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Images of 'NASA' found, 7,390

 
Tenoumer impact crater, Mauritania - Tenoumer impact crater, Mauritania - The Tenoumer impact crater in Mauritania is said to have been formed 10,000 to 30,000 years ago and has a diameter of 1.9 km. Image made from the International Space Station on 1 March 2007. Tenoumer impact crater, Mauritania, as seen by the International Space Station on march 1st 2007. Nearly a perfect circle, it is 1.9 kilometers (1.2 miles) wide, and sports a rim 100 meters (330 feet) high. The crater sits in a vast plain of rocks so ancient they were deposited hundreds of millions of years before the first dinosaurs walked the Earth. Modern geologists long debated what caused this crater, some of them favoring a volcano. But closer examination of the structure revealed that the crater's hardened lava”” was actually rock that had melted from a meteorite impact. Although it resides in ancient rock, Tenoumer is geologically young, ranging in age between roughly 10,000 and 30,000 years old.

PIX4630656

Tenoumer impact crater, Mauritania - Tenoumer impact crater, Mauritania - The Tenoumer impact crater in Mauritania is said to have been formed 10,000 to 30,000 years ago and has a diameter of 1.9 km. Image made from the International Space Station on 1 March 2007. Tenoumer impact crater, Mauritania, as seen by the International Space Station on march 1st 2007. Nearly a perfect circle, it is 1.9 kilometers (1.2 miles) wide, and sports a rim 100 meters (330 feet) high. The crater sits in a vast plain of rocks so ancient they were deposited hundreds of millions of years before the first dinosaurs walked the Earth. Modern geologists long debated what caused this crater, some of them favoring a volcano. But closer examination of the structure revealed that the crater's hardened lava”” was actually rock that had melted from a meteorite impact. Although it resides in ancient rock, Tenoumer is geologically young, ranging in age between roughly 10,000 and 30,000 years old.

PIX4630656

 
Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

PIX4630749

Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

PIX4630749

 
The dwarf planet Eris - Illustration - Dwarf planet Eris - Artwork - Artist's view of the dwarf planet Eris and its satellite Dysnomia. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 with its moon Dysnomia. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

PIX4629642

The dwarf planet Eris - Illustration - Dwarf planet Eris - Artwork - Artist's view of the dwarf planet Eris and its satellite Dysnomia. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 with its moon Dysnomia. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

PIX4629642

 
Artist's view of the solar system - Solar system artwork - Artist's view of the solar system. Planets are represented in order of proximity to the sun. From left to right: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune and Pluto. Other dwarf planets are not represented. The planets are shown in the correct order of distance from the Sun, the correct relative sizes, and the correct relative orbital distances. The sizes of the bodies are greatly exaggerated relative to the orbital distances. The faint rings of Jupiter, Uranus, and Neptune are not shown. Eris, Haumea, and Makemake do not appear in the illustration owing to their highly tilted orbits. The dwarf planet Ceres is not shown separately; it resides in the asteroid belt between Mars and Jupiter

PIX4630249

Artist's view of the solar system - Solar system artwork - Artist's view of the solar system. Planets are represented in order of proximity to the sun. From left to right: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune and Pluto. Other dwarf planets are not represented. The planets are shown in the correct order of distance from the Sun, the correct relative sizes, and the correct relative orbital distances. The sizes of the bodies are greatly exaggerated relative to the orbital distances. The faint rings of Jupiter, Uranus, and Neptune are not shown. Eris, Haumea, and Makemake do not appear in the illustration owing to their highly tilted orbits. The dwarf planet Ceres is not shown separately; it resides in the asteroid belt between Mars and Jupiter

PIX4630249

 
Tenerife - Tenerife, the largest island in the Canary Islands, seen by the Landsat-8 satellite on 25 January 2016. The Teide Peak is a stratovolcano that reaches 3718 metres above sea level. But from its base under the sea it rises to 7500 metres, making it the third largest volcano in the world. Tenerife, the largest of Spain's Canary Islands seen from space by Landsat 8 satellite on January 25, 2016. The summit of the Teide stratovolcano reaches 3,718 meters (12,198 feet) above sea level. If you include what's below the water line, the volcano rises 7,500 meters (24,606 feet) from the ocean floor, making it the third tallest volcanic structure on Earth

