'Boundary' Bilder und Clips Suchergebnisse

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Bilder zu 'Boundary' gefunden, 3,055

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Border between Pakistan and India at night: India, on the right and Pakistan (left) seen from the International Space Station (ISS) on September 23, 2015. The border between the two countries is clearly visible at night, illuminated by strong safety bulbs. Karachi is the bright spot at the bottom left of the picture - An astronaut aboard the International Space Station took this nighttime panorama while looking north across Pakistan's Indus River valley. The port city of Karachi is the bright cluster of lights facing the Arabian Sea, which appears completely black. City lights and the dark color of dense agriculture closely track with the great curves of the Indus valley. For scale, the distance from Karachi to the foothills of the Himalaya Mountains is 1,160 kilometers (720 miles) - This photograph shows one of the few places on Earth where an international boundary can be seen at night. The winding border between Pakistan and India is lit by security lights that have a distinct orang

Border between Pakistan and India at night: India, on the right and Pakistan (left) seen from the International Space Station (ISS) on September 23, 2015. The border between the two countries is clearly visible at night, illuminated by strong safety bulbs. Karachi is the bright spot at the bottom left of the picture - An astronaut aboard the International Space Station took this nighttime panorama while looking north across Pakistan's Indus River valley. The port city of Karachi is the bright cluster of lights facing the Arabian Sea, which appears completely black. City lights and the dark color of dense agriculture closely track with the great curves of the Indus valley. For scale, the distance from Karachi to the foothills of the Himalaya Mountains is 1,160 kilometers (720 miles) - This photograph shows one of the few places on Earth where an international boundary can be seen at night. The winding border between Pakistan and India is lit by security lights that have a distinct orang

PIX4661321

March: chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles and Sacra Fossae. To the north, the large impact crater 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 image shows an old 35 km - diameter impact crater in the north. The crater's southwestern rim is eroded strongly, mostly by flowing water. The source of the water was located in Etus Chasma, which lies about 850 km to the southwest. The crater floor and the northwestern part are remarkably flat, formed by sediments and basaltic lava fl

March: chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles and Sacra Fossae. To the north, the large impact crater 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 image shows an old 35 km - diameter impact crater in the north. The crater's southwestern rim is eroded strongly, mostly by flowing water. The source of the water was located in Etus Chasma, which lies about 850 km to the southwest. The crater floor and the northwestern part are remarkably flat, formed by sediments and basaltic lava fl

PIX4616176

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

Iceland, True Colour Satellite Image. Iceland, satellite image. This is a European country surrounded by the northern Atlantic Ocean. It lies just south of the Arctic Circle. Its capital, Reykjavik (in the bay at centre left), is the northernmost in the world. Iceland has a population of around 300,000 (2006). It is situation on a plate boundary and is thus very geologically active. This allows it to derive a large amount of its energy from geothermal sources, which it supplements with hydroelectric power. Together they provide around 99% of the country's energy. Composite image using data from LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Iceland, True Colour Satellite Image. Iceland, satellite image. This is a European country surrounded by the northern Atlantic Ocean. It lies just south of the Arctic Circle. Its capital, Reykjavik (in the bay at centre left), is the northernmost in the world. Iceland has a population of around 300,000 (2006). It is situation on a plate boundary and is thus very geologically active. This allows it to derive a large amount of its energy from geothermal sources, which it supplements with hydroelectric power. Together they provide around 99% of the country's energy. Composite image using data from LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5421292

Portrait, probably of Ayodeya Prasad, brother of Dina Nath, 1845 circa (miniature on ivory)

Portrait, probably of Ayodeya Prasad, brother of Dina Nath, 1845 circa (miniature on ivory)

Unknown Artist, (19th century)

NAM5926804

Cleave Collection 2: Survey of International Frontier between Uganda and Kenya, 1959-1960 (Part 1 of 5)

Cleave Collection 2: Survey of International Frontier between Uganda and Kenya, 1959-1960 (Part 1 of 5)

BRV7424744

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

PIX4615396

The Oberbaum Bridge (Oberbaumbrücke Bridge), Berlin, Germany (photo)

The Oberbaum Bridge (Oberbaumbrücke Bridge), Berlin, Germany (photo)

