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Artwork from ' Ron Miller (b.1947)' found, 578

 
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Exoplanete around a neutron star - Neutron Star Planet - Illustration

Miller, Ron (b.1947)

PIX4574288

Exoplanete around a neutron star - Neutron Star Planet - Illustration

Miller, Ron (b.1947)

PIX4574288

 
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Core of a Comet - Illustration - Comet nucleus Artwork

Miller, Ron (b.1947)

PIX4588722

Core of a Comet - Illustration - Comet nucleus Artwork

Miller, Ron (b.1947)

PIX4588722

 
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Moon Formation: Hypotheses of impact giant - Moon Formation: Giant impact hypothesis: The hypotheses of impact giant suggests that the Moon was created from material ejecteated by a collision between the young Earth and a body the size of Mars named Theia, 4.5 billion years ago - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, approximately 4.5 billion years ago

Miller, Ron (b.1947)

PIX4614839

Moon Formation: Hypotheses of impact giant - Moon Formation: Giant impact hypothesis: The hypotheses of impact giant suggests that the Moon was created from material ejecteated by a collision between the young Earth and a body the size of Mars named Theia, 4.5 billion years ago - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, approximately 4.5 billion years ago

Miller, Ron (b.1947)

PIX4614839

 
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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

Miller, Ron (b.1947)

PIX4607542

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

 
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Ice structures on the Europe satellite - Illustration - Europa ice features

Miller, Ron (b.1947)

PIX4614387

Ice structures on the Europe satellite - Illustration - Europa ice features

Miller, Ron (b.1947)

PIX4614387

 
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Ice structures on the Europe satellite - Illustration - Europa ice features: Europa Iceberg

Miller, Ron (b.1947)

PIX4614409

Ice structures on the Europe satellite - Illustration - Europa ice features: Europa Iceberg

Miller, Ron (b.1947)

PIX4614409

 
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Jupiter and the Sun seen from the volcanic surface of Io.

Miller, Ron (b.1947)

PIX4614428

Jupiter and the Sun seen from the volcanic surface of Io.

Miller, Ron (b.1947)

PIX4614428

 
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A Day on Io - 5/6 - Illustration - A Day on Io - 5/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-5. Ten and a half hours later, the sun set on the horizon of Io. Jupiter is in his last quarter phase. In the distance, a volcano erupts and the gases emitted into the thin atmosphere of Io illuminate in the magnetic field surrounding Jupiter and Io - Io keeps the same face towards Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 5. Ten and a half hours later and the sun has now set below Io's horizon. Jupiter is in its last quarter phase. A distant vo

Miller, Ron (b.1947)

PIX4614156

A Day on Io - 5/6 - Illustration - A Day on Io - 5/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-5. Ten and a half hours later, the sun set on the horizon of Io. Jupiter is in his last quarter phase. In the distance, a volcano erupts and the gases emitted into the thin atmosphere of Io illuminate in the magnetic field surrounding Jupiter and Io - Io keeps the same face towards Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 5. Ten and a half hours later and the sun has now set below Io's horizon. Jupiter is in its last quarter phase. A distant vo

Miller, Ron (b.1947)

PIX4614156

 
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Astronauts on Io - Illustration - Astronauts on Io - Artwork: Astronauts admire a volcanic eruption on Io

Miller, Ron (b.1947)

PIX4614231

Astronauts on Io - Illustration - Astronauts on Io - Artwork: Astronauts admire a volcanic eruption on Io

Miller, Ron (b.1947)

PIX4614231

 
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Io vu du satellite Thebe - Illustration - Io seen from Thebe

Miller, Ron (b.1947)

PIX4614241

Io vu du satellite Thebe - Illustration - Io seen from Thebe

Miller, Ron (b.1947)

PIX4614241

 
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Jupiter Ring - Illustration - Jupiter Ring: Jupiter is surrounded by a system of very dark rings composed of dust torn from some of its satellites. This system consists of a main ring, located between the satellites Metis and Adrastee, then rings very held on the orbits of the satellites Amalthee and Thebe - Jupiter's Main ring is believed to be composed of dust and debris from meteoroid impacts with Jupiter's tiny innermost satellites Metis and Adrastea. Jupiter hosts two other broader and more diffuse rings which are believed to be generated and replenished by meteoroid impacts on the tiny satellites Thebe and Amalthea

Miller, Ron (b.1947)

PIX4614259

Jupiter Ring - Illustration - Jupiter Ring: Jupiter is surrounded by a system of very dark rings composed of dust torn from some of its satellites. This system consists of a main ring, located between the satellites Metis and Adrastee, then rings very held on the orbits of the satellites Amalthee and Thebe - Jupiter's Main ring is believed to be composed of dust and debris from meteoroid impacts with Jupiter's tiny innermost satellites Metis and Adrastea. Jupiter hosts two other broader and more diffuse rings which are believed to be generated and replenished by meteoroid impacts on the tiny satellites Thebe and Amalthea

Miller, Ron (b.1947)

PIX4614259

 
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Pust Tempete sur Mars - Illustration - Channel and dust storm on Mars: Landscape on Mars with dust devils - Mars with dust devils

Miller, Ron (b.1947)

PIX4617018

Pust Tempete sur Mars - Illustration - Channel and dust storm on Mars: Landscape on Mars with dust devils - Mars with dust devils

Miller, Ron (b.1947)

PIX4617018

 
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Fog in a Martian Vallee - Illustration - Foggy Mars valley

Miller, Ron (b.1947)

PIX4617030

Fog in a Martian Vallee - Illustration - Foggy Mars valley

Miller, Ron (b.1947)

PIX4617030

 
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Surface de Mercure - Artist View - Pit-like features on Mercury

Miller, Ron (b.1947)

PIX4617440

Surface de Mercure - Artist View - Pit-like features on Mercury

Miller, Ron (b.1947)

PIX4617440

 
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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

Miller, Ron (b.1947)

PIX4607862

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

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

Miller, Ron (b.1947)

PIX4607866

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

Miller, Ron (b.1947)

PIX4607866

 
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Artist's view of the exoplanet Gliese 581c - Artwork of exoplanet Gliese 581c: The star Gliese 581 seen from the surface of the exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible alien life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super-earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super-earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.””

Miller, Ron (b.1947)

PIX4607996

Artist's view of the exoplanet Gliese 581c - Artwork of exoplanet Gliese 581c: The star Gliese 581 seen from the surface of the exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible alien life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super-earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super-earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.””

Miller, Ron (b.1947)

PIX4607996

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

Miller, Ron (b.1947)

PIX4608132

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

Miller, Ron (b.1947)

PIX4608132

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

Miller, Ron (b.1947)

PIX4608244

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

Miller, Ron (b.1947)

PIX4608244

 
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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 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

 
Special Instructions
  • No additional copyright fee required
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 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

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