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Images de 'Meteorites' médias trouvés, 476

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The Hayabusa and Itokawa probe - Hayabusa spacecraft near the asteroid Itokawa: Artist's view of the Hayabusa probe near the asteroid Itokawa. The Japanese probe Hayabusa (MUSES-C) was launched on 9 May 2003 to reach the asteroid 25143 Itokawa in September 2005 and to take samples from it. His return to Earth took place in June 2010

The Hayabusa and Itokawa probe - Hayabusa spacecraft near the asteroid Itokawa: Artist's view of the Hayabusa probe near the asteroid Itokawa. The Japanese probe Hayabusa (MUSES-C) was launched on 9 May 2003 to reach the asteroid 25143 Itokawa in September 2005 and to take samples from it. His return to Earth took place in June 2010

Miller, Ron (b.1947)

PIX4643666

Detourning a threatening asteroid - Illustration - Deflecting an asteroid - Illustration - Attempt to deflect an asteroid threatening the Earth using spacecraft using an electromagnetic catapult as a means of propulsion. Several mass drivers are attached to an asteroid to push it into a non-earth impacting course. A mass driver or electromagnetic catapult is a proposed method of non-rocket spacelaunch that would use a linear motor to accelerate and catapult payloads up to high speeds

Detourning a threatening asteroid - Illustration - Deflecting an asteroid - Illustration - Attempt to deflect an asteroid threatening the Earth using spacecraft using an electromagnetic catapult as a means of propulsion. Several mass drivers are attached to an asteroid to push it into a non-earth impacting course. A mass driver or electromagnetic catapult is a proposed method of non-rocket spacelaunch that would use a linear motor to accelerate and catapult payloads up to high speeds

PIX4583928

1970s: Boys speak and gesture

1970s: Boys speak and gesture

AVE6329895

Based on an asteroid-Artist's view - Base on an asteroid - Illustratio

Based on an asteroid-Artist's view - Base on an asteroid - Illustratio

S. Numazawa

PIX4639693

Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf

Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf

Walter B Myers

PIX4572527

Impact on the Europe satellite - Illustration - Impact on Europa - Illustration: Impact of an asteroid on the ice surface of the Europe satellite. Artist view - Asteroid impact on the icy surface of the moon Europa with planet Jupiter in background

Impact on the Europe satellite - Illustration - Impact on Europa - Illustration: Impact of an asteroid on the ice surface of the Europe satellite. Artist view - Asteroid impact on the icy surface of the moon Europa with planet Jupiter in background

PIX4614077

Artist's view of the double asteroid 90 Antiope - Artist impression of the binary asteroid 90 Antiope - Artist's view of the double asteroid 90 Antiope located in the asteroid belt between Mars and Jupiter. The two asteroids that make up this system are approximately 86 km long and 170 km apart. Artwork of the binary asteroid 90 Antiope, which orbits in the main part of the outer asteroid belt. Each asteroid is about 86 km across, orbiting its partner from a distance of 170 km

Artist's view of the double asteroid 90 Antiope - Artist impression of the binary asteroid 90 Antiope - Artist's view of the double asteroid 90 Antiope located in the asteroid belt between Mars and Jupiter. The two asteroids that make up this system are approximately 86 km long and 170 km apart. Artwork of the binary asteroid 90 Antiope, which orbits in the main part of the outer asteroid belt. Each asteroid is about 86 km across, orbiting its partner from a distance of 170 km

PIX4583618

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwork - Artist view

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwork - Artist view

S. Numazawa

PIX4583643

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Alex Tudorica

PIX4598903

An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration

An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration

Miller, Ron (b.1947)

PIX4583829

An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration

An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration

Miller, Ron (b.1947)

PIX4583830

The asteroid belt - The asteroid belt- Artwork - View of the main asteroid belt, from planetary orbits to jupiter, with Trojan asteroids. Artist view of the asteroid belt located between Mars and Jupiter orbits plus the trojan asteroids

The asteroid belt - The asteroid belt- Artwork - View of the main asteroid belt, from planetary orbits to jupiter, with Trojan asteroids. Artist view of the asteroid belt located between Mars and Jupiter orbits plus the trojan asteroids

