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Images of 'Extrasolar Planet' found, 246

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Exoplanete Kelt-11b - Artist's view of Kelt-11b orbiting his star KELT-11, located 320 light years from Earth in the constellation of the Lion. Kelt-11b is an exoplanet larger than Jupiter and very close to its star. It was discovered in 2016. Kelt-11b is an exoplanet orbiting around the yellow subgiant star KELT-11 about 320 light-years away from Earth

Exoplanete Kelt-11b - Artist's view of Kelt-11b orbiting his star KELT-11, located 320 light years from Earth in the constellation of the Lion. Kelt-11b is an exoplanet larger than Jupiter and very close to its star. It was discovered in 2016. Kelt-11b is an exoplanet orbiting around the yellow subgiant star KELT-11 about 320 light-years away from Earth

Miller, Ron (b.1947)

PIX4945226

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

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

D. Ducros

PIX4573918

Voyager and Exoplanets Probe - Voyager entering an alien solar system Artist's view showing one of the probes approaching another solar system

Voyager and Exoplanets Probe - Voyager entering an alien solar system Artist's view showing one of the probes approaching another solar system

Miller, Ron (b.1947)

PIX4643456

Exoplanete HD 188015 b: HD 188015 b is an exoplanet slightly larger than Jupiter, located in the constellation Little Fox. HD 188015 b is an extrasolar planet with a minimum mass about quarter greater than Jupiter. Discovered in 2005 it is located in Vulpecula constellation

Exoplanete HD 188015 b: HD 188015 b is an exoplanet slightly larger than Jupiter, located in the constellation Little Fox. HD 188015 b is an extrasolar planet with a minimum mass about quarter greater than Jupiter. Discovered in 2005 it is located in Vulpecula constellation

Miller, Ron (b.1947)

PIX4608499

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

Artist's view of the 1st discovered exoplanet-51 Peg b - Artwork of 51 Peg b, the first exoplanet discovered: This exoplanet located in the constellation of Pegase, about 48 light years from Earth, is the first discovered exoplanet in 1995. It is a big gas planet very close to its star 51 Pegasi. This type of exoplanet is called a hot Jupiter. Artistic view of 51 Peg b, the first exoplanet discovered in 1995. It is a hot Jupiter type located 48 light-year from the earth in Pegasus constellation

Artist's view of the 1st discovered exoplanet-51 Peg b - Artwork of 51 Peg b, the first exoplanet discovered: This exoplanet located in the constellation of Pegase, about 48 light years from Earth, is the first discovered exoplanet in 1995. It is a big gas planet very close to its star 51 Pegasi. This type of exoplanet is called a hot Jupiter. Artistic view of 51 Peg b, the first exoplanet discovered in 1995. It is a hot Jupiter type located 48 light-year from the earth in Pegasus constellation

Miller, Ron (b.1947)

PIX4607862

Exoplanete Kepler-64 b: Kepler-64 b or PH1 b (Planet Hunters 1b), is a circumbinary extrasolar planet belonging to the Quadruple Star System Kepler-64 (PH1). PH1b would be a giant gas planet. pH1b (standing for “” Planet Hunters 1””), or by its NASA designation Kepler-64b, is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The giant planet is Neptune-sized, about 20-55 Earth-masses, located 5000 light years from Earth in Cygnus constellation

Exoplanete Kepler-64 b: Kepler-64 b or PH1 b (Planet Hunters 1b), is a circumbinary extrasolar planet belonging to the Quadruple Star System Kepler-64 (PH1). PH1b would be a giant gas planet. pH1b (standing for “” Planet Hunters 1””), or by its NASA designation Kepler-64b, is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The giant planet is Neptune-sized, about 20-55 Earth-masses, located 5000 light years from Earth in Cygnus constellation

Miller, Ron (b.1947)

PIX4608219

Life on a low gravity exoplanet - Life on a low gravity world

Life on a low gravity exoplanet - Life on a low gravity world

Miller, Ron (b.1947)

PIX4607766

Artist view of exoplanets - Artist view of exoplanets - Vue d'artiste d'une planete extrasolaire de type telluric et son satellite, devant leur star. A rocky extrasolar planet with its satellite in front of their star

Artist view of exoplanets - Artist view of exoplanets - Vue d'artiste d'une planete extrasolaire de type telluric et son satellite, devant leur star. A rocky extrasolar planet with its satellite in front of their star

D. Ducros

PIX4573926

Detection of an exoplanet: transit method - Detection of an exoplanet: transit method - This method of indirect detection is based on the study of star luminosite (yellow line). If the latter varies periodically, it may indicate the passage of a planet in front of its star. If a planet crosses in front of its star, then the observed brightness of the star (yellow line) is modified

Detection of an exoplanet: transit method - Detection of an exoplanet: transit method - This method of indirect detection is based on the study of star luminosite (yellow line). If the latter varies periodically, it may indicate the passage of a planet in front of its star. If a planet crosses in front of its star, then the observed brightness of the star (yellow line) is modified

PIX4573950

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

Observation of an exoplanete by interferometry - Observation of an exoplanet with interferometry - Illustration of the principle of direct observation of an exoplanete by interferometry with space telescopes. Places in different places, each telescope observes the light of the star with a slight decay relative to each other. Together these observations would reduce the apparent luminosite of the star and amplify the luminosite of the planet. Optical interferometry combines the light of multiple telescopes to perform the work of a single, much larger telescope. This is possible due to the interaction of light waves, also called interference. Their interaction can be used to cancel out the blinding glare of bright stars or to measure distances and angles precisely

Observation of an exoplanete by interferometry - Observation of an exoplanet with interferometry - Illustration of the principle of direct observation of an exoplanete by interferometry with space telescopes. Places in different places, each telescope observes the light of the star with a slight decay relative to each other. Together these observations would reduce the apparent luminosite of the star and amplify the luminosite of the planet. Optical interferometry combines the light of multiple telescopes to perform the work of a single, much larger telescope. This is possible due to the interaction of light waves, also called interference. Their interaction can be used to cancel out the blinding glare of bright stars or to measure distances and angles precisely

