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Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

PIX4623720

Framed Youth — Revenge of the Teenage Perverts 1986 (Credits)

Framed Youth — Revenge of the Teenage Perverts 1986 (Credits)

LCV7247019

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 4)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 4)

LCV7247025

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 2)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 2)

LCV7247022

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 3)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 3)

LCV7247024

Group of Galaxies HCG 31 - Hickson Compact Group 31 - This group of interacting galaxies is located 166 million years of light from Earth in the constellation Eridan. Dwarf galaxies are merging causing intense star formation. This long fusion process will lead to the birth of a large elliptical galaxy. Image obtained by the Hubble Space Telescope on August 8, 2006. These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow. Such encounters between dwarf galaxies are normally seen billions of light - years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light - years away. In this image, taken by Nasa's Hubble Space Telescope, the

Group of Galaxies HCG 31 - Hickson Compact Group 31 - This group of interacting galaxies is located 166 million years of light from Earth in the constellation Eridan. Dwarf galaxies are merging causing intense star formation. This long fusion process will lead to the birth of a large elliptical galaxy. Image obtained by the Hubble Space Telescope on August 8, 2006. These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow. Such encounters between dwarf galaxies are normally seen billions of light - years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light - years away. In this image, taken by Nasa's Hubble Space Telescope, the

PIX4565530

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

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

Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

PIX4623214

Eagle Nebula (IC 4703) in the Snake - detail - Young stars in the Eagle nebula - Detail on young stars located in the north - west part of the Eagle Nebula (M16). Image obtained by the Hubble Space Telescope. This picture shows the northwestern part of the Eagle nebula (M16), well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow. The star cluster is very bright and was discovered in the mid - eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed The Pillars of Creation”” ever since the Hubble S

Eagle Nebula (IC 4703) in the Snake - detail - Young stars in the Eagle nebula - Detail on young stars located in the north - west part of the Eagle Nebula (M16). Image obtained by the Hubble Space Telescope. This picture shows the northwestern part of the Eagle nebula (M16), well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow. The star cluster is very bright and was discovered in the mid - eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed The Pillars of Creation”” ever since the Hubble S

PIX4620062

Orion nebula centre - Trapeze - Orion nebula center - Mosaic of images obtained by the space telescope in 1994 and 1995 showing the center of Orion nebula, the region around the Trapeze, a cluster of 4 very young and massive stars that make this nebula shine. The picture shows a churning turbulent star factory set within a maelstrom of flowing, luminescent gas. Although this 2.5 light - years wide view is still a small portion of the entire Orion nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. Hubble reveals details as small as 4.1 billion miles across. Hubble Space Telescope observing time was devoted to making this panorama because the nebula is a vast laboratory for studying the processes which gave birth to our own Sun and solar system 4.5 billion years ago. Gas are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, whi

Orion nebula centre - Trapeze - Orion nebula center - Mosaic of images obtained by the space telescope in 1994 and 1995 showing the center of Orion nebula, the region around the Trapeze, a cluster of 4 very young and massive stars that make this nebula shine. The picture shows a churning turbulent star factory set within a maelstrom of flowing, luminescent gas. Although this 2.5 light - years wide view is still a small portion of the entire Orion nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. Hubble reveals details as small as 4.1 billion miles across. Hubble Space Telescope observing time was devoted to making this panorama because the nebula is a vast laboratory for studying the processes which gave birth to our own Sun and solar system 4.5 billion years ago. Gas are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, whi

PIX4617855

WW2 Documentary 'Invasion Of Europe: Normandy - Volume 1' 1944

WW2 Documentary 'Invasion Of Europe: Normandy - Volume 1' 1944

BOF6287535

Machine gunner's body armour (Sappenpanzer), 1916-17 (steel)

Machine gunner's body armour (Sappenpanzer), 1916-17 (steel)

German School, (20th century)

AMR3548830

Chest-of-drawers, 1780 (wood & marble)

Chest-of-drawers, 1780 (wood & marble)

Riesener, Jean-Henri (1734-1806)

TWC5899281

Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

PIX4621545

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

PIX4672819

Chest-of-drawers, 1780 (wood & marble)

Chest-of-drawers, 1780 (wood & marble)

Riesener, Jean-Henri (1734-1806)

TWC5899282

Chest-of-drawers, 1780 (wood & marble)

Chest-of-drawers, 1780 (wood & marble)

Riesener, Jean-Henri (1734-1806)

TWC65549

Stars cluster in the Nebula of the Eagle - Young stars in the Eagle nebula - Detail on young stars located in the cluster of stars NGC 6611 of the Nebula of the Eagle (M16). Image obtained by the Hubble Space Telescope. A spectacular section of the well - known Eagle Nebula has been targeted by the NASA/ESA Hubble Space Telescope. This collection of dazzling stars is called NGC 6611, an open star cluster that formed about 5.5 million years ago and is found approximately 6500 light - years from the Earth. It is a very young cluster, containing many hot, blue stars, whose fierce ultraviolet glow make the surrounding Eagle Nebula glow brightly. The cluster and the associated nebula together are also known as Messier 16. Astronomers refer to areas like the Eagle Nebula as HII regions. This is the scientific notation for ionised hydrogen from which the region is largely made. Extrapolating far into the future, this HII region will eventually disperse, helped along by shockwaves from superno