L. Bret

PIX4584064

Inner Solar system seen from an asteroid: Artist's view of the orbits of the inner planets (Mercury, Venus, Earth and Mars) seen from the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter

Inner Solar system seen from an asteroid: Artist's view of the orbits of the inner planets (Mercury, Venus, Earth and Mars) seen from the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter

Miller, Ron (b.1947)

PIX4569111

This Hubble picture, taken on 23 July 2009, is the sharpest visible

This Hubble picture, taken on 23 July 2009, is the sharpest visible

PIX5619661

Last September

premium — Last September

JAN1078160

Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

PIX4583494

Engraving depicting the great daylight bolide of 1886. Dated 19th Century

Engraving depicting the great daylight bolide of 1886. Dated 19th Century

UIG5426103

Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line

Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line

Walter B Myers

PIX4572539

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor

PIX4583808

The Osiris-Rex probe and the Bennu asteroid - Artist's view - Osiris-rex and asteroid Bennu - Artwork - Artist view of the Osiris-Rex probe collecting a sample of the Bennu asteroid. OSIRIS-REX was launched on 8 September 2016 to reach the asteroid Bennu in 2018 and bring a sample back to Earth in 2023. OSIRIS-REX contacts the asteroid Bennu with the Touch-And-Go Sample Arm Mechanism. The spaceprobe was launched on Sept. 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023

The Osiris-Rex probe and the Bennu asteroid - Artist's view - Osiris-rex and asteroid Bennu - Artwork - Artist view of the Osiris-Rex probe collecting a sample of the Bennu asteroid. OSIRIS-REX was launched on 8 September 2016 to reach the asteroid Bennu in 2018 and bring a sample back to Earth in 2023. OSIRIS-REX contacts the asteroid Bennu with the Touch-And-Go Sample Arm Mechanism. The spaceprobe was launched on Sept. 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023

PIX4643777

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

Fall of a Meteorite in the Appennines, Italy, 1937, illustration from 'La Domenica del Corriere' 14th February 1937 (colour litho)

Fall of a Meteorite in the Appennines, Italy, 1937, illustration from 'La Domenica del Corriere' 14th February 1937 (colour litho)

Beltrame, Achille (1871-1945)

CHT184904

The Rosetta probe and the Steins asteroid - Rosetta spacecraft near asteroid Steins - Artist's view of the passage of the Rosetta probe near the Steins asteroid (2867) on September 5, 2008. The Rosetta probe was launched on 2 March 2004 in order to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Esa's Rosetta spacecraft flew by asteroid (2867) Steins on 5 September 2008 at 20:58 CEST, ground received time (= spacecraft time CEST+20 minutes), with a closest approach distance of 800 km. Steins is Rosetta's first nominal scientific target. The spacecraft encountered the asteroid in the course of its first incursion into the main asteroid belt located between the orbits of Mars and Jupiter, while on its way to Comet 67P/Churyumov - Gerasimenko

The Rosetta probe and the Steins asteroid - Rosetta spacecraft near asteroid Steins - Artist's view of the passage of the Rosetta probe near the Steins asteroid (2867) on September 5, 2008. The Rosetta probe was launched on 2 March 2004 in order to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Esa's Rosetta spacecraft flew by asteroid (2867) Steins on 5 September 2008 at 20:58 CEST, ground received time (= spacecraft time CEST+20 minutes), with a closest approach distance of 800 km. Steins is Rosetta's first nominal scientific target. The spacecraft encountered the asteroid in the course of its first incursion into the main asteroid belt located between the orbits of Mars and Jupiter, while on its way to Comet 67P/Churyumov - Gerasimenko

C. Carreau

PIX4607105

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor

Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor

S. Numazawa

PIX4583641

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen August 11, 2008. In the sky, the constellations of Persee and Cassiopee. Composite image of perseid meteors seen on august 11 2008. Above, is the constellation of Cassiopeia, and constellation of Perseus is visible at bottom right

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen August 11, 2008. In the sky, the constellations of Persee and Cassiopee. Composite image of perseid meteors seen on august 11 2008. Above, is the constellation of Cassiopeia, and constellation of Perseus is visible at bottom right

PIX4598896

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - 15 minutes in the direction of the constellation Lion. A fifteen minute exposure captures the shower radiant in Leo along with dozens on meteor trails. Nov 19, 2001

