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Church of Virgin Mary (Council Church)

Church of Virgin Mary (Council Church)

SAP693774

Where the Anzacs dug themselves in on the shelterless slopes of barren hills exposed to enemy fire, 1915 (b/w photo)

Where the Anzacs dug themselves in on the shelterless slopes of barren hills exposed to enemy fire, 1915 (b/w photo)

Unknown photographer, (20th century)

NAM5923026

Temple of Artemis

Temple of Artemis

SAP694640

Church of Virgin Mary (Council Church)

Church of Virgin Mary (Council Church)

SAP693777

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662356

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662358

Carboniferous flora and fauna - Carboniferous riverbank - Carboniferous landscape with its ferns, giant lycopods, sigillaria (sigillaria), calamites. Among the fauna are an amphibian, a scorpion and insects that dominated the landscape, such as the Meganeura, giant dragonfly with a wingspan of more than 80 cm, or the 2-metre-long arthropleura climbing here in a tree. Ferns, seed ferns, and giant lycopods (primitive moss - like plants with long slender leaves) flourished during the Carboniferous period, from about 360 to 300 million years ago. Some lycopods, such as the arboreal Sigillaria illustrated here, grew as high as 130 feet. (100 feet is considered tall for a modern Maple tree). Other tree - like plants included many varieties of the Calamites, extinct ancestors of modern horsetails. While the first dinosaurs were not to appear for another 130 million years, the Carboniferous forests were home to a plethora of terrestrial animals, including many species of invertebrates and some

Carboniferous flora and fauna - Carboniferous riverbank - Carboniferous landscape with its ferns, giant lycopods, sigillaria (sigillaria), calamites. Among the fauna are an amphibian, a scorpion and insects that dominated the landscape, such as the Meganeura, giant dragonfly with a wingspan of more than 80 cm, or the 2-metre-long arthropleura climbing here in a tree. Ferns, seed ferns, and giant lycopods (primitive moss - like plants with long slender leaves) flourished during the Carboniferous period, from about 360 to 300 million years ago. Some lycopods, such as the arboreal Sigillaria illustrated here, grew as high as 130 feet. (100 feet is considered tall for a modern Maple tree). Other tree - like plants included many varieties of the Calamites, extinct ancestors of modern horsetails. While the first dinosaurs were not to appear for another 130 million years, the Carboniferous forests were home to a plethora of terrestrial animals, including many species of invertebrates and some

Walter B Myers

PIX4632863

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

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585223

Temple of Zeus Olympios, Temple of Olympian Zeus,

Temple of Zeus Olympios, Temple of Olympian Zeus,

SAP616515

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662360

Church of Virgin Mary (Council Church)

Church of Virgin Mary (Council Church)

SAP693775

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

The Bahamas satellite views - Satellite image of the Bahamas - The Bahamas viewed by the Aqua satellite on 12 February 2009. East of southern Florida, large swaths of ocean water glow peacock blue. These waters owe their iridescence to their shallow depths. Near Florida and Cuba, the underwater terrain is hilly, and the crests of many of these hills including the islands of the Bahamas. On February 12, 2009, relatively clear skies allowed the Moderate Resolution Imaging Spectroradiometer (MODIS) on Nasa's Aqua satellite an unobstructed view of the region. The most striking feature of this image is the Great Bahama Bank, a massive underwater hill underlying Andros Island in the west, Eleuthera Island in the east, and multiple islands in between. To the north, another bank underlies another set of islands, including Grand Bahama. The varied colors of these banks suggest their surfaces are somewhat uneven. The banks' distinct contours, sharply outlined in dark blue, indicate that the ocea

The Bahamas satellite views - Satellite image of the Bahamas - The Bahamas viewed by the Aqua satellite on 12 February 2009. East of southern Florida, large swaths of ocean water glow peacock blue. These waters owe their iridescence to their shallow depths. Near Florida and Cuba, the underwater terrain is hilly, and the crests of many of these hills including the islands of the Bahamas. On February 12, 2009, relatively clear skies allowed the Moderate Resolution Imaging Spectroradiometer (MODIS) on Nasa's Aqua satellite an unobstructed view of the region. The most striking feature of this image is the Great Bahama Bank, a massive underwater hill underlying Andros Island in the west, Eleuthera Island in the east, and multiple islands in between. To the north, another bank underlies another set of islands, including Grand Bahama. The varied colors of these banks suggest their surfaces are somewhat uneven. The banks' distinct contours, sharply outlined in dark blue, indicate that the ocea

