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Noctulescent clouds in Alaska, august 2009 (photo)

Noctulescent clouds in Alaska, august 2009 (photo)

Dennis Anderson

PIX4671632

Astronauts in weightlessness - Astronauts in Tranquility Module - Astronauts in the STS mission - 130 Terry Virts (bottom), Stephen Robinson (top right) and Soichi Noguchi weightlessness photographs in the new Tranquility module of the International Space Station (ISS). 14 February 2010. NASA astronauts Terry Virts (bottom), STS - 130 pilot; Stephen Robinson (top right), STS - 130 mission specialist; and Japan Aerospace Exploration Agency (JAXA) astronaut Soichi Noguchi, Expedition 22 flight engineer, are pictured in the newly - installed Tranquility node of the International Space Station while space shuttle Endeavour remains docked with the station. February 14, 2010

Astronauts in weightlessness - Astronauts in Tranquility Module - Astronauts in the STS mission - 130 Terry Virts (bottom), Stephen Robinson (top right) and Soichi Noguchi weightlessness photographs in the new Tranquility module of the International Space Station (ISS). 14 February 2010. NASA astronauts Terry Virts (bottom), STS - 130 pilot; Stephen Robinson (top right), STS - 130 mission specialist; and Japan Aerospace Exploration Agency (JAXA) astronaut Soichi Noguchi, Expedition 22 flight engineer, are pictured in the newly - installed Tranquility node of the International Space Station while space shuttle Endeavour remains docked with the station. February 14, 2010

PIX4602801

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250497

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250596

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250624

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250531

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250566

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250595

Tombs of the Kings, Remains of the funeral chambers and loculi of tomb 6, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of burial chambers and tomb loculi 6 of the necropolis known as the “Tombs of the Kings”, Ptolemaic Necropolis of Hellenistic style - Doric, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD, Paphos, Cyprus,

Tombs of the Kings, Remains of the funeral chambers and loculi of tomb 6, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of burial chambers and tomb loculi 6 of the necropolis known as the “Tombs of the Kings”, Ptolemaic Necropolis of Hellenistic style - Doric, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD, Paphos, Cyprus,

Frank Buffetrille

FBU4243819

Tombs of the Kings, Remains of the atrium of tomb 6 and entrance of the funeral chamber, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of the tomb atrium 6 and portico of the funerary chamber, Necropole called “Tombs of the Kings”, Necropole Ptolemaic Hellenistic-Doric style, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD-C, Paphos, Cyprus,

Tombs of the Kings, Remains of the atrium of tomb 6 and entrance of the funeral chamber, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of the tomb atrium 6 and portico of the funerary chamber, Necropole called “Tombs of the Kings”, Necropole Ptolemaic Hellenistic-Doric style, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD-C, Paphos, Cyprus,

Frank Buffetrille

FBU4243506

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Stairs leading to the remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250486

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250554

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Archaeological site of Gournia. Gournia is the best preserved of all Minoan cities, and has been characterized as the “” Pompei Minoan Crete””. The cities has been found as it is now and has never been rebuilt. Gournia offers a picture of the daily life of the Minoan, who were engaged in agricultural, animal husbandry, fishing and range-making as shown by the tools discovered in the settlement. Remains of the Palace. The palace was the most luxurious building in town, probably the administrative center and the residence of the town's leader. Crete

Frank Buffetrille

FBU4250632

Tombs of the Kings, Remains of the atrium of tomb 6 and entrance of the funeral chamber, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of the tomb atrium 6 and portico of the funerary chamber, Necropole called “Tombs of the Kings”, Necropole Ptolemaic Hellenistic-Doric style, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD-C, Paphos, Cyprus,

Tombs of the Kings, Remains of the atrium of tomb 6 and entrance of the funeral chamber, Early Ptolemaic necropolis in a Hellenistic Doric style, dating from 300 BC, The necropolis was continuously used as a burial area during the Hellenistic and Roman periods (3rd century BC-beginning of 4th century AD) Paphos, Cyprus - Remains of the tomb atrium 6 and portico of the funerary chamber, Necropole called “Tombs of the Kings”, Necropole Ptolemaic Hellenistic-Doric style, Place that served as a cemetery during the Hellenistic and Roman periods and place of refuge for the first Christian during the persecutions, UNESCO site, 3rd century BC - 3rd century AD-C, Paphos, Cyprus,

Frank Buffetrille

FBU4243913

Tunguska event -Artist view-3/3 - Tunguska valley - Artist view (3/3) - Artist view of the Tungouska region a few minutes after the explosion, June 30, 1908. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. Precisely what the Tunguska Event was remains a mystery. Despite the enormous scale of the explosion, there was no impact crater. Instead some 2000 sq/kms of taiga forest was flattened like matchwood and incinerated. This is the scene some minutes after the explosion. Most of the forest has been blown away, the few remaining stumps are burning and the air is full of acrid smoke. June 30 190

Tunguska event -Artist view-3/3 - Tunguska valley - Artist view (3/3) - Artist view of the Tungouska region a few minutes after the explosion, June 30, 1908. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. Precisely what the Tunguska Event was remains a mystery. Despite the enormous scale of the explosion, there was no impact crater. Instead some 2000 sq/kms of taiga forest was flattened like matchwood and incinerated. This is the scene some minutes after the explosion. Most of the forest has been blown away, the few remaining stumps are burning and the air is full of acrid smoke. June 30 190

PIX4583798

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

PIX4593469

Remains of the supernova Cassiopee A/HST - Cassiopeia A: Colorful, Shredded Remains of Old Supernova Glowing gaseous streamers of red, white, and blue - - as well as green and pink - - illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by Nasa's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a blow. The dead star's shredded remains are called Cassiopeia A, or “” Cas A”” for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light - years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astrono

Remains of the supernova Cassiopee A/HST - Cassiopeia A: Colorful, Shredded Remains of Old Supernova Glowing gaseous streamers of red, white, and blue - - as well as green and pink - - illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by Nasa's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a blow. The dead star's shredded remains are called Cassiopeia A, or “” Cas A”” for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light - years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astrono

PIX4582924

Tue 03, 1953 - Camera takes 50,000 pictures a second: A new camera claimed capable of taking 50,000 pictures a second being developed for use in scientific research by the British Admiralty Research Laboratory, in conjunction with a Glasgow firm of optical instrument makers. The camera is of the drum type, in which the film remains stationary. Incorporating many different size lenses, glass prisms and reflecting mirrors, it uses 35 mm. film at the rate of 10 feet for every 50,000 pictures. Picture shows Professor Home Dickson of the British Admiralty Research Laboratory examines the camera's lens holder in a Glasgow workshop.

