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This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

UIG866228

China: Livestock market and bazaar in Shufu County near Kashgar, Xinjiang Province

China: Livestock market and bazaar in Shufu County near Kashgar, Xinjiang Province

David Henley

PFH4072212

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

PFH1773939

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

PFH1773940

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

PFH1773942

Bristol Docks with St Mary Redcliffe Church beyond

Bristol Docks with St Mary Redcliffe Church beyond

English School, (19th century)

USB1160061

China: A variety of powders, pigments and minerals used for making dyes at a market in the Old Town, Kashgar, Xinjiang Province (photo)

China: A variety of powders, pigments and minerals used for making dyes at a market in the Old Town, Kashgar, Xinjiang Province (photo)

PFH5302807

Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon

Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon

Walter B Myers

PIX4575211

The banded iron formations exposed in this sedimentary rock, originated more than 2..., 2000 (photo)

premium — The banded iron formations exposed in this sedimentary rock, originated more than 2..., 2000 (photo)

The banded iron formations exposed in this sedimentary rock, originated more than 2..., 2000 (photo)

Wolinsky, Cary (1947-2023)

CWO8718989

Map of Mecca - 19th century

Map of Mecca - 19th century

Unknown Artist, (19th century)

Giancarlo Costa

GIA4755660

The boiler room of HMS Kelly after the torpedo damage, Hawthorn Leslie Yard, Hebburn on Tyne, UK, 1940 (b/w photo)

The boiler room of HMS Kelly after the torpedo damage, Hawthorn Leslie Yard, Hebburn on Tyne, UK, 1940 (b/w photo)

TW3661077

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

PFH1773938

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

Wales / UK: Alfred Russel Wallace, British naturalist, explorer, geographer, anthropologist and biologist (1823-1913)

PFH1773943

Ireland, True Colour Satellite Image. Ireland. True-colour satellite image of Ireland. North is at top. The island's main cities are Dublin (centre right) and Belfast (upper right). Ireland is often called the """"Emerald Isle"""" because of the vivid greenness of its countryside ; this is largely due to the warm, wet winds from the Atlantic Ocean to the West. Topographically, the island is shaped like a basin, having lowlands in its centre & hilly ranges around its coastline. Ireland has many lakes, including the largest in the British Isles, Lough Neagh (at upper right). The longest river in the British Isles, the Shannon, empties into a long, narrow estuary at lower left. Image taken by the Landsat-5 satellite ©Planet Observer/UIG/Leemage

Ireland, True Colour Satellite Image. Ireland. True-colour satellite image of Ireland. North is at top. The island's main cities are Dublin (centre right) and Belfast (upper right). Ireland is often called the """"Emerald Isle"""" because of the vivid greenness of its countryside ; this is largely due to the warm, wet winds from the Atlantic Ocean to the West. Topographically, the island is shaped like a basin, having lowlands in its centre & hilly ranges around its coastline. Ireland has many lakes, including the largest in the British Isles, Lough Neagh (at upper right). The longest river in the British Isles, the Shannon, empties into a long, narrow estuary at lower left. Image taken by the Landsat-5 satellite ©Planet Observer/UIG/Leemage

UIG5421004

The first Battle of Schooneveld, 28 May 1673, 1684 (pen, grisaille on canvas)

The first Battle of Schooneveld, 28 May 1673, 1684 (pen, grisaille on canvas)

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

MMM7337621

Princess Juliena Airport on the island of Saint Martin 2007

Princess Juliena Airport on the island of Saint Martin 2007

IMO2122551

Houston Training Pool - NBL facilities (Neutral Buoyancy Laboratory) - The Houston Pool (Neutral Buoyancy Laboratory) is used for astronaut training. Measuring 60 metres long, 30 metres wide and 12 metres deep, this basin hosts models of the International Space Station modules allowing astronauts to train in a state close to weightlessness on their future outings into space. The Neutral Buoyancy Laboratory pool at Nasa's Johnson Space Center in Houston, Texas, where astronauts, wearing a 65 - kg Extravehicular Mobility Unit (EMU) spacesuit, practice spacewalking and working outside the International Space Station during underwater simulated extravehicular activities (EVAs). This facility consists in a 60 - m - long, 30 - m - wide and 12 - m - deep water reservoir, with a capacity of 23,500 cubic meters. Two overhead bridge cranes are used to display mock space station modules for training. The spacesuit buoyancy provides a simulated weightlessness for astronaut trainees. Most ESA astro