PIX4672775

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

PIX4653092

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

PIX4582252

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP692759

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662357

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662359

Temple of Zeus Olympios

Temple of Zeus Olympios

SAP662361

Temple of Artemis

Temple of Artemis

SAP694635

Church of Virgin Mary (Council Church)

Church of Virgin Mary (Council Church)

SAP693776

Church of Virgin Mary (Council Church)

Church of Virgin Mary (Council Church)

SAP693778

Sarcosuchus & crocodiles compared - The Sarcosuchus or Sarcosuchus imperator was a reptile of the order of crocodilians that was between 11 and 14 metres long and weighed nearly 10 tonnes. He lived about 110 million years ago in the cretace. It was one of the biggest crocodiles that existed on Earth. It is here compared to a Crocodylus porosus, on the left, and a Gavialis gangeticus, on the right. An adult crocodyliform reptile of the genus Sarcosuchus from 110 million years ago is compared to a modern saltwater crocodile (Crocodylus porosus) on the left and a modern gharial (Gavialis gangeticus) on the right. The Sarcosuchus is about 40 feet long and weighs 10 tons* while the saltwater crocodile is 20 feet long and weighs 2 tons and the gharial is 20 feet long and weighs about 350 pounds The saltwater crocodile is currently the largest of all living reptiles, as well as the largest terrestrial and riparian predator in the world, while the gharial, aka fish-eating crocodile, is the lon

Sarcosuchus & crocodiles compared - The Sarcosuchus or Sarcosuchus imperator was a reptile of the order of crocodilians that was between 11 and 14 metres long and weighed nearly 10 tonnes. He lived about 110 million years ago in the cretace. It was one of the biggest crocodiles that existed on Earth. It is here compared to a Crocodylus porosus, on the left, and a Gavialis gangeticus, on the right. An adult crocodyliform reptile of the genus Sarcosuchus from 110 million years ago is compared to a modern saltwater crocodile (Crocodylus porosus) on the left and a modern gharial (Gavialis gangeticus) on the right. The Sarcosuchus is about 40 feet long and weighs 10 tons* while the saltwater crocodile is 20 feet long and weighs 2 tons and the gharial is 20 feet long and weighs about 350 pounds The saltwater crocodile is currently the largest of all living reptiles, as well as the largest terrestrial and riparian predator in the world, while the gharial, aka fish-eating crocodile, is the lon

Walter B Myers

PIX4662477

Chimborazo - Chimborazo and Milky Way - The lactee road over the Chimborazo volcano (6268 metres) in Ecuador. Mosaic of 28 images. With an altitude of 6268 meters (20564 ft) above sea level, Chimborazo volcano is the highest summit in Ecuador but of course not the highest summit on the planet. This record belongs to Mount Everest (8848 metres/29029 ft above sea level). However, because the Earth is not a perfect sphere but rather an oblate spheroid (a sphere flattened along the axis from pole to pole such that there is a bulge around the equator) and that Chimborazo is very close to the equator line (only -1 degree in latitude), Chimborazo is known as the “” the farthest location from the center of the Earth”. 6384.687 Km against 6382.467 Km for Everest that is, a difference of 2.220 Km/1.38 miles. The image is a mosaic of 28 images in order to cover all the sky with a 35 mm focal length lens. The exposure time for each image is only 15 seconds with a modified Canon 5Dii camera. The au

Chimborazo - Chimborazo and Milky Way - The lactee road over the Chimborazo volcano (6268 metres) in Ecuador. Mosaic of 28 images. With an altitude of 6268 meters (20564 ft) above sea level, Chimborazo volcano is the highest summit in Ecuador but of course not the highest summit on the planet. This record belongs to Mount Everest (8848 metres/29029 ft above sea level). However, because the Earth is not a perfect sphere but rather an oblate spheroid (a sphere flattened along the axis from pole to pole such that there is a bulge around the equator) and that Chimborazo is very close to the equator line (only -1 degree in latitude), Chimborazo is known as the “” the farthest location from the center of the Earth”. 6384.687 Km against 6382.467 Km for Everest that is, a difference of 2.220 Km/1.38 miles. The image is a mosaic of 28 images in order to cover all the sky with a 35 mm focal length lens. The exposure time for each image is only 15 seconds with a modified Canon 5Dii camera. The au