Sergi Reboredo

SRB1202555

Piyain River is a tributary of the Surma River, and originates from the Umgat river of Assam. The Umgat's source is from the hilly areas of Assam. Flowing south, the river enters Bangladesh through the Sylhet district and branches out into two: the Piyain and the Dauki, also known as Jaflong. After entering Bangladesh, the Piyain follows a 7km route westward along the international boundary and turns southwest to meet the Surma River at Chatak. The total length of the Piyain is about 145 km. As the river is a hilly stream, it often causes flash floods and transports a huge amount of stones from its source area. Goainghat, Jaflong, Sylhet, Bangladesh. October 19, 2007. . (photo)

Piyain River is a tributary of the Surma River, and originates from the Umgat river of Assam. The Umgat's source is from the hilly areas of Assam. Flowing south, the river enters Bangladesh through the Sylhet district and branches out into two: the Piyain and the Dauki, also known as Jaflong. After entering Bangladesh, the Piyain follows a 7km route westward along the international boundary and turns southwest to meet the Surma River at Chatak. The total length of the Piyain is about 145 km. As the river is a hilly stream, it often causes flash floods and transports a huge amount of stones from its source area. Goainghat, Jaflong, Sylhet, Bangladesh. October 19, 2007. . (photo)

UIG795322

Piyain River is a tributary of the Surma River, and originates from the Umgat river of Assam. The Umgat's source is from the hilly areas of Assam. Flowing south, the river enters Bangladesh through the Sylhet district and branches out into two: the Piyain and the Dauki, also known as Jaflong. After entering Bangladesh, the Piyain follows a 7km route westward along the international boundary and turns southwest to meet the Surma River at Chatak. The total length of the Piyain is about 145 km. As the river is a hilly stream, it often causes flash floods and transports a huge amount of stones from its source area. Goainghat, Jaflong, Sylhet, Bangladesh. October 19, 2007. . (photo)

Piyain River is a tributary of the Surma River, and originates from the Umgat river of Assam. The Umgat's source is from the hilly areas of Assam. Flowing south, the river enters Bangladesh through the Sylhet district and branches out into two: the Piyain and the Dauki, also known as Jaflong. After entering Bangladesh, the Piyain follows a 7km route westward along the international boundary and turns southwest to meet the Surma River at Chatak. The total length of the Piyain is about 145 km. As the river is a hilly stream, it often causes flash floods and transports a huge amount of stones from its source area. Goainghat, Jaflong, Sylhet, Bangladesh. October 19, 2007. . (photo)

UIG795325

Kerameikos

Kerameikos

SAP629178

Kerameikos, olive tree

Kerameikos, olive tree

SAP629199

Kerameikos

Kerameikos

SAP692763

Kerameikos

Kerameikos

SAP629180

Kerameikos

Kerameikos

SAP629186

Kerameikos

Kerameikos

SAP629191

Pile carpet, Pazyryk Culture, early Iron Age, 5th - 4th century BC (wool)

Pile carpet, Pazyryk Culture, early Iron Age, 5th - 4th century BC (wool)

XBH2634795

Stela A, Quirigua, 1883 (platinum print)

Stela A, Quirigua, 1883 (platinum print)

Maudslay, Alfred Percival (1850-1931)

PRM479397

Brinton Collection 2: A Sporting Medley, 1939 (Part 3 of 3)

Brinton Collection 2: A Sporting Medley, 1939 (Part 3 of 3)

BAF7424763

Kerameikos, olive tree

Kerameikos, olive tree

SAP629188

Kerameikos

Kerameikos

SAP629224

Kerameikos

Kerameikos

SAP629227

Kerameikos

Kerameikos

SAP629218

Kerameikos

Kerameikos

SAP629220

Kerameikos

Kerameikos

SAP629234

Map of Hampstead. The individual settlements that make up this area of London are shown by red blocks, with boundary lines indicating the fields separating them. Shading and soft interlining indicate relief, neatly illustrated at Primrose Hill, the summit of which is left bare. The barracks at the edge of Hyde Park are illustrated at the very bottom of the map. The dark blue-black line running from West Drayton to Brentford and Paddington is the Grand Junction Canal. This was London's principal link to the rest of Britain's canals, allowing the passage of goods to and from the industrial towns of the North and Midlands. Hyett includes a ground plan of Kenwood House in Hampstead, showing a level of detail much greater than might be expected from a map with a scale of two inches-to-the-mile.