Houston Training Pool - NBL facilities (Neutral Buoyancy Laboratory) - The Houston Pool (Neutral Buoyancy Laboratory) is used for astronaut training. Measuring 60 metres long, 30 metres wide and 12 metres deep, this basin hosts models of the International Space Station modules allowing astronauts to train in a state close to weightlessness on their future outings into space. The Neutral Buoyancy Laboratory pool at Nasa's Johnson Space Center in Houston, Texas, where astronauts, wearing a 65 - kg Extravehicular Mobility Unit (EMU) spacesuit, practice spacewalking and working outside the International Space Station during underwater simulated extravehicular activities (EVAs). This facility consists in a 60 - m - long, 30 - m - wide and 12 - m - deep water reservoir, with a capacity of 23,500 cubic meters. Two overhead bridge cranes are used to display mock space station modules for training. The spacesuit buoyancy provides a simulated weightlessness for astronaut trainees. Most ESA astro

S. Corvaja

PIX4650176

Adriace bay, Lycia, Turkey

Adriace bay, Lycia, Turkey

SAP694690

Brother Carlo Saving the Head of Ulysses, 2011 (oil on canvas)

premium — Brother Carlo Saving the Head of Ulysses, 2011 (oil on canvas)

Brother Carlo Saving the Head of Ulysses, 2011 (oil on canvas)

DRN3090562

Adriace bay, Lycia, Turkey

Adriace bay, Lycia, Turkey

SAP694689

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

PIX4614997

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

Ireland, True Colour Satellite Image With Mask. Ireland. True colour satellite image of Ireland, with mask. North is at top. The island's main cities are Dublin (centre right) and Belfast (upper right). Ireland is often called the """"Emerald Isle"""" because of the vivid greenness of its countryside ; this is largely due to the warm, wet winds from the Atlan- tic Ocean to the West. Topographically, the island is shaped like a basin, having lowlands in its centre & hilly ranges around its coastline. Ireland has many lakes, including the largest in the British Isles, Lough Neagh (at upper right). The longest river in the British Isles, the Shannon, empties into a long, narrow estuary at lower left. Image taken by the Landsat-5 satellite ©Planet Observer/UIG/Leemage

Ireland, True Colour Satellite Image With Mask. Ireland. True colour satellite image of Ireland, with mask. North is at top. The island's main cities are Dublin (centre right) and Belfast (upper right). Ireland is often called the """"Emerald Isle"""" because of the vivid greenness of its countryside ; this is largely due to the warm, wet winds from the Atlan- tic Ocean to the West. Topographically, the island is shaped like a basin, having lowlands in its centre & hilly ranges around its coastline. Ireland has many lakes, including the largest in the British Isles, Lough Neagh (at upper right). The longest river in the British Isles, the Shannon, empties into a long, narrow estuary at lower left. Image taken by the Landsat-5 satellite ©Planet Observer/UIG/Leemage

UIG5421010

South America, True Colour Satellite Image. South America. True colour satellite image centred on South America. North is at top. Water is blue, arid areas are brown, vegetation is green, and snow and ice are white. The terrain of South America is marked by the Andes mountains along the western coast, tropical rainforests (dark green) in the Amazon river basin in the north, and swamps and plains (lighter green) in the south. Surrounding South America (clockwise from upper left) is part of Central America, the islands of the Caribbean, the Atlantic Ocean (right) and the Pacific Ocean (left). A small part of Antarctica is at bottom centre. The image used data from LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

South America, True Colour Satellite Image. South America. True colour satellite image centred on South America. North is at top. Water is blue, arid areas are brown, vegetation is green, and snow and ice are white. The terrain of South America is marked by the Andes mountains along the western coast, tropical rainforests (dark green) in the Amazon river basin in the north, and swamps and plains (lighter green) in the south. Surrounding South America (clockwise from upper left) is part of Central America, the islands of the Caribbean, the Atlantic Ocean (right) and the Pacific Ocean (left). A small part of Antarctica is at bottom centre. The image used data from LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5420997

Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

PIX4630745

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

PIX4616154

An Unknown Man and a Boy (formerly said to be Sir Henry Arundell Bedingfeld, 3rd Bt (1689-1760) as a Boy with his Tutor Thomas Marwood (d.1718))

An Unknown Man and a Boy (formerly said to be Sir Henry Arundell Bedingfeld, 3rd Bt (1689-1760) as a Boy with his Tutor Thomas Marwood (d.1718))