Tue 03, 1953 - Camera takes 50,000 pictures a second: A new camera claimed capable of taking 50,000 pictures a second being developed for use in scientific research by the British Admiralty Research Laboratory, in conjunction with a Glasgow firm of optical instrument makers. The camera is of the drum type, in which the film remains stationary. Incorporating many different size lenses, glass prisms and reflecting mirrors, it uses 35 mm. film at the rate of 10 feet for every 50,000 pictures. Picture shows Professor Home Dickson of the British Admiralty Research Laboratory examines the camera's lens holder in a Glasgow workshop.

ZUM4875067

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

PIX4593478

Devonian Landscape, England, 2011 (photo)

Devonian Landscape, England, 2011 (photo)

Walter B Myers

PIX4632919

Apr. 07, 1953 - Detective remove chimney at the house of Death. work on roof in Rillington Place: Blue - overalled detectives today made a brick by brick interior examination of the chimney stack of No.10. Rillington place, Notting Hill, where the remains of two unidentified women were found in the garden ten days ago. The search of the stack followed a probe of the chimney with a stick. The stick met with resistance so it was decided to make further investigation there

Apr. 07, 1953 - Detective remove chimney at the house of Death. work on roof in Rillington Place: Blue - overalled detectives today made a brick by brick interior examination of the chimney stack of No.10. Rillington place, Notting Hill, where the remains of two unidentified women were found in the garden ten days ago. The search of the stack followed a probe of the chimney with a stick. The stick met with resistance so it was decided to make further investigation there

ZUM4837276

Einiosaurus - The Einiosaurs were herbivorous dinosaurs of the cretace, of the same family as the triceratops. A herd of plant-eating Einiosaurus roam the plains in what is today the Two Medicine Formation in northwestern Montana. In the distance a long-dormant volcano signals its return to activity by cauterizing snowcover into great clouds of steam. Within weeks the volcano will bury this scene beneath a massive ash fall, preserving the remains of the flora a fauna for future exhumation and examination by Homo sapiens 75 million years later. Einiosaurus was from the same family as the better known Triceratops. These dinosaurs were about 20 feet long, 6 feet tall at the hips and weighed about 2 tons

Einiosaurus - The Einiosaurs were herbivorous dinosaurs of the cretace, of the same family as the triceratops. A herd of plant-eating Einiosaurus roam the plains in what is today the Two Medicine Formation in northwestern Montana. In the distance a long-dormant volcano signals its return to activity by cauterizing snowcover into great clouds of steam. Within weeks the volcano will bury this scene beneath a massive ash fall, preserving the remains of the flora a fauna for future exhumation and examination by Homo sapiens 75 million years later. Einiosaurus was from the same family as the better known Triceratops. These dinosaurs were about 20 feet long, 6 feet tall at the hips and weighed about 2 tons

Walter B Myers

PIX4662929

Remnants of the supernova Cassiopee A in X-rays - Chandra 3 - color X - ray Image of Cassiopeia A This spectacular image of the supernova remnant Cassiopeia A is the most detailed image ever made of the remains of an exploded star. The one million second image shows a bright outer ring (green) ten light years in diameter that marks the location of a shock wave generated by the supernova explosion. A large jet - like structure that protrudes beyond the shock wave can be seen in the upper left. In this image, the colors represent different ranges of X - rays with red, green, and blue representing, low, medium, and higher X - ray energies

Remnants of the supernova Cassiopee A in X-rays - Chandra 3 - color X - ray Image of Cassiopeia A This spectacular image of the supernova remnant Cassiopeia A is the most detailed image ever made of the remains of an exploded star. The one million second image shows a bright outer ring (green) ten light years in diameter that marks the location of a shock wave generated by the supernova explosion. A large jet - like structure that protrudes beyond the shock wave can be seen in the upper left. In this image, the colors represent different ranges of X - rays with red, green, and blue representing, low, medium, and higher X - ray energies

PIX4582936

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Milicians carrying the coffin of the remains of the founder of the Falange Jose Antonio Primo de Rivera. Photography. SPAIN

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Milicians carrying the coffin of the remains of the founder of the Falange Jose Antonio Primo de Rivera. Photography. SPAIN

Unknown photographer, (20th century)

CUL4882845

The Zulu army, 1849 (lithograph)

The Zulu army, 1849 (lithograph)

Angas, George French (1822-86)

AMD8939307

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Albacete (24/11/1939), the provincial head of Spanish Falange Fulgencio Lozano, carrying the coffin of the remains of Jose Antonio Primo de Rivera on his shoulders. Photography. SPAIN. Albacete

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Albacete (24/11/1939), the provincial head of Spanish Falange Fulgencio Lozano, carrying the coffin of the remains of Jose Antonio Primo de Rivera on his shoulders. Photography. SPAIN. Albacete

Unknown photographer, (20th century)

CUL4882871

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Militias of Falange over funeral procession with lighted torches during the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. Madrid

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Militias of Falange over funeral procession with lighted torches during the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. Madrid

Unknown photographer, (20th century)

CUL4882721

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The remains of Jose Antonio Primo de Rivera arriving at El Escorial. Photography. SPAIN. San Lorenzo de El Escorial. Royal Monastery of San Lorenzo de El Escorial

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The remains of Jose Antonio Primo de Rivera arriving at El Escorial. Photography. SPAIN. San Lorenzo de El Escorial. Royal Monastery of San Lorenzo de El Escorial

Unknown photographer, (20th century)

CUL4882739

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Citizens making the fascist salute to the coffin with the remains of Jose Antonio Primo de Rivera that were carried from Alicante to El Escorial. Photography. SPAIN. Madrid

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Citizens making the fascist salute to the coffin with the remains of Jose Antonio Primo de Rivera that were carried from Alicante to El Escorial. Photography. SPAIN. Madrid

Unknown photographer, (20th century)

CUL4882759

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Girls from the Auxilio Social organitation waving his arm up to the remains of the founder of the Falange. Photography. SPAIN. Madrid

