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Earth by satellite - Earth seen by satellite

Earth by satellite - Earth seen by satellite

PIX4669205

Earth - The geoid - Earth's geoid - The Earth's geoid, an image of the inegalites of the Earth's gravitation field. Image centred on Indonesia. Image obtained by the GOCE satellite in 2011. ESA's GOCE mission has delivered the most accurate model of the 'geoid' ever produced, which will be used to further our understanding of how Earth works. A precise model of Earth's geoid is crucial for deriving accurate measurements of ocean circulation, sea - level change and terrestrial ice dynamics. The geoid is also used as a reference surface from which to map the topographical features on the planet. In addition, a better understanding of variations in the gravity field will lead to a deeper understanding of Earth's interior, such as the physics and dynamics associated with volcanic activity and earthquakes

Earth - The geoid - Earth's geoid - The Earth's geoid, an image of the inegalites of the Earth's gravitation field. Image centred on Indonesia. Image obtained by the GOCE satellite in 2011. ESA's GOCE mission has delivered the most accurate model of the 'geoid' ever produced, which will be used to further our understanding of how Earth works. A precise model of Earth's geoid is crucial for deriving accurate measurements of ocean circulation, sea - level change and terrestrial ice dynamics. The geoid is also used as a reference surface from which to map the topographical features on the planet. In addition, a better understanding of variations in the gravity field will lead to a deeper understanding of Earth's interior, such as the physics and dynamics associated with volcanic activity and earthquakes

PIX4632050

Earth from space - Earth from space - Image of Earth recomposed from different satellite images Composite images obtained with data collected from several satellites

Earth from space - Earth from space - Image of Earth recomposed from different satellite images Composite images obtained with data collected from several satellites

PIX4632062

Earth by satellite - Earth from space - The Earth from satellite centred on Australia. Image recomposed from satellite data. Global Earth centered on Australia seen by satellites

Earth by satellite - Earth from space - The Earth from satellite centred on Australia. Image recomposed from satellite data. Global Earth centered on Australia seen by satellites

PIX4631886

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

PIX4629876

Comparison between Earth, Mercury and the Moon - Earth, Mercury, and Earth's Moon compared - Comparison at the scale of the Earth's size, the planet Mercury and the Moon. The diameter of Mercury is about one third of that of the Earth. Mercury is a little larger than the Earth's Moon and is believed to be composed mostly of iron and rock, making it considerably denser than the Moon. Mercury also has a magnetic field about 1% as strong as the Earth's. Mercury's diameter is only one third that of the Earth's. It has only 6% the mass. If you weigh 180 pounds on the Earth, you would weigh 64 pounds on Mercury. Is only one-third the Earth's distance from the Su

Comparison between Earth, Mercury and the Moon - Earth, Mercury, and Earth's Moon compared - Comparison at the scale of the Earth's size, the planet Mercury and the Moon. The diameter of Mercury is about one third of that of the Earth. Mercury is a little larger than the Earth's Moon and is believed to be composed mostly of iron and rock, making it considerably denser than the Moon. Mercury also has a magnetic field about 1% as strong as the Earth's. Mercury's diameter is only one third that of the Earth's. It has only 6% the mass. If you weigh 180 pounds on the Earth, you would weigh 64 pounds on Mercury. Is only one-third the Earth's distance from the Su

Walter B Myers

PIX4629901

The End of Oceans on Earth - Artist's View - Earth's oceans end - Artist view: When the Sun swells to become a giant yellow star, the heat on Earth will evaporate the oceans. As the sun gets older, it begins to swell. As it enters the yellow giant stage, the earth becomes so warm that the oceans dry up

The End of Oceans on Earth - Artist's View - Earth's oceans end - Artist view: When the Sun swells to become a giant yellow star, the heat on Earth will evaporate the oceans. As the sun gets older, it begins to swell. As it enters the yellow giant stage, the earth becomes so warm that the oceans dry up

Miller, Ron (b.1947)

PIX4669608

Earth seen by satellite - Earth seen by satellite - Mosaic of Earth images obtained by the Suomi NPP satellite in January 2012. This composite image uses a number of swaths of the Earth's surface taken on January 23, 2012 by Suomi NPP satellite