Stars cluster in the Nebula of the Eagle - Young stars in the Eagle nebula - Detail on young stars located in the cluster of stars NGC 6611 of the Nebula of the Eagle (M16). Image obtained by the Hubble Space Telescope. A spectacular section of the well - known Eagle Nebula has been targeted by the NASA/ESA Hubble Space Telescope. This collection of dazzling stars is called NGC 6611, an open star cluster that formed about 5.5 million years ago and is found approximately 6500 light - years from the Earth. It is a very young cluster, containing many hot, blue stars, whose fierce ultraviolet glow make the surrounding Eagle Nebula glow brightly. The cluster and the associated nebula together are also known as Messier 16. Astronomers refer to areas like the Eagle Nebula as HII regions. This is the scientific notation for ionised hydrogen from which the region is largely made. Extrapolating far into the future, this HII region will eventually disperse, helped along by shockwaves from superno

PIX4620069

'Road To Interdependence' History Of U.S. Foreign Relations Documentary (part 5/10)

'Road To Interdependence' History Of U.S. Foreign Relations Documentary (part 5/10)

BOF5914642

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

PIX4612940

Ball and evening dresses'. Figure 253: 'Front hair cropped ...; double bandeau of sliver band, ornamented with artificial flowers; white ostrich feather, fixed with a diamind pin. White crape petticoat, spotted with silver. Body and train of green satin; short sleeves of satin-strped muslin. Gold bracelets. Four rows of pearls round the neck. Pearl ear-rings. White gloves and shoes. Figure 254: Hair cropped. Turban cap of white crape, trimmed with broad white lace, and a silver band on the left side. White muslin petticoat. Robe of white muslin, the train trimmed with a broad lace; short sleeves; epaulettes a la polonoise, trimmed with lace, and tied with a string of pearls. Diamond hoop ear-rings. White gloves and shoes. Figure 255: Hair cropped, ornamented with pearls, behind with a muslin handkerchief, formed into a bow. Jacket and petticoat of white muslin; short sleeves trimmed with lace; high ruff round the neck. Gold hoop ear-rings. White gloves and shoes. Figure: 256: Front ha

Ball and evening dresses'. Figure 253: 'Front hair cropped ...; double bandeau of sliver band, ornamented with artificial flowers; white ostrich feather, fixed with a diamind pin. White crape petticoat, spotted with silver. Body and train of green satin; short sleeves of satin-strped muslin. Gold bracelets. Four rows of pearls round the neck. Pearl ear-rings. White gloves and shoes. Figure 254: Hair cropped. Turban cap of white crape, trimmed with broad white lace, and a silver band on the left side. White muslin petticoat. Robe of white muslin, the train trimmed with a broad lace; short sleeves; epaulettes a la polonoise, trimmed with lace, and tied with a string of pearls. Diamond hoop ear-rings. White gloves and shoes. Figure 255: Hair cropped, ornamented with pearls, behind with a muslin handkerchief, formed into a bow. Jacket and petticoat of white muslin; short sleeves trimmed with lace; high ruff round the neck. Gold hoop ear-rings. White gloves and shoes. Figure: 256: Front ha

BL3294789

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

British School, (19th century)

NAM5920622

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

British School, (19th century)

NAM5920624

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

British School, (19th century)

NAM5920625

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

General Officers sword used by Lieutenant-General Sir John Moore, 1809 circa (metal)

British School, (19th century)

NAM5920623

Bust of a 'Barbary pirate', c.1700 (terracotta)

Bust of a 'Barbary pirate', c.1700 (terracotta)

Unknown artist, (18th century)

MMM7342403

The English Yacht 'Portsmouth' at Anchor, 1675 (oil on panel)

The English Yacht 'Portsmouth' at Anchor, 1675 (oil on panel)

Velde, Willem van de, the Elder (1611-93)

MMM7342590

Battipaglia, 1969

Battipaglia, 1969

MOD6428900

Switzerland Lambachschule Habkern, 1945 (b/w photo)

Switzerland Lambachschule Habkern, 1945 (b/w photo)

Walter Studer

KES6234395

Compagnie Lubat Uzeste, 1991 (b/w photo)

premium — Compagnie Lubat Uzeste, 1991 (b/w photo)

Compagnie Lubat Uzeste, 1991 (b/w photo)

MWL7390346

Switzerland Helvetik Napoleon Basel (b/w photo)

Switzerland Helvetik Napoleon Basel (b/w photo)

KES6249743

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

PIX4665861

History of the Founding of the Geppoji Temple, Muromachi Period, c.1495 (ink, colour & gold on paper)

History of the Founding of the Geppoji Temple, Muromachi Period, c.1495 (ink, colour & gold on paper)

Mitsunobu, Tosa (1434-1525)

FSG483276

Illustration from the Founding of the Buddhist Temple, Tsukiminedera, Muromachi Period, 1495 (ink, colour & gold on paper)

Illustration from the Founding of the Buddhist Temple, Tsukiminedera, Muromachi Period, 1495 (ink, colour & gold on paper)

Mitsunobu, Tosa (1434-1525)

FSG483282

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