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Tenerife - Tenerife, the largest island in the Canary Islands, seen by the Landsat-8 satellite on 25 January 2016. The Teide Peak is a stratovolcano that reaches 3718 metres above sea level. But from its base under the sea it rises to 7500 metres, making it the third largest volcano in the world. Tenerife, the largest of Spain's Canary Islands seen from space by Landsat 8 satellite on January 25, 2016. The summit of the Teide stratovolcano reaches 3,718 meters (12,198 feet) above sea level. If you include what's below the water line, the volcano rises 7,500 meters (24,606 feet) from the ocean floor, making it the third tallest volcanic structure on Earth

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Saturn and Titan seen by Pioneer 11 31 - 08 - 197

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Saturn and Titan seen by Pioneer 11 31 - 08 - 197

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Condensation trains seen from ISS. - Contrails over Rhone valley seen from ISS. - Condensation trains caused by air traffic. Upstairs, Leman Lake. Image obtained from the International Space Station on May 15, 2002. This digital photograph taken through the windows of the International Space Station on May 15, 2002, shows condensation trails over the Rhone Valley. Condensation trails - - or contrails - - are straight lines of ice crystals that form in the wake of jet liners where air temperatures at altitude are lower than about - 40* C. Newer contrails are thin whereas older trails have widened with time as a result of light winds. Because of this tendency for thin contrails to cover greater areas with time, it is estimated that these artificial clouds”” cover 0.1% of the planet's surface. Percentages are far higher in some places such as southern California, the Ohio River Valley and parts of Europe, as illustrated here.

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Condensation trains seen from ISS. - Contrails over Rhone valley seen from ISS. - Condensation trains caused by air traffic. Upstairs, Leman Lake. Image obtained from the International Space Station on May 15, 2002. This digital photograph taken through the windows of the International Space Station on May 15, 2002, shows condensation trails over the Rhone Valley. Condensation trails - - or contrails - - are straight lines of ice crystals that form in the wake of jet liners where air temperatures at altitude are lower than about - 40* C. Newer contrails are thin whereas older trails have widened with time as a result of light winds. Because of this tendency for thin contrails to cover greater areas with time, it is estimated that these artificial clouds”” cover 0.1% of the planet's surface. Percentages are far higher in some places such as southern California, the Ohio River Valley and parts of Europe, as illustrated here.

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Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

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Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

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Baghdad - Copper Mine in Arizona - USA - Baghdad Copper Mine - Arizona: Baghdad is a copper mining community located in the western state of Arizona in the United States. It is one of the only two labourers that still exist in Arizona. Image taken from the International Space Station (ISS) on 1 March 2007. The Baghdad Mine is a large copper mine located in Arizona, in the southwestern part of the United States. Baghdad represents one of the largest copper reserves in the United States and in the world. The town of Baghdad, Arizona was built as a company town to house mine workers. Astronaut photograph was acquired on March 1, 2007 from the International Space Station (ISS)

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Baghdad - Copper Mine in Arizona - USA - Baghdad Copper Mine - Arizona: Baghdad is a copper mining community located in the western state of Arizona in the United States. It is one of the only two labourers that still exist in Arizona. Image taken from the International Space Station (ISS) on 1 March 2007. The Baghdad Mine is a large copper mine located in Arizona, in the southwestern part of the United States. Baghdad represents one of the largest copper reserves in the United States and in the world. The town of Baghdad, Arizona was built as a company town to house mine workers. Astronaut photograph was acquired on March 1, 2007 from the International Space Station (ISS)