Earth seen by satellite - Earth seen by satellite - Mosaic of Earth images obtained by the Suomi NPP satellite in January 2012. This composite image uses a number of swaths of the Earth's surface taken on January 23, 2012 by Suomi NPP satellite

PIX4631980

Earth seen by Apollo 13 - Apollo 13: Earth - 04/1970 - Earth seen by Apollo 13 in April 1970. Earth as seen from Apollo 13 in April 1970. North America

Earth seen by Apollo 13 - Apollo 13: Earth - 04/1970 - Earth seen by Apollo 13 in April 1970. Earth as seen from Apollo 13 in April 1970. North America

PIX4632210

Earth - Day and Night - Australia - Earth - Day and night - Australia - Composite of two images of the Earth, entirely illuminated by the Sun, and of the Earth entirely in darkness, showing the light of inhabited areas. This image of the Earth is a composite of two data images - one of the globe fully illuminated by the Sun, and one of the globe in full darkness, showing only the city lights of inhabited areas

Earth - Day and Night - Australia - Earth - Day and night - Australia - Composite of two images of the Earth, entirely illuminated by the Sun, and of the Earth entirely in darkness, showing the light of inhabited areas. This image of the Earth is a composite of two data images - one of the globe fully illuminated by the Sun, and one of the globe in full darkness, showing only the city lights of inhabited areas

PIX4632546

Earth: The four seasons - Earth: The four seasons - Equinoxes and solstices mark the four seasons on Earth. Earth's orbit showing seasons. Illustration

Earth: The four seasons - Earth: The four seasons - Equinoxes and solstices mark the four seasons on Earth. Earth's orbit showing seasons. Illustration

Sebastien Beaucourt

PIX4633352

Asteroids Families - Asteroids Families- Artwork - Artist's view of the different Asteroids families

Asteroids Families - Asteroids Families- Artwork - Artist's view of the different Asteroids families

L. Bret

PIX4584051

Comparison between Earth and Venus - Earth and Venus compared - Comparison at the scale of the sizes of Earth and Venus, seen here without their atmosphere. The size of the Venus planet is roughly the same as that of the Earth. This to-scale image suggests how the Earth and Venus might appear without their atmospheres. Venus' diameter is 86% that of the Earth's. It has 82% the mass. If you weigh 180 pounds on the Earth, you would weigh 163 pounds on Venus. Venus is about three-quarters the Earth's distance from the Sun. While Venus is roughly the same size and density as the Earth, it is otherwise a very different world. Earth's surface is a varied one, with liquid water covering three quarters of its surface. Those areas not under water have been highly modified by plate tectonics, weather, and life itself. Venus on the other hand is far too hot to host liquid water. Volcanoes, massive lava flows and the occasional impact crater characterize its surface. Latest observations suggest th

Comparison between Earth and Venus - Earth and Venus compared - Comparison at the scale of the sizes of Earth and Venus, seen here without their atmosphere. The size of the Venus planet is roughly the same as that of the Earth. This to-scale image suggests how the Earth and Venus might appear without their atmospheres. Venus' diameter is 86% that of the Earth's. It has 82% the mass. If you weigh 180 pounds on the Earth, you would weigh 163 pounds on Venus. Venus is about three-quarters the Earth's distance from the Sun. While Venus is roughly the same size and density as the Earth, it is otherwise a very different world. Earth's surface is a varied one, with liquid water covering three quarters of its surface. Those areas not under water have been highly modified by plate tectonics, weather, and life itself. Venus on the other hand is far too hot to host liquid water. Volcanoes, massive lava flows and the occasional impact crater characterize its surface. Latest observations suggest th

Walter B Myers

PIX4629857

Venus Express Probe leaves Earth orbit - Venus Express spacecraft leaving Earth orbit - The European Venus Express probe was launched on 9 November 2005 by a Soyuz - Fregat rocket and placed in orbit around Venus on 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 by a Soyuz - Fregat rocket and reaches the planet Venus on april 11 2006

Venus Express Probe leaves Earth orbit - Venus Express spacecraft leaving Earth orbit - The European Venus Express probe was launched on 9 November 2005 by a Soyuz - Fregat rocket and placed in orbit around Venus on 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 by a Soyuz - Fregat rocket and reaches the planet Venus on april 11 2006

