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Bilder zu 'Brauner Zwerg' gefunden, 31

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Brown dwarf star Gliese 229b: Artist's view of the brown dwarf star Gliese 229 B seen from a possible satellite. Discovered in 1995 in the constellation Lievre at 18 light years from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and would be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a satellite. Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun

Brown dwarf star Gliese 229b: Artist's view of the brown dwarf star Gliese 229 B seen from a possible satellite. Discovered in 1995 in the constellation Lievre at 18 light years from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and would be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a satellite. Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun

Miller, Ron (b.1947)

PIX4607542

Different types of brown dwarves - Artist's view - Different types of brown dwarves. Artwork - From left to right: brown dwarf type M, the youngest and most massive, temperature between 200 and 3000 degres Kelvin; brown dwarf type L, between 1500 and 2000 degres Kelvin; brown dwarf type T, between 1200 and 1500 degres Kelvin; brown dwarf type T but colder, from 1200 to 600 degres Kelvin; brown dwarf type still indefinite, less than 600 degres Kelvin; finally, on the right, Jupiter for size comparison. From left to right: a brown dwarf of type M (the youngest and most massive brown dwarves), a brown dwarf of type L, then a type T, another type T but colder, then another brown dwarf with a type unidentified yet which is colder, at last Jupiter for comparison

Different types of brown dwarves - Artist's view - Different types of brown dwarves. Artwork - From left to right: brown dwarf type M, the youngest and most massive, temperature between 200 and 3000 degres Kelvin; brown dwarf type L, between 1500 and 2000 degres Kelvin; brown dwarf type T, between 1200 and 1500 degres Kelvin; brown dwarf type T but colder, from 1200 to 600 degres Kelvin; brown dwarf type still indefinite, less than 600 degres Kelvin; finally, on the right, Jupiter for size comparison. From left to right: a brown dwarf of type M (the youngest and most massive brown dwarves), a brown dwarf of type L, then a type T, another type T but colder, then another brown dwarf with a type unidentified yet which is colder, at last Jupiter for comparison

L. Bret

PIX4572495

Brunette dwarves and young stars - Artist's view - Brown dwarves and young stars. Artwork - Surface of a brown dwarf in the foreground; in the background of the young stars and another brown dwarf. In foreground the surface of a brown dwarf; in the sky, young stars and another brown dwarf

Brunette dwarves and young stars - Artist's view - Brown dwarves and young stars. Artwork - Surface of a brown dwarf in the foreground; in the background of the young stars and another brown dwarf. In foreground the surface of a brown dwarf; in the sky, young stars and another brown dwarf

L. Bret

PIX4572522

The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison

The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison

L. Bret

PIX4572490

Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As

Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As

Walter B Myers

PIX4572553

Double star Gliese 623 - Double star system Gliese 623 in Hercules - Gliese 623 is a double star located about 25 years ago - light in the constellation Hercules. The Hubble space telescope was able for the first time to obtain an image of the two stars that make up this system, in June 1994. The two stars are separated by about twice the distance from Earth to Sun. On the right, 623b, a star 60,000 times less bright than the Sun, and 10 times less massive. Its nature is misidentified, it's a red dwarf or a brown dwarf. A dim double star system cataloged as Gliese 623 lies 25 light - years from Earth, in the constellation of Hercules. The individual stars of this binary system were distinguished for the first time when the Hubble Space Telescope's Faint Object Camera recorded this image in June 1994. They are separated by 200 million miles - about twice the Earth/Sun distance. On the right, the fainter Gliese 623b is 60,000 times less luminous than the Sun and approximately 10 times le

Double star Gliese 623 - Double star system Gliese 623 in Hercules - Gliese 623 is a double star located about 25 years ago - light in the constellation Hercules. The Hubble space telescope was able for the first time to obtain an image of the two stars that make up this system, in June 1994. The two stars are separated by about twice the distance from Earth to Sun. On the right, 623b, a star 60,000 times less bright than the Sun, and 10 times less massive. Its nature is misidentified, it's a red dwarf or a brown dwarf. A dim double star system cataloged as Gliese 623 lies 25 light - years from Earth, in the constellation of Hercules. The individual stars of this binary system were distinguished for the first time when the Hubble Space Telescope's Faint Object Camera recorded this image in June 1994. They are separated by 200 million miles - about twice the Earth/Sun distance. On the right, the fainter Gliese 623b is 60,000 times less luminous than the Sun and approximately 10 times le