Stephane Guisard

PIX4636564

Malaspina Glacier, Alaska. 08/1989 - Malaspina Glacier, Alaska, U.S.A. August 1989 - Malaspina Glacier, Alaska, observes from Space Shuttle Columbia. Malaspina Glacier can be seen just left of the center of this northeast - looking, low - oblique photograph. Located in southern Alaska on the shore of the Gulf of Alaska, Malaspina Glacier is a classic example of a piedmont glacier lying at the foot of a mountain range - - in this case, the Saint Elias Mountains (just north of the glacier). The glacier covers an area of 1500 square miles (3900 square kilometers) on the coastal plain, is almost 60 miles (97 kilometers) long, and is more than 1000 feet (300 meters) thick. The Seward Ice Field is the main source of ice for the glacier. The glacier moves in surges that push earlier - formed moraines outward into expanding concentric patterns, which you can see along the flanks of the ice mass. To the northwest of Malaspina Glacier is the curved and pointed Agassiz Glacier, which is also fed

Malaspina Glacier, Alaska. 08/1989 - Malaspina Glacier, Alaska, U.S.A. August 1989 - Malaspina Glacier, Alaska, observes from Space Shuttle Columbia. Malaspina Glacier can be seen just left of the center of this northeast - looking, low - oblique photograph. Located in southern Alaska on the shore of the Gulf of Alaska, Malaspina Glacier is a classic example of a piedmont glacier lying at the foot of a mountain range - - in this case, the Saint Elias Mountains (just north of the glacier). The glacier covers an area of 1500 square miles (3900 square kilometers) on the coastal plain, is almost 60 miles (97 kilometers) long, and is more than 1000 feet (300 meters) thick. The Seward Ice Field is the main source of ice for the glacier. The glacier moves in surges that push earlier - formed moraines outward into expanding concentric patterns, which you can see along the flanks of the ice mass. To the northwest of Malaspina Glacier is the curved and pointed Agassiz Glacier, which is also fed

PIX4672451

America, mexico, zacatecas, malpaso valley,pre hispanic, archaeological site la quemada, salon de las columnas, columns hall. this 41 by 32 metre enclosure, probably reached a height of more than five metres before the fire that caused its destruction. in their interior eleven columns supported the roof. until now its specific function is not known. although works made in the 1950s indicate a ceremonial use possibly related to human sacrifice.it is supposed that this place could be the legendary chicomostoc, a caxcan site, a teotihuacan fortress, a purepecha centre, a fort against chichimeca intruders, a toltec trading post, or simply consequence of independent development and a city of all the native groups established north of the rio grande de santiago

America, mexico, zacatecas, malpaso valley,pre hispanic, archaeological site la quemada, salon de las columnas, columns hall. this 41 by 32 metre enclosure, probably reached a height of more than five metres before the fire that caused its destruction. in their interior eleven columns supported the roof. until now its specific function is not known. although works made in the 1950s indicate a ceremonial use possibly related to human sacrifice.it is supposed that this place could be the legendary chicomostoc, a caxcan site, a teotihuacan fortress, a purepecha centre, a fort against chichimeca intruders, a toltec trading post, or simply consequence of independent development and a city of all the native groups established north of the rio grande de santiago

Charles Mahaux

AGF5457155

Dilini (8 years old) lies on a bed in surgical ward for children in Matara General Hospital in Southern Sri Lanka. Dilini and her older sister Nadisa with their parents were waiting at Matara Bus Terminal for a bus, only meters from the sea, to go to their home village for the new-year holidays, when first wave came. They were hit by tsunami water that destroyed everything around. Many were trapped at the Matara Bus Terminal and died when furniture, luggage and even big busses were tossed around by water. Nadisha, Dilina and their mother Malkanti were found in three different places and were eventually taken to the hospital for their injuries. Over two week now, they are still in the hospital receiving treatment. Nadishas sister and father died. Surgical ward, Matara General Hospital. Southern Sri Lanka. (photo)

Dilini (8 years old) lies on a bed in surgical ward for children in Matara General Hospital in Southern Sri Lanka. Dilini and her older sister Nadisa with their parents were waiting at Matara Bus Terminal for a bus, only meters from the sea, to go to their home village for the new-year holidays, when first wave came. They were hit by tsunami water that destroyed everything around. Many were trapped at the Matara Bus Terminal and died when furniture, luggage and even big busses were tossed around by water. Nadisha, Dilina and their mother Malkanti were found in three different places and were eventually taken to the hospital for their injuries. Over two week now, they are still in the hospital receiving treatment. Nadishas sister and father died. Surgical ward, Matara General Hospital. Southern Sri Lanka. (photo)

