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Type # for projects,to access projects, > for users, and ? for help.

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Bilder zu 'Zwergplanet' gefunden, 108

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Pluto.

Pluto.

UIG2628618

Pluto.

Pluto.

UIG2628615

Pluto.

Pluto.

UIG2628617

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

The dwarf planet Pluto.

The dwarf planet Pluto.

UIG2628619

Pluto.

Pluto.

UIG2628614

Pluto's Atmosphere - Artist's View - Pluto's Atmosphere - Pluto's Artist's View surrounded by its thin atmosphere. In 1985 it was discovered that Pluto has an atmosphere, albeit a very tenuous one. Pluto's atmosphere arises only when it approaches closer to the Sun during its highly eccentric, 248 earth years long orbit. The atmosphere likely consists of nitrogen, methane, and carbon monoxide, which sublimate directly from Pluto's frozen surface. As Pluto's orbit moves it away from the Sun, these gases are believed to slowly precipitate back to Pluto's surface

Pluto's Atmosphere - Artist's View - Pluto's Atmosphere - Pluto's Artist's View surrounded by its thin atmosphere. In 1985 it was discovered that Pluto has an atmosphere, albeit a very tenuous one. Pluto's atmosphere arises only when it approaches closer to the Sun during its highly eccentric, 248 earth years long orbit. The atmosphere likely consists of nitrogen, methane, and carbon monoxide, which sublimate directly from Pluto's frozen surface. As Pluto's orbit moves it away from the Sun, these gases are believed to slowly precipitate back to Pluto's surface

Walter B Myers

PIX4624547

Pluto - Artist's view - Artist's view of Pluto surrounded by its thin atmosphere. An artist's concept of the crescent of Pluto in deep space

Pluto - Artist's view - Artist's view of Pluto surrounded by its thin atmosphere. An artist's concept of the crescent of Pluto in deep space

PIX4624533

Surface of Ceres - Ceres' surface - Surface of the dwarf planet Ceres. Artist's view. What is known about Ceres' surface is that it has an albedo (surface brightness) about the same as the Earth's Moon and never gets warmer than minus 30o F. In this image the artist is suggesting a lunar-like terrain modified by the presence of water ice

Surface of Ceres - Ceres' surface - Surface of the dwarf planet Ceres. Artist's view. What is known about Ceres' surface is that it has an albedo (surface brightness) about the same as the Earth's Moon and never gets warmer than minus 30o F. In this image the artist is suggesting a lunar-like terrain modified by the presence of water ice

Walter B Myers

PIX4584135

Surface of Pluto - Artist view - Pluto surface- Artist view: The icy surface of Pluto. Icy surface of Pluto. Lake of liquid neon

Surface of Pluto - Artist view - Pluto surface- Artist view: The icy surface of Pluto. Icy surface of Pluto. Lake of liquid neon

Miller, Ron (b.1947)

PIX4624516

Artist's View of Ceres Degazages - Outgassing on Ceres: Artist's View of the Dwarf Planet Ceres with Panaches of Water Vapour

Artist's View of Ceres Degazages - Outgassing on Ceres: Artist's View of the Dwarf Planet Ceres with Panaches of Water Vapour

Miller, Ron (b.1947)

PIX4584153

Pluto and Charon - Artist view - Pluto and Charon - Artist view: Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Pluto and Charon - Artist view - Pluto and Charon - Artist view: Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Miller, Ron (b.1947)

PIX4624494

Pluto and Charon - Artist view - Pluto and Charon - Artist view: Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Pluto and Charon - Artist view - Pluto and Charon - Artist view: Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Miller, Ron (b.1947)

PIX4624510

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view - Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view - Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Miller, Ron (b.1947)

PIX4624485

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Miller, Ron (b.1947)

