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Images of 'Artist's Impression' found, 346

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Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

PIX4608398

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

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

PIX4608435

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

PIX4653093

Exoplanete Gliese 581d - Illustration - Artist's view of the star Gliese 581 in the sky of the extrasolar planet Gliese 581 d. Discovered in 20074, this exoplanet in the constellation Libra is considered to be potentially habitable. The atmosphere is dense and its thick cloud layer would plunge the surface into a reddish shade. Artist's impression of the star red dwarf Gliese 581 shining in the sky of the extrasolar planet Gliese 581 d. This exoplanet located in the habitable zone of its star could harbor extraterrestrial life

Exoplanete Gliese 581d - Illustration - Artist's view of the star Gliese 581 in the sky of the extrasolar planet Gliese 581 d. Discovered in 20074, this exoplanet in the constellation Libra is considered to be potentially habitable. The atmosphere is dense and its thick cloud layer would plunge the surface into a reddish shade. Artist's impression of the star red dwarf Gliese 581 shining in the sky of the extrasolar planet Gliese 581 d. This exoplanet located in the habitable zone of its star could harbor extraterrestrial life

Miller, Ron (b.1947)

PIX4574024

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

D. Ducros

PIX4604495

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

PIX4653094

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

PIX4608442

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

D. Ducros

PIX4604515

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

PIX4653104

H.M.S. Pinafore

H.M.S. Pinafore

XLE3749481

Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of Planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the image. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of Planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the image. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

Miller, Ron (b.1947)

PIX4608073

Future Concepts Drawing of future lunar outpost, 1988

Future Concepts Drawing of future lunar outpost, 1988

UIS5073168

Artist's view of an asteroid Amor near Mars - Artist impression of Amor asteroid near Mars: Amor asteroids are a family of asteroids that cross the orbit of Mars but not that of Earth. They are thus named after the asteroid (1221) Amor. The Amor asteroids are a group of near-earth asteroids named after the asteroid 1221 Amor. They approach the orbit of Earth from beyond, but do not cross it

Artist's view of an asteroid Amor near Mars - Artist impression of Amor asteroid near Mars: Amor asteroids are a family of asteroids that cross the orbit of Mars but not that of Earth. They are thus named after the asteroid (1221) Amor. The Amor asteroids are a group of near-earth asteroids named after the asteroid 1221 Amor. They approach the orbit of Earth from beyond, but do not cross it

Miller, Ron (b.1947)

PIX4584181

Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune

Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune

PIX4607276

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

PIX4653099

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

PIX4572892

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

PIX4572795

Supernova 1993J exploding (artist's impression) - In 1993 the supernova SN 1993J appeared in the galaxy M81. The illustration shows the supergiant red star exploding after transferring a huge mass of hydrogen to its companion star (right). In this artist's view the red supergiant supernova progenitor star (left) is exploding after having transferred about 10 solar masses of hydrogen gas to the blue companion star (right). This interaction process happened over about 250 years and affected the supernova explosion to such an extent that SN 1993J was later known as one of the most peculiar supernovae ever seen

Supernova 1993J exploding (artist's impression) - In 1993 the supernova SN 1993J appeared in the galaxy M81. The illustration shows the supergiant red star exploding after transferring a huge mass of hydrogen to its companion star (right). In this artist's view the red supergiant supernova progenitor star (left) is exploding after having transferred about 10 solar masses of hydrogen gas to the blue companion star (right). This interaction process happened over about 250 years and affected the supernova explosion to such an extent that SN 1993J was later known as one of the most peculiar supernovae ever seen

PIX4583292

H.M.S. Pinafore

H.M.S. Pinafore

XLE3750165

Fusee Ariane 5 ECA - Illustration - The Ariane 5 ECA rocket - Illustration - Cross-section view of the Ariane 5 ECA rocket, the version of Ariane 5 can put into geostationary transfer orbit a load of up to ten tons. Artist's impression of the Ariane 5 ECA, the version of Ariane 5 with a Geostationary Transfer Orbit launch capacity of 10,000 kilograms