UIG797727

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Rainer Krack

PFH2635904

Malaysia / China: Carving of Mei Bo, depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

Malaysia / China: Carving of Mei Bo, depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

PFH3277868

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Rainer Krack

PFH2635990

Feet With Rings Of A Just Married Man Surrounded By Rose Petals At His Wedding In Trichy, India, 2008 (photo)

Feet With Rings Of A Just Married Man Surrounded By Rose Petals At His Wedding In Trichy, India, 2008 (photo)

Eric Lafforgue

LFG7355783

A view taken on the Clifton Suspension Bridge, looking east towards the Clifton Observatory, showing pedestrians on either side of the road, and a detailed look at the central span chains, Clifton Suspension Bridge, Clifton, City Of Bristol, City Of Bristol, City Of Bristol, UK, c. 1955-c.1980 (b/w photo)

A view taken on the Clifton Suspension Bridge, looking east towards the Clifton Observatory, showing pedestrians on either side of the road, and a detailed look at the central span chains, Clifton Suspension Bridge, Clifton, City Of Bristol, City Of Bristol, City Of Bristol, UK, c. 1955-c.1980 (b/w photo)

EHT5055570

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

PIX4675641

Nepal: Two schoolgirls stand in front of a door at the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Nepal: Two schoolgirls stand in front of a door at the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Chaweewan Chuchuay

PFH2635903

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Nepal: A courtyard in the Pujari Math (formerly living quarters for Hindu priests and now the Woodcarving Museum), Tachupal Tol, or Dattatreya Square, Bhaktapur, Kathmandu Valley (1997)

Rainer Krack

PFH2635905

The yacht of Roman Abramowitsch

The yacht of Roman Abramowitsch

IMO2119802

German prisoners of war captured during the battle of the Menin Road, 1917 (b/w photo)

German prisoners of war captured during the battle of the Menin Road, 1917 (b/w photo)

Unknown photographer, (20th century)

NAM5921668

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Team with a 6.5 m mirror, he will observe the universe mainly in infrared - Six of the 18 James Webb Space Telescope mirror segments are being moved into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors: Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2018. Team with a 6.5 m mirror, he will observe the universe mainly in infrared - Six of the 18 James Webb Space Telescope mirror segments are being moved into the X-ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling -414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X-ray & Cryogenic Facility is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb

PIX4645800

Deities Carved on Rriver Rocks, Kabal Spean, Cambodia (photo)

Deities Carved on Rriver Rocks, Kabal Spean, Cambodia (photo)

Sergi Reboredo

SRB1202753

Aerial view of the Victoria Falls, Zambia (photo)

Aerial view of the Victoria Falls, Zambia (photo)

Sergi Reboredo

SRB1202558

Deane Adams .50 inch percussion revolver, c.1852 (revolver, percussion, Deane Adams, .50 in improved self-cocking)

Deane Adams .50 inch percussion revolver, c.1852 (revolver, percussion, Deane Adams, .50 in improved self-cocking)

English School, (19th century)

NAM5930104

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

PIX4616152

Mars - View of the north pole - Mars north pole - Image of a portion of the northern polar cap of Mars obtained by the Mars Express probe on May 17, 2010. This image was acquired by the Mars Express High - Resolution Stereo Camera on 17 May 2010 and shows a part of the northern polar region of Mars at the northern hemisphere summer solstice. The polar ice deposits follow the seasonal cycles. Studies made by Mars Express's OMEGA instrument shows that the cap is covered by frozen water and carbon dioxide ice in winter and spring but by this point in the martian year all of the carbon dioxide ice has warmed and evaporated into the planet's atmosphere. Only water ice is left behind, which shows up as bright white areas in this picture. From these layers, large bursts of water vapour are occasionally released into the atmosphere. In winter, part of the atmosphere recondenses as frost and snow on the northern cap. These seasonal deposits can extend as far south as 45* N latitude and be up to