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Lake Ontario, Lake Erie, seen from space shuttle Discovery - Lake Ontario, lake Erie seen from space shuttle - In this picture taken at sunset, water bodies stand out, relaying the light of the Sun. In the foreground is Lake Ontario with the St. Lawrence River; above, Lake Erie. Image obtained by the shuttle Discovery on October 21, 2000. The STS - 92 Space Shuttle astronauts photographed upstate New York at sunset on October 21, 2000. Water bodies (Lake Ontario, Lake Erie, the Finger Lakes, the St. Lawrence and Niagara Rivers) are highlighted by sunglint (sun reflecting off the water surface), making for a dramatic and unusual regional view. The photograph was taken looking toward the southwest from southern Canada, and captures a regional smog layer extending across central New York, western Lake Erie and Ohio, and further west. The layer of atmospheric pollution layer is capped by an atmospheric inversion, which is marked by the layer of clouds at the top of the photograph

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Lake Ontario, Lake Erie, seen from space shuttle Discovery - Lake Ontario, lake Erie seen from space shuttle - In this picture taken at sunset, water bodies stand out, relaying the light of the Sun. In the foreground is Lake Ontario with the St. Lawrence River; above, Lake Erie. Image obtained by the shuttle Discovery on October 21, 2000. The STS - 92 Space Shuttle astronauts photographed upstate New York at sunset on October 21, 2000. Water bodies (Lake Ontario, Lake Erie, the Finger Lakes, the St. Lawrence and Niagara Rivers) are highlighted by sunglint (sun reflecting off the water surface), making for a dramatic and unusual regional view. The photograph was taken looking toward the southwest from southern Canada, and captures a regional smog layer extending across central New York, western Lake Erie and Ohio, and further west. The layer of atmospheric pollution layer is capped by an atmospheric inversion, which is marked by the layer of clouds at the top of the photograph

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Highland Valley Copper Mine - Canada - Highland Valley Copper Mine - Canada: The Highland Valley Mine is an open pit copper and molybdene mine located in British Columbia, Canada. Image taken from the International Space Station (ISS) on September 28, 2009. The north is downstairs. The Highland Valley Copper mine is the largest open pit copper mine in Canada, located near Logan Lake, British Columbia. Astronaut photograph was acquired on September 28 2009 from the International Space Station (ISS)

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Highland Valley Copper Mine - Canada - Highland Valley Copper Mine - Canada: The Highland Valley Mine is an open pit copper and molybdene mine located in British Columbia, Canada. Image taken from the International Space Station (ISS) on September 28, 2009. The north is downstairs. The Highland Valley Copper mine is the largest open pit copper mine in Canada, located near Logan Lake, British Columbia. Astronaut photograph was acquired on September 28 2009 from the International Space Station (ISS)

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Cananea Copper Mine - Mexico - Cananea Copper Mine - Sonora - Mexico: The Cananea Mine is an open pit copper and gold mine located in Mexico. Its production began in 1899. Image taken from the International Space Station (ISS) on March 3, 2008. One of the largest open-pit copper mines in the world, the Cananea mine produced over 164,000 tonnes of copper in 2006. The mine is located approximately 40 km south of the border between the USA (Arizona) and Mexico (Sonora). Copper and gold ores at Cananea are found in a porphyry copper deposit, a geological structure formed by crystal-rich magma moving upwards through pre-existing rock layers. A porphyry - an igneous rock with large crystals in a fine-grained matrix - is formed as the magma cools and crystallizes. While crystallization is occurring, hot fluids can circulate through the magma and surrounding rocks via fractures. This hydrothermal alteration of the rocks typically forms copper-bearing and other minerals. The active, 2 km in dia

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Cananea Copper Mine - Mexico - Cananea Copper Mine - Sonora - Mexico: The Cananea Mine is an open pit copper and gold mine located in Mexico. Its production began in 1899. Image taken from the International Space Station (ISS) on March 3, 2008. One of the largest open-pit copper mines in the world, the Cananea mine produced over 164,000 tonnes of copper in 2006. The mine is located approximately 40 km south of the border between the USA (Arizona) and Mexico (Sonora). Copper and gold ores at Cananea are found in a porphyry copper deposit, a geological structure formed by crystal-rich magma moving upwards through pre-existing rock layers. A porphyry - an igneous rock with large crystals in a fine-grained matrix - is formed as the magma cools and crystallizes. While crystallization is occurring, hot fluids can circulate through the magma and surrounding rocks via fractures. This hydrothermal alteration of the rocks typically forms copper-bearing and other minerals. The active, 2 km in dia

