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Bilder zu 'Hot Jupiter' gefunden, 32

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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

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

Jupiter Terrace, Yellowstone, 1893 (oil on canvas)

Jupiter Terrace, Yellowstone, 1893 (oil on canvas)

Moran, Thomas (1837-1926)

CH985289

Star HD 189733 and nebula planetary Dumbbell (M27) - A star field with HD 189733 and Dumbell nebula - Image centree on the star HD 189733 located 63 years ago - light in the constellation Petite Fox. Astronomers discovered around this star an exoplanet (HD 189733b). This gas planet a little bigger than Jupiter is very close to its star; this type of planet is called hot Jupiter. We detected the presence of mists in his atmosphere. To the right of this star is the planetary nebula Dumbbell (M27) located about 1400 years from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. A star field image showing the star HD 189733 (centre) with Dumbell nebula. Orbiting close to its parent star, is an extrasolar planet, HD 189733b, a 'hot - Jupiter' type of gas giant slightly larger than Jupiter. The observations provide clear evidence of the presence of hazes in its atmosphere. To the right

Star HD 189733 and nebula planetary Dumbbell (M27) - A star field with HD 189733 and Dumbell nebula - Image centree on the star HD 189733 located 63 years ago - light in the constellation Petite Fox. Astronomers discovered around this star an exoplanet (HD 189733b). This gas planet a little bigger than Jupiter is very close to its star; this type of planet is called hot Jupiter. We detected the presence of mists in his atmosphere. To the right of this star is the planetary nebula Dumbbell (M27) located about 1400 years from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. A star field image showing the star HD 189733 (centre) with Dumbell nebula. Orbiting close to its parent star, is an extrasolar planet, HD 189733b, a 'hot - Jupiter' type of gas giant slightly larger than Jupiter. The observations provide clear evidence of the presence of hazes in its atmosphere. To the right

PIX4623483

Exoplanete HAT-P-32 b - Artist's view: HAT-P-32 b is an exoplanet orbiting around the star HAT-P-32. Discovered on 8 June 2011 by the transit method, it is 0.941 times the mass of Jupiter. Its radius makes it the largest exoplanet known at the end of 2012. Hat-P-32b is a planet in the orbit of the star HAT-P-32, which is approximately 1,044 light years away from Earth in Andromeda constellation. The planet is considered a Hot Jupiter, and although it is slightly less massive than Jupiter, it is bloated to nearly twice Jupiter's size. At the time of its discovery, Hat-p-32b had one of the largest radii known among extrasolar planets

Exoplanete HAT-P-32 b - Artist's view: HAT-P-32 b is an exoplanet orbiting around the star HAT-P-32. Discovered on 8 June 2011 by the transit method, it is 0.941 times the mass of Jupiter. Its radius makes it the largest exoplanet known at the end of 2012. Hat-P-32b is a planet in the orbit of the star HAT-P-32, which is approximately 1,044 light years away from Earth in Andromeda constellation. The planet is considered a Hot Jupiter, and although it is slightly less massive than Jupiter, it is bloated to nearly twice Jupiter's size. At the time of its discovery, Hat-p-32b had one of the largest radii known among extrasolar planets

Miller, Ron (b.1947)

PIX4607841

Exoplanete WASP-142b: WASP-142b is a warm Jupiter exoplanet in the constellation Hydra. An artist's impression of the planet WASP-142b, depicted as seen from a hypothetical moon

Exoplanete WASP-142b: WASP-142b is a warm Jupiter exoplanet in the constellation Hydra. An artist's impression of the planet WASP-142b, depicted as seen from a hypothetical moon

Miller, Ron (b.1947)

PIX4608335

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

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter

Miller, Ron (b.1947)

PIX4608293

Exoplanete WASP-18b: WASP-18b is a hot Jupiter exoplanet orbiting in less than a day around the star WASP-18. WASP-18b is a “” hot Jupiter,””” a giant exoplanet that orbits very close to its star, located about 330 light years from Earth. Specifically, the mass of WASP-18b is estimated to be about ten times that of Jupiter, yet it orbits its star about once every 23 hours

Exoplanete WASP-18b: WASP-18b is a hot Jupiter exoplanet orbiting in less than a day around the star WASP-18. WASP-18b is a “” hot Jupiter,””” a giant exoplanet that orbits very close to its star, located about 330 light years from Earth. Specifically, the mass of WASP-18b is estimated to be about ten times that of Jupiter, yet it orbits its star about once every 23 hours

PIX4608353

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

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter - HD 149026b (in the background) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 years - light in the constellation Hercules. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b, is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the hottest. HD 149026b is located 256 light -

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter - HD 149026b (in the background) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 years - light in the constellation Hercules. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b, is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the hottest. HD 149026b is located 256 light -