PIX4573974

Detection of an exoplanet by microlens effect - Detection of an exoplanet: Gravitational microlensing - On the left, the observation of a distant star whose light is diluted. On the right, the light of this star is amplified by gravitational lens effect. The gravitational lens effect occurs when the gravitational field of a star acts as a magnifying glass by amplifying the light emitted by a farther star. This amplification is measurable, and when the foreground star is accompanied by a planet, a second peak of intensity in the life rays appears more weakly. Illustration showing at left the observation of faint light emitted by a distant star, at right, the light of the same star magnified by a gravitational lens. Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. Possible planets orbiting the foreground star can cause detectable anomalies in the lensing event light curve

Detection of an exoplanet by microlens effect - Detection of an exoplanet: Gravitational microlensing - On the left, the observation of a distant star whose light is diluted. On the right, the light of this star is amplified by gravitational lens effect. The gravitational lens effect occurs when the gravitational field of a star acts as a magnifying glass by amplifying the light emitted by a farther star. This amplification is measurable, and when the foreground star is accompanied by a planet, a second peak of intensity in the life rays appears more weakly. Illustration showing at left the observation of faint light emitted by a distant star, at right, the light of the same star magnified by a gravitational lens. Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. Possible planets orbiting the foreground star can cause detectable anomalies in the lensing event light curve

PIX4573970

Exoplanete Kepler-22b: Kepler-22b is an exoplanet orbiting Kepler-22, a star of spectral type G5, similar to the Sun, located about 620 light years (190 pc) from the Solar System in the constellation of Swan. This is the first planet discovered by the Kepler space telescope in the habitable area of a yellow dwarf in December 2011. Kepler-22b is an extrasolar planet orbiting G-type star Kepler-22. It is located 600 light years away from Earth in the constellation of Cygnus. It was discovered by Nasa's Kepler Space Telescope and is the first known transiting planet to orbit within the habitable zone of a Sun-like star

Exoplanete Kepler-22b: Kepler-22b is an exoplanet orbiting Kepler-22, a star of spectral type G5, similar to the Sun, located about 620 light years (190 pc) from the Solar System in the constellation of Swan. This is the first planet discovered by the Kepler space telescope in the habitable area of a yellow dwarf in December 2011. Kepler-22b is an extrasolar planet orbiting G-type star Kepler-22. It is located 600 light years away from Earth in the constellation of Cygnus. It was discovered by Nasa's Kepler Space Telescope and is the first known transiting planet to orbit within the habitable zone of a Sun-like star

Miller, Ron (b.1947)

PIX4608034

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth-like”” planet went to Kepler-62F, which is 40 percent larger than the size of Earth and orbits in its star's habitable zone. Kepler-186f orbits its star once every 130 days and receives one-third the energy that Earth does from the sun, placing it near the outer edge of the habitable zone. If you could stand on the surface of Kepler-186f, the brightness of its star at high noon would appear as bright as our sun is about an hour before sunset on Earth. Kepler-186f resides in the Kepler-186 system about 500 light-years from Earth in the constellation Cygnus. The system is also home to four inner planets, seen lined up in orbit around a host star that is half the size and mass of the sun — Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Miller, Ron (b.1947)

PIX4608153

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant 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. 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 - or Astronomical Units - which is about the distance Saturn is from the Sun. The planet has a mass of about nine Jupiter masses and is right mass and location to explain the observed warp in the inner parts of the disc — Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant 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. 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 1

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant 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. 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 1

Miller, Ron (b.1947)

PIX4608449

Exoplanetes - Artist's view - Exoplanets - Illustration - Artist's view of extrasolar planets. Extrasolar planets in a starry sky

Exoplanetes - Artist's view - Exoplanets - Illustration - Artist's view of extrasolar planets. Extrasolar planets in a starry sky

PIX4574273

Life on an exoplanet - Alien flora - Artist's view of an extrasolar planet where plant life developed there. Artwork showing an exoplanet with vegetal life

Life on an exoplanet - Alien flora - Artist's view of an extrasolar planet where plant life developed there. Artwork showing an exoplanet with vegetal life

PIX4573280

Planet Formation - Artist View - Planet Birth - Artist view - Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A new born planet in a star's dusty, planet - forming disc

Planet Formation - Artist View - Planet Birth - Artist view - Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A new born planet in a star's dusty, planet - forming disc

PIX4633462

Exoplanete Gliese 849 b: Artist's view of the extrasolar planet Gliese 849 b, an exoplanet whose mass is less than that of Jupiter, discovered in 2006 and located 29 light years from Earth in the constellation Aquarius. Gliese 849 b is an extrasolar planet approximately 29 light years away in the constellation of Aquarius. It is the first long-period Jupiter-like planet discovered around a red dwarf

Exoplanete Gliese 849 b: Artist's view of the extrasolar planet Gliese 849 b, an exoplanet whose mass is less than that of Jupiter, discovered in 2006 and located 29 light years from Earth in the constellation Aquarius. Gliese 849 b is an extrasolar planet approximately 29 light years away in the constellation of Aquarius. It is the first long-period Jupiter-like planet discovered around a red dwarf

Miller, Ron (b.1947)

PIX4607959

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

Exoplanete Kepler-70b: Kepler-70b (KOI-55.01) is a confirmed extrasolar planet orbiting the star Kepler-70 (KOI-55), located in the constellation Swan. Kepler-70 b is probably a rocky exoplanet whose surface temperature is one of the warmest known surface temperatures on all exoplanets. Kepler-70b (KOI-55.01) is an exoplanet discovered orbiting the subdwarf B star Kepler-70. It is the hottest exoplanet as of mid-2013, with a surface temperature of 7,143 K (6,870* C)

Exoplanete Kepler-70b: Kepler-70b (KOI-55.01) is a confirmed extrasolar planet orbiting the star Kepler-70 (KOI-55), located in the constellation Swan. Kepler-70 b is probably a rocky exoplanet whose surface temperature is one of the warmest known surface temperatures on all exoplanets. Kepler-70b (KOI-55.01) is an exoplanet discovered orbiting the subdwarf B star Kepler-70. It is the hottest exoplanet as of mid-2013, with a surface temperature of 7,143 K (6,870* C)