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Girls from the Auxilio Social organitation waving his arm up to the remains of the founder of the Falange. Photography. SPAIN. Madrid

Unknown photographer, (20th century)

CUL4882816

Column Medicis (Paris 1er) - Medicis Column - Paris - High of 31 metres, built in 1575, this column is the only vestige of the palace of Catherine de Medicis, deconstructed in 1748. The astrologers of the sovereign ensured their forecasts from the top of the platform, access to which is via a screw staircase located inside the column. A sundial, made by astronomer Guy Pingre, was installed on this column from 1764 to 1889. Located in the garden of Les Halles near the Bourse du Commerce (Stockmarket) of Paris, the Medicis column, built in 1575 is what remains of the Queen s hotel. This column is 31 meters (100 feet) high, with interior stairs counting 147 steps; its real function was never established. It is believed that due to the Queen s interest for astrology, it used to be an observatory for Cosimo Ruggieri, Catherine de Medicis astrologist

Column Medicis (Paris 1er) - Medicis Column - Paris - High of 31 metres, built in 1575, this column is the only vestige of the palace of Catherine de Medicis, deconstructed in 1748. The astrologers of the sovereign ensured their forecasts from the top of the platform, access to which is via a screw staircase located inside the column. A sundial, made by astronomer Guy Pingre, was installed on this column from 1764 to 1889. Located in the garden of Les Halles near the Bourse du Commerce (Stockmarket) of Paris, the Medicis column, built in 1575 is what remains of the Queen s hotel. This column is 31 meters (100 feet) high, with interior stairs counting 147 steps; its real function was never established. It is believed that due to the Queen s interest for astrology, it used to be an observatory for Cosimo Ruggieri, Catherine de Medicis astrologist

Sebastien Beaucourt

PIX4585387

Barnard's Star Movement - The proper motion of Barnard's star - Barnard's Star is a red dwarf less than six years from Earth in the constellation Ophiuchus. Its proximity makes it move quickly ahead of the other stars. Barnard's star is known for having the most important clean movement. This composite image made from three images taken in 1988 (blue), 1991 (red) and 1993 (green) shows the shift of the star in 15 years. Barnard's Star is red dwarf star approximately 6 light - years away from Earth in the constellation of Ophiuchus Its proper motion is 10.3 arcseconds per year, which remains the largest known proper motion of any star relative to the Sun. The monochrome plates from which this 3 - colour picture were made were taken in 1988 (blue), 1991 (red) and 1993 (green) showing its movement over 15 years

Barnard's Star Movement - The proper motion of Barnard's star - Barnard's Star is a red dwarf less than six years from Earth in the constellation Ophiuchus. Its proximity makes it move quickly ahead of the other stars. Barnard's star is known for having the most important clean movement. This composite image made from three images taken in 1988 (blue), 1991 (red) and 1993 (green) shows the shift of the star in 15 years. Barnard's Star is red dwarf star approximately 6 light - years away from Earth in the constellation of Ophiuchus Its proper motion is 10.3 arcseconds per year, which remains the largest known proper motion of any star relative to the Sun. The monochrome plates from which this 3 - colour picture were made were taken in 1988 (blue), 1991 (red) and 1993 (green) showing its movement over 15 years

PIX4571864

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Spanish workers of the Transport and Communications Union making the fascist salute to the remains of Jose Antonio Primo de Rivera at its pass through the streets of Madrid. Photography. SPAIN. Madrid

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Spanish workers of the Transport and Communications Union making the fascist salute to the remains of Jose Antonio Primo de Rivera at its pass through the streets of Madrid. Photography. SPAIN. Madrid

Unknown photographer, (20th century)

CUL4882796

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image obtained with a telescope 61 cm in diameter. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova. Image taken with a 24 - inch telescope

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image obtained with a telescope 61 cm in diameter. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova. Image taken with a 24 - inch telescope

Adam Block

PIX4582731

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The militias from Albacete passed the coffin with Jose Antonio Primo de Rivera remains to the militias from Tarragona during their trip to El Escorial, on 11/24/1939. Photography. SPAIN. TARRAGONA

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The militias from Albacete passed the coffin with Jose Antonio Primo de Rivera remains to the militias from Tarragona during their trip to El Escorial, on 11/24/1939. Photography. SPAIN. TARRAGONA

Unknown photographer, (20th century)

CUL4882565

Venus Surface - Artist View - A venusian volcanic valley - Artist view - Venus's surface looks young, about 500 million years old. Active volcanism could be the cause. Based upon analysis of the number and distribution of impact craters across the whole of Venus, the entire surface appears to be the same age: about 500 million years old. This is an astonishing result since 500 million years is young for a planet in our solar system. Like the Earth, Venus is thought to be about 4.5 billion years old. This suggests that 500 million years ago (1/9th Venus' current age) Venus completely resurfaced itself - - turned itself inside out. What caused such a cataclysmic event, or if indeed this is what really happened, remains a mystery

Venus Surface - Artist View - A venusian volcanic valley - Artist view - Venus's surface looks young, about 500 million years old. Active volcanism could be the cause. Based upon analysis of the number and distribution of impact craters across the whole of Venus, the entire surface appears to be the same age: about 500 million years old. This is an astonishing result since 500 million years is young for a planet in our solar system. Like the Earth, Venus is thought to be about 4.5 billion years old. This suggests that 500 million years ago (1/9th Venus' current age) Venus completely resurfaced itself - - turned itself inside out. What caused such a cataclysmic event, or if indeed this is what really happened, remains a mystery

Walter B Myers

PIX4635439

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. NGC 3521 is located about 35 million light years in the distance towards the northern constellation of Leo. This new deep image depicts multiple debris shells that evidence previous mergers with one or more satellite galaxies. NGC 3521 is an example of a flocculent galaxy. Galaxies are assigned this classification because they exhibit short, fragmented and somewhat disorganized spiral arms. Almost one third of all spiral galaxies display this characteristic to some extent. The cause of this condition remains elusive but recent observations have revealed that this galaxy has experienced a merger with one or more satellite galaxies