USB1157757

Tikal - Temple V and the constellation Orion - Tikal - Orion constellation above Temple V - Temple V was built around 700, and rises to 57 meters high. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. Temple V stands south of the Central Acropolis and is the mortuary pyramid of an as yet unidentified ruler. The temple stands 57 meters (187 ft) high, making it the second tallest structure at Tikal - only Temple IV is taller. The temple has been dated to about AD 700, in the Late Classic period, via radiocarbon analysis and the dating of ceramics associated with the structure places its construction during the reign of Nun Bak Chak in the second half of the 7th century. Tikal (or Tik'al according to the modern Mayan orthography) is one of the largest archaeological sites and urban centres

Tikal - Temple V and the constellation Orion - Tikal - Orion constellation above Temple V - Temple V was built around 700, and rises to 57 meters high. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. Temple V stands south of the Central Acropolis and is the mortuary pyramid of an as yet unidentified ruler. The temple stands 57 meters (187 ft) high, making it the second tallest structure at Tikal - only Temple IV is taller. The temple has been dated to about AD 700, in the Late Classic period, via radiocarbon analysis and the dating of ceramics associated with the structure places its construction during the reign of Nun Bak Chak in the second half of the 7th century. Tikal (or Tik'al according to the modern Mayan orthography) is one of the largest archaeological sites and urban centres

Stephane Guisard

PIX4673092

Miss Elsie (Elspeth) Thomson, later Mrs Kenneth Grahame, 1881 (oil on canvas)

Miss Elsie (Elspeth) Thomson, later Mrs Kenneth Grahame, 1881 (oil on canvas)

Dicksee, Frank (1853-1928)

USB1157627

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965909

China: The steps leading to the summit near Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The steps leading to the summit near Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965910

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965919

Globe South America, True Colour Satellite Image. Earth. True colour satellite image of the Earth, centred on South America. North is at top. Water is blue, vegetation is green, arid areas are brown, and snow and ice are white. Both land and ocean floor topography are shown. The terrain of South America is marked by the Andes mountains along the western coast, tropical rainforests (dark green) in the Amazon river basin in the north, and swamps and plains (lighter green) in the south. Surrounding South America (clockwise from upper left) is North America and the Caribbean islands, the Atlantic Ocean (right) and the Pacific Ocean (left). Parts of Greenland, Europe, Africa and Antarctica are also seen on the edges of the globe. The image used data from LANDSAT 5 & 7 satellites. Print size 42x42cm ©Planet Observer/UIG/Leemage

Globe South America, True Colour Satellite Image. Earth. True colour satellite image of the Earth, centred on South America. North is at top. Water is blue, vegetation is green, arid areas are brown, and snow and ice are white. Both land and ocean floor topography are shown. The terrain of South America is marked by the Andes mountains along the western coast, tropical rainforests (dark green) in the Amazon river basin in the north, and swamps and plains (lighter green) in the south. Surrounding South America (clockwise from upper left) is North America and the Caribbean islands, the Atlantic Ocean (right) and the Pacific Ocean (left). Parts of Greenland, Europe, Africa and Antarctica are also seen on the edges of the globe. The image used data from LANDSAT 5 & 7 satellites. Print size 42x42cm ©Planet Observer/UIG/Leemage

UIG5421007

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

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965915

China: A statue to the two Uighur lovers, Princess Tzuhola and her lover, the shepherd Tayir near the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: A statue to the two Uighur lovers, Princess Tzuhola and her lover, the shepherd Tayir near the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965912

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965916

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965917

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The tomb of Princess Tzuhola and her lover, the shepherd Tayir, at the summit of the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965914

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The narrow artery that forced all travellers into the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965918

1994 Northridge California earthquake, USA, Part2

1994 Northridge California earthquake, USA, Part2

BOF3281680

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965907

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The harsh, crumbling mountains surrounding Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965908

China: The steps leading to the summit near Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: The steps leading to the summit near Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965911

China: A statue to the two Uighur lovers, Princess Tzuhola and her lover, the shepherd Tayir near the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

China: A statue to the two Uighur lovers, Princess Tzuhola and her lover, the shepherd Tayir near the Tiemenguan (The Iron Gate Pass), the ancient strategic strongpoint controlling the Silk Road near Korla, Xinjiang Province (photo)

PFH2965913

Trukkee, 28th February 1845, an incident during Sir Charles Napiers Hill campaign in Baluchistan, 1845 (oil on board)

Trukkee, 28th February 1845, an incident during Sir Charles Napiers Hill campaign in Baluchistan, 1845 (oil on board)

English School, (19th century)