D. Ducros

PIX4606242

Asteroids hit the Earth - Asteroids hit the Earth - Asteroids hit the Earth. Asteroids collide with the earth

Asteroids hit the Earth - Asteroids hit the Earth - Asteroids hit the Earth. Asteroids collide with the earth

PIX4583708

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - This image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits.: Europe at night - Europe by night

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - This image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits.: Europe at night - Europe by night

PIX4669265

Earth - artist's view - Earth. Artwork - The Earth centred on the Indian Ocean. The Earth centered on Indian ocean

Earth - artist's view - Earth. Artwork - The Earth centred on the Indian Ocean. The Earth centered on Indian ocean

Walter B Myers

PIX4633167

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

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

Walter B Myers

PIX4629809

A neutron star at the scale of France - Size comparison: a neutron star with France - A neutron star is a very dense star resulting from the explosion of a massive supernova star. These stars are very small as in this illustration on scale. Neutron stars are incredibly dense remnants of older stars that have blown off their outer gas layers. Many are only as far across as a city. In this cosmic comparison, we see a typical neutron star compared to France and northern Spain

A neutron star at the scale of France - Size comparison: a neutron star with France - A neutron star is a very dense star resulting from the explosion of a massive supernova star. These stars are very small as in this illustration on scale. Neutron stars are incredibly dense remnants of older stars that have blown off their outer gas layers. Many are only as far across as a city. In this cosmic comparison, we see a typical neutron star compared to France and northern Spain

M. Carroll

PIX4572449

Kepler's Law - Illustration - The segment that connects the planet to the Sun sweeps equal areas in equal times. In other words, the speed of a planet becomes greater when the planet approaches the Sun. It is maximum in the vicinity of the shortest radius (perihelie), and minimal in the vicinity of the largest radius (aphelie). Second Kepler's law, the line joining a planet and the Sun sweeps out equal areas during equal intervals of time. The planet moves faster near the Sun, so the same area is swept out in a given time as at larger distances, where the planet moves more slowl

Kepler's Law - Illustration - The segment that connects the planet to the Sun sweeps equal areas in equal times. In other words, the speed of a planet becomes greater when the planet approaches the Sun. It is maximum in the vicinity of the shortest radius (perihelie), and minimal in the vicinity of the largest radius (aphelie). Second Kepler's law, the line joining a planet and the Sun sweeps out equal areas during equal intervals of time. The planet moves faster near the Sun, so the same area is swept out in a given time as at larger distances, where the planet moves more slowl

Sebastien Beaucourt

PIX4629399

Mission to Phobos - Appointment in Earth orbit - Phobos mission rendezvous in Earth orbit - An Orion-type space capsule (left), with three astronauts on board, joins a launcher in Earth orbit to reach Phobos, one of Mars's satellites. An Orion class command module, lower left, with a crew of three approaches an awaiting rocket already in Earth orbit. The rocket and command module are destined for Mars' moon Phobos

Mission to Phobos - Appointment in Earth orbit - Phobos mission rendezvous in Earth orbit - An Orion-type space capsule (left), with three astronauts on board, joins a launcher in Earth orbit to reach Phobos, one of Mars's satellites. An Orion class command module, lower left, with a crew of three approaches an awaiting rocket already in Earth orbit. The rocket and command module are destined for Mars' moon Phobos

Walter B Myers

PIX4639605

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521039

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521040

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521054

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521057

Globe Showing Northern America, True Colour Satellite Image

Globe Showing Northern America, True Colour Satellite Image

UIG521113

South America With Country Borders, True Colour Satellite Image

South America With Country Borders, True Colour Satellite Image

UIG520944

South America At Night With Cloud Coverage, True Colour Satellite Image

South America At Night With Cloud Coverage, True Colour Satellite Image

UIG520951

Earth- Illustration - Earth from space. Artwork

Earth- Illustration - Earth from space. Artwork

S. Numazawa

PIX4669558

Ocean level rise - Hemisphere oriental - Earth's Eastern hemisphere with sea level+100m - Artist's view showing Asia and Oceania as they would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how the Earth's Eastern hemisphere may appear with mean sea level about 100 meters (330 feet) above today's.