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. NGC 3521 is located about 35 million light years in the distance towards the northern constellation of Leo. This new deep image depicts multiple debris shells that evidence previous mergers with one or more satellite galaxies. NGC 3521 is an example of a flocculent galaxy. Galaxies are assigned this classification because they exhibit short, fragmented and somewhat disorganized spiral arms. Almost one third of all spiral galaxies display this characteristic to some extent. The cause of this condition remains elusive but recent observations have revealed that this galaxy has experienced a merger with one or more satellite galaxies

R. Jay GaBany

PIX4610751

Swan Lace - detail ngc 6960 - This image of the Veil Nebula was taken with the Mosaic camera on the WIYN 0.9 - meter telescope at the National Science Foundation's Kitt Peak National Observatory near Tucson, AZ. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light - years from Earth in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova

Swan Lace - detail ngc 6960 - This image of the Veil Nebula was taken with the Mosaic camera on the WIYN 0.9 - meter telescope at the National Science Foundation's Kitt Peak National Observatory near Tucson, AZ. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light - years from Earth in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova

PIX4582687

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Funeral procession through the villages of La Mancha with torches by militia of the Falange Party (24/11/1939). The coffin conteined the remains of the founder of the Falange Jose Antonio Primo de Rivera. Photography. SPAIN. CASTILE LA MANCHA

PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Funeral procession through the villages of La Mancha with torches by militia of the Falange Party (24/11/1939). The coffin conteined the remains of the founder of the Falange Jose Antonio Primo de Rivera. Photography. SPAIN. CASTILE LA MANCHA

Unknown photographer, (20th century)

CUL4882540

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image obtained with a telescope 61 cm in diameter. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova. Image taken with a 24 - inch telescope

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image obtained with a telescope 61 cm in diameter. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova. Image taken with a 24 - inch telescope

PIX4582737

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The Caudillo, Francisco Franco, upon arrival at the Escorial Monastery during the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. San Lorenzo de El Escorial

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The Caudillo, Francisco Franco, upon arrival at the Escorial Monastery during the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. San Lorenzo de El Escorial

Unknown photographer, (20th century)

CUL4882673

Cryolophosaur - Cryolophosaurus - Cryolophosaur is the first dinosaur found in Antarctica by paleontologists. About 7 metres long, this carnivore lived at the beginning of the Jurassic about 190 million years ago. Over 20 feet long and weighing as much as a ton, Cryolophosaurus is the first dinosaur to have been unearthed by paleontologists in Antarctica. This formidable predator hunted 190 million years ago during the Early Jurassic period. While the Earth was warmer and Antarctica closer to the equator during Cryolophosaurus' time, the continent was still far enough south for the climate to be temperate rather than tropical. Much of Antarctica was likely covered by dense forests, at least near the coasts. Cryolophosaurus 'remains were found on a mountain range that would have placed it at an altitude of about 10,000 feet and 1,000 miles from the South Pole during its reign

Cryolophosaur - Cryolophosaurus - Cryolophosaur is the first dinosaur found in Antarctica by paleontologists. About 7 metres long, this carnivore lived at the beginning of the Jurassic about 190 million years ago. Over 20 feet long and weighing as much as a ton, Cryolophosaurus is the first dinosaur to have been unearthed by paleontologists in Antarctica. This formidable predator hunted 190 million years ago during the Early Jurassic period. While the Earth was warmer and Antarctica closer to the equator during Cryolophosaurus' time, the continent was still far enough south for the climate to be temperate rather than tropical. Much of Antarctica was likely covered by dense forests, at least near the coasts. Cryolophosaurus 'remains were found on a mountain range that would have placed it at an altitude of about 10,000 feet and 1,000 miles from the South Pole during its reign

Walter B Myers

PIX4661960

Open cluster of Pleiades - Open cluster of Pleiades - The north is at top. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lies some 440 light years away from the Earth, in the constellation of Taurus. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

Open cluster of Pleiades - Open cluster of Pleiades - The north is at top. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lies some 440 light years away from the Earth, in the constellation of Taurus. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

D. De Martin

PIX4568766

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image in false colors obtained with a telescope measuring 40 cm in diameter through various filters that highlight the oxygen (in blue), and the hydrogen (in red). The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star at right, known as 52 Cygnus, is not associated with the supernova. Image taken with a 16 - inch telescope. Red is Hydrogen, Blue is Oxygen

Les Dentelles du Cygne - Detail - NGC 6960 - Part of the Veil nebula - NGC 6960 - Part of the rest of the supernova of the Dentelles du Swan lies about 1500 years - light from the Earth. The bright star is 52 Cygnus, a star visible to the naked eye that is not associated with lace. Image in false colors obtained with a telescope measuring 40 cm in diameter through various filters that highlight the oxygen (in blue), and the hydrogen (in red). The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded less than 10,000 years ago in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star at right, known as 52 Cygnus, is not associated with the supernova. Image taken with a 16 - inch telescope. Red is Hydrogen, Blue is Oxygen

PIX4582749

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Madrid citizens while milicians were walking throught Madrid streets with the remains of the founder of the Falange Jose Antonio Primo de Rivera on their shoulders. Photography. SPAIN. MADRID (AUTONOMOUS COMMUNITY)

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. Madrid citizens while milicians were walking throught Madrid streets with the remains of the founder of the Falange Jose Antonio Primo de Rivera on their shoulders. Photography. SPAIN. MADRID (AUTONOMOUS COMMUNITY)

Unknown photographer, (20th century)

CUL4882824

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) on the left and M110 (NGC 205) (off-field). Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. The several distinct stars that surround Andromeda's image are actually stars in our Galaxy that are well in front of the background object. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) on the left and M110 (NGC 205) (off-field). Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. The several distinct stars that surround Andromeda's image are actually stars in our Galaxy that are well in front of the background object. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei

R. Gendler

PIX4608837

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

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

R. Gendler

PIX4568697

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

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

Walter B Myers

PIX4629809

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

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

PIX4568835

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The Head of State, Francisco Franco, leaving the basilica accompanied by the ministers after the celebration of the religious act after the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. San Lorenzo de El Escorial. Royal Monastery of San Lorenzo de El Escorial