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Manhattan Region, New York, view from space - 11/09/2001 - Smoke plume from Manhattan, New York City - 11/09/2001 - The smoke plume escaping from Manhattan Island to New York seen from the International Space Station on 11 September 2001 11 September 2001 - One of a series of pictures taken of metropolitan New York City (and other parts of New York as well as New Jersey) by one of the Expedition Three crew members onboard the International Space Station (ISS) at various times during the day of September 11, 2001. The image shows a smoke plume rising from the Manhattan area. The orbital outpost was flying at an altitude of approximately 250 miles. The image was recorded with a digital still camera

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Manhattan Region, New York, view from space - 11/09/2001 - Smoke plume from Manhattan, New York City - 11/09/2001 - The smoke plume escaping from Manhattan Island to New York seen from the International Space Station on 11 September 2001 11 September 2001 - One of a series of pictures taken of metropolitan New York City (and other parts of New York as well as New Jersey) by one of the Expedition Three crew members onboard the International Space Station (ISS) at various times during the day of September 11, 2001. The image shows a smoke plume rising from the Manhattan area. The orbital outpost was flying at an altitude of approximately 250 miles. The image was recorded with a digital still camera

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The Great Barrier Reef in Australia from space - The Great Barrier Reef is the largest coral reef in the world, extending over 2000 km off Queensland, Australia. At the bottom of the picture is Cape Melville. Image obtained from the International Space Station (ISS) on 22 November 2007. The Great Barrier Reef arches over 2000 kilometers along the northeast coast of Australia. The white calcium carbonate that coats the coral reflects light, making the water above the reef appear bright blue from space. Image taken from the International space station (ISS) on November 22, 2007

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The Great Barrier Reef in Australia from space - The Great Barrier Reef is the largest coral reef in the world, extending over 2000 km off Queensland, Australia. At the bottom of the picture is Cape Melville. Image obtained from the International Space Station (ISS) on 22 November 2007. The Great Barrier Reef arches over 2000 kilometers along the northeast coast of Australia. The white calcium carbonate that coats the coral reflects light, making the water above the reef appear bright blue from space. Image taken from the International space station (ISS) on November 22, 2007

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North-West Australia, seen by shuttle Columbia - 80 mile beach - 24 July 199

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North-West Australia, seen by shuttle Columbia - 80 mile beach - 24 July 199

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Argyle Diamond Mine - Australia - Argyle Diamond Mine - Australia: The Argyle Diamond Mine is a mine located in the Eastern Kimberley region of northern Australia. It is the largest diamond mine in the world in volume terms, although due to the low proportion of quality diamonds, it is not a leader in value. Image taken from the International Space Station (ISS) on 22 June 2006. The Argyle Diamond Mine is a diamond mine located in the East Kimberley region in the remote north of Western Australia. Argyle is the largest diamond producer in the world by volume, although due to the low proportion of gemquality diamonds it is set to close by 2020. Image taken from the international space station on June 22 2006.

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Argyle Diamond Mine - Australia - Argyle Diamond Mine - Australia: The Argyle Diamond Mine is a mine located in the Eastern Kimberley region of northern Australia. It is the largest diamond mine in the world in volume terms, although due to the low proportion of quality diamonds, it is not a leader in value. Image taken from the International Space Station (ISS) on 22 June 2006. The Argyle Diamond Mine is a diamond mine located in the East Kimberley region in the remote north of Western Australia. Argyle is the largest diamond producer in the world by volume, although due to the low proportion of gemquality diamonds it is set to close by 2020. Image taken from the international space station on June 22 2006.

