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Bilder zu 'Neptun-Satellit' gefunden, 34

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Neptune view from Naiade - Illustration - Neptune seen from Naiad: Neptune with its satellite Naiade in the foreground

Neptune view from Naiade - Illustration - Neptune seen from Naiad: Neptune with its satellite Naiade in the foreground

Miller, Ron (b.1947)

PIX4624108

Neptune from Triton - Illustration - Neptune from the surface of Triton - Neptune seen from the icy surface of his Triton satellite. White cirrus clouds race across a crescent Neptune as it presides over Triton's bleak and frozen south polar region. Sheets of frozen nitrogen ice with traces of other substances, including frozen methane and carbon monoxide, overlie Triton's darker material. The ice has turned pink due to the interaction with ultraviolet light from the distant Sun. Further south all of the surface of Triton is covered by such ices

Neptune from Triton - Illustration - Neptune from the surface of Triton - Neptune seen from the icy surface of his Triton satellite. White cirrus clouds race across a crescent Neptune as it presides over Triton's bleak and frozen south polar region. Sheets of frozen nitrogen ice with traces of other substances, including frozen methane and carbon monoxide, overlie Triton's darker material. The ice has turned pink due to the interaction with ultraviolet light from the distant Sun. Further south all of the surface of Triton is covered by such ices

Walter B Myers

PIX4624055

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Miller, Ron (b.1947)

PIX4624114

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Miller, Ron (b.1947)

PIX4624116

Ice Volcano on Triton - Illustration - Ice volcano on Triton - Cryovolcanoes and geysers of nitrogen and methane have been observed on the surface of the Triton satellite. There is evidence that the south pole of Neptune's satellite Triton is host to dozens of ice volcanoes, or geysers. One such eruption was observed to shoot a towering jet of material to a height of five miles, while the tenuous nitrogen atmosphere carried the smoky plume over 80 miles “” downwind.” The eruptive material is believed to be a combination of liquid nitrogen, dust, and methane compounds driven by seasonal heating from the Sun

Ice Volcano on Triton - Illustration - Ice volcano on Triton - Cryovolcanoes and geysers of nitrogen and methane have been observed on the surface of the Triton satellite. There is evidence that the south pole of Neptune's satellite Triton is host to dozens of ice volcanoes, or geysers. One such eruption was observed to shoot a towering jet of material to a height of five miles, while the tenuous nitrogen atmosphere carried the smoky plume over 80 miles “” downwind.” The eruptive material is believed to be a combination of liquid nitrogen, dust, and methane compounds driven by seasonal heating from the Sun

Walter B Myers

PIX4624061

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Neptune from Nereide - Illustration - Neptune seen from Nereid - Illustration: Neptune with its Nereide satellite foreground

Miller, Ron (b.1947)

PIX4624110

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Miller, Ron (b.1947)

PIX4624089

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Miller, Ron (b.1947)

PIX4624092

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration: Artist's view of nitrogen geysers on the surface of Triton, Neptune's largest satellite - Artist's impression of nitrogen geysers on Triton surface, the largest moon of the planet Neptune

Miller, Ron (b.1947)

PIX4624102

Neptune from Triton - Illustration - Triton's shadow on Neptune - Neptune seen from the icy surface of his Triton satellite. The satellite projects its shadow on the Giant Planet. A full Neptune washes Triton's frozen surface with an indigo light, the only source of illumination on this now Triton's dark side. Fortuitous alignment of the Sun, Triton and Neptune causes this satellite's shadow to fall on Neptune's distant cloud tops 220 thousand miles away. This view is from within a deep, crater - like depression on Triton's northern hemisphere

Neptune from Triton - Illustration - Triton's shadow on Neptune - Neptune seen from the icy surface of his Triton satellite. The satellite projects its shadow on the Giant Planet. A full Neptune washes Triton's frozen surface with an indigo light, the only source of illumination on this now Triton's dark side. Fortuitous alignment of the Sun, Triton and Neptune causes this satellite's shadow to fall on Neptune's distant cloud tops 220 thousand miles away. This view is from within a deep, crater - like depression on Triton's northern hemisphere

Walter B Myers

PIX4624072

Neptune seen from its satellite Triton - Illustration - Neptune as seen from Triton - Illustratio

Neptune seen from its satellite Triton - Illustration - Neptune as seen from Triton - Illustratio