FRANCO BAHAMONDE, Francisco (1892-1975). Spanish military man and politician. Dictator of Spain from 1939 to 1975. PRIMO DE RIVERA, Jose Antonio (1903-1936). Spanish lawyer, nobleman, politician, and founder of the Falange Espanola ('Spanish Phalanx'). Military accused of conspiracy and rebellion against the government of the Second Spanish Republic and sentenced to death. He got finally executed during the first months of the Spanish Civil War. At the end of the Civil War, the body was exhumed and carried on the shoulders from Alicante to El Escorial to honor him. Once the Basilica of the Valle de los Caidos was built, Francisco Franco ordered to bury the body there. The Head of State, Francisco Franco, leaving the basilica accompanied by the ministers after the celebration of the religious act after the transfer of the remains of Jose Antonio Primo de Rivera Escorial. Photography. SPAIN. San Lorenzo de El Escorial. Royal Monastery of San Lorenzo de El Escorial

Unknown photographer, (20th century)

CUL4882688

Swan Lace Detail - The Veil nebula, IC 1340 - IC 1340 is a detail of the Swan lace, a remnant of supernova located about 1900 years - light in the constellation Swan. The supernova exploded 5,000 or 8,000 years ago. Image in false colors obtained with a telescope measuring 40 cm in diameter through various filters that highlight the oxygen (in blue), and the hydrogen (in red). This image shows a faint portion of the eastern veil nebula in Cygnus, a large, almost spherical glowing shell of gas, the expanding remains of a star that exploded between 5,000 and 8,000 years ago. The nebula (and thus its precursor star) is about 1900 light years distant and about 100 light years across. It is the result of the shockwave from the explosion exciting the tenuous interstellar medium and making it glow. Shooting in these wavelengths and with the color combine choices yielded a spooky view of something resembling a Bat or Owl. Red is Hydrogen, Blue is Oxygen, Green is the product of both

Swan Lace Detail - The Veil nebula, IC 1340 - IC 1340 is a detail of the Swan lace, a remnant of supernova located about 1900 years - light in the constellation Swan. The supernova exploded 5,000 or 8,000 years ago. Image in false colors obtained with a telescope measuring 40 cm in diameter through various filters that highlight the oxygen (in blue), and the hydrogen (in red). This image shows a faint portion of the eastern veil nebula in Cygnus, a large, almost spherical glowing shell of gas, the expanding remains of a star that exploded between 5,000 and 8,000 years ago. The nebula (and thus its precursor star) is about 1900 light years distant and about 100 light years across. It is the result of the shockwave from the explosion exciting the tenuous interstellar medium and making it glow. Shooting in these wavelengths and with the color combine choices yielded a spooky view of something resembling a Bat or Owl. Red is Hydrogen, Blue is Oxygen, Green is the product of both

PIX4582768

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

Woolly rhinoceros - Woolly rhinoceros - Woolly rhinoceros (Coelodonta antiquitatis), also known as cloisonnee nostrils, was a species of large rhinoceros (1.6 to 2 metres high at withers and up to 3.5 metres long, weighing 2 to 3 tonnes) characterized by A thick woolly fleece. He lived in the cold steppes which covered in Pleistocene much of Eurasia. At its peak, less than 30,000 years ago, it was found from central Spain and southern England to Mongolia and southern Siberia. A woolly rhinoceros (Coelodonta antiquitatis) wanders the snow-covered terrain of Northern Europe 200 thousand years ago. In the foreground is a common rabbit of the family Leporidae. About the size, and maybe a little larger, than today's white rhinoceros, the woolly rhinoceros is believed to be related to the modern Sumatran rhinoceros. Covered with thick fur (AKA pelage), this stocky herbivore was well-suited to the cold climates associated with the Pleistocene glaciations. Woolly rhinoceros remains have been f

Woolly rhinoceros - Woolly rhinoceros - Woolly rhinoceros (Coelodonta antiquitatis), also known as cloisonnee nostrils, was a species of large rhinoceros (1.6 to 2 metres high at withers and up to 3.5 metres long, weighing 2 to 3 tonnes) characterized by A thick woolly fleece. He lived in the cold steppes which covered in Pleistocene much of Eurasia. At its peak, less than 30,000 years ago, it was found from central Spain and southern England to Mongolia and southern Siberia. A woolly rhinoceros (Coelodonta antiquitatis) wanders the snow-covered terrain of Northern Europe 200 thousand years ago. In the foreground is a common rabbit of the family Leporidae. About the size, and maybe a little larger, than today's white rhinoceros, the woolly rhinoceros is believed to be related to the modern Sumatran rhinoceros. Covered with thick fur (AKA pelage), this stocky herbivore was well-suited to the cold climates associated with the Pleistocene glaciations. Woolly rhinoceros remains have been f

Walter B Myers

PIX4664585

Astronauts in the International Space Station - Astronauts in ISS - Astronauts in the STS-131 mission (in light blue jerseys) and Expedition 23 pose for a group photo in the Kibo module of the International Space Station (ISS). The astronauts of the STS-131 mission are Alan Poindexter, James P. Dutton Jr., Clayton Anderson, Rick Mastracchio, Dorothy Metcalf-Lindenburger, Stephanie Wilson and Naoko Yamazaki. The members of Expedition 23 are Oleg Kotov, Mikhail Kornienko, Alexander Skvortsov, Soichi Noguchi, T.J. Creamer and Tracy Caldwell Dyson. April 14, 2010. STS-131 and Expedition 23 crew members gather for a group portrait in the Kibo laboratory of the International Space Station while space shuttle Discovery remains docked with the station. STS - 131 crew members pictured (light blue shirts) are NASA astronauts Alan Poindexter, commander; James P. Dutton Jr., pilot; Clayton Anderson, Rick Mastracchio, Dorothy Metcalf - Lindenburger, Stephanie Wilson and Japan Aerospace Exploration

Astronauts in the International Space Station - Astronauts in ISS - Astronauts in the STS-131 mission (in light blue jerseys) and Expedition 23 pose for a group photo in the Kibo module of the International Space Station (ISS). The astronauts of the STS-131 mission are Alan Poindexter, James P. Dutton Jr., Clayton Anderson, Rick Mastracchio, Dorothy Metcalf-Lindenburger, Stephanie Wilson and Naoko Yamazaki. The members of Expedition 23 are Oleg Kotov, Mikhail Kornienko, Alexander Skvortsov, Soichi Noguchi, T.J. Creamer and Tracy Caldwell Dyson. April 14, 2010. STS-131 and Expedition 23 crew members gather for a group portrait in the Kibo laboratory of the International Space Station while space shuttle Discovery remains docked with the station. STS - 131 crew members pictured (light blue shirts) are NASA astronauts Alan Poindexter, commander; James P. Dutton Jr., pilot; Clayton Anderson, Rick Mastracchio, Dorothy Metcalf - Lindenburger, Stephanie Wilson and Japan Aerospace Exploration