Miller, Ron (b.1947)

PIX4608244

Solar sail near an exoplanet - Artist view - Solar sail and exoplanet - Artist view - View of a probe using solar wind and photons emitted by the Sun as a means of propulsion. The radiation pressure of sunlight on a huge expanse of very thin reflective material can gradually build up enough speed to reach another star

Solar sail near an exoplanet - Artist view - Solar sail and exoplanet - Artist view - View of a probe using solar wind and photons emitted by the Sun as a means of propulsion. The radiation pressure of sunlight on a huge expanse of very thin reflective material can gradually build up enough speed to reach another star

PIX4640485

Exoplanete Corot - 7b - Artist's impression of Corot - 7b - Artist's view of the extrasolar planet Corot - 7b, a small terrestrial exoplanet located in the constellation Unicorn. Artist's impression of the extrasolar planet Corot - 7b a small exoplanet located in the constellation of Monoceros. The exoplanet Corot - 7b is so close to its Sun - like host star that it must experience extreme conditions. This planet has a mass five times that of Earth's and is in fact the closest known exoplanet to its host star, which also makes it the fastest - - - it orbits its star at a speed of more than 750,000 kilometres per hour. The probable temperature on its day - face”” is above 2,000 degrees, but minus 200 degrees on its night face. Theoretical models suggest that the planet may have lava or boiling oceans on its surface. The artist has provided an impression of how it may look like if it were covered by lava. The sister planet, Corot - 7c, is seen in the distance.

Exoplanete Corot - 7b - Artist's impression of Corot - 7b - Artist's view of the extrasolar planet Corot - 7b, a small terrestrial exoplanet located in the constellation Unicorn. Artist's impression of the extrasolar planet Corot - 7b a small exoplanet located in the constellation of Monoceros. The exoplanet Corot - 7b is so close to its Sun - like host star that it must experience extreme conditions. This planet has a mass five times that of Earth's and is in fact the closest known exoplanet to its host star, which also makes it the fastest - - - it orbits its star at a speed of more than 750,000 kilometres per hour. The probable temperature on its day - face”” is above 2,000 degrees, but minus 200 degrees on its night face. Theoretical models suggest that the planet may have lava or boiling oceans on its surface. The artist has provided an impression of how it may look like if it were covered by lava. The sister planet, Corot - 7c, is seen in the distance.

PIX4573791

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

PIX4573350

Exoplanets around a white dwarf - Illustration - White dwarf system - Artwork

Exoplanets around a white dwarf - Illustration - White dwarf system - Artwork

Miller, Ron (b.1947)

PIX4574228

Exoplanete around a binary star - Artist view - Binary Star Exoplanet - Artist rendering

Exoplanete around a binary star - Artist view - Binary Star Exoplanet - Artist rendering

Miller, Ron (b.1947)

PIX4607698

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, en transit devant son etoile. Transit of a rocky extrasolar planet in front of its star

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, en transit devant son etoile. Transit of a rocky extrasolar planet in front of its star

D. Ducros

PIX4573917

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Miller, Ron (b.1947)

PIX4607656

Exoplanete Corot-7b - Exoplanet Corot-7b: Artist's view of the extrasolar planet Corot-7b, a small terrestrial exoplanet located in the constellation of the Unicorn. Artist's impression of the extrasolar planet Corot-7b a small exoplanet located in the constellation of Monoceros

Exoplanete Corot-7b - Exoplanet Corot-7b: Artist's view of the extrasolar planet Corot-7b, a small terrestrial exoplanet located in the constellation of the Unicorn. Artist's impression of the extrasolar planet Corot-7b a small exoplanet located in the constellation of Monoceros

Miller, Ron (b.1947)

PIX4607875

Artist's view of an exoplanet covered with water on its surface.

Artist's view of an exoplanet covered with water on its surface.

Miller, Ron (b.1947)

PIX4608560

Exoplanete around Beta Hydri: Beta Hydri is the brightest star in the constellation of the male Hydra. Located about 24.4 light years from Earth, Beta Hydri is often studied as it could give information about what could happen to the Sun in the next 2.5 billion years. Larger and slightly more massive than the latter, it probably has planets. Beta Hydri is a star in the southern circumpolar constellation of Hydrus. Located 24.33 light-years away, it could harbor a true Jupiter-analogue, though 4 times more massive

Exoplanete around Beta Hydri: Beta Hydri is the brightest star in the constellation of the male Hydra. Located about 24.4 light years from Earth, Beta Hydri is often studied as it could give information about what could happen to the Sun in the next 2.5 billion years. Larger and slightly more massive than the latter, it probably has planets. Beta Hydri is a star in the southern circumpolar constellation of Hydrus. Located 24.33 light-years away, it could harbor a true Jupiter-analogue, though 4 times more massive

Miller, Ron (b.1947)

PIX4608343

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

PIX4573359

Exoplanete near a star at the end of life - A dying star sheds its outer layers - An artist's view of a star that, like the Sun at the end of life, turns into a red giant, and expels its upper layers into concentric circles, before becoming a white dwarf. In the foreground, an exoplanet distant from its star that sees its surface reheat. When a star like our sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant. Then over the next several tens of thousands of years the star episodically ejects its outer layers into space, sometimes producing concentric shells. These ejected layers eventually form a planetary nebula. What will subsequently remain of the star is a small, extremely hot core which cools off to become a white dwarf. In this image a red giant star expels its first of many shells of gas into space. In the years to come this spherical shell will grow outward, its circumference eventually expanding far beyond the orbit of this planet. As for this planet, being so far from its parent sun for most of its life has kept it in a deep, dark freeze for the past ten billion years (think Pluto). It has been during only the past 100 million years, when its sun first blossomed into a red giant, that this planet has experienced such light and warmth. This effluence is short - lived, however; in about another million years darkness and cold will again be the norm for this world — Exoplanete near a star at the end of life - A dying star sheds its outer layers - An artist's view of a star that, like the Sun at the end of life, turns into a red giant, and expels its upper layers into concentric circles, before becoming a white dwarf. In the foreground, an exoplanet distant from its star that sees its surface reheat. When a star like our sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant. Then over the next several tens of thousands of years the star episodically ejects its outer layers into space, sometimes producing concentric shells. These ejected layers eventually form a planetary nebula. What will subsequently remain of the star is a small, extremely hot core which cools off to become a white dwarf. In this image a red giant star expels its first of many shells of gas into space. In the years to come this spherical shell will grow outward, its circumference eventually expanding far beyond the orbit of th