PIX4572158

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,

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,

Walter B Myers

PIX4572545

Brown dwarf around the red dwarf star Gliese 229 - Brown dwarf around red dwarf Gliese 229 - First false-colored image of a brown dwarf. With a mass of 20 to 50 times that of Jupiter, but of a diameter equivalent to the gas planet, GL229B, is orbiting around the red dwarf star Gliese 229, about 18 years - light from Earth in the constellation Lievre. On the left, the observation made from the ground in adaptive optics at Mount Palomar, October 27, 1994. On the right, the image obtained by the Hubble space telescope on November 17, 1995. These two false - color telescope images reveal the faintest object ever seen around a star beyond our Sun, and the first unambiguous detection of a brown dwarf. The brown dwarf, called GL229B, orbits the red dwarf star Gliese 229, located approximately 18 light - years away in the constellation Lepus. The brown dwarf is about 20 - 50 times the mass of Jupiter, but is so dense it is about the same diameter as Jupiter (80,000 miles). Brown dwarfs are a m

Brown dwarf around the red dwarf star Gliese 229 - Brown dwarf around red dwarf Gliese 229 - First false-colored image of a brown dwarf. With a mass of 20 to 50 times that of Jupiter, but of a diameter equivalent to the gas planet, GL229B, is orbiting around the red dwarf star Gliese 229, about 18 years - light from Earth in the constellation Lievre. On the left, the observation made from the ground in adaptive optics at Mount Palomar, October 27, 1994. On the right, the image obtained by the Hubble space telescope on November 17, 1995. These two false - color telescope images reveal the faintest object ever seen around a star beyond our Sun, and the first unambiguous detection of a brown dwarf. The brown dwarf, called GL229B, orbits the red dwarf star Gliese 229, located approximately 18 light - years away in the constellation Lepus. The brown dwarf is about 20 - 50 times the mass of Jupiter, but is so dense it is about the same diameter as Jupiter (80,000 miles). Brown dwarfs are a m

PIX4572124

Brown dwarves Oph 1622 - Artist's view - Brown dwarves Oph 1622 - These two stars orbit each other in the constellation Ophiuchus. First identified as floating planets, isolated planets without nearby stars, they are now identified as two brown dwarf stars. Artwork of the two brown dwarves Oph 1622 in Ophiuchus

Brown dwarves Oph 1622 - Artist's view - Brown dwarves Oph 1622 - These two stars orbit each other in the constellation Ophiuchus. First identified as floating planets, isolated planets without nearby stars, they are now identified as two brown dwarf stars. Artwork of the two brown dwarves Oph 1622 in Ophiuchus

H. Piraud

PIX4572535

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

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

Walter B Myers

PIX4572527

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

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

Walter B Myers

PIX4572539

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)

PIX4607656

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

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

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

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

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

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

Walter B Myers

PIX4572541

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 light years away 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 light years away 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)

PIX4607648

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

PIX4568892

Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field

Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field

Dixon, Don (b.1951)

PIX4572525

Exploration of the exoplanet 2M1207B - Artist view - Exoplanet 2M1207B - Artist rendering: A probe studies the atmosphere of the extrasolar planet 2M1207B. 2M1207B is 5 times more massive than Jupiter and is located about 200 light years away in the constellation of Hydra. It is orbiting a brown dwarf star, visible in the sky. Artwork of the extrasolar planet 2M1207B atmosphere studied by a spaceprobe. 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

Exploration of the exoplanet 2M1207B - Artist view - Exoplanet 2M1207B - Artist rendering: A probe studies the atmosphere of the extrasolar planet 2M1207B. 2M1207B is 5 times more massive than Jupiter and is located about 200 light years away in the constellation of Hydra. It is orbiting a brown dwarf star, visible in the sky. Artwork of the extrasolar planet 2M1207B atmosphere studied by a spaceprobe. 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)

PIX4607635

The evolution of stars - Illustration - The evolution of the stars - Illustration - All stars are born in interstellar clouds but depending on their masses, they will follow different destinies. Stars are all born in interstellar clouds but according to their mass, they will follow different destinies

The evolution of stars - Illustration - The evolution of the stars - Illustration - All stars are born in interstellar clouds but depending on their masses, they will follow different destinies. Stars are all born in interstellar clouds but according to their mass, they will follow different destinies