Fusee Ariane 5 ECA - Illustration - The Ariane 5 ECA rocket - Illustration - Cross-section view of the Ariane 5 ECA rocket, the version of Ariane 5 can put into geostationary transfer orbit a load of up to ten tons. Artist's impression of the Ariane 5 ECA, the version of Ariane 5 with a Geostationary Transfer Orbit launch capacity of 10,000 kilograms

D. Ducros

PIX4604451

Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a Wolf-Rayet star orbiting a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. This artist's impression depicts a star-mass black hole. The black hole has a mass of about twenty times the mass of the Sun and is associated with a Wolf-Rayet star: a star that will become a black hole itself. The black hole is stripping matter away from the star as they orbit each other

Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a Wolf-Rayet star orbiting a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. This artist's impression depicts a star-mass black hole. The black hole has a mass of about twenty times the mass of the Sun and is associated with a Wolf-Rayet star: a star that will become a black hole itself. The black hole is stripping matter away from the star as they orbit each other

PIX4584795

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 40 - metre - class E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 40 - metre - class E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

PIX4653079

Fusee Ariane 5 ECA - Illustration - The Ariane 5 ECA rocket - Illustration - Cross-section view of the Ariane 5 ECA rocket, the version of Ariane 5 can put into geostationary transfer orbit a load of up to ten tons. Artist's impression of the Ariane 5 ECA, the version of Ariane 5 with a Geostationary Transfer Orbit launch capacity of 10,000 kilograms

Fusee Ariane 5 ECA - Illustration - The Ariane 5 ECA rocket - Illustration - Cross-section view of the Ariane 5 ECA rocket, the version of Ariane 5 can put into geostationary transfer orbit a load of up to ten tons. Artist's impression of the Ariane 5 ECA, the version of Ariane 5 with a Geostationary Transfer Orbit launch capacity of 10,000 kilograms

D. Ducros

PIX4604449

Satellite ENVISAT - Artist's impression of Envisat - Artist's view of the cover of the Ariane 5 rocket opening to put the European ENVISAT satellite into orbit around the Earth. Launched on March 1, 2002, it is the largest scientific Earth observation satellite ever designed, observing the Earth in visible, infrared and radar. Artwork showing the Ariane 5 fairing ejection before Envisat separation from the upper stage. Launched in 2002, Envisat is the largest Earth Observation spacecraft ever built. It carries ten sophisticated optical and radar instruments to provide continuous observation and monitoring of the Earth's land, atmosphere, oceans and ice caps

Satellite ENVISAT - Artist's impression of Envisat - Artist's view of the cover of the Ariane 5 rocket opening to put the European ENVISAT satellite into orbit around the Earth. Launched on March 1, 2002, it is the largest scientific Earth observation satellite ever designed, observing the Earth in visible, infrared and radar. Artwork showing the Ariane 5 fairing ejection before Envisat separation from the upper stage. Launched in 2002, Envisat is the largest Earth Observation spacecraft ever built. It carries ten sophisticated optical and radar instruments to provide continuous observation and monitoring of the Earth's land, atmosphere, oceans and ice caps

D. Ducros

PIX4644506

George Stephenson (1781-1848)

George Stephenson (1781-1848)

UIG863791

Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a star orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space where gravity is so strong that it stops any form of material or radiation from escaping. Combining observations done with Eso's Very Large Telescope and Nasa's Chandra X-ray telescope, astronomers have uncovered the most powerful pair of jets ever seen from a stellar black hole. The black hole blows a huge bubble of hot gas, 1000 light-years across or twice as large and tens of times more powerful than the other such microquasars. The stellar black hole belongs to a binary system as pictured in this artist's impression

Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a star orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space where gravity is so strong that it stops any form of material or radiation from escaping. Combining observations done with Eso's Very Large Telescope and Nasa's Chandra X-ray telescope, astronomers have uncovered the most powerful pair of jets ever seen from a stellar black hole. The black hole blows a huge bubble of hot gas, 1000 light-years across or twice as large and tens of times more powerful than the other such microquasars. The stellar black hole belongs to a binary system as pictured in this artist's impression

PIX4584773

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

PIX4643733

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a huge exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a huge exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc

Miller, Ron (b.1947)

PIX4608453

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected; the probe measures 32 meters with its deployed panels; the core of the comet about 4 km.; Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko.; The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays; while the comet nucleus is thought to be about 4 km wide

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected; the probe measures 32 meters with its deployed panels; the core of the comet about 4 km.; Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko.; The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays; while the comet nucleus is thought to be about 4 km wide

PIX4607178

World War II. Futuristic German weapons to attack Britain.