Exoplanete near a star at the end of life - A dying star sheds its outer layers - An artist's view of a star that, like the Sun at the end of life, turns into a red giant, and expels its upper layers into concentric circles, before becoming a white dwarf. In the foreground, an exoplanet distant from its star that sees its surface reheat. When a star like our sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant. Then over the next several tens of thousands of years the star episodically ejects its outer layers into space, sometimes producing concentric shells. These ejected layers eventually form a planetary nebula. What will subsequently remain of the star is a small, extremely hot core which cools off to become a white dwarf. In this image a red giant star expels its first of many shells of gas into space. In the years to come this spherical shell will grow outward, its circumference eventually expanding far beyond the orbit of th

Walter B Myers

PIX4573888

Exoplanete type Super-Jupiter - Artist view - Super-Jupiter Exoplanet - Artist rendering: A Super-Jupiter seen from one of its satellites. A super-Jupiter, is a planet of mass higher than that of Jupiter. A Super-Jupiter is an astronomical object that is more massive than the planet Jupiter

Exoplanete type Super-Jupiter - Artist view - Super-Jupiter Exoplanet - Artist rendering: A Super-Jupiter seen from one of its satellites. A super-Jupiter, is a planet of mass higher than that of Jupiter. A Super-Jupiter is an astronomical object that is more massive than the planet Jupiter

Miller, Ron (b.1947)

PIX4607707

Exoplanete type Super-Jupiter - Artist view - Super-Jupiter Exoplanet - Artist rendering: A Super-Jupiter seen from one of its satellites. A super-Jupiter, is a planet of mass higher than that of Jupiter. A Super-Jupiter is an astronomical object that is more massive than the planet Jupiter

Exoplanete type Super-Jupiter - Artist view - Super-Jupiter Exoplanet - Artist rendering: A Super-Jupiter seen from one of its satellites. A super-Jupiter, is a planet of mass higher than that of Jupiter. A Super-Jupiter is an astronomical object that is more massive than the planet Jupiter

Miller, Ron (b.1947)

PIX4607705

Artist's view of Kelt-11b orbiting his star KELT-11, located 320 light years from Earth in the constellation of the Lion. Kelt-11b is an exoplanet larger than Jupiter and very close to its star. It was discovered in 2016.

Artist's view of Kelt-11b orbiting his star KELT-11, located 320 light years from Earth in the constellation of the Lion. Kelt-11b is an exoplanet larger than Jupiter and very close to its star. It was discovered in 2016.

Miller, Ron (b.1947)

PIX4608601

Exoplanets around Kepler-47 - Artist's impression of the Kepler-47 system: Kepler-47 c is a giant gas extrasolar planet located in the habitable area of its binary star Kepler-47. Kepler-47 c is a gas giant that orbits the two stars in the habitable zone of Kepler-47 system

Exoplanets around Kepler-47 - Artist's impression of the Kepler-47 system: Kepler-47 c is a giant gas extrasolar planet located in the habitable area of its binary star Kepler-47. Kepler-47 c is a gas giant that orbits the two stars in the habitable zone of Kepler-47 system

PIX4574140

Artist's view of an ocean planet - Ocean planet - Artist's view of an exoplanet covered with water on its surface

Artist's view of an ocean planet - Ocean planet - Artist's view of an exoplanet covered with water on its surface

Miller, Ron (b.1947)

PIX4945162

Artist's view of a hot Jupiter - Exoplanet - Hot Jupiter - Artist's view of a gas giant exoplanet very close to its star. Many of the extra - solar planets which have been discovered in recent years are large, massive, and orbit surprisingly close to their parent stars. These are believed to be gas giant planets similar to Jupiter. Since they're so close to their sun, they're hot. Thus the common term for them has become “” hot Jupiter””. This one is hot enough to glow a dull red even on its night side. The existence of these planets has proven that the arrangement of other solar systems need not closely resemble our own

Artist's view of a hot Jupiter - Exoplanet - Hot Jupiter - Artist's view of a gas giant exoplanet very close to its star. Many of the extra - solar planets which have been discovered in recent years are large, massive, and orbit surprisingly close to their parent stars. These are believed to be gas giant planets similar to Jupiter. Since they're so close to their sun, they're hot. Thus the common term for them has become “” hot Jupiter””. This one is hot enough to glow a dull red even on its night side. The existence of these planets has proven that the arrangement of other solar systems need not closely resemble our own

PIX4574132

Artist view of the Exoplanete Gliese 581c - Artwork of exoplanet Gliese 581c - Artist view of the Exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” This image of a rocky and variegated Gliese 581 c with an atmosphere and clouds is purely speculative

Artist view of the Exoplanete Gliese 581c - Artwork of exoplanet Gliese 581c - Artist view of the Exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” This image of a rocky and variegated Gliese 581 c with an atmosphere and clouds is purely speculative