PIX4573429

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter: HD 149026b (or Smertrios) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 light-years in the constellation Hercules. Here, the planet represented by day. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b (or Smertrios), is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter: HD 149026b (or Smertrios) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 light-years in the constellation Hercules. Here, the planet represented by day. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b (or Smertrios), is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the

Miller, Ron (b.1947)

PIX4607859

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter - HD 149026b (in the background) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 years - light in the constellation Hercules. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b, is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the hottest. HD 149026b is located 256 light -

Artist's view of a hot Jupiter HD 149026b - Exoplanet HD 149026b - Hot Jupiter - HD 149026b (in the background) is to date the hottest exoplanet in the universe. This warm Jupiter reaches a temperature of 2000 degrees; it absorbs almost all the light of its star and is therefore also the darkest planet in the universe. HD 149026b is located 256 years - light in the constellation Hercules. This artist's concept illustrates the hottest planet yet observed in the universe. This “” hot Jupiter”” called HD 149026b, is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) - about 3 times hotter than the rocky surface of Venus, the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet in the universe, in addition to the hottest. HD 149026b is located 256 light -

PIX4573447

Star HD 209458 in Pegase - Star HD 209458 in Pegasus - This star, located in the center of the image, is about 150 years from Earth and is observable with a pair of binoculars. In orbit around this star, invisible in this image, we discovered a giant planet called Osiris (HD 209458b). This extrasolar planet of a new type is a hot Jupiter, a massive planet very close to its star. The star located in the center of this image is called HD 209458. It is similar to our Sun and lies 150 light - years from Earth. It is visible with binoculars as a seventh magnitude star in the constellation of Pegasus. In orbit around this star (but invisible on this picture) is an exoplanet named Osiris (HD 209458b). It is a hot jupiter, a giant planet orbiting very close to its star

Star HD 209458 in Pegase - Star HD 209458 in Pegasus - This star, located in the center of the image, is about 150 years from Earth and is observable with a pair of binoculars. In orbit around this star, invisible in this image, we discovered a giant planet called Osiris (HD 209458b). This extrasolar planet of a new type is a hot Jupiter, a massive planet very close to its star. The star located in the center of this image is called HD 209458. It is similar to our Sun and lies 150 light - years from Earth. It is visible with binoculars as a seventh magnitude star in the constellation of Pegasus. In orbit around this star (but invisible on this picture) is an exoplanet named Osiris (HD 209458b). It is a hot jupiter, a giant planet orbiting very close to its star

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

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

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Cyclones encircle Jupiter's North Pole (photo)

Cyclones encircle Jupiter's North Pole (photo)

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Jupiter's Aurora Illustration, 2015

Jupiter's Aurora Illustration, 2015

Roetsch, Tobias

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Lava lake on Io - Illustration - Lava lake on Io - Artist's view of a lava lake on the surface of Io, one of Jupiter's satellites. There are places on Io where molten lava has been observed actively welling up from beneath the surface of this otherwise frozen world. Lavas on Io were originally thought to be molten sulfur, but with caldera temperatures far exceeding 1,000o F - - too hot for liquid sulfur - - these eruptions are now thought to be primarily molten silicate rocks. In this image a dormant volcanic caldera re - awakens with a surge of new lava that breaks up and melts a frozen crust. A gibbous Jupiter hangs over the horizon

Lava lake on Io - Illustration - Lava lake on Io - Artist's view of a lava lake on the surface of Io, one of Jupiter's satellites. There are places on Io where molten lava has been observed actively welling up from beneath the surface of this otherwise frozen world. Lavas on Io were originally thought to be molten sulfur, but with caldera temperatures far exceeding 1,000o F - - too hot for liquid sulfur - - these eruptions are now thought to be primarily molten silicate rocks. In this image a dormant volcanic caldera re - awakens with a surge of new lava that breaks up and melts a frozen crust. A gibbous Jupiter hangs over the horizon

Walter B Myers

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Front view of Mammoth Hot Springs, Cleopatra and Jupiter Terraces (b/w photo)

Front view of Mammoth Hot Springs, Cleopatra and Jupiter Terraces (b/w photo)

American Photographer (19th century) (after)

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Size comparison: Earth, Moon and Galilean satellites - Jupiter's four largest satellites and Earth and the Moon compared - Jupiter's four largest satellites, called Galilean satellites, compared to Earth and Moon. At the top, from left to right, in order of their distance to the planet Jupiter, we find Io, Europe, Ganymede and Callisto. Ganymede is the largest satellite in the solar system. Jupiter's four largest satellites, also known as the “” Galilean”” satellites since they were first observed by the Italian astronomer Galileo over 400 years ago, are worlds in their own right. Top row, left to right, in order from their distances from Jupiter, are: Io, Europa, Ganymede, Callisto Io is the most volcanic world in the Solar System, resurfacing itself continually with extremely hot and massive eruptions that spew material over 200 miles into space. Europa is about the same size as Earth's Moon, however unlike the Moon which is made up mostly of dry silicate materials, Europa is believe