NAM5929032

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

PIX4625574

Mars - View of the south pole - Mars South pole - Image of part of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. While it looks smooth in this image, at close quarters the cap is a layered mix of peaks, troughs and flat plains, and has been likened in appearance to swiss cheese. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. The cap is around 150 km north of Mars' geographical south pole and Mars Express has shed light on why this ice cap is displaced. Deep impact craters - notably the Hellas Basin, the largest impact structure on the entire planet at 7 km deep and 2300 km across - funne

Mars - View of the south pole - Mars South pole - Image of part of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. While it looks smooth in this image, at close quarters the cap is a layered mix of peaks, troughs and flat plains, and has been likened in appearance to swiss cheese. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. The cap is around 150 km north of Mars' geographical south pole and Mars Express has shed light on why this ice cap is displaced. Deep impact craters - notably the Hellas Basin, the largest impact structure on the entire planet at 7 km deep and 2300 km across - funne

PIX4616189

A typical British passenger locomotive.

A typical British passenger locomotive.

UIG5308492

Ocean level rise - West Hemisphere - Earth's Western hemisphere with sea level+100m - Artist's view showing North and South America as they would appear if ocean levels increased by 100 metres. This would happen if all glaciers on Earth melt. This is how the Earth's Western hemisphere may appear with mean sea level about 100 meters (330 feet) above today's. Such a dramatic rise in sea level could occur if all of the Earth's glaciers were to melt. In this image the Gulf of Mexico and Atlantic ocean have inundated almost all of southeastern United State including the entire state of Florida, almost all of Louisiana, and significant portions of the other southeastern states and the District of Columbia. Major US cities submerged include New York City, Boston, and Houston, and on the west coast Los Angeles, San Francisco, and much of San Diego. In addition to land claimed from the United States this 100 meter rise in sea level has also claimed much of Central America including the Yucatan

Ocean level rise - West Hemisphere - Earth's Western hemisphere with sea level+100m - Artist's view showing North and South America as they would appear if ocean levels increased by 100 metres. This would happen if all glaciers on Earth melt. This is how the Earth's Western hemisphere may appear with mean sea level about 100 meters (330 feet) above today's. Such a dramatic rise in sea level could occur if all of the Earth's glaciers were to melt. In this image the Gulf of Mexico and Atlantic ocean have inundated almost all of southeastern United State including the entire state of Florida, almost all of Louisiana, and significant portions of the other southeastern states and the District of Columbia. Major US cities submerged include New York City, Boston, and Houston, and on the west coast Los Angeles, San Francisco, and much of San Diego. In addition to land claimed from the United States this 100 meter rise in sea level has also claimed much of Central America including the Yucatan

Walter B Myers

PIX4633147

Tikal - The Pyramid of the Lost World and the constellation Orion - Tikal - Orion constellation above Mundo Perdido Temple - 30 m tall, the Pyramid of the Lost World (Structure 5C - 54) constituted the largest edifice of Tikal until the seventh century. It is located in the south-west part of the central core of Tikal, south of Temple III and west of Temple V. The pyramid forms, with three small buildings located to the east, an Ensemble E which would have had astronomical significance. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. The Lost World Pyramid (Structure 5C - 54) lies in the southwest portion of Tikal's central core, south of Temple III and west of Temple V. It was decorated with stucco masks of the sun god and dates to the Late Preclassic; this pyramid is part of an enclos

Tikal - The Pyramid of the Lost World and the constellation Orion - Tikal - Orion constellation above Mundo Perdido Temple - 30 m tall, the Pyramid of the Lost World (Structure 5C - 54) constituted the largest edifice of Tikal until the seventh century. It is located in the south-west part of the central core of Tikal, south of Temple III and west of Temple V. The pyramid forms, with three small buildings located to the east, an Ensemble E which would have had astronomical significance. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. The Lost World Pyramid (Structure 5C - 54) lies in the southwest portion of Tikal's central core, south of Temple III and west of Temple V. It was decorated with stucco masks of the sun god and dates to the Late Preclassic; this pyramid is part of an enclos

Stephane Guisard

PIX4673089

Tikal - The Pyramid of the Lost World and the constellation Orion - Tikal - Orion constellation above Mundo Perdido Temple - 30 m tall, the Pyramid of the Lost World (Structure 5C - 54) constituted the largest edifice of Tikal until the seventh century. It is located in the south-west part of the central core of Tikal, south of Temple III and west of Temple V. The pyramid forms, with three small buildings located to the east, an Ensemble E which would have had astronomical significance. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. The Lost World Pyramid (Structure 5C - 54) lies in the southwest portion of Tikal's central core, south of Temple III and west of Temple V. It was decorated with stucco masks of the sun god and dates to the Late Preclassic; this pyramid is part of an enclos