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - 15 minutes in the direction of the constellation Lion. A fifteen minute exposure captures the shower radiant in Leo along with dozens on meteor trails. Nov 19, 2001

F.Espenak

PIX4598750

Detourner un asteroide menacant - Illustration - Moving an asteroid - Illustration: Attempt to devier an asteroid threatening Earth - A spaceprobe is attached to an asteroid to push it into a non-earth impacting course

Detourner un asteroide menacant - Illustration - Moving an asteroid - Illustration: Attempt to devier an asteroid threatening Earth - A spaceprobe is attached to an asteroid to push it into a non-earth impacting course

Miller, Ron (b.1947)

PIX4583934

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

L. Bret

PIX4584062

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Walter B Myers

PIX4573224

An asteroid passes near Saturn - Artist view - Asteroid near Saturn - Artist view: A near-earth asteroid close to Saturn

An asteroid passes near Saturn - Artist view - Asteroid near Saturn - Artist view: A near-earth asteroid close to Saturn

PIX4583905

Engraving depicting a meteor shower. Dated 19th Century

Engraving depicting a meteor shower. Dated 19th Century

UIG5426073

Engraving depicting a meteor shower. Dated 19th Century

Engraving depicting a meteor shower. Dated 19th Century

UIG5426074

Asteroide P/2010 A2 seen by the space telescope Hubble - Comet-like Asteroid P/2010 A2 - P/2010 A2 is not a comet but the result of the collision between two asteroides located in the asteroid belt between Mars and Jupiter. This remains of asteroid (lower left) is about 150 metres in diameter and is accompanied by a long trail of debris and dust

Asteroide P/2010 A2 seen by the space telescope Hubble - Comet-like Asteroid P/2010 A2 - P/2010 A2 is not a comet but the result of the collision between two asteroides located in the asteroid belt between Mars and Jupiter. This remains of asteroid (lower left) is about 150 metres in diameter and is accompanied by a long trail of debris and dust

PIX4583555

Asteroids rush on Earth - Asteroids threaten the Eart

Asteroids rush on Earth - Asteroids threaten the Eart

PIX4583996

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Walter B Myers

PIX4616824

Primitive Earth - Artist's View - Early Earth: Artist's View of Earth Bombed by Asteroids About 4 Billion Years ago - This is an artist's concept of the young Earth being bombarded by asteroids

Primitive Earth - Artist's View - Early Earth: Artist's View of Earth Bombed by Asteroids About 4 Billion Years ago - This is an artist's concept of the young Earth being bombarded by asteroids

PIX4669364

Asteroids threatening the Earth - Artist view - Asteroids threaten to hit the Earth. Threatening asteroids going forward to impact Earth

Asteroids threatening the Earth - Artist view - Asteroids threaten to hit the Earth. Threatening asteroids going forward to impact Earth

P. Carril

PIX4583866

Engraving depicting the Leonids meteor shower, which was associated with the comet Tempel-Tuttle, as seen over Niagara Falls in 1833, 19th century

Engraving depicting the Leonids meteor shower, which was associated with the comet Tempel-Tuttle, as seen over Niagara Falls in 1833, 19th century

UIG5309303

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - Shooting stars and constellation Lion. On the right, the bright spot is Jupiter. November 19, 2001. The radiant of the Leonid shower is clearly seen from the many meteor trails diverging from the sickle shaped head of Leo. The Beehive Cluster (M44) is near the center while the bright 'star' to the upper right is Jupiter in Gemini. Nov 19 2001

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - Shooting stars and constellation Lion. On the right, the bright spot is Jupiter. November 19, 2001. The radiant of the Leonid shower is clearly seen from the many meteor trails diverging from the sickle shaped head of Leo. The Beehive Cluster (M44) is near the center while the bright 'star' to the upper right is Jupiter in Gemini. Nov 19 2001

F.Espenak

PIX4598734

Primitive Earth - Artist's View - Ancient terrestrial landscape - Artist's view of the Earth about 4 billion years ago. Volcanoes dominate the landscape. This is how the surface of the Earth may have appeared beneath its clouds about 500 million years after its birth. Massive volcanoes and lava fields still dominate the landscape. In a few million years rain will begin falling, further cooling the crust. In about another 200 million years the first living microbes will call the Earth home