Walter B Myers

PIX4573773

Exoplanete Kepler-452 b - Artist's impression of the Kepler-452 b exoplanet: Kepler-452 b is an extrasolar planet probably of the Earth type, located in the habitable area of its star Kepler-452, a star similar to our Sun. This super-earth is located in the constellation Swan, about 1400 light years from Earth. This artist's concept depicts one possible appearance of the planet Kepler-452b, the first near-earth-size world to be found in the habitable zone of star that is similar to our sun. The habitable zone is a region around a star where temperatures are right for water to pool on the surface. Scientists do not know if Kepler-452b can support life or not. What is known about the planet is that it is about 60 percent larger than Earth, placing it in a class of planets dubbed “” Super-earths.”” While its mass and composition are not yet determined, previous research suggests that planets the size of Kepler-452b have a better than even chance of being rocky. Kepler-452b orbits its star every 385 days. The planet's star is about 1,400 light-years away in the constellation Cygnus. It is a G2-type star like our sun, with almost the same temperature and mass. This star is 6 billion years old, 1.5 billion years older than our sun — Exoplanete Kepler-452 b - Artist's impression of the Kepler-452 b exoplanet: Kepler-452 b is an extrasolar planet probably of the Earth type, located in the habitable area of its star Kepler-452, a star similar to our Sun. This super-earth is located in the constellation Swan, about 1400 light years from Earth. This artist's concept depicts one possible appearance of the planet Kepler-452b, the first near-earth-size world to be found in the habitable zone of star that is similar to our sun. The habitable zone is a region around a star where temperatures are right for water to pool on the surface. Scientists do not know if Kepler-452b can support life or not. What is known about the planet is that it is about 60 percent larger than Earth, placing it in a class of planets dubbed “” Super-earths.”” While its mass and composition are not yet determined, previous research suggests that planets the size of Kepler-452b have a better than even chance of being rocky. Kepler-452b orbits its star

Exoplanete Kepler-452 b - Artist's impression of the Kepler-452 b exoplanet: Kepler-452 b is an extrasolar planet probably of the Earth type, located in the habitable area of its star Kepler-452, a star similar to our Sun. This super-earth is located in the constellation Swan, about 1400 light years from Earth. This artist's concept depicts one possible appearance of the planet Kepler-452b, the first near-earth-size world to be found in the habitable zone of star that is similar to our sun. The habitable zone is a region around a star where temperatures are right for water to pool on the surface. Scientists do not know if Kepler-452b can support life or not. What is known about the planet is that it is about 60 percent larger than Earth, placing it in a class of planets dubbed “” Super-earths.”” While its mass and composition are not yet determined, previous research suggests that planets the size of Kepler-452b have a better than even chance of being rocky. Kepler-452b orbits its star

PIX4574146

Exoplanete Kepler - 69c - Kepler - 69c is an exoplanet orbiting Kepler - 69, a star similar to the Sun, located about 2700 light years from the Solar System in the constellation of Swan. Kepler - 69c is a super Earth located in the living area of its star. Artist's concept of planet Kepler - 69c, a super - Earth - size planet (70% larger than Earth). It is the smallest yet found orbiting in the habitable zone of a sun - like star. Its orbit of 242 days resemble that of our neighboring planet Venus

Exoplanete Kepler - 69c - Kepler - 69c is an exoplanet orbiting Kepler - 69, a star similar to the Sun, located about 2700 light years from the Solar System in the constellation of Swan. Kepler - 69c is a super Earth located in the living area of its star. Artist's concept of planet Kepler - 69c, a super - Earth - size planet (70% larger than Earth). It is the smallest yet found orbiting in the habitable zone of a sun - like star. Its orbit of 242 days resemble that of our neighboring planet Venus

PIX4574115

Detection of an exoplanet by radial velocity - Detection of an exoplanet: Radial velocity or Doppler method - This detection method is based on the study of the light spectrum of the star. A planet orbiting around a star periodically influences the movement of that star. By Doppler effect (the star's light wave shifts to blue when it approaches and decals to red when it moves away), we can measure the radial velocity of the star and know the position of the planet's orbit. An exoplanet orbiting a larger star could produce changes in position and velocity of the star as they orbit their common center of mass. Those variations in the radial velocity are known in studying the spectral lines of the star due to the Doppler effect (blue shift when the star is approaching, redshift when it is receding)

Detection of an exoplanet by radial velocity - Detection of an exoplanet: Radial velocity or Doppler method - This detection method is based on the study of the light spectrum of the star. A planet orbiting around a star periodically influences the movement of that star. By Doppler effect (the star's light wave shifts to blue when it approaches and decals to red when it moves away), we can measure the radial velocity of the star and know the position of the planet's orbit. An exoplanet orbiting a larger star could produce changes in position and velocity of the star as they orbit their common center of mass. Those variations in the radial velocity are known in studying the spectral lines of the star due to the Doppler effect (blue shift when the star is approaching, redshift when it is receding)

PIX4573959

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Miller, Ron (b.1947)

PIX4573470

L'exoplanete HD 69830 d - Artist view - Exoplanet HD 69830 d - Artwork - Artist view of the extrasolar planet HD 69830 d. This planet, located in the habitability area, is represented here with several satellites. Artwork showing the extrasolar planet HD 69830 d. This planet resides in the habitable zone and is shown here with several moons

L'exoplanete HD 69830 d - Artist view - Exoplanet HD 69830 d - Artwork - Artist view of the extrasolar planet HD 69830 d. This planet, located in the habitability area, is represented here with several satellites. Artwork showing the extrasolar planet HD 69830 d. This planet resides in the habitable zone and is shown here with several moons

Miller, Ron (b.1947)

PIX4573252

Exoplanete - An Earthlike Moon - Artist's view of a satellite of a gas planet where water is present in abundance. There are likely earthlike planets that themselves are satellites of larger worlds

Exoplanete - An Earthlike Moon - Artist's view of a satellite of a gas planet where water is present in abundance. There are likely earthlike planets that themselves are satellites of larger worlds

Walter B Myers

PIX4573259

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Miller, Ron (b.1947)

PIX4607669

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Miller, Ron (b.1947)

PIX4607660

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Miller, Ron (b.1947)

PIX4607909

Exoplanete Trappist-1b - Artist's impression of Trappist-1b: Artist's view of the surface of the extrasolar planet Trappist-1b.

Exoplanete Trappist-1b - Artist's impression of Trappist-1b: Artist's view of the surface of the extrasolar planet Trappist-1b.