Tikal - The Pyramid of the Lost World and the constellation Orion - Tikal - Orion constellation above Mundo Perdido Temple - 30 m tall, the Pyramid of the Lost World (Structure 5C - 54) constituted the largest edifice of Tikal until the seventh century. It is located in the south-west part of the central core of Tikal, south of Temple III and west of Temple V. The pyramid forms, with three small buildings located to the east, an Ensemble E which would have had astronomical significance. Tikal (or Tik'al according to modern Mayan spelling) is one of the largest archaeological sites and urban centers of the Mayan precolombian civilization. Located in what is now northern Guatemala, it was declared a UNESCO World Heritage Site in 1979. The Lost World Pyramid (Structure 5C - 54) lies in the southwest portion of Tikal's central core, south of Temple III and west of Temple V. It was decorated with stucco masks of the sun god and dates to the Late Preclassic; this pyramid is part of an enclos

Stephane Guisard

PIX4673091

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

PIX4625616

Lakes of Nayriz, Iran, seen by satellite - Neyriz Lakes, Iran - In southern Iran's Fars province, the lakes of Bakhtegan and Tashk, better known as lakes of Nayriz “” appear on this image taken by ALOS, a four-ton Japanese observation satellite. Lake Bakhtegan (central) and Lake Tashk (upper), located in the Nayriz basin, are dirty lakes in the south-east of the Zagros Mountains, whose water levels fluctuate with rain and snow in the mountains. Lake Bakhtegan, the second largest lake in Iran, is fed mainly by the Kour River, while Lake Tashk receives the overflow from the marecages at its western extremite and from an important permanent north-west source. Although normally separated by narrow strips of land, during the years of heavy rain they can join and form only one lake. Similarly, after several years of low rains, as in 1934 and 1971, the lakes can be completely low except for the points closest to the springs. The two lakes, their delta and the morecages associated with the spr

Lakes of Nayriz, Iran, seen by satellite - Neyriz Lakes, Iran - In southern Iran's Fars province, the lakes of Bakhtegan and Tashk, better known as lakes of Nayriz “” appear on this image taken by ALOS, a four-ton Japanese observation satellite. Lake Bakhtegan (central) and Lake Tashk (upper), located in the Nayriz basin, are dirty lakes in the south-east of the Zagros Mountains, whose water levels fluctuate with rain and snow in the mountains. Lake Bakhtegan, the second largest lake in Iran, is fed mainly by the Kour River, while Lake Tashk receives the overflow from the marecages at its western extremite and from an important permanent north-west source. Although normally separated by narrow strips of land, during the years of heavy rain they can join and form only one lake. Similarly, after several years of low rains, as in 1934 and 1971, the lakes can be completely low except for the points closest to the springs. The two lakes, their delta and the morecages associated with the spr

PIX4660585

Martian surface seen by Spirit in 2008 - Martian surface seen from the rover Spirit in 2008 - 360 degres panorama obtained by the Martian rover Spirit from February 28 to October 5, 2008. The 246 images that make up this panorama were taken from a tray called the Home Plate. The hill has the horizon on the right is Husband Hill. The hill on the left is McCool Hill. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Spirit has spent its third Martian southern - hemisphere winter inside Mars' Gusev Crater. The rover's overwintering location is on the northern edge of a low plateau informally called “Home Plate,””” which is about 80 meters or 260 feet in diameter. This view combines 246 different exposures taken with Spirit's panoramic camera (Pancam) - - 82 pointings, with three filters at each pointing. Spirit took the first of these frames during the mission's 1,477th

Martian surface seen by Spirit in 2008 - Martian surface seen from the rover Spirit in 2008 - 360 degres panorama obtained by the Martian rover Spirit from February 28 to October 5, 2008. The 246 images that make up this panorama were taken from a tray called the Home Plate. The hill has the horizon on the right is Husband Hill. The hill on the left is McCool Hill. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Spirit has spent its third Martian southern - hemisphere winter inside Mars' Gusev Crater. The rover's overwintering location is on the northern edge of a low plateau informally called “Home Plate,””” which is about 80 meters or 260 feet in diameter. This view combines 246 different exposures taken with Spirit's panoramic camera (Pancam) - - 82 pointings, with three filters at each pointing. Spirit took the first of these frames during the mission's 1,477th

PIX4615764

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

PIX4625361

President Bill Clinton - Affirmative Action Speech, 1995

President Bill Clinton - Affirmative Action Speech, 1995

BOF6286734

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