Primitive Earth - Artist's View - Ancient terrestrial landscape - Artist's view of the Earth about 4 billion years ago. Volcanoes dominate the landscape. This is how the surface of the Earth may have appeared beneath its clouds about 500 million years after its birth. Massive volcanoes and lava fields still dominate the landscape. In a few million years rain will begin falling, further cooling the crust. In about another 200 million years the first living microbes will call the Earth home

Walter B Myers

PIX4632690

An asteroid hits the Earth - An asteroid hits the Earth - An asteroid hits the Earth. An asteroid collides with the earth

An asteroid hits the Earth - An asteroid hits the Earth - An asteroid hits the Earth. An asteroid collides with the earth

PIX4583694

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

Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to tran

Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to tran

Walter B Myers

PIX4640726

Engraving depicting the Leonids meteor shower, which was associated with the comet Tempel-Tuttle, as seen over Niagara Falls in 1833, 19th century

Engraving depicting the Leonids meteor shower, which was associated with the comet Tempel-Tuttle, as seen over Niagara Falls in 1833, 19th century

UIG5309420

An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie

An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie

P. Carril

PIX4583907

Engraving depicting a meteor shower. Dated 19th Century

Engraving depicting a meteor shower. Dated 19th Century

UIG5426069

Engraving depicting a meteor shower. Dated 19th Century

Engraving depicting a meteor shower. Dated 19th Century

UIG5426084

Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

PIX4569144

An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie

An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie

P. Carril

PIX4583913

Exoplanete in formation - NGC 2547-ID8: Illustration of the collision between two asteroids in the habitable zone of the star NGC 2547-ID8. This could result in an accretion-forming rocky exoplanet. Planets, including those like our own Earth, form from epic collisions between asteroids and even bigger bodies, called proto-planets. Sometimes the colliding bodies are ground to dust, and sometimes they stick together to ultimately form larger, mature planets. This artist's conception shows one such smash-up. Spitzer's infrared vision detected a huge eruption around the star NGC 2547-ID8 between August 2012 and 2013. Scientists think the dust was kicked up by a massive collision between two large asteroids. They say the smashup took place in the star's “” terrestrial zone,””” the region around stars where rocky planets like Earth take shape. NGC 2547-ID8 is a sun-like star located about 1,200 light-years from Earth in the constellation Vela. It is about 35 million years old, the same age

Exoplanete in formation - NGC 2547-ID8: Illustration of the collision between two asteroids in the habitable zone of the star NGC 2547-ID8. This could result in an accretion-forming rocky exoplanet. Planets, including those like our own Earth, form from epic collisions between asteroids and even bigger bodies, called proto-planets. Sometimes the colliding bodies are ground to dust, and sometimes they stick together to ultimately form larger, mature planets. This artist's conception shows one such smash-up. Spitzer's infrared vision detected a huge eruption around the star NGC 2547-ID8 between August 2012 and 2013. Scientists think the dust was kicked up by a massive collision between two large asteroids. They say the smashup took place in the star's “” terrestrial zone,””” the region around stars where rocky planets like Earth take shape. NGC 2547-ID8 is a sun-like star located about 1,200 light-years from Earth in the constellation Vela. It is about 35 million years old, the same age

PIX4608473

Lunar base - Illustration - Small lunar base - Artist's view of a first lunar base, ahead of a larger permanent installation. This is an artist's concept of a small lunar outpost. Someday, larger lunar outposts may serve as a backup for civilization in case of a global catastrophe, like an asteroid impact or a pandemic

Lunar base - Illustration - Small lunar base - Artist's view of a first lunar base, ahead of a larger permanent installation. This is an artist's concept of a small lunar outpost. Someday, larger lunar outposts may serve as a backup for civilization in case of a global catastrophe, like an asteroid impact or a pandemic

PIX4638830

La formation du système solaire - Vue d'artiste - Artist's impression of the development of the Solar System - Vue d'artiste de planete en formation dans le disque de gaz et de dusts (disque protoplanetaire) autour de son toile. This artist's impression shows four stages of the development of the inner Solar System over a period of almost five billion years. The top panel shows the earliest stage where the debris disc around the Sun was composed of gas and tiny particles, typically less than one millimetre across. At the second stage the particles have formed large clumps, roughly 100 kilometers across and, similar to the asteroid Lutetia. These bodies in turn formed the rocky planets including the Earth, shown in the third panel down. Over the subsequent four billion years the surface of the Earth developed to what we know now under the influence of meteor bombardment that delivered volatile materials including water, and the evolution of life on its surface