P. Carril

PIX4573031

The evolution of stars - Illustration - The evolution of stars - Illustration - All stars are born in interstellar clouds but according to their masses they will follow different destinies. From top to bottom: - The brown dwarf - The red dwarf, a small star that will become a white dwarf and then a black dwarf. - A star of the same type as the Sun, which will evolve into a red giant then planetary nebula to become a white dwarf and end up as a black dwarf. - A blue giant star that becomes supergeant red to explode in supernova and finish either black hole or neutron star. Every stars come to life in interstellar clouds, but their evolution will depend on their mass; from top to bottom: - A brown dwarf - A red dwarf, a small star which will slowly collapse to become a white dwarf then a black dwarf. - A Sun - like star will become a red giant then a planetary nebula, a white dwarf and will end as a black dwarf. - A blue star will become a red supergiant, then will explode in a supernova

The evolution of stars - Illustration - The evolution of stars - Illustration - All stars are born in interstellar clouds but according to their masses they will follow different destinies. From top to bottom: - The brown dwarf - The red dwarf, a small star that will become a white dwarf and then a black dwarf. - A star of the same type as the Sun, which will evolve into a red giant then planetary nebula to become a white dwarf and end up as a black dwarf. - A blue giant star that becomes supergeant red to explode in supernova and finish either black hole or neutron star. Every stars come to life in interstellar clouds, but their evolution will depend on their mass; from top to bottom: - A brown dwarf - A red dwarf, a small star which will slowly collapse to become a white dwarf then a black dwarf. - A Sun - like star will become a red giant then a planetary nebula, a white dwarf and will end as a black dwarf. - A blue star will become a red supergiant, then will explode in a supernova

PIX4573087

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

PIX4568835

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Sebastian Voltmer

PIX4568871

NASA's WISE has uncovered the coldest brown dwarf known so far (green dot in very center of this infrared image). Called WISE 1828+2650, this chilly star-like body isn't even as warm as a human body.

NASA's WISE has uncovered the coldest brown dwarf known so far (green dot in very center of this infrared image). Called WISE 1828+2650, this chilly star-like body isn't even as warm as a human body.

UIG867321

The green dot in the middle of this image is a dim star belonging to a class called brown dwarfs. This particular object is named "WISEPC J045853.90+643451.9" after its location in the sky. WISE.

The green dot in the middle of this image is a dim star belonging to a class called brown dwarfs. This particular object is named "WISEPC J045853.90+643451.9" after its location in the sky. WISE.

UIG867233

Dwarf (earthenware, tan slip)

Dwarf (earthenware, tan slip)

Chinese School, Han Dynasty (100-300 AD)

IMA484788

Star, Planet and Brown Dwarf Formation - Schema illustrating how stars (left), planets (middle) and brown dwarf (right) form based on the mass of their primitive nebula. Infographic showing how stars (left arrow), planets (middle), and brown dwarfs (right) form depending on the mass of their parent nebula. Artwor

Star, Planet and Brown Dwarf Formation - Schema illustrating how stars (left), planets (middle) and brown dwarf (right) form based on the mass of their primitive nebula. Infographic showing how stars (left arrow), planets (middle), and brown dwarfs (right) form depending on the mass of their parent nebula. Artwor

Dixon, Don (b.1951)

PIX4572945

Exoplanete BD+48 738c - Illustration of an extrasolar planet orbiting a red dwarf star. In the sky, close to the dwarf star, the giant red star BD+48 738. It's a large planet, which may be a small brown dwarf, that orbits a red dwarf star. According to one reference: “”... one of the massive, dying stars - - BD+48 738 - - is accompanied not only by an enormous, Jupiter - like planet, but also by a second, mystery object. According to the team, this object could be another planet, a low - mass star, or - - most interestingly - - a brown dwarf, which is a star - like body that is intermediate in mass between the coolest stars and giant planets.

Exoplanete BD+48 738c - Illustration of an extrasolar planet orbiting a red dwarf star. In the sky, close to the dwarf star, the giant red star BD+48 738. It's a large planet, which may be a small brown dwarf, that orbits a red dwarf star. According to one reference: “”... one of the massive, dying stars - - BD+48 738 - - is accompanied not only by an enormous, Jupiter - like planet, but also by a second, mystery object. According to the team, this object could be another planet, a low - mass star, or - - most interestingly - - a brown dwarf, which is a star - like body that is intermediate in mass between the coolest stars and giant planets.

Miller, Ron (b.1947)

PIX4574061

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