World War II. Futuristic German weapons to attack Britain.

XLF3781096

World War II,futuristic German weapons to invade Britain.'

World War II,futuristic German weapons to invade Britain.'

XLF3781095

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide

PIX4607171

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

Gravitational Waves - Gravitational Waves: Two colliding neutron stars create a gravitational wave that spreads over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017.

Gravitational Waves - Gravitational Waves: Two colliding neutron stars create a gravitational wave that spreads over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017.

Dixon, Don (b.1951)

PIX4607592

The Rosetta probe near the Earth - Rosetta spacecraft over Earth - Artist's view of the passage of the Rosetta probe near the Earth. The purpose of this passage is to use the gravity of the planet to modify the velocity and trajectory of the probe. The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Artist's impression of Rosetta spacecraft over Earth. The aim of the transit is to use the planet's gravity to modify the speed and the trajectory of the probe. The European Space Agency spacecraft was launched on March 02 2004 and intended to study the comet 67P/Churyumov - Gerasimenko. Rosetta is expected to enter in orbit around the comet for releasing a lander in May 2014

The Rosetta probe near the Earth - Rosetta spacecraft over Earth - Artist's view of the passage of the Rosetta probe near the Earth. The purpose of this passage is to use the gravity of the planet to modify the velocity and trajectory of the probe. The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Artist's impression of Rosetta spacecraft over Earth. The aim of the transit is to use the planet's gravity to modify the speed and the trajectory of the probe. The European Space Agency spacecraft was launched on March 02 2004 and intended to study the comet 67P/Churyumov - Gerasimenko. Rosetta is expected to enter in orbit around the comet for releasing a lander in May 2014

C. Carreau

PIX4607029

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702152

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702153

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of a gravitational wave generated by a system of two neutron stars in collision, spreading over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017. A couple of seconds after that, ESA's Integral and Nasa's Fermi satellites detected a burst of gamma rays, the luminous counterpart to the gravitational waves emitted by the cosmic clash. This is the first discovery of gravitational waves and light coming from the same source

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of a gravitational wave generated by a system of two neutron stars in collision, spreading over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017. A couple of seconds after that, ESA's Integral and Nasa's Fermi satellites detected a burst of gamma rays, the luminous counterpart to the gravitational waves emitted by the cosmic clash. This is the first discovery of gravitational waves and light coming from the same source

PIX4607575

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Miller, Ron (b.1947)

PIX4974341

German railway gun on the English Channel coast, World War II, 1940 (lithograph)

German railway gun on the English Channel coast, World War II, 1940 (lithograph)

Liska, Hans (1907-84)

XLF3781098

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702151

August 24, 2016: Artist's view of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible between the planet and the star Proxima. Proxima b is a little more massive than Earth, orbit in habitable area or temperature would allow the presence of liquid water on its surface - This artist's impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

August 24, 2016: Artist's view of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible between the planet and the star Proxima. Proxima b is a little more massive than Earth, orbit in habitable area or temperature would allow the presence of liquid water on its surface - This artist's impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

PIX4650952

Satellite ENVISAT - Artist's impression of Envisat - ENVISAT artist view Location: Credit line: ESA - Silicon Worlds View of European satellite artist ENVISAT orbit the Earth. Launched on March 1, 2002, it is the largest scientific Earth observation satellite ever designed, observing the Earth in visible, infrared and radar. Launched in 2002, Envisat is the largest Earth Observation spacecraft ever built. It carries ten sophisticated optical and radar instruments to provide continuous observation and monitoring of the Earth's land, atmosphere, oceans and ice caps

Satellite ENVISAT - Artist's impression of Envisat - ENVISAT artist view Location: Credit line: ESA - Silicon Worlds View of European satellite artist ENVISAT orbit the Earth. Launched on March 1, 2002, it is the largest scientific Earth observation satellite ever designed, observing the Earth in visible, infrared and radar. Launched in 2002, Envisat is the largest Earth Observation spacecraft ever built. It carries ten sophisticated optical and radar instruments to provide continuous observation and monitoring of the Earth's land, atmosphere, oceans and ice caps