Ocean level rise - Hemisphere oriental - Earth's Eastern hemisphere with sea level+100m - Artist's view showing Asia and Oceania as they would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how the Earth's Eastern hemisphere may appear with mean sea level about 100 meters (330 feet) above today's.

Walter B Myers

PIX4633107

Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete

Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete

Walter B Myers

PIX4633164

100m ocean level rise - South Asia - South Asia with sea level+100m - Artist's view showing South Asia as it would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how South Asia 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 over half of Pakistan along with the Indian state of Gujarat have become part of the Arabian Sea while the Persian Gulf has consumed Iran's border with Kuwait and some of Iraq. Bangladesh has succumbed entirely to the Bay of Bengal. The Gulf of Martaban now flows into much of Myanmar

100m ocean level rise - South Asia - South Asia with sea level+100m - Artist's view showing South Asia as it would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how South Asia 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 over half of Pakistan along with the Indian state of Gujarat have become part of the Arabian Sea while the Persian Gulf has consumed Iran's border with Kuwait and some of Iraq. Bangladesh has succumbed entirely to the Bay of Bengal. The Gulf of Martaban now flows into much of Myanmar

Walter B Myers

PIX4633202

Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view

Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view

E. Graeff

PIX4583678

Tungouska event -Artist's view-2/3 - Tunguska Valley - Artist view (2/3) - On June 30, 1908 a car, several ten metres in diameter, exploded over the Tounguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

Tungouska event -Artist's view-2/3 - Tunguska Valley - Artist view (2/3) - On June 30, 1908 a car, several ten metres in diameter, exploded over the Tounguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

PIX4583789

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG520984

Mission to Phobos - Appointment in Earth orbit - Phobos mission docking in Earth orbit - An Orion-type space capsule (right), with three astronauts on board, joins in Earth orbit a launcher to reach Phobos, one of Mars's satellites. An Orion class command module, upper right, prepares to dock with a Phobos mission rocket in Earth orbit. Below at a distance of approximately 200 miles is the eastern Sahara desert. Lower left are the crew quarters for the 16 month mission

Mission to Phobos - Appointment in Earth orbit - Phobos mission docking in Earth orbit - An Orion-type space capsule (right), with three astronauts on board, joins in Earth orbit a launcher to reach Phobos, one of Mars's satellites. An Orion class command module, upper right, prepares to dock with a Phobos mission rocket in Earth orbit. Below at a distance of approximately 200 miles is the eastern Sahara desert. Lower left are the crew quarters for the 16 month mission

Walter B Myers

PIX4639615

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

PIX4669194

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

PIX4625315

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

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

PIX4583798

Globe Showing Europe And Africa, True Colour Satellite Image

Globe Showing Europe And Africa, True Colour Satellite Image

UIG521114

Globe Showing Europe And Northern Africa, True Colour Satellite Image

Globe Showing Europe And Northern Africa, True Colour Satellite Image

UIG521108

Earth at night - Asia - Earth at night - Asia - Earth centred on Asia observed at night by satellite. The Earth with city lights seen from satellite, centered on Asia

Earth at night - Asia - Earth at night - Asia - Earth centred on Asia observed at night by satellite. The Earth with city lights seen from satellite, centered on Asia

PIX4632487

Moon and Jupiter - Moon and Jupiter - Planet Jupiter (the bright spot on the left) near the Moon. Image obtained on July 17, 2008. To the left of nearly full moon is the bright planet Jupiter. Image taken on July 17, 2008

Moon and Jupiter - Moon and Jupiter - Planet Jupiter (the bright spot on the left) near the Moon. Image obtained on July 17, 2008. To the left of nearly full moon is the bright planet Jupiter. Image taken on July 17, 2008

Laurent Laveder

PIX4587513

The solar system - Partial view - Our solar system. Artwork - Artist's view of the solar system. The planets represented are Mars, Earth, Neptune, Saturn, Jupiter. The Sun and a comet are also represented. Partial view of the planets of our solar system showing Mars, the Earth, Neptune, Saturn, Jupiter, a comet and the Sun

The solar system - Partial view - Our solar system. Artwork - Artist's view of the solar system. The planets represented are Mars, Earth, Neptune, Saturn, Jupiter. The Sun and a comet are also represented. Partial view of the planets of our solar system showing Mars, the Earth, Neptune, Saturn, Jupiter, a comet and the Sun