Miller, Ron (b.1947)

PIX4608411

Exoplanete HD 156668 b: HD 156668 b is an exoplanet orbiting the star HD 156668 has 78.5 light years of Earth, in the constellation of Hercules. With 4.15 times the mass of the Earth, it is, on the date of its discovery in 2010, the second smallest super-earth after Gliese 581 e. HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses

Exoplanete HD 156668 b: HD 156668 b is an exoplanet orbiting the star HD 156668 has 78.5 light years of Earth, in the constellation of Hercules. With 4.15 times the mass of the Earth, it is, on the date of its discovery in 2010, the second smallest super-earth after Gliese 581 e. HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses

Miller, Ron (b.1947)

PIX4608494

Galaxy in the sky of an exoplanet - Galaxy seen from a rogue planet: Artist's view of a galaxy in the sky of an isolated exoplanet

Galaxy in the sky of an exoplanet - Galaxy seen from a rogue planet: Artist's view of a galaxy in the sky of an isolated exoplanet

Miller, Ron (b.1947)

PIX4573513

Exoplanete Tau Bootis b - Tau Booetes b - Artist's view of the extrasolar planet Tau Bootis b view of a hypothetical satellite. Tau Bootis b is located 50 years of light from Earth in the constellation Bovier. It is a gas exoplanet about four times the mass of Jupiter, located very close to its star. The extrasolar planet Tau Booetes b reigns over the airless, baked and battered terrain of a hypothetical moon. Tau Booetes b orbits very close to Tau Booetes, a type F7V star about 50 light years from the Earth. Tau Booetes b is believed to have about four times the mass of the planet Jupiter and orbits around its sun at the astonishing pace of once every 3.3 days. Tau Booetes b is so close to its host sun that the force of the solar wind may be enough to constantly blow off the planet's outer atmosphere

Exoplanete Tau Bootis b - Tau Booetes b - Artist's view of the extrasolar planet Tau Bootis b view of a hypothetical satellite. Tau Bootis b is located 50 years of light from Earth in the constellation Bovier. It is a gas exoplanet about four times the mass of Jupiter, located very close to its star. The extrasolar planet Tau Booetes b reigns over the airless, baked and battered terrain of a hypothetical moon. Tau Booetes b orbits very close to Tau Booetes, a type F7V star about 50 light years from the Earth. Tau Booetes b is believed to have about four times the mass of the planet Jupiter and orbits around its sun at the astonishing pace of once every 3.3 days. Tau Booetes b is so close to its host sun that the force of the solar wind may be enough to constantly blow off the planet's outer atmosphere

Walter B Myers

PIX4573262

Kappa Andromedae b: Kappa Andromedae b is a hot, young, gaseous Giant Planet with about 13 times the mass of Jupiter. The “” Super-Jupiter”” Kappa Andromedae b, shown here in an artist's rendering, circles its star at almost twice the distance that Neptune orbits the sun. With a mass about 13 times Jupiter's, the object glows with a reddish color

Kappa Andromedae b: Kappa Andromedae b is a hot, young, gaseous Giant Planet with about 13 times the mass of Jupiter. The “” Super-Jupiter”” Kappa Andromedae b, shown here in an artist's rendering, circles its star at almost twice the distance that Neptune orbits the sun. With a mass about 13 times Jupiter's, the object glows with a reddish color

PIX4608283

L'exoplanete HD 69830 d - Artist view: Artist view of the extrasolar planet HD 69830 d. This planet, located in the habitability area, is represented here with several satellites. Artwork showing the extrasolar planet HD 69830 d. This planet resides in the habitable zone and is shown here with several moons

L'exoplanete HD 69830 d - Artist view: Artist view of the extrasolar planet HD 69830 d. This planet, located in the habitability area, is represented here with several satellites. Artwork showing the extrasolar planet HD 69830 d. This planet resides in the habitable zone and is shown here with several moons

Miller, Ron (b.1947)

PIX4607818

Exoplanete around 55 Cancri - Artist's view - Exoplanet 55 Cancri e -Artwork: Artist's view of the surface of the extrasolar planet 55 Cancri e, orbiting around 55 Cancri, a star similar to our Sun, located 41 light years from Earth in the constellation of Cancer. This superland, very close to its star, was discovered in 2004 and its transit was observed in 2011. This artist's concept shows exoplanet 55 Cancri and that orbits 55 Cancri, a star much like our own located 41 light years away

Exoplanete around 55 Cancri - Artist's view - Exoplanet 55 Cancri e -Artwork: Artist's view of the surface of the extrasolar planet 55 Cancri e, orbiting around 55 Cancri, a star similar to our Sun, located 41 light years from Earth in the constellation of Cancer. This superland, very close to its star, was discovered in 2004 and its transit was observed in 2011. This artist's concept shows exoplanet 55 Cancri and that orbits 55 Cancri, a star much like our own located 41 light years away

Miller, Ron (b.1947)

PIX4607917

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 - - or Astronomical Units - - which is about the distance Saturn is from the Sun. The planet has a mass of about nine Jupiter masses and is right mass and location to explain the observed warp in the inner parts of the disc — 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 -

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

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b in the constellation Scorpio. Its mass is estimated at 5.5 times that of Earth, distinguishing it from the smallest of our gas planets, Uranus (15 Earth masses) and Neptune (17). It is most likely solid, composed of ice and rocks. But if her mass is higher, then she could be an ice giant like Uranus and Neptune.

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b in the constellation Scorpio. Its mass is estimated at 5.5 times that of Earth, distinguishing it from the smallest of our gas planets, Uranus (15 Earth masses) and Neptune (17). It is most likely solid, composed of ice and rocks. But if her mass is higher, then she could be an ice giant like Uranus and Neptune.