PIX4624077

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration - Artist's view of geysers on the surface of Triton, the largest satellite in Neptune. Artist's impression of geysers on Triton surface, the largest moon of the planet Neptun

Geyser on the Triton satellite - Illustration - Geyser on Triton - Illustration - Artist's view of geysers on the surface of Triton, the largest satellite in Neptune. Artist's impression of geysers on Triton surface, the largest moon of the planet Neptun

Miller, Ron (b.1947)

PIX4624130

Triton could break and form a new ring - Triton could break to give Neptune a new rings system.: Neptune and Triton- Illustration - Neptune with its moon Triton. Artwork

Triton could break and form a new ring - Triton could break to give Neptune a new rings system.: Neptune and Triton- Illustration - Neptune with its moon Triton. Artwork

S. Numazawa

PIX4623948

Neptune et Triton- Illustration - Neptune with its moon Triton Artwork

Neptune et Triton- Illustration - Neptune with its moon Triton Artwork

S. Numazawa

PIX4623956

Sunrise seen from Triton - Artist view - Sunrise on Triton - Artist view - Sunrise seen from Triton, the largest satellite in Neptune. A diminutive sun rises over Triton's hard and glistening landscape of rock, frozen water, carbon dioxide, nitrogen, and methane. The little warmth that reaches Triton's surface induces a nitrogen and methane haze, forming a very tenuous atmosphere. It is very cold on Triton with temperatures falling as low as minus 391o F. While as much as 25% of Triton may be composed of water ice, it is very unlikely that there is any liquid water, or life, on this world

Sunrise seen from Triton - Artist view - Sunrise on Triton - Artist view - Sunrise seen from Triton, the largest satellite in Neptune. A diminutive sun rises over Triton's hard and glistening landscape of rock, frozen water, carbon dioxide, nitrogen, and methane. The little warmth that reaches Triton's surface induces a nitrogen and methane haze, forming a very tenuous atmosphere. It is very cold on Triton with temperatures falling as low as minus 391o F. While as much as 25% of Triton may be composed of water ice, it is very unlikely that there is any liquid water, or life, on this world

Walter B Myers

PIX4624014

Neptune and Triton - Illustration - Neptune from Triton orbit - Neptune and its Triton satellite (foreground). Looking like an over - ripe cantaloupe, Neptune's satellite Triton is in the foreground while Neptune itself looms on the upper right. At a distance of 220 thousand miles, Triton is about the same distance from Neptune as the moon is from the Earth. A frozen world that's somewhat smaller than the moon, Triton is the seventh and largest of Neptune's satellites, completing an orbit every six days. Triton is believed to be composed primarily of rock and water ice with traces of methane and other compounds

Neptune and Triton - Illustration - Neptune from Triton orbit - Neptune and its Triton satellite (foreground). Looking like an over - ripe cantaloupe, Neptune's satellite Triton is in the foreground while Neptune itself looms on the upper right. At a distance of 220 thousand miles, Triton is about the same distance from Neptune as the moon is from the Earth. A frozen world that's somewhat smaller than the moon, Triton is the seventh and largest of Neptune's satellites, completing an orbit every six days. Triton is believed to be composed primarily of rock and water ice with traces of methane and other compounds

Walter B Myers

PIX4624052

Neptune - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This image suggests how Neptune might look from a position in space above the plane of its rings. Like Uranus, Neptune is a Gas Giant, composed primarily of hydrogen and helium gases surrounding a relatively small, dense core of molten rock and metal. Also like Uranus, Neptune has charcoal - colored rings, although they appear to be fewer in number than Uranus's. While Neptune's diameter is slightly less than Uranus ', it has more mass. Neptune's blue color is due to the presence of methane in its upper atmosphere. The dark spot in the southern hemisphere beneath the rings, dubbed “” The Great Dark Spot,””” is believed to be a giant storm which was active in 1989 when Voyager 2 photographed Neptune. Just beyond the rings at Neptune's 7 o'clock position, barely discernable from the background stars, is the tiny satellite Proteus. With an average diameter of