PIX4602885

Apollo 16: decolving the Lem from the lunar surface - Apollo 16: lunar module liftoff - The Orion lunar module decolves from the moon. View obtained by the television camera mounted on the lunar jeep, April 24, 1972. The Apollo 16 Lunar Module “” Orion”” ascent stage makes its liftoff from the lunar surface in this reproduction taken from a color television transmission made by the RCA color TV camera mounted on the Lunar Roving Vehicle (LRV). Remotely controlled from NASA's Mission Control Center (MCC) in Houston, the LRV - mounted camera made it possible for persons on Earth to watch the LM's launch from the moon. Liftoff occurred at 175:44 ground elapsed time, 7:26 p.m. (CST), April 23, 1972. The “Orion”” ascent stage, with astronauts John W. Young and Charles M. Duke Jr. aboard, returned from the lunar surface to rejoin the Command and Service Modules (CSM) orbiting the moon. Astronaut Thomas K. (Ken) Mattingly II remained with the CSM in lunar orbit while Young and Duke descended

Apollo 16: decolving the Lem from the lunar surface - Apollo 16: lunar module liftoff - The Orion lunar module decolves from the moon. View obtained by the television camera mounted on the lunar jeep, April 24, 1972. The Apollo 16 Lunar Module “” Orion”” ascent stage makes its liftoff from the lunar surface in this reproduction taken from a color television transmission made by the RCA color TV camera mounted on the Lunar Roving Vehicle (LRV). Remotely controlled from NASA's Mission Control Center (MCC) in Houston, the LRV - mounted camera made it possible for persons on Earth to watch the LM's launch from the moon. Liftoff occurred at 175:44 ground elapsed time, 7:26 p.m. (CST), April 23, 1972. The “Orion”” ascent stage, with astronauts John W. Young and Charles M. Duke Jr. aboard, returned from the lunar surface to rejoin the Command and Service Modules (CSM) orbiting the moon. Astronaut Thomas K. (Ken) Mattingly II remained with the CSM in lunar orbit while Young and Duke descended

PIX4597653

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in infrared by the Hubble space telescope. The image reveals in the center of the image a young star accompanied by a jet of material. NGC 3372 is located about 7000 light years away from Earth. Image obtained in July 2009. Composed of gas and dust, the pictured pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. Taken in infrared light, the image shows the dense column and the surrounding greenish - coloured gas all but disappear. Only a faint outline of the pillar remains. By penetrating the wall of gas and dust, the infrared vision of WFC3 reveals the infant star that is probably blasting the jet. Part of the jet nearest the star is more prominent in this view. These features can be seen because infrared light, unlike visible light, can pass through the dust. Hubble's Wide

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in infrared by the Hubble space telescope. The image reveals in the center of the image a young star accompanied by a jet of material. NGC 3372 is located about 7000 light years away from Earth. Image obtained in July 2009. Composed of gas and dust, the pictured pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. Taken in infrared light, the image shows the dense column and the surrounding greenish - coloured gas all but disappear. Only a faint outline of the pillar remains. By penetrating the wall of gas and dust, the infrared vision of WFC3 reveals the infant star that is probably blasting the jet. Part of the jet nearest the star is more prominent in this view. These features can be seen because infrared light, unlike visible light, can pass through the dust. Hubble's Wide

PIX4619096

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

Colorful Torosaurus - Torosaurus lived 75 million years ago in southeastern Wyoming, USA. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A colorful Torosaurus wonders a Cretaceous forest 75 million years ago in what is today southeastern Wyoming. Like the better known Triceratops, Torosaurus was a ceratopsid, a family of large four-legged plant-eating dinosaurs characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a purpose other than protecting against a brute force attack. One p

Colorful Torosaurus - Torosaurus lived 75 million years ago in southeastern Wyoming, USA. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A colorful Torosaurus wonders a Cretaceous forest 75 million years ago in what is today southeastern Wyoming. Like the better known Triceratops, Torosaurus was a ceratopsid, a family of large four-legged plant-eating dinosaurs characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a purpose other than protecting against a brute force attack. One p

Walter B Myers

PIX4662996

Detail in the nebula Omega (M17) - Part of M17 nebula - Detail in the nebula Omega (M17), a region of star formation. Image obtained from the 3.5-metre NTT telescope of the European Observatory of La Silla in Chile. The Omega Nebula (M17) is one of the youngest and most massive star - forming regions in the Milky Way. Active star - birth started a few million years ago and continues through today. The brightly shining gas shown in this picture is just a blister erupting from the side of a much larger dark cloud of molecular gas. The dust that is so prominent in this picture comes from the remains of massive hot stars that have ended their brief lives and ejected material back into space, as well as the cosmic detritus from which future suns form. Three - colour composite image of the Omega Nebula (Messier 17), based on images obtained with the EMMI instrument on the ESO 3.58 - metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the imag

Detail in the nebula Omega (M17) - Part of M17 nebula - Detail in the nebula Omega (M17), a region of star formation. Image obtained from the 3.5-metre NTT telescope of the European Observatory of La Silla in Chile. The Omega Nebula (M17) is one of the youngest and most massive star - forming regions in the Milky Way. Active star - birth started a few million years ago and continues through today. The brightly shining gas shown in this picture is just a blister erupting from the side of a much larger dark cloud of molecular gas. The dust that is so prominent in this picture comes from the remains of massive hot stars that have ended their brief lives and ejected material back into space, as well as the cosmic detritus from which future suns form. Three - colour composite image of the Omega Nebula (Messier 17), based on images obtained with the EMMI instrument on the ESO 3.58 - metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the imag

PIX4620256

Colorful Albertaceratops - Albertaceratops lived 77 million years ago in Alberta, Canada; it was 2 metres tall at the withers and weighed more than 2 tonnes. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A 20 foot long Albertaceratops wonders a Cretaceous forest 77 million years ago in what is today Alberta, Canada. Like the better known Triceratops, Albertaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a