Miller, Ron (b.1947)

PIX4607912

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

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

PIX4573338

Gas exoplanete - Gas exoplanet - Artist's view of an extrasolar gas planet in the sky of one of its satellites. Recent discoveries of what appear to be giant planets orbiting very close to distant stars inspired this image. Due to the close proximity to its own sun, this gas planet would shine brilliantly in this moon's sky

Gas exoplanete - Gas exoplanet - Artist's view of an extrasolar gas planet in the sky of one of its satellites. Recent discoveries of what appear to be giant planets orbiting very close to distant stars inspired this image. Due to the close proximity to its own sun, this gas planet would shine brilliantly in this moon's sky

Walter B Myers

PIX4573237

Exoplanete Gliese 1214 b - Gliese 1214 b (or GJ 1214 b) is a super-Earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on 16 December 2009. It is located about 40 years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light - years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super - Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT - 7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low density — Exoplanete Gliese 1214 b - Gliese 1214 b (or GJ 1214 b) is a super-Earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on 16 December 2009. It is located about 40 years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light - years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super - Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT - 7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low dens

Exoplanete Gliese 1214 b - Gliese 1214 b (or GJ 1214 b) is a super-Earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on 16 December 2009. It is located about 40 years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light - years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super - Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT - 7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low dens

Miller, Ron (b.1947)

PIX4574069

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering

Miller, Ron (b.1947)

PIX4607680

Exoplanets around Kepler-11: Kepler-11 is a star similar to the Sun, located about 2,000 light years from the Solar System in the constellation Swan. It has a planetary system consisting of at least six exoplanets detected by the Kepler space telescope in 2011. Kepler-11 is a Sun-like star in the constellation Cygnus, located some 2,000 light years from Earth. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size

Exoplanets around Kepler-11: Kepler-11 is a star similar to the Sun, located about 2,000 light years from the Solar System in the constellation Swan. It has a planetary system consisting of at least six exoplanets detected by the Kepler space telescope in 2011. Kepler-11 is a Sun-like star in the constellation Cygnus, located some 2,000 light years from Earth. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size

Miller, Ron (b.1947)

PIX4608132

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

Patrick Lécureuil

PIX4655293

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Miller, Ron (b.1947)

PIX4607920

Exoplanete MOA-2007-BLG-192L b: MOA-2007-BLG-192L b is a confirmed extrasolar planet (exoplanet) orbiting the brown dwarf star MOA-2007-BLG-192L. Its temperature is freezing (< -200* C). MOA-2007-BLG-192LB, occasionally shortened to MOA-192 b, is an extrasolar planet approximately 3,000 light-years away in the constellation of Sagittarius. The planet was discovered orbiting the brown dwarf or low-mass star MOA-2007-BLG-192L. At a mass of approximately 3.3 times Earth, it is one of the lowest-mass extrasolar planets at the time of discovery

Exoplanete MOA-2007-BLG-192L b: MOA-2007-BLG-192L b is a confirmed extrasolar planet (exoplanet) orbiting the brown dwarf star MOA-2007-BLG-192L. Its temperature is freezing (< -200* C). MOA-2007-BLG-192LB, occasionally shortened to MOA-192 b, is an extrasolar planet approximately 3,000 light-years away in the constellation of Sagittarius. The planet was discovered orbiting the brown dwarf or low-mass star MOA-2007-BLG-192L. At a mass of approximately 3.3 times Earth, it is one of the lowest-mass extrasolar planets at the time of discovery

Miller, Ron (b.1947)

PIX4608349

Exoplanete Kepler-36 c: Kepler-36 c view from the surface of Kepler-36 b. These two planets have close orbits and revolve around the star Kepler-36 in the constellation Swan. Kepler-36c is a gas giant that orbits very close to Kepler-36b, a rocky world, in the Kepler-36 system

Exoplanete Kepler-36 c: Kepler-36 c view from the surface of Kepler-36 b. These two planets have close orbits and revolve around the star Kepler-36 in the constellation Swan. Kepler-36c is a gas giant that orbits very close to Kepler-36b, a rocky world, in the Kepler-36 system

Miller, Ron (b.1947)

PIX4608186

Exoplanete Corot-7b: Artist's view of the extrasolar planet Corot-7b, a small terrestrial exoplanet located in the constellation of Unicorn. Artist's impression of the extrasolar planet Corot-7b a small exoplanet located in the constellation of Monoceros

Exoplanete Corot-7b: Artist's view of the extrasolar planet Corot-7b, a small terrestrial exoplanet located in the constellation of Unicorn. Artist's impression of the extrasolar planet Corot-7b a small exoplanet located in the constellation of Monoceros

Miller, Ron (b.1947)

PIX4608021

Exoplanete Kepler-64 b: Kepler-64 b or PH1 b (Planet Hunters 1b), is a circumbinary extrasolar planet belonging to the Quadruple Star System Kepler-64 (PH1). PH1b would be a giant gas planet. pH1b (standing for “” Planet Hunters 1””), or by its NASA designation Kepler-64b, is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The giant planet is Neptune-sized, about 20-55 Earth-masses, located 5000 light years from Earth in Cygnus constellation

Exoplanete Kepler-64 b: Kepler-64 b or PH1 b (Planet Hunters 1b), is a circumbinary extrasolar planet belonging to the Quadruple Star System Kepler-64 (PH1). PH1b would be a giant gas planet. pH1b (standing for “” Planet Hunters 1””), or by its NASA designation Kepler-64b, is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The giant planet is Neptune-sized, about 20-55 Earth-masses, located 5000 light years from Earth in Cygnus constellation

Miller, Ron (b.1947)

PIX4608221

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Miller, Ron (b.1947)

PIX4607866

Planete pres d'un amas globulaire - Artist view - Planet close to a globular cluster - Artist view - A globular cluster seen from the surface of a hypothetical planet. This cluster contains about 50,000 stars and is riding high above our own Milky Way galaxy. Like other globular clusters, it may be the remnant of the core of a small galaxy long ago adsorbed by the larger Milky Way. There may even be a black hole lurking at its center. Globular clusters usually contain very old stars. Any planets to be found in one would likely be much older than the Earth

Planete pres d'un amas globulaire - Artist view - Planet close to a globular cluster - Artist view - A globular cluster seen from the surface of a hypothetical planet. This cluster contains about 50,000 stars and is riding high above our own Milky Way galaxy. Like other globular clusters, it may be the remnant of the core of a small galaxy long ago adsorbed by the larger Milky Way. There may even be a black hole lurking at its center. Globular clusters usually contain very old stars. Any planets to be found in one would likely be much older than the Earth

Walter B Myers

PIX4573519

Artist's view of an exoplanet - Exoplanet - Illustration - Artist's view of a gas giant exoplanet accompanied by satellites. A gas giant exoplanet with satellites

Artist's view of an exoplanet - Exoplanet - Illustration - Artist's view of a gas giant exoplanet accompanied by satellites. A gas giant exoplanet with satellites