Neptune - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This image suggests how Neptune might look from a position in space above the plane of its rings. Like Uranus, Neptune is a Gas Giant, composed primarily of hydrogen and helium gases surrounding a relatively small, dense core of molten rock and metal. Also like Uranus, Neptune has charcoal - colored rings, although they appear to be fewer in number than Uranus's. While Neptune's diameter is slightly less than Uranus ', it has more mass. Neptune's blue color is due to the presence of methane in its upper atmosphere. The dark spot in the southern hemisphere beneath the rings, dubbed “” The Great Dark Spot,””” is believed to be a giant storm which was active in 1989 when Voyager 2 photographed Neptune. Just beyond the rings at Neptune's 7 o'clock position, barely discernable from the background stars, is the tiny satellite Proteus. With an average diameter of

Walter B Myers

PIX4624079

Comparison of the largest satellites in the solar system - Largest moons of the solar system - Photomontage showing the largest satellites in the solar system at the scale. Largest moons of the solar system shown to scale

Comparison of the largest satellites in the solar system - Largest moons of the solar system - Photomontage showing the largest satellites in the solar system at the scale. Largest moons of the solar system shown to scale

PIX4629974

Neptune seen from his satellite Triton - Illustration - Neptune and Triton - Illustration - Geyser artist's view on the surface of Neptune's largest satellite, Triton. Artist's impression of geyser on Triton surface, the largest moon of the planet Neptun

Neptune seen from his satellite Triton - Illustration - Neptune and Triton - Illustration - Geyser artist's view on the surface of Neptune's largest satellite, Triton. Artist's impression of geyser on Triton surface, the largest moon of the planet Neptun

M. Carroll

PIX4624009

Voyager 2 probe near Neptune - Voyager 2 spacecraft near Neptune - Artwork - The Voyager 2 probe orbited around Neptune in August 1989. Artist View Voyager 2 passes Neptune and Triton, its largest moon before leaving the Solar System forever

Voyager 2 probe near Neptune - Voyager 2 spacecraft near Neptune - Artwork - The Voyager 2 probe orbited around Neptune in August 1989. Artist View Voyager 2 passes Neptune and Triton, its largest moon before leaving the Solar System forever

Steven Hobbs

PIX4605819

Orbits of planets of Solar System and, in box, detail of Neptune and Pluto revolution around sun, Drawing (photo)

Orbits of planets of Solar System and, in box, detail of Neptune and Pluto revolution around sun, Drawing (photo)

DGA1135706

Earth and Moon - Artist view - Earth and Moon. Artwork - The Earth and the Moon represented on the scale (size but not distance) against the background of stars. Artist view of the Earth and the Moon showing their actual relative size (but not the actual distance between the two). Earth's equatorial diameter is 12,756 km while the Moon's diameter is 3,476 km. The Moon is actually one of the largest natural satellites in the Solar System, smaller only than Jupiter's Ganymede, Callisto and Io as well as Saturn's Titan, but bigger than Jupiter's Europa, Neptune's Triton and the planet Pluto

Earth and Moon - Artist view - Earth and Moon. Artwork - The Earth and the Moon represented on the scale (size but not distance) against the background of stars. Artist view of the Earth and the Moon showing their actual relative size (but not the actual distance between the two). Earth's equatorial diameter is 12,756 km while the Moon's diameter is 3,476 km. The Moon is actually one of the largest natural satellites in the Solar System, smaller only than Jupiter's Ganymede, Callisto and Io as well as Saturn's Titan, but bigger than Jupiter's Europa, Neptune's Triton and the planet Pluto

PIX4577456

The solar system - Our solar system. Artwork - Illustration of the solar system. Planets and their main satellites are represented in order of proximity to the sun. From right to left, the Sun, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. Planets and major moons to scale

The solar system - Our solar system. Artwork - Illustration of the solar system. Planets and their main satellites are represented in order of proximity to the sun. From right to left, the Sun, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. Planets and major moons to scale

Miller, Ron (b.1947)

PIX4630070

Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Miller, Ron (b.1947)

PIX4629567

Triton, Neptune satellite - Voyager 2 - High resolution mosaic of Triton, the largest satellite of Neptun

Triton, Neptune satellite - Voyager 2 - High resolution mosaic of Triton, the largest satellite of Neptun

PIX4623079

Neptune and its largest Triton satellite - Editing showing Neptune with its largest satellite in the foreground, Triton

Neptune and its largest Triton satellite - Editing showing Neptune with its largest satellite in the foreground, Triton