Colorful Albertaceratops - Albertaceratops lived 77 million years ago in Alberta, Canada; it was 2 metres tall at the withers and weighed more than 2 tonnes. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A 20 foot long Albertaceratops wonders a Cretaceous forest 77 million years ago in what is today Alberta, Canada. Like the better known Triceratops, Albertaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a

Walter B Myers

PIX4663088

Remains of the Crab Supernova (M1) in the Taurus - M1, the Crab Nebula, is a supernova remnant from a star that exploded in July or August of 1054 AD and was witnessed and described by Chinese astronomers as being six times brighter than Venus. The supernova, located in the constellation of Taurus and about 7,000 light years away from the Earth, shined with the light of 400 million suns, was visible in the daytime for almost a month, and remained visible in the evening sky for more than a year. Today, some 900 years later, we see the remains of the exploded star as a cloud of gaseous debris, illuminated by the remnants of the core of the original star, which is now a rapidly spinning neutron star called a pulsar. The colors in the nebula come from two different sources. The red filaments come from typical hydrogen emission such as in emission nebula like M8. The diffuse blue background has a continuous spectrum composed of synchrotron radiation which is emitted by high energy electrons

Remains of the Crab Supernova (M1) in the Taurus - M1, the Crab Nebula, is a supernova remnant from a star that exploded in July or August of 1054 AD and was witnessed and described by Chinese astronomers as being six times brighter than Venus. The supernova, located in the constellation of Taurus and about 7,000 light years away from the Earth, shined with the light of 400 million suns, was visible in the daytime for almost a month, and remained visible in the evening sky for more than a year. Today, some 900 years later, we see the remains of the exploded star as a cloud of gaseous debris, illuminated by the remnants of the core of the original star, which is now a rapidly spinning neutron star called a pulsar. The colors in the nebula come from two different sources. The red filaments come from typical hydrogen emission such as in emission nebula like M8. The diffuse blue background has a continuous spectrum composed of synchrotron radiation which is emitted by high energy electrons

Jerry Lodriguss

PIX4583001

Colorful Pentaceratops - The Pentaceratops lived 75 million years ago in the southwestern United States. Herbivore, it was 8 meters long and weighed 6 tons. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A six ton, 27 foot long Pentaceratops wonders a Cretaceous forest 75 million years ago in what is today the southwestern United States. Like the better known Triceratops, Pentaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that the

Colorful Pentaceratops - The Pentaceratops lived 75 million years ago in the southwestern United States. Herbivore, it was 8 meters long and weighed 6 tons. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A six ton, 27 foot long Pentaceratops wonders a Cretaceous forest 75 million years ago in what is today the southwestern United States. Like the better known Triceratops, Pentaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that the

Walter B Myers

PIX4663157

The First Life Forms on Earth - Eoarchean Earth - 3.8 billion years ago, 770 million years after the formation of the Earth, the first life forms appeared as a unicellular organism. Bacteries and archeobacteries (archaea) began to populate the Earth's surface while the atmosphere was still filled with volcanic gases and probably without oxygen. In this illustration, these micro-organisms came out of the ocean to attach themselves to the rock remains of a caldera, bringing colour to this monochrome landscape. 770 million years after the formation of the Earth - - 3.8 billion years ago - - the first life may have appeared in the form of simple, single - celled organisms. Bacteria and archaea may have even found a way to populate the otherwise sterile and inhospitable surface. The atmosphere would likely have consisted solely of gases vented by volcanoes: carbon dioxide, carbon monoxide, sulfur dioxide, nitrogen, methane, hydrogen, methane, ammonia, and water vapor. In this image, a varie

The First Life Forms on Earth - Eoarchean Earth - 3.8 billion years ago, 770 million years after the formation of the Earth, the first life forms appeared as a unicellular organism. Bacteries and archeobacteries (archaea) began to populate the Earth's surface while the atmosphere was still filled with volcanic gases and probably without oxygen. In this illustration, these micro-organisms came out of the ocean to attach themselves to the rock remains of a caldera, bringing colour to this monochrome landscape. 770 million years after the formation of the Earth - - 3.8 billion years ago - - the first life may have appeared in the form of simple, single - celled organisms. Bacteria and archaea may have even found a way to populate the otherwise sterile and inhospitable surface. The atmosphere would likely have consisted solely of gases vented by volcanoes: carbon dioxide, carbon monoxide, sulfur dioxide, nitrogen, methane, hydrogen, methane, ammonia, and water vapor. In this image, a varie

Walter B Myers

PIX4632742

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of

PIX4608823

Apollo 17: decolving the Lem from the lunar surface - Apollo 17: lunar module liftoff - The Challenger lunar module decolves from the Moon. View obtained by the television camera mounted on the lunar jeep, December 14, 1972. The Apollo 17 Lunar Module (LM) “” Challenger”” ascent stage leaves the Taurus - Littrow landing site as it makes its spectacular liftoff from the lunar surface, as seen in this reproduction taken from a color television transmission made by the color RCA TV camera mounted on the Lunar Roving Vehicle (LRV). The LRV - mounted TV camera, remotely controlled from the Mission Control Center (MCC) in Houston, made it possible for people on Earth to watch the fantastic event. The LM liftoff was at 188:01:36 ground elapsed time, 4:54:36 p.m. (CST), Thursday, Dec. 14, 1972. The LM ascent stage, with astronauts Eugene A. Cernan and Harrison H. Schmitt aboard, returned from the lunar surface to rejoin the Command and Service Modules (CSM) orbiting the moon. Astronaut Ronald

Apollo 17: decolving the Lem from the lunar surface - Apollo 17: lunar module liftoff - The Challenger lunar module decolves from the Moon. View obtained by the television camera mounted on the lunar jeep, December 14, 1972. The Apollo 17 Lunar Module (LM) “” Challenger”” ascent stage leaves the Taurus - Littrow landing site as it makes its spectacular liftoff from the lunar surface, as seen in this reproduction taken from a color television transmission made by the color RCA TV camera mounted on the Lunar Roving Vehicle (LRV). The LRV - mounted TV camera, remotely controlled from the Mission Control Center (MCC) in Houston, made it possible for people on Earth to watch the fantastic event. The LM liftoff was at 188:01:36 ground elapsed time, 4:54:36 p.m. (CST), Thursday, Dec. 14, 1972. The LM ascent stage, with astronauts Eugene A. Cernan and Harrison H. Schmitt aboard, returned from the lunar surface to rejoin the Command and Service Modules (CSM) orbiting the moon. Astronaut Ronald