PIX4574352

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”” planet went to Kepler - 62f, which is 40 percent larger than the size of Earth and orbits in its star's habitable zone. Kepler - 186f orbits its star once every 130 days and receives one - third the energy that Earth does from the sun, placing it near the outer edge of the habitable zone. If you could stand on the surface of Kepler - 186f, the brightness of its star at high noon would appear as bright as our sun is about an hour before sunset on Earth. Kepler - 186f resides in the Kepler - 186 system about 500 light - years from Earth in the constellation Cygnus. The system is also home to four inner planets, seen lined up in orbit around a host star that is half the size and mass of the sun. The artistic concept of Kepler - 186f is the result of scientists and artists collaborating to imagine the appearance of these distant worlds — Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

PIX4574126

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

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 WASP-12b: WASP-12b is a hot Jupiter-type exoplanet orbiting in 1.09 days around the star WASP-12, located about 870 light-years from the Sun, in the constellation of Coach. This planet is so close to its star that it is stretched by the maree forces of the latter so that it presents an ovoid shape and its atmosphere is little by little torn away by the star. WASP-12b is an extrasolar planet orbiting the star WASP-12, discovered by the SuperWasp planetary transit survey. Due to its extremely close orbit to its star, the star's tidal forces are distorting it into an egg shape and pulling away its atmosphere. The planet takes only a little over a day to orbit the star

Exoplanete WASP-12b: WASP-12b is a hot Jupiter-type exoplanet orbiting in 1.09 days around the star WASP-12, located about 870 light-years from the Sun, in the constellation of Coach. This planet is so close to its star that it is stretched by the maree forces of the latter so that it presents an ovoid shape and its atmosphere is little by little torn away by the star. WASP-12b is an extrasolar planet orbiting the star WASP-12, discovered by the SuperWasp planetary transit survey. Due to its extremely close orbit to its star, the star's tidal forces are distorting it into an egg shape and pulling away its atmosphere. The planet takes only a little over a day to orbit the star

Miller, Ron (b.1947)

PIX4608333

L'exoplanete 2M1207B - Vue d'artiste - Exoplanet 2M1207B - Artist rendering - Illustration of the extrasolar planet 2M1207B seen from one of its satellites. 2M1207B is 5 times more massive than Jupiter and is located about 200 years ago - light in the constellation of Hydra. It is orbiting a brown dwarf star, visible at the top left of the image. Artwork of the extrasolar planet 2M1207b seen from one of its moons. This exoplanet is five times the Jupiter mass and is located at about 200 light years in the constellation of Hydra. It orbits around a brown dwarf

L'exoplanete 2M1207B - Vue d'artiste - Exoplanet 2M1207B - Artist rendering - Illustration of the extrasolar planet 2M1207B seen from one of its satellites. 2M1207B is 5 times more massive than Jupiter and is located about 200 years ago - light in the constellation of Hydra. It is orbiting a brown dwarf star, visible at the top left of the image. Artwork of the extrasolar planet 2M1207b seen from one of its moons. This exoplanet is five times the Jupiter mass and is located at about 200 light years in the constellation of Hydra. It orbits around a brown dwarf

Miller, Ron (b.1947)

PIX4573104

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

Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view 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. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view 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. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

PIX4573412

Exoplanete Kepler-16 b seen from one of its satellites: Kepler-16 b is an extrasolar planet (exoplanete) orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. Kepler-16b is a saturn-mass extrasolar planet orbiting a binary star, Kepler-16

Exoplanete Kepler-16 b seen from one of its satellites: Kepler-16 b is an extrasolar planet (exoplanete) orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. Kepler-16b is a saturn-mass extrasolar planet orbiting a binary star, Kepler-16

Miller, Ron (b.1947)

PIX4608161

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view

Miller, Ron (b.1947)

PIX4607858

Exoplanete near the galactic center - Exoplanet near the galactic center Artwork

Exoplanete near the galactic center - Exoplanet near the galactic center Artwork

Miller, Ron (b.1947)

PIX4573504

Sunset on Kepler-11g - Kepler-11g sunset: Kepler-11g is an exoplanet the size of Neptune belonging to the system of 6 planets orbiting the star Kepler-11. Kepler-11g is an exoplanet discovered in the orbit of the sunlike star Kepler-11 by the Kepler spacecraft. Kepler-11g is the outermost of the star's six planets and is comparable to Neptune's size

Sunset on Kepler-11g - Kepler-11g sunset: Kepler-11g is an exoplanet the size of Neptune belonging to the system of 6 planets orbiting the star Kepler-11. Kepler-11g is an exoplanet discovered in the orbit of the sunlike star Kepler-11 by the Kepler spacecraft. Kepler-11g is the outermost of the star's six planets and is comparable to Neptune's size

Miller, Ron (b.1947)

PIX4608144

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

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 devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

D. Ducros

PIX4573924

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

Exoplanete devant son etoile - Artist view of an exoplanet - Vue d'artiste d'une planete extrasolaire de type telluric, devant son etoile. A rocky extrasolar planet in front of its star

D. Ducros

PIX4573958

Exoplanete around 70 Virginis - A jovian planet orbiting 70 Virginis: Artist's view of the extrasolar planet 70 Vir B, a gas-like planet orbiting around a solar star, about 60 light years from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. About 60 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun

Exoplanete around 70 Virginis - A jovian planet orbiting 70 Virginis: Artist's view of the extrasolar planet 70 Vir B, a gas-like planet orbiting around a solar star, about 60 light years from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. About 60 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun

Miller, Ron (b.1947)

PIX4607837

Surface of an uninhabitable exoplanet - Exoplanet too hot for life. Artwork - Artist's view of the surface of a planet where extreme temperatures make life impossible. There are likely earthlike planets that miss being hospitable to life because they are a little too close to their host sun (s)

Surface of an uninhabitable exoplanet - Exoplanet too hot for life. Artwork - Artist's view of the surface of a planet where extreme temperatures make life impossible. There are likely earthlike planets that miss being hospitable to life because they are a little too close to their host sun (s)

Walter B Myers

PIX4573941

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