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'Artist's Telescope' images and/or videos results page 91 of 2

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Images of 'Artist's Telescope' found, 106

 
Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France

PIX4573375

Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France

PIX4573375

 
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Imaginary solar system, c 2005

UIS5104217

Imaginary solar system, c 2005

UIS5104217

 
Beta Pictoris b - Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbiting 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. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell - tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth - Sun separation -

PIX4574181

Beta Pictoris b - Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbiting 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. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell - tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth - Sun separation -

PIX4574181

 
Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

PIX4573193

Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

PIX4573193

 
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573989

Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573989

 
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4574021

Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4574021

 
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Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

Miller, Ron (b.1947)

PIX4574012

Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

Miller, Ron (b.1947)

PIX4574012

 
Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

PIX4573201

Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

PIX4573201

 
Hypergeante Star HR 5171 - Illustration: This artist view shows the yellow hypergeant star HR 5171. It is a very rare star of which only a dozen people our galaxy. Its dimensions are more than 1300 times greater than those of the Sun, making it one of the ten largest stars discovered to date. Observations have shown that it is actually a double star, whose companion is in direct contact with the main star. This artist's impression shows the yellow hypergiant star HR 5171. This is a very rare type of star with only a dozen known in our galaxy. Its size is over 1300 times that of our Sun - one of the largest ten stars found so far. Observations with Eso's Very Large Telescope Interferometer have shown that it is actually a double star, with the companion in contact with the main star

PIX4572123

Hypergeante Star HR 5171 - Illustration: This artist view shows the yellow hypergeant star HR 5171. It is a very rare star of which only a dozen people our galaxy. Its dimensions are more than 1300 times greater than those of the Sun, making it one of the ten largest stars discovered to date. Observations have shown that it is actually a double star, whose companion is in direct contact with the main star. This artist's impression shows the yellow hypergiant star HR 5171. This is a very rare type of star with only a dozen known in our galaxy. Its size is over 1300 times that of our Sun - one of the largest ten stars found so far. Observations with Eso's Very Large Telescope Interferometer have shown that it is actually a double star, with the companion in contact with the main star

PIX4572123

 
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573980

Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573980

 
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573990

Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist

PIX4573990

 
Exoplanete Gliese 667 Cb - The system Gliese 667 (Artist's impression) - Gliese 667 Cb is an exoplanet orbiting the star Gliese 667 C, located about 23 years ago - light 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. 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 telescope, reported on the incredible discovery of some 32 new exoplanets, cementing Harps's position as the world's foremost exoplanet hunter. One of these is surrounding the star Gliese 667 C, which belongs to a triple system. The 6 Earth - mass exoplanet circulates around its low - mass host star at a distance equal to only 1/20th of the Earth - Sun distance. The host star is a companion to two other low - mass stars, which are seen here in the distance

PIX4574001

Exoplanete Gliese 667 Cb - The system Gliese 667 (Artist's impression) - Gliese 667 Cb is an exoplanet orbiting the star Gliese 667 C, located about 23 years ago - light 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. 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 telescope, reported on the incredible discovery of some 32 new exoplanets, cementing Harps's position as the world's foremost exoplanet hunter. One of these is surrounding the star Gliese 667 C, which belongs to a triple system. The 6 Earth - mass exoplanet circulates around its low - mass host star at a distance equal to only 1/20th of the Earth - Sun distance. The host star is a companion to two other low - mass stars, which are seen here in the distance

PIX4574001

 
Primitive black hole - Artist view - Primitive Black hole - Artist view - Artist view of a primitive galactic black hole. The presence of 13 billion-year-old black holes was observed by the Spitzer space telescope. These distant black holes appear in the early stages of their formation; their accretion disc contains no dust. This artist's conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy. Astronomers using Nasa's Spitzer Space Telescope have uncovered two of these early objects, dating back to about 13 billion years ago. The monstrous black holes are among the most distant known, and appear to be in the very earliest stages of formation, earlier than any observed so far. Unlike all other supermassive black holes probed to date, this primitive duo, called J0005-0006 and J0303-0019, lacks dust. As the drawing shows, gas swirls around a black hole in what is called an accretion disk. Usually, the ac

PIX4584544

Primitive black hole - Artist view - Primitive Black hole - Artist view - Artist view of a primitive galactic black hole. The presence of 13 billion-year-old black holes was observed by the Spitzer space telescope. These distant black holes appear in the early stages of their formation; their accretion disc contains no dust. This artist's conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy. Astronomers using Nasa's Spitzer Space Telescope have uncovered two of these early objects, dating back to about 13 billion years ago. The monstrous black holes are among the most distant known, and appear to be in the very earliest stages of formation, earlier than any observed so far. Unlike all other supermassive black holes probed to date, this primitive duo, called J0005-0006 and J0303-0019, lacks dust. As the drawing shows, gas swirls around a black hole in what is called an accretion disk. Usually, the ac

PIX4584544

 
Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

PIX4573892

Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

PIX4573892

 
Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Walter B Myers

PIX4639150

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Walter B Myers

PIX4639150

 
Artemis communication satellite - Artemis satellite communication. Artwork - Artist's view of the European satellite Artemis (Advanced Relay and Technology Mission). Communication and relay satellite for other satellites, it was launched in July 2001. Built by ESA with an industrial team led by Italy's Alenia Spazio, Artemis carries three payloads plus a number of experiments developed to demonstrate new telecommunications technologies. The L - band Land Mobile (LLM) payload provides relay for two - way voice and data communications between fixed Earth stations and land mobiles - trucks, trains or cars - anywhere in Europe and North Africa. LLM is also broadcasting corrective GPS - like navigation signals for the European Global Navigation Overlay Service (EGNOS) programme, Europe's first satellite navigation system and a forerunner to the Galileo global navigation system. The other two primary payloads are designed to provide direct high data rate communications links between satellit

J. Huart

PIX4642928

Artemis communication satellite - Artemis satellite communication. Artwork - Artist's view of the European satellite Artemis (Advanced Relay and Technology Mission). Communication and relay satellite for other satellites, it was launched in July 2001. Built by ESA with an industrial team led by Italy's Alenia Spazio, Artemis carries three payloads plus a number of experiments developed to demonstrate new telecommunications technologies. The L - band Land Mobile (LLM) payload provides relay for two - way voice and data communications between fixed Earth stations and land mobiles - trucks, trains or cars - anywhere in Europe and North Africa. LLM is also broadcasting corrective GPS - like navigation signals for the European Global Navigation Overlay Service (EGNOS) programme, Europe's first satellite navigation system and a forerunner to the Galileo global navigation system. The other two primary payloads are designed to provide direct high data rate communications links between satellit

J. Huart

PIX4642928

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