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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

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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

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Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

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Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

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Hurricane Emilie 07/1994 - Hurricane Emilia as seen from the space shuttle 07/1994 - Hurricane Emilie over the Pacific Ocean seen by Shuttle Columbia in July 1994. STS - 65 Earth observation taken aboard Columbia, Orbiter Vehicle (OV) 102, shows Hurricane Emilia in the Eastern Pacific Ocean. Hurricane Emilia's wind speeds exceeded 150 knots. This high oblique view of the storm shows numerous spiral bands of thunderstorms, overshooting thunderstorm tops at the tropopause, and a well developed eye at the center of the picture. Shuttle photography provides high resolution details of these powerful and destructive systems that are not fully possible from lower - resolution, unmanned satellites

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Hurricane Emilie 07/1994 - Hurricane Emilia as seen from the space shuttle 07/1994 - Hurricane Emilie over the Pacific Ocean seen by Shuttle Columbia in July 1994. STS - 65 Earth observation taken aboard Columbia, Orbiter Vehicle (OV) 102, shows Hurricane Emilia in the Eastern Pacific Ocean. Hurricane Emilia's wind speeds exceeded 150 knots. This high oblique view of the storm shows numerous spiral bands of thunderstorms, overshooting thunderstorm tops at the tropopause, and a well developed eye at the center of the picture. Shuttle photography provides high resolution details of these powerful and destructive systems that are not fully possible from lower - resolution, unmanned satellites

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Hurricane Ike seen from space - Hurricane Ike seen from space - Hurricane Ike seen over Cuba on 9 September 2008 from the International Space Station (ISS). 9 Sep. 2008 - Hurricane Ike covers more than half of Cuba in this image, photographed by the crew of ISS - 17 aboard the International Space Station from a vantage point of 220 statute miles above Earth. The center of Ike was near 22.4 degrees north latitude and 82.4 degrees west longitude and moving 290 degrees at 11.7 miles per hour. Sustained winds were at 80.6 miles per hour, with gusts to 97.9 miles per hour and were forced to strengthen as the eye moved back over the warm water in the gulf of Mexico City

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Hurricane Ike seen from space - Hurricane Ike seen from space - Hurricane Ike seen over Cuba on 9 September 2008 from the International Space Station (ISS). 9 Sep. 2008 - Hurricane Ike covers more than half of Cuba in this image, photographed by the crew of ISS - 17 aboard the International Space Station from a vantage point of 220 statute miles above Earth. The center of Ike was near 22.4 degrees north latitude and 82.4 degrees west longitude and moving 290 degrees at 11.7 miles per hour. Sustained winds were at 80.6 miles per hour, with gusts to 97.9 miles per hour and were forced to strengthen as the eye moved back over the warm water in the gulf of Mexico City

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Hurricane Igor seen from space - Hurricane Igor seen from space - Hurricane Igor seen from space over the Lesser Antilles on 14 September 2010 from the International Space Station (ISS). Hurricane Igor is featured in this Sept. 14 2010 image photographed by an Expedition 24 crew member on the International Space Station. At the time this image was taken, Hurricane Igor was about 648 miles east of Barbuda Island in the Lesser Antilles. It was travelling to the northeast (290 degrees) at 6.2 mph. The winds were already 132.5 mph gusting to 161.3 mph and forecast to intensify. Igor's well - defined eye was a dynamic area of swift rising winds in the outer wall and sinking winds in the center. His strong eye wall surrounded a low level cloud deck of clouds containing additional vortices

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Hurricane Igor seen from space - Hurricane Igor seen from space - Hurricane Igor seen from space over the Lesser Antilles on 14 September 2010 from the International Space Station (ISS). Hurricane Igor is featured in this Sept. 14 2010 image photographed by an Expedition 24 crew member on the International Space Station. At the time this image was taken, Hurricane Igor was about 648 miles east of Barbuda Island in the Lesser Antilles. It was travelling to the northeast (290 degrees) at 6.2 mph. The winds were already 132.5 mph gusting to 161.3 mph and forecast to intensify. Igor's well - defined eye was a dynamic area of swift rising winds in the outer wall and sinking winds in the center. His strong eye wall surrounded a low level cloud deck of clouds containing additional vortices

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Clouds 03/02 - Clouds seen by the shuttle STS - 109 in March 2002

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Clouds 03/02 - Clouds seen by the shuttle STS - 109 in March 2002

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