PIX4644503

Future Concepts Boeing high-speed civil transport concept, 1994

Future Concepts Boeing high-speed civil transport concept, 1994

UIS5073913

Satellite Sentinel - 2 - Artist view - Sentinel - 2 satellite - Artist view - Viewing of European satellite Sentinel - 2. This Earth observation satellite belongs to the Global Monitoring for Environment and Security (GMES) Earth Monitoring Satellite Network, which will study the changes in the Earth's environment. The launch of Sentinel-2 is scheduled for 2012. Artist's impression of the European Sentinel - 2 spacecraft in Earth orbit. The ESA Sentinels, composed of five satellites are responding to the needs of the GMES (Global Monitoring for Environment and Security) programme. Sentinel - 2 is scheduled to be launched in 2012

Satellite Sentinel - 2 - Artist view - Sentinel - 2 satellite - Artist view - Viewing of European satellite Sentinel - 2. This Earth observation satellite belongs to the Global Monitoring for Environment and Security (GMES) Earth Monitoring Satellite Network, which will study the changes in the Earth's environment. The launch of Sentinel-2 is scheduled for 2012. Artist's impression of the European Sentinel - 2 spacecraft in Earth orbit. The ESA Sentinels, composed of five satellites are responding to the needs of the GMES (Global Monitoring for Environment and Security) programme. Sentinel - 2 is scheduled to be launched in 2012

P. Carril

PIX4644339

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (front view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (front view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

PIX4607164

Arches star cluster, c 2000

Arches star cluster, c 2000

UIS5104188

Artist's impression of sunset on the super - Earth world Gliese 667 Cc - This artist's view represents a sunset seen from Super Earth Gliese 667Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B also appear right in the sky. Gliese 667 Cc is an exoplanet orbiting the star Gliese 667 C, located about 23 years from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. This artist's impression shows a sunset seen from the super - Earth Gliese 667 Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B appear in the sky also to the right. On 19 October 2009, the team who built the High Accuracy Radial Velocity Planet Searcher, better known as HARPS, the spectrograph for ESO's 3.6 - metre te

Artist's impression of sunset on the super - Earth world Gliese 667 Cc - This artist's view represents a sunset seen from Super Earth Gliese 667Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B also appear right in the sky. Gliese 667 Cc is an exoplanet orbiting the star Gliese 667 C, located about 23 years from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. This artist's impression shows a sunset seen from the super - Earth Gliese 667 Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B appear in the sky also to the right. On 19 October 2009, the team who built the High Accuracy Radial Velocity Planet Searcher, better known as HARPS, the spectrograph for ESO's 3.6 - metre te

PIX4573998

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Miller, Ron (b.1947)

PIX4643682

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

PIX4607586

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (back view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (back view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

PIX4607152

Artist's view of the Exoplanet HD 189733b - Exoplanet HD 189733b - Artist's view of the transit of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. Using the Hubble space telescope, astronomers have detected carbon dioxide and monoxide in the atmosphere of this planet. Previously, methane and water vapour had already been detected in his atmosphere. But with a surface temperature of over 900 degrees, this planet remains too hot to shelter life. This is an artist's impression of the Jupiter - size extrasolar planet, HD 189733b, being eclipsed by its parent star. Astronomers using the Hubble Space Telescope have measured carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a “” hot Jupiter,””” which is so close to its star that it completes an orbit in only 2.2 days. The planet is too hot for life as we know it. But under the right conditions,

Artist's view of the Exoplanet HD 189733b - Exoplanet HD 189733b - Artist's view of the transit of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. Using the Hubble space telescope, astronomers have detected carbon dioxide and monoxide in the atmosphere of this planet. Previously, methane and water vapour had already been detected in his atmosphere. But with a surface temperature of over 900 degrees, this planet remains too hot to shelter life. This is an artist's impression of the Jupiter - size extrasolar planet, HD 189733b, being eclipsed by its parent star. Astronomers using the Hubble Space Telescope have measured carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a “” hot Jupiter,””” which is so close to its star that it completes an orbit in only 2.2 days. The planet is too hot for life as we know it. But under the right conditions,