PIX4598316

Interacting galaxies NGC 1614 - Interacting galaxies NGC 1614 - The galaxy NGC 1614 is located about 200 million light years away from Earth in the southern constellation of Eridan. This system is composed of interacting galaxies. Image obtained by the Hubble Space Telescope on August 13, 2002. The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one - sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. The galaxy appears to be the result of a tidal interaction and the resulting merger of two predecessor systems. The system has a nuclear region of quasar - like luminosity, but shows no direct evidence for an active nucleus. It is heavily and unevenly reddened across its nucleus, while infrared imaging also shows a ridge of d

Interacting galaxies NGC 1614 - Interacting galaxies NGC 1614 - The galaxy NGC 1614 is located about 200 million light years away from Earth in the southern constellation of Eridan. This system is composed of interacting galaxies. Image obtained by the Hubble Space Telescope on August 13, 2002. The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one - sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. The galaxy appears to be the result of a tidal interaction and the resulting merger of two predecessor systems. The system has a nuclear region of quasar - like luminosity, but shows no direct evidence for an active nucleus. It is heavily and unevenly reddened across its nucleus, while infrared imaging also shows a ridge of d

PIX4609963

AVE8920960

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - 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 large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not stellar'. The tiny bright nebula that captures H

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - 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 large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not stellar'. The tiny bright nebula that captures H

Adam Block

PIX4619672

Burial pit (photo)

Burial pit (photo)

Ken Welsh

KW227423

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - 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 large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. Image made with Siding Spring's 3.9m telescope. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - 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 large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. Image made with Siding Spring's 3.9m telescope. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not

PIX4619615

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

PIX4594061

Detail of Civilisation Remains, 2010 (projection on glass slide)

Detail of Civilisation Remains, 2010 (projection on glass slide)

Bucher, Willi (b.1948)

STF452332

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

PIX4594065

St. Helene Island - St. Helena Island - St. Helene Island seen from the International Space Station (ISS) on 7 May 2009. Sainte-Helene is located 1860 km off the African coast in the Atlantic Ocean. Saint Helena Island, located in the South Atlantic Ocean approximately 1,860 kilometers (1,156 miles) west of Africa, was one of the many isolated islands that naturalist Charles Darwin visited during his scientific voyages in the nineteenth century. This image was acquired by astronauts onboard the International Space Station on May 7, 2009. This astronaut photograph shows the island's sharp peaks and deep ravines; the rugged topography results from erosion of the volcanic rocks that make up the island. The change in elevation from the coast to the interior creates a climate gradient. The higher, wetter center is covered with green vegetation, whereas the lower coastal areas are drier and hotter, with little vegetation cover. Human presence on the island has also caused dramatic changes to

St. Helene Island - St. Helena Island - St. Helene Island seen from the International Space Station (ISS) on 7 May 2009. Sainte-Helene is located 1860 km off the African coast in the Atlantic Ocean. Saint Helena Island, located in the South Atlantic Ocean approximately 1,860 kilometers (1,156 miles) west of Africa, was one of the many isolated islands that naturalist Charles Darwin visited during his scientific voyages in the nineteenth century. This image was acquired by astronauts onboard the International Space Station on May 7, 2009. This astronaut photograph shows the island's sharp peaks and deep ravines; the rugged topography results from erosion of the volcanic rocks that make up the island. The change in elevation from the coast to the interior creates a climate gradient. The higher, wetter center is covered with green vegetation, whereas the lower coastal areas are drier and hotter, with little vegetation cover. Human presence on the island has also caused dramatic changes to

PIX4659322

Roman Villa discovered in Lower Thames-Street (engraving)

Roman Villa discovered in Lower Thames-Street (engraving)

Fairholt, Frederick William (1814-66)

LIP1607005

Cannibalised face found at Gough's Cave.

Cannibalised face found at Gough's Cave.

UIG5305210

Human Head from Necropolis, Bovila de Madurell

Human Head from Necropolis, Bovila de Madurell

IND49353

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

PIX4634727

Roman remains found in Thames Street (engraving)

Roman remains found in Thames Street (engraving)

English School, (19th century)

LLJ583099

General view of the ruins (photo)

General view of the ruins (photo)

EDF291299

Opened sarcophagus, containing a lead coffin and a skeleton of a woman in her 20s

Opened sarcophagus, containing a lead coffin and a skeleton of a woman in her 20s

Roman, (4th century AD)

MOL225967

Remains of City of Bam, Iran

Remains of City of Bam, Iran

Stephen Coyne

SCN3477135

The last remains of the Fleet Prison (engraving)

The last remains of the Fleet Prison (engraving)

English School, (19th century)

LLM654153

Remains of Osney Abbey (engraving)

Remains of Osney Abbey (engraving)

English School, (19th century)

LLM662618

The Last Remains of the Fleet (engraving)

The Last Remains of the Fleet (engraving)

English School, (19th century)

LLR2776966

Cannibalised face found at Gough's Cave.

Cannibalised face found at Gough's Cave.

UIG5305209

Dead bodies of Lipniki Village residents in Volhynia. The Ukrainian Insurgent Army murdered 182 people. Photograph from the Independence museum in Warsaw under the title ' Volhynia extermination'.

Dead bodies of Lipniki Village residents in Volhynia. The Ukrainian Insurgent Army murdered 182 people. Photograph from the Independence museum in Warsaw under the title ' Volhynia extermination'.

FRM564655

Temple of Minerva viewed through Antonine Gate, 139 AD. Sbeitla, Roman city remains.

Temple of Minerva viewed through Antonine Gate, 139 AD. Sbeitla, Roman city remains.

Stephen Coyne

SCN3477734

Add. 22912, ff.307v-308, from 'Autograph journal of Dr. John Covel during his travels in Asia and Italy', 1670-78 (pen & ink on paper)

Add. 22912, ff.307v-308, from 'Autograph journal of Dr. John Covel during his travels in Asia and Italy', 1670-78 (pen & ink on paper)

English School, (17th century)

BL4819887

Column base and architectural element with a stork (photo)

Column base and architectural element with a stork (photo)

Roman, (3rd century AD)

Gerard Degeorge

GDG287821

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