PIX4623032

Neptune view of Triton, its largest satellite - Artist view - Neptune view of Triton, its largest satellite - Vue d'artiste

Neptune view of Triton, its largest satellite - Artist view - Neptune view of Triton, its largest satellite - Vue d'artiste

Dixon, Don (b.1951)

PIX4624002

The Triton satellite seen by Voyager 2 - Faux-colored image of Triton, the largest satellite of Neptune, obtained by the Voyager 2 probe on August 24, 1989, has a distance of 530,000 km from the satellite

The Triton satellite seen by Voyager 2 - Faux-colored image of Triton, the largest satellite of Neptune, obtained by the Voyager 2 probe on August 24, 1989, has a distance of 530,000 km from the satellite

PIX4623044

Planets of the solar system -2006 - Our solar system. 2006 - Planets are represented in order of proximity to the sun. From top to bottom: Mercury, Venus, Earth and Moon, its satellite, Mars, Jupiter, Saturn, Uranus, Neptune. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. This is a montage of planetary images taken by spacecraft managed by the Jet Propulsion Laboratory in Pasadena, CA. Included are (from top to bottom) images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus and Neptune. The spacecraft responsible for these images are as follows: the Mercury image was taken by Mariner 10, the Venus image by Magellan, the Earth and Moon images by Galileo, the Mars image by Mars Global Surveyor, the Jupiter image by Cassini, and the Saturn, Uranus and Neptune images by Voyager. Pluto is not shown as no spacecraft has yet visited it. The inner planets (Mercury, Venus, Earth, Moon, and Mars) are roug

Planets of the solar system -2006 - Our solar system. 2006 - Planets are represented in order of proximity to the sun. From top to bottom: Mercury, Venus, Earth and Moon, its satellite, Mars, Jupiter, Saturn, Uranus, Neptune. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. This is a montage of planetary images taken by spacecraft managed by the Jet Propulsion Laboratory in Pasadena, CA. Included are (from top to bottom) images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus and Neptune. The spacecraft responsible for these images are as follows: the Mercury image was taken by Mariner 10, the Venus image by Magellan, the Earth and Moon images by Galileo, the Mars image by Mars Global Surveyor, the Jupiter image by Cassini, and the Saturn, Uranus and Neptune images by Voyager. Pluto is not shown as no spacecraft has yet visited it. The inner planets (Mercury, Venus, Earth, Moon, and Mars) are roug

PIX4630291

The Transneptunien object 2007 OR10 - Illustration - Transneptunian Object 2007 OR10 - Artwork: (225088) 2007 OR10 is a Transneptunian object with a probable diameter of more than 1,000 km, making it a candidate for the status of a dwarf planet. It is the largest celestial body in the solar system that did not receive a name in 2016, it is also the third largest object known beyond Neptune. It has a satellite with a diameter of about 300 km - (225088) 2007 OR10 is a trans-Neptunian object (TNO) approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System beyond Neptune, and the largest known body in the Solar System without a name. According to current estimates as of May 2016, it is slightly larger than Makemake or Haumea, and is hence almost certainly a dwarf planet. It has one known moon

The Transneptunien object 2007 OR10 - Illustration - Transneptunian Object 2007 OR10 - Artwork: (225088) 2007 OR10 is a Transneptunian object with a probable diameter of more than 1,000 km, making it a candidate for the status of a dwarf planet. It is the largest celestial body in the solar system that did not receive a name in 2016, it is also the third largest object known beyond Neptune. It has a satellite with a diameter of about 300 km - (225088) 2007 OR10 is a trans-Neptunian object (TNO) approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System beyond Neptune, and the largest known body in the Solar System without a name. According to current estimates as of May 2016, it is slightly larger than Makemake or Haumea, and is hence almost certainly a dwarf planet. It has one known moon

Miller, Ron (b.1947)

PIX4629575

William Lassell, English astronomer, c 1866-1879

William Lassell, English astronomer, c 1866-1879

UIS5071468

Callisto, one of the moons of Jupiter, 1979

Callisto, one of the moons of Jupiter, 1979

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Callisto, one of the moons of Jupiter, 1979

Callisto, one of the moons of Jupiter, 1979

UIS5071209

Close up of Ganymede, one of the moons of Jupiter, 1979

Close up of Ganymede, one of the moons of Jupiter, 1979

UIS5071200

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