Mars - View of the north pole - Mars north pole - Image of a portion of the northern polar cap of Mars obtained by the Mars Express probe on May 17, 2010. This image was acquired by the Mars Express High - Resolution Stereo Camera on 17 May 2010 and shows a part of the northern polar region of Mars at the northern hemisphere summer solstice. The polar ice deposits follow the seasonal cycles. Studies made by Mars Express's OMEGA instrument shows that the cap is covered by frozen water and carbon dioxide ice in winter and spring but by this point in the martian year all of the carbon dioxide ice has warmed and evaporated into the planet's atmosphere. Only water ice is left behind, which shows up as bright white areas in this picture. From these layers, large bursts of water vapour are occasionally released into the atmosphere. In winter, part of the atmosphere recondenses as frost and snow on the northern cap. These seasonal deposits can extend as far south as 45* N latitude and be up to

PIX4616313

Greek Agora, Bases of the Eponymous Hero

Greek Agora, Bases of the Eponymous Hero

SAP780899

Greek Agora, Odeon of Agrippa

Greek Agora, Odeon of Agrippa

SAP780978

Repulsing the Famous Prussian Guard at Ypres, 1914 (photogravure)

Repulsing the Famous Prussian Guard at Ypres, 1914 (photogravure)

Matania, Fortunino (1881-1963) (after)

NAM5926167

Deane Adams .50 inch percussion revolver, c.1852 (revolver, percussion, Deane Adams, .50 in improved self-cocking)

Deane Adams .50 inch percussion revolver, c.1852 (revolver, percussion, Deane Adams, .50 in improved self-cocking)

English School, (19th century)

NAM5930103

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

Greek Agora, Odeon of Agrippa

Greek Agora, Odeon of Agrippa

SAP780931

Greek Agora, Bases of the Eponymous Hero

Greek Agora, Bases of the Eponymous Hero

SAP780952

Greek Agora, Odeon of Agrippa

Greek Agora, Odeon of Agrippa

SAP780894

Sepoy Ali Haidar VC (right) at the Frontier Force Rifles depot, Abbottabad, 13 August 1945 (b/w photo)

Sepoy Ali Haidar VC (right) at the Frontier Force Rifles depot, Abbottabad, 13 August 1945 (b/w photo)

Unknown photographer, (20th century)

NAM5923536

Sepoy Ali Haidar VC, 13th Frontier Force Rifles, 13 August 1945 (b/w photo)

Sepoy Ali Haidar VC, 13th Frontier Force Rifles, 13 August 1945 (b/w photo)

Unknown photographer, (20th century)

NAM5923535

The Shanghai World Financial Center, Shanghai, China (photo)

The Shanghai World Financial Center, Shanghai, China (photo)

Sergi Reboredo

SRB1202611

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

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

PIX4625061

March - Spirit - View during the descent of Husband Hill. 11/2005 - Martian surface seen from the rover Spirit. 11/2005 - Panorama of 360 degres obtained by Spirit from 23 to 28 November 2005. The summit of Husband Hill rises 100 m above the surrounding plateau. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. In late November 2005 while descending “” Husband Hill,””” Nasa's Mars Exploration Rover Spirit took the most detailed panorama so far of the “” Inner Basin,”” the rover's next target destination. Spirit acquired the 405 individual images that make up this 360 - degree view of the surrounding terrain using five different filters on the panoramic camera. The rover took the images on Martian days, or sols, 672 to 677 (Nov. 23 to 28, 2005). Spirit acquired this more oblique view, known as the “” Seminole panorama,”” from about halfway down the south flank of Husband Hill, 50 meters (164 feet) or so below the summit. Near the center of the panorama, on the ho

March - Spirit - View during the descent of Husband Hill. 11/2005 - Martian surface seen from the rover Spirit. 11/2005 - Panorama of 360 degres obtained by Spirit from 23 to 28 November 2005. The summit of Husband Hill rises 100 m above the surrounding plateau. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. In late November 2005 while descending “” Husband Hill,””” Nasa's Mars Exploration Rover Spirit took the most detailed panorama so far of the “” Inner Basin,”” the rover's next target destination. Spirit acquired the 405 individual images that make up this 360 - degree view of the surrounding terrain using five different filters on the panoramic camera. The rover took the images on Martian days, or sols, 672 to 677 (Nov. 23 to 28, 2005). Spirit acquired this more oblique view, known as the “” Seminole panorama,”” from about halfway down the south flank of Husband Hill, 50 meters (164 feet) or so below the summit. Near the center of the panorama, on the ho

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March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

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March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

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Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585215

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