La formation du système solaire - Vue d'artiste - Artist's impression of the development of the Solar System - Vue d'artiste de planete en formation dans le disque de gaz et de dusts (disque protoplanetaire) autour de son toile. This artist's impression shows four stages of the development of the inner Solar System over a period of almost five billion years. The top panel shows the earliest stage where the debris disc around the Sun was composed of gas and tiny particles, typically less than one millimetre across. At the second stage the particles have formed large clumps, roughly 100 kilometers across and, similar to the asteroid Lutetia. These bodies in turn formed the rocky planets including the Earth, shown in the third panel down. Over the subsequent four billion years the surface of the Earth developed to what we know now under the influence of meteor bombardment that delivered volatile materials including water, and the evolution of life on its surface

PIX4630355

Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems

Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems

Walter B Myers

PIX4572541

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

An asteroid threatens the Earth - An asteroid threatens the Earth - Photomontage Composite image

An asteroid threatens the Earth - An asteroid threatens the Earth - Photomontage Composite image

PIX4583850

Mine sur un asteroide - Illustration - Asteroid mining outpost - Artist's view a mining base installed on an asteroid. A massive manned mining outpost is built around a rocky near - Earth asteroid about 300 million miles from Earth. In the foreground are arrays of solar photovoltaic panels similar to those currently supplying power to the International Space Station (ISS). This oblong asteroid is approximately 2,000 feet long by 1,000 feet wide. The mining base and its supporting structure is almost one - half statute mile long

Mine sur un asteroide - Illustration - Asteroid mining outpost - Artist's view a mining base installed on an asteroid. A massive manned mining outpost is built around a rocky near - Earth asteroid about 300 million miles from Earth. In the foreground are arrays of solar photovoltaic panels similar to those currently supplying power to the International Space Station (ISS). This oblong asteroid is approximately 2,000 feet long by 1,000 feet wide. The mining base and its supporting structure is almost one - half statute mile long

Walter B Myers

PIX4640719

Mine sur un asteroide - Illustration - Asteroid mining outpost - Artist's view a mining base installed on an asteroid. A massive manned mining outpost is built around a rocky near - Earth asteroid about 300 million miles from Earth. This oblong asteroid is approximately 2,000 feet long by 1,000 feet wide. The mining base and its supporting structure is almost one - half statute mile long

Mine sur un asteroide - Illustration - Asteroid mining outpost - Artist's view a mining base installed on an asteroid. A massive manned mining outpost is built around a rocky near - Earth asteroid about 300 million miles from Earth. This oblong asteroid is approximately 2,000 feet long by 1,000 feet wide. The mining base and its supporting structure is almost one - half statute mile long

Walter B Myers

PIX4640756

Megatsunami - Artist's view - While a tsunami is affected by the movements of the earth's crust, a megatsunami can be caused by a colossal collapse or the fall of an asteroid, causing powerful waves up to hundreds of metres in height. Megatsunami is an informal term to describe a tsunami that has initial wave heights that are much larger than normal tsunamis. Unlike usual tsunamis - which originate from tectonic activity and the raising or lowering of the sea floor - known megatsunamis have originated from a large scale landslide, collision, or volcanic eruption event

Megatsunami - Artist's view - While a tsunami is affected by the movements of the earth's crust, a megatsunami can be caused by a colossal collapse or the fall of an asteroid, causing powerful waves up to hundreds of metres in height. Megatsunami is an informal term to describe a tsunami that has initial wave heights that are much larger than normal tsunamis. Unlike usual tsunamis - which originate from tectonic activity and the raising or lowering of the sea floor - known megatsunamis have originated from a large scale landslide, collision, or volcanic eruption event

PIX4632948

Mini Moons Earth Collision Illustration, 2018

Mini Moons Earth Collision Illustration, 2018

Roetsch, Tobias

KBS7281917

Know Your London, 1951 (colour litho)

Know Your London, 1951 (colour litho)

Nevin (fl.1951)

PST2907119

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