des train the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584746

 
Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584744

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584744

 
San Francisco Bay area view from space - San Francisco Bay area seen from space - San Francisco Bay area seen from space on April 17, 1998 from space shuttle Columbia. San Francisco Bay Area, California April 17, 1998. Considered one of the best natural harbors in the world, San Francisco Bay, with its various sediment patterns, can be seen in this unique near - vertical view. Surrounded by the San Francisco Metropolitan area to the west and southwest, the Berkeley and Oakland Metropolitan area to the east, and the San Jose Metropolitan (not visible on the image) to the southeast, San Francisco Bay is 50 miles (80 km) long and from 3 to 13 miles (5 to 21 km) wide. Waters of the Pacific Ocean (bottom of image) enter the bay through Golden Gate, a strait between two peninsulas. The world famous Golden Gate Bridge is discernible on the image connecting the two peninsulas. The bay is as deep as 100 feet (30 meters) in spots, with a channel 50 feet (15 meters) deep maintained through the sa

PIX4672866

San Francisco Bay area view from space - San Francisco Bay area seen from space - San Francisco Bay area seen from space on April 17, 1998 from space shuttle Columbia. San Francisco Bay Area, California April 17, 1998. Considered one of the best natural harbors in the world, San Francisco Bay, with its various sediment patterns, can be seen in this unique near - vertical view. Surrounded by the San Francisco Metropolitan area to the west and southwest, the Berkeley and Oakland Metropolitan area to the east, and the San Jose Metropolitan (not visible on the image) to the southeast, San Francisco Bay is 50 miles (80 km) long and from 3 to 13 miles (5 to 21 km) wide. Waters of the Pacific Ocean (bottom of image) enter the bay through Golden Gate, a strait between two peninsulas. The world famous Golden Gate Bridge is discernible on the image connecting the two peninsulas. The bay is as deep as 100 feet (30 meters) in spots, with a channel 50 feet (15 meters) deep maintained through the sa

PIX4672866

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584745

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584745

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

 
Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

 
Milky way all around the horizon and Gegenschein - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Stephane Guisard

PIX4636032

Milky way all around the horizon and Gegenschein - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Stephane Guisard

PIX4636032

 
Map of the sky seen by Planck - The microwave sky as seen by Planck - 380,000 years after the formation of the universe, when the temperature had become low enough, the light could be released from the extremely dense material that imprisoned it and spread throughout the universe. This moment appears to us today in the form of a radiation called fossil radiation, or cosmological diffuse background. This image is the map of temperature fluctuations of the cosmological diffuse background (in orange) seen by the Planck satellite between August 2009 and June 2010. Overlay, in blue, the Lactee Way and clear, filamentary structures that extend beyond the plane of our Lactee Way. This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure orig

PIX4634312

Map of the sky seen by Planck - The microwave sky as seen by Planck - 380,000 years after the formation of the universe, when the temperature had become low enough, the light could be released from the extremely dense material that imprisoned it and spread throughout the universe. This moment appears to us today in the form of a radiation called fossil radiation, or cosmological diffuse background. This image is the map of temperature fluctuations of the cosmological diffuse background (in orange) seen by the Planck satellite between August 2009 and June 2010. Overlay, in blue, the Lactee Way and clear, filamentary structures that extend beyond the plane of our Lactee Way. This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure orig

PIX4634312

 
Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

PIX4616544

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

PIX4616544

 
Fracture in the Petermann Glacier, Greenland - Crack in the Petermann Glacier, Greenland - View of Petermann Glacier northwest of Greenland September 7, 2008. The glacier occupies an area of about 1300 km and occasionally releases large icebergs (at the top of the picture). This glacier already lost 87 km of its surface between 2000 and 2001. Between 10 and 24 July 2008, the glacier lost another 29 km. A huge breche with a fine fracture is visible at the bottom of the image; if it continues to expand, the glacier could see a third of its mass detach. Image obtained from the Terra satellite. Covering some 1,295 square kilometers (500 square miles) along the northwestern coast of Greenland, Petermann Glace's floating ice tongue is the Northern Hemisphere's largest, and it has occasionally calved large icebergs. Between 2000 and 2001, the glacier lost nearly 87 square kilometers (34 square miles). Between July 10 and July 24, 2008, the glacier lost another 29 square kilometers (11 square

PIX4666067

Fracture in the Petermann Glacier, Greenland - Crack in the Petermann Glacier, Greenland - View of Petermann Glacier northwest of Greenland September 7, 2008. The glacier occupies an area of about 1300 km and occasionally releases large icebergs (at the top of the picture). This glacier already lost 87 km of its surface between 2000 and 2001. Between 10 and 24 July 2008, the glacier lost another 29 km. A huge breche with a fine fracture is visible at the bottom of the image; if it continues to expand, the glacier could see a third of its mass detach. Image obtained from the Terra satellite. Covering some 1,295 square kilometers (500 square miles) along the northwestern coast of Greenland, Petermann Glace's floating ice tongue is the Northern Hemisphere's largest, and it has occasionally calved large icebergs. Between 2000 and 2001, the glacier lost nearly 87 square kilometers (34 square miles). Between July 10 and July 24, 2008, the glacier lost another 29 square kilometers (11 square

PIX4666067

 
Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

PIX4660095

Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

PIX4660095

 
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Coffer, c.1700 (wood, brass & turtleshell)

Boulle, Andre Charles (1642-1732) (workshop of) (attr. to)

TWC5902041

Coffer, c.1700 (wood, brass & turtleshell)

Boulle, Andre Charles (1642-1732) (workshop of) (attr. to)

TWC5902041

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
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Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

 
The knight Bayard (Pierre Terrail) (1476-1524) fatally wounded Rebec on 29 April 1524 while covering the retreat of the French army of Francois I, replied to the Connetable of Bourbon who had betrayed the king of France and said: There is no need for pity for me, for I die as a good man; but I have mercy on you, for you serve against your Prince and your homeland! “” avant de die dans le camp de ses adversaires admiratifs”” (The death of Pierre Terrail de Bayard mortally wounded by an arquebus ball, on April 30, 1524, by his old comrade, Charles, Duke of Bourbon, who was now fighting on the opposite side) Engraving from “Les-Celebrites-Francaises” by Alfred des Essarts, 1862 Collection privee

ELD4883216

The knight Bayard (Pierre Terrail) (1476-1524) fatally wounded Rebec on 29 April 1524 while covering the retreat of the French army of Francois I, replied to the Connetable of Bourbon who had betrayed the king of France and said: There is no need for pity for me, for I die as a good man; but I have mercy on you, for you serve against your Prince and your homeland! “” avant de die dans le camp de ses adversaires admiratifs”” (The death of Pierre Terrail de Bayard mortally wounded by an arquebus ball, on April 30, 1524, by his old comrade, Charles, Duke of Bourbon, who was now fighting on the opposite side) Engraving from “Les-Celebrites-Francaises” by Alfred des Essarts, 1862 Collection privee

ELD4883216

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