Map of Hampstead. The individual settlements that make up this area of London are shown by red blocks, with boundary lines indicating the fields separating them. Shading and soft interlining indicate relief, neatly illustrated at Primrose Hill, the summit of which is left bare. The barracks at the edge of Hyde Park are illustrated at the very bottom of the map. The dark blue-black line running from West Drayton to Brentford and Paddington is the Grand Junction Canal. This was London's principal link to the rest of Britain's canals, allowing the passage of goods to and from the industrial towns of the North and Midlands. Hyett includes a ground plan of Kenwood House in Hampstead, showing a level of detail much greater than might be expected from a map with a scale of two inches-to-the-mile.

BL3304897

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. A row of houses ablaze on a street in Nihonbashi

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. A row of houses ablaze on a street in Nihonbashi

PFH1773703

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

PFH1773692

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

PFH1773695

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Piles of bodies of those caught in the great fire that swept the city after the quake

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Piles of bodies of those caught in the great fire that swept the city after the quake

PFH1773704

Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

PIX4622776

Elephant Scratching His Head in Chobe River Front, Chobe National Park, Botswana (photo)

Elephant Scratching His Head in Chobe River Front, Chobe National Park, Botswana (photo)

Sergi Reboredo

SRB1202642

Kerameikos

Kerameikos

SAP692663

Kerameikos

Kerameikos

SAP692764

Kerameikos

Kerameikos

SAP629247

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

PFH1773696

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Crowds of refugees struggling to board trains at Nippori Station

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Crowds of refugees struggling to board trains at Nippori Station

PFH1773701

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

PFH1773691

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. The metropolitan police building ablaze

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. The metropolitan police building ablaze

PFH1773693

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923

PFH1773694

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Central Tokyo viewed from the roof of the Imperial Hotel

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Central Tokyo viewed from the roof of the Imperial Hotel

PFH1773699

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Crowds of refugees struggling to board a train to escape the devastation

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. Crowds of refugees struggling to board a train to escape the devastation

PFH1773702

2 St Barnabas' Square, Douglas, Isle of Man, 1932-34 (b/w photo)

2 St Barnabas' Square, Douglas, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5052653

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. View from Tokyo across Yokohama to Tokyo Bay

Japan: Scene of destruction in Tokyo after the Great Kanto Earthquake of 1923. View from Tokyo across Yokohama to Tokyo Bay

PFH1773700

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

PIX4616082

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616090

Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

PIX4630564

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616083

Seneschal Lane, Douglas, Isle of Man, 1932 (b/w photo)

Seneschal Lane, Douglas, Isle of Man, 1932 (b/w photo)

Frowde, John James (1868-1946)

MNX5052739

Panorama of galactic center seen in infrared

Panorama of galactic center seen in infrared

PIX4637943

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036715

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036724

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036716

Glacier Bay, Alaska - Glacier Bay in Alaska - Glacier Bay from perspective. This image is the result of joint observations made by the Landsat-7 satellite in visible and infrared, combined with elevation radar data obtained by the Shuttle Radar Topography Mission (SRTM) in February 2000. At the bottom left of the picture, the Brady Glacier. Glacier Bay National Park and Preserve lies on the Pacific Coast of Alaska south of the St. Elias mountain range. The bay was set aside as a National Monument in 1925 and became its current National Park and Preserve in 1980, when approximately 85 percent of the park was designated a Wilderness Area. It has since been recognized as a UN Biosphere Reserve, in 1986, and a World Heritage Site, in 1992. The water in the foreground in the southwest (bottom left) corner of the image is the Gulf of Alaska, with Icy Strait running roughly west to east (horizontally) in from Cape Spencer where the strait meets the Pacific. The foreground glacier is the Brady

Glacier Bay, Alaska - Glacier Bay in Alaska - Glacier Bay from perspective. This image is the result of joint observations made by the Landsat-7 satellite in visible and infrared, combined with elevation radar data obtained by the Shuttle Radar Topography Mission (SRTM) in February 2000. At the bottom left of the picture, the Brady Glacier. Glacier Bay National Park and Preserve lies on the Pacific Coast of Alaska south of the St. Elias mountain range. The bay was set aside as a National Monument in 1925 and became its current National Park and Preserve in 1980, when approximately 85 percent of the park was designated a Wilderness Area. It has since been recognized as a UN Biosphere Reserve, in 1986, and a World Heritage Site, in 1992. The water in the foreground in the southwest (bottom left) corner of the image is the Gulf of Alaska, with Icy Strait running roughly west to east (horizontally) in from Cape Spencer where the strait meets the Pacific. The foreground glacier is the Brady

PIX4672471

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