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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
Exoplanete - Artist's View
Spaceship - Artist's View - Spaceship - Artist vie
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
Artist's impression of the Exoplanète Proxima Centauri
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Voyager and Exoplanets Probe - Voyager entering an alien solar system  Artist's view showing one of the probes approaching another solar system
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
Exoplanete around a neutron star - Neutron Star Planet - Illustration
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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
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
Exoplanetes - Artist's view - Exoplanets - Illustration - Artist's view of extrasolar planets. Extrasolar planets in a starry sky
Exoplanete PSR B1620-26 b - Mathusalem - Exoplanet PSR B1620-26 b - Methuselah: PSR B1620-26 b, unofficially nicknamed Mathusalem is a circumbinary exoplanet of about 2.5 Jovian masses. It would be the oldest known planet, perhaps 13 billion years old. Discovered in 1993 around the binary system formed by PSR B1620-26 and WD B1620-26, respectively a pulsar and a white dwarf orbiting around each other. This system is approximately 12,400 light-years away from Earth in the M4 globular cluster of the constellation Scorpio. PSR B1620-26 b is an extrasolar planet located approximately 12,400 light-years away from Earth in the constellation of Scorpius. It bears the unofficial nickname “” Methuselah”” due to its extreme age. The planet is in a circumbinary orbit around a pulsar (PSR B1620-26) and a white dwarf (WD B1620-26)) and is the first circumbinary planet ever confirmed. It is also the first planet found in a globular cluster. The planet is one of the oldest known extrasolar planets, believed to be about 12.7 billion years old
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
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.
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
Exoplanets around a white dwarf - Illustration - White dwarf system - Artwork
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Exoplanete around a binary star - Artist view - Binary Star Exoplanet - Artist rendering
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
Life on a low gravity exoplanet - Life on a low gravity world
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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
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
Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
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-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
Artist's view of an exoplanet covered with water on its surface.
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Exoplanete Trappist-1b - Artist's impression of Trappist-1b: Artist's view of the surface of the extrasolar planet Trappist-1b.
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
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 a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
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 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
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)
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
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 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
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)
Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view
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 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
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
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 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 in formation - LKCA 15 b - Exoplanet forming - LKCA 15 b: Artist's view showing the exoplanet LKCA 15 b, an exoplanet in formation by accretion. LKCA 15 b or Lick-Calcium 15b is a candidate protoplanetary object in orbit around LKCA 15, a star in the Taurus-Auriga Star Forming Region. It was discovered by direct imaging techniques using the Keck II telescope in 2011. A 2015 study of observations from the Magellan Telescopes and the Large Binocular Telescope argued that the planet is forming though accretion. It is the first observed exoplanet seen in the process of active accretion.
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
The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees
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
Brown dwarf star Teide 1 - Brown dwarf Teide 1 - Artist view of the brown dwarf star Teide 1. Discovered in 1995 in the Pleiades cluster, about 55 times the mass of Jupiter, this brown dwarf is represented here in the sky of a young exoplanet lit by the star. This is how Teide 1 might appear from the surface of a hypothetical, March - like planet. Discovered in 1995, Teide 1 is a type of mysterious object called a brown dwarf (failed star or super planet). Bigger than a planet, but smaller than a star, this brown dwarf is about 400 light years from the Earth in the Pleiades star cluster. It is thought that Teide 1 has the mass equivalent of about 55 Jupiters, which is considered large for a brown dwarf. Teide 1 is massive enough, and hence hot enough, to sustain lithium fusion in its core, but is unable to initiate hydrogen fusion like our sun. Teide 1 is probably only about 120 million years old (compared to our sun's age of 4.5 billion years) and shines at a temperature of 4,000o F, less than half as hot as the surface of our sun. In this image a young planet orbits Teide 1 from distance of about four million miles. The planet has acquired enough atmosphere to host clouds and put a lower limit on size of meteors that reach its surface (the smaller ones burn up before reaching the ground), but it is still very early in its evolution. Teide 1 looms large in this planet's sky, but in fact Teide 1's diameter is only about twice that of Jupiter's. All brown dwarfs are roughly the size of Jupiter - - the more massive brown dwarfs are simply more dense. As for this planet, it is very unlikely that life will ever evolve here due to its host's relatively short life span; in just another billion years Teide 1 will have cooled to a modest 1,700o F
Planete near a globular cluster - Artist view - Planet close to a globular cluster - Artist view
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
Planetary system around Trappist-1 - Artist's impression 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. This artist's impression shows the view from the surface of one of the planets in the TRAPPIST-1 system. At least seven planets orbit this ultra cool dwarf star 40 light-years from Earth in Aquarius constellation and they are all roughly the same size as the Earth. They are at the right distances from their star for liquid water to exist on the surfaces of several of them.
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 December 16, 2009. It is located about 40 light 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 around a binary star - Artist view - Binary Red Giants Exoplanet - Artist rendering