Size comparison: Earth, Moon and Galilean satellites - Jupiter's four largest satellites and Earth and the Moon compared - Jupiter's four largest satellites, called Galilean satellites, compared to Earth and Moon. At the top, from left to right, in order of their distance to the planet Jupiter, we find Io, Europe, Ganymede and Callisto. Ganymede is the largest satellite in the solar system. Jupiter's four largest satellites, also known as the “” Galilean”” satellites since they were first observed by the Italian astronomer Galileo over 400 years ago, are worlds in their own right. Top row, left to right, in order from their distances from Jupiter, are: Io, Europa, Ganymede, Callisto Io is the most volcanic world in the Solar System, resurfacing itself continually with extremely hot and massive eruptions that spew material over 200 miles into space. Europa is about the same size as Earth's Moon, however unlike the Moon which is made up mostly of dry silicate materials, Europa is believe

Walter B Myers

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Artist's view of a hot Jupiter. - Artist's view of an exoplanet gas very close to its star. Artist's impression of a hot Jupiter

Artist's view of a hot Jupiter. - Artist's view of an exoplanet gas very close to its star. Artist's impression of a hot Jupiter

H. Piraud

PIX4573858

Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star

Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star

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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

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Artist's View of a Hot Jupiter - Artist's View of a Giant Gas Exoplanet Very Close to its Star

Artist's View of a Hot Jupiter - Artist's View of a Giant Gas Exoplanet Very Close to its Star

Dixon, Don (b.1951)

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Infrared and visible images of Jupiter, 1979

Infrared and visible images of Jupiter, 1979

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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

Miller, Ron (b.1947)

PIX4608303

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

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In the sapphire winds of the exoplanet HAT-P-7b

In the sapphire winds of the exoplanet HAT-P-7b

Miller, Ron (b.1947)

PIX7223406

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter. This illustration presents a purely speculative view of what such a “” hot Jupiter”” might look like. It could have a powerful magnetic field that traps charged particles from the star. These particles create glowing auroral rings around the planet's magnetic poles

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter. This illustration presents a purely speculative view of what such a “” hot Jupiter”” might look like. It could have a powerful magnetic field that traps charged particles from the star. These particles create glowing auroral rings around the planet's magnetic poles

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Exoplanet Kelt-9b - Illustration

Exoplanet Kelt-9b - Illustration

Miller, Ron (b.1947)

PIX7223407

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

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Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light 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. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light 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. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Walter B Myers

PIX4573224

Planetary nebula NGC 3242 ultraviolet view - Planetary nebula NGC 3242 seen in ultraviolet - The planetary nebula NGC 3242, also called the ghost of Jupiter, ultraviolet view by the GALEX satellite. NGC 3242 is located between 1400 and 2500 years - light of the Earth, in the constellation Hydra (hydra, or female hydra). This ultraviolet image from NASA's Galaxy Evolution Explorer (GALEX) shows NGC 3242, a planetary nebula frequently referred to as “” Jupiter's Ghost.””” When stars with a mass similar to our sun approach the end of their lives by exhausting supplies of hydrogen and helium fuel in their cores, they swell up into cool red - giant stars. In a last gasp before death, they expel the layers of gas in their outer atmosphere. This exposes the core of the dying star, a dense hot ball of carbon and oxygen called a white dwarf. The white dwarf is so hot that it shines very brightly in the ultraviolet. The ultraviolet light from the white dwarf, in turn, ionizes the gaseous materia

Planetary nebula NGC 3242 ultraviolet view - Planetary nebula NGC 3242 seen in ultraviolet - The planetary nebula NGC 3242, also called the ghost of Jupiter, ultraviolet view by the GALEX satellite. NGC 3242 is located between 1400 and 2500 years - light of the Earth, in the constellation Hydra (hydra, or female hydra). This ultraviolet image from NASA's Galaxy Evolution Explorer (GALEX) shows NGC 3242, a planetary nebula frequently referred to as “” Jupiter's Ghost.””” When stars with a mass similar to our sun approach the end of their lives by exhausting supplies of hydrogen and helium fuel in their cores, they swell up into cool red - giant stars. In a last gasp before death, they expel the layers of gas in their outer atmosphere. This exposes the core of the dying star, a dense hot ball of carbon and oxygen called a white dwarf. The white dwarf is so hot that it shines very brightly in the ultraviolet. The ultraviolet light from the white dwarf, in turn, ionizes the gaseous materia

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