D. Ducros

PIX4630060

Earth Globe Showing North Pole With Country Borders

Earth Globe Showing North Pole With Country Borders

UIG675257

Globe Showing Asia, True Colour Satellite Image

Globe Showing Asia, True Colour Satellite Image

UIG521119

Oceania With Country Borders And Major Rivers, True Colour Satellite Image

Oceania With Country Borders And Major Rivers, True Colour Satellite Image

UIG520965

Oceania At Night With Country Borders And Cloud Coverage, True Colour Satellite Image

Oceania At Night With Country Borders And Cloud Coverage, True Colour Satellite Image

UIG520970

Globe Centred On The Americas, True Colour Satellite Image

Globe Centred On The Americas, True Colour Satellite Image

UIG520994

Globe Centred On The Americas, True Colour Satellite Image

Globe Centred On The Americas, True Colour Satellite Image

UIG521009

Ice on the Moon - Illustration - Lunar ice - Illustration - Artist's view of ice on the surface of a crater that remains perpetually in the shade of the Sun, near the poles. Water from an encounter with an icy comet has collected in the perpetual shade of a deep crater where the temperature is a constant - 380o F. In 1998, the unmanned Lunar Prospector probe discovered evidence for water ice on the surface of the moon. Some scientists believe that as much as 10 to 300 million tons of ice may reside at the moon's North and South poles. The source of the ice is thought to be from one or more comets that struck the moon's surface four billion years ago. (It is thought that Earth's water may have come from comets as well.) Unfortunately, the moon's small size and lack of an atmosphere caused it to lose almost all of its accumulated water to space. Any water that does remain on the moon would likely be on the poles, hidden in craters and depressions shaded from the Sun

Ice on the Moon - Illustration - Lunar ice - Illustration - Artist's view of ice on the surface of a crater that remains perpetually in the shade of the Sun, near the poles. Water from an encounter with an icy comet has collected in the perpetual shade of a deep crater where the temperature is a constant - 380o F. In 1998, the unmanned Lunar Prospector probe discovered evidence for water ice on the surface of the moon. Some scientists believe that as much as 10 to 300 million tons of ice may reside at the moon's North and South poles. The source of the ice is thought to be from one or more comets that struck the moon's surface four billion years ago. (It is thought that Earth's water may have come from comets as well.) Unfortunately, the moon's small size and lack of an atmosphere caused it to lose almost all of its accumulated water to space. Any water that does remain on the moon would likely be on the poles, hidden in craters and depressions shaded from the Sun

Walter B Myers

PIX4580041

Size Comparison: Earth, Titan satellite and Moon - Earth, Titan, and Earth's Moon compared - Saturn's largest satellite, Titan compares to Earth and Moon. Titan may be larger than the planet Mercury - and (the dwarf planet) Pluto- but it is still considerably smaller than the Earth. Despite Titan's diminutive size, its atmosphere is dense enough that the barometric pressure at Titan's surface is one and-a-half times greater than that of the Earth's at sea level

Size Comparison: Earth, Titan satellite and Moon - Earth, Titan, and Earth's Moon compared - Saturn's largest satellite, Titan compares to Earth and Moon. Titan may be larger than the planet Mercury - and (the dwarf planet) Pluto- but it is still considerably smaller than the Earth. Despite Titan's diminutive size, its atmosphere is dense enough that the barometric pressure at Titan's surface is one and-a-half times greater than that of the Earth's at sea level

Walter B Myers

PIX4629987

Earth Globe Showing North and South American Continents

Earth Globe Showing North and South American Continents

UIG675232

Earth Globe Showing North and South American Continents

Earth Globe Showing North and South American Continents

UIG675234

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521036

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521043

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521045

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521053

Globe Centred On Europe And Africa, True Colour Satellite Image

Globe Centred On Europe And Africa, True Colour Satellite Image

UIG521058

NASA's Kepler mission confirmed the discovery of its first rocky planet, named Kepler-10b, 2000

NASA's Kepler mission confirmed the discovery of its first rocky planet, named Kepler-10b, 2000

UIG3508220

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