PIX4573420

The Huygens probe is on Titan - Artist view - Huygens Titan descent - Artist view - Artist view of the descent of the European probe Huygens on Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's impression shows the Probe Huygens suspended from the stabilizer parachute passing through the clouds that are expected at around 20 km altitude. The descent will occur during daylight to provide the best illumination conditions for imaging the clouds and surface

The Huygens probe is on Titan - Artist view - Huygens Titan descent - Artist view - Artist view of the descent of the European probe Huygens on Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's impression shows the Probe Huygens suspended from the stabilizer parachute passing through the clouds that are expected at around 20 km altitude. The descent will occur during daylight to provide the best illumination conditions for imaging the clouds and surface

PIX4606129

August 24, 2016: Artist's view of the surface of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the star Proxima. Proxima b is a little more massive than the Earth, orbit in habitable area where the temperature would allow the presence of liquid water on its surface - This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

August 24, 2016: Artist's view of the surface of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the star Proxima. Proxima b is a little more massive than the Earth, orbit in habitable area where the temperature would allow the presence of liquid water on its surface - This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

PIX4650935

Exoplanete Alpha Centauri Bb - Artist's impression of the planet orbiting Alpha Centauri B: Artist's view of the planet Alpha Centauri Bb, also known as Gliese 559 Bb. Discovered in 2012 its existence is questioned. It would be orbiting the dwarf star Alpha Centauri B at a distance of 4.37 light years in the constellation Centauri. The planet is not in the habitable zone of the star, as it orbits far too close to the star. Alpha Centauri Bb was a proposed exoplanet orbiting the K-type main-sequence star Alpha Centauri B, located 4.37 light-years from Earth in the southern constellation of Centaurus. Its existence was announced in October 2012 but in October 2015, a scientific paper disproved the existence of the planet. Alpha Centauri B dominates the sky. Just above it to the right is a very bright star: Alpha Centauri A. And above that to the right is another star: our sun

Exoplanete Alpha Centauri Bb - Artist's impression of the planet orbiting Alpha Centauri B: Artist's view of the planet Alpha Centauri Bb, also known as Gliese 559 Bb. Discovered in 2012 its existence is questioned. It would be orbiting the dwarf star Alpha Centauri B at a distance of 4.37 light years in the constellation Centauri. The planet is not in the habitable zone of the star, as it orbits far too close to the star. Alpha Centauri Bb was a proposed exoplanet orbiting the K-type main-sequence star Alpha Centauri B, located 4.37 light-years from Earth in the southern constellation of Centaurus. Its existence was announced in October 2012 but in October 2015, a scientific paper disproved the existence of the planet. Alpha Centauri B dominates the sky. Just above it to the right is a very bright star: Alpha Centauri A. And above that to the right is another star: our sun

Miller, Ron (b.1947)

PIX4608127

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606969

Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings

Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings

Miller, Ron (b.1947)

PIX4584199

Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings

Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings

Miller, Ron (b.1947)

PIX4584208

Satellite Sentinel - 2 - Artist view - Sentinel - 2 satellite - Artist view - Artist view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite belongs to the Global Monitoring for Environment and Security (GMES) Earth Monitoring Satellite Network, which will study the changes in the Earth's environment. The launch of Sentinel-2 is scheduled for 2012. Artist's impression of the European Sentinel - 2 spacecraft in Earth orbit. The ESA Sentinels, composed of five satellites are responding to the needs of the GMES (Global Monitoring for Environment and Security) programme. Sentinel - 2 is scheduled to be launched in 2012

Satellite Sentinel - 2 - Artist view - Sentinel - 2 satellite - Artist view - Artist view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite belongs to the Global Monitoring for Environment and Security (GMES) Earth Monitoring Satellite Network, which will study the changes in the Earth's environment. The launch of Sentinel-2 is scheduled for 2012. Artist's impression of the European Sentinel - 2 spacecraft in Earth orbit. The ESA Sentinels, composed of five satellites are responding to the needs of the GMES (Global Monitoring for Environment and Security) programme. Sentinel - 2 is scheduled to be launched in 2012

P. Carril

PIX4644325

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