PIX4624582

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto seen by the New Horizons probe on July 7, 2015 at a distance of 8 million km from the dwarf planet. In the early morning hours of July 8, 2015, mission scientists received this new view of Pluto - - the most detailed yet returned by the Long Range Reconnaissance Imager (LORRI) aboard New Horizons. The image was taken on July 7, when the NASA spacecraft was just under 5 million miles (8 million kilometers) from Pluto, and is the first to be received since the July 4 anomaly that sent the spacecraft into safe mode. This view is centered roughly on the area that will be seen close - up during New Horizons' July 14 closest approach. This side of Pluto is dominated by three broad regions of varying brightness. Most prominent are an elongated dark feature at the equator, informally known as “” the whale,”” and a large heart - shaped bright area measuring some 1,200 miles (2,000 kilometers) across on the right. Above th

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto seen by the New Horizons probe on July 7, 2015 at a distance of 8 million km from the dwarf planet. In the early morning hours of July 8, 2015, mission scientists received this new view of Pluto - - the most detailed yet returned by the Long Range Reconnaissance Imager (LORRI) aboard New Horizons. The image was taken on July 7, when the NASA spacecraft was just under 5 million miles (8 million kilometers) from Pluto, and is the first to be received since the July 4 anomaly that sent the spacecraft into safe mode. This view is centered roughly on the area that will be seen close - up during New Horizons' July 14 closest approach. This side of Pluto is dominated by three broad regions of varying brightness. Most prominent are an elongated dark feature at the equator, informally known as “” the whale,”” and a large heart - shaped bright area measuring some 1,200 miles (2,000 kilometers) across on the right. Above th

PIX4624339

Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will b

Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will b

PIX4624313

Ring around Pluto - View d'artiste - Pluto's ring - Artist view: View of hypothetical rings around Pluto; in the background, the satellite Charon. Hypothetical rings system around Pluto. Background is Charon.

Ring around Pluto - View d'artiste - Pluto's ring - Artist view: View of hypothetical rings around Pluto; in the background, the satellite Charon. Hypothetical rings system around Pluto. Background is Charon.

Miller, Ron (b.1947)

PIX4624600

Surface de Ceres - Ceres ice field: Ice surface of the dwarf planet Ceres. Artist view

Surface de Ceres - Ceres ice field: Ice surface of the dwarf planet Ceres. Artist view

Miller, Ron (b.1947)

PIX4584200

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto seen by the New Horizons probe. Composite image created from four images obtained on 13 July 2015 at a distance of 450,000 km from the dwarf planet. Four images from New Horizons' Long Range Recognition Imager (LORRI) were combined with color data from the Ralph instrument to create this global view of Pluto. (The lower right edge of Pluto in this view currently lacks high - resolution color coverage.) The images, taken when the spacecraft was 280,000 miles (450,000 kilometers) away, show features as small as 1.4 miles (2.2 kilometers), twice the resolution of the single - image view taken on July 13

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto seen by the New Horizons probe. Composite image created from four images obtained on 13 July 2015 at a distance of 450,000 km from the dwarf planet. Four images from New Horizons' Long Range Recognition Imager (LORRI) were combined with color data from the Ralph instrument to create this global view of Pluto. (The lower right edge of Pluto in this view currently lacks high - resolution color coverage.) The images, taken when the spacecraft was 280,000 miles (450,000 kilometers) away, show features as small as 1.4 miles (2.2 kilometers), twice the resolution of the single - image view taken on July 13

PIX4624351

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

PIX4624317

The Dwarf Planet Ceres seen by the Dawn probe - Dwarf Planet Ceres: Image reconstructed in very high resolution from observations made by the Dawn probe, showing the dwarf planet Ceres with the occator crater in the center. This orthographic projection shows dwarf planet Ceres as seen by Nasa's Dawn spacecraft. The projection is centered on Occator Crater, home to the brightest area on Ceres. Occator is centered at 20 degrees north latitude, 239 degrees east longitude. This image was made from views Dawn took during its low-altitude mapping orbit, at about 240 miles (385 kilometers) above the surface. The image resolution is about 120 feet (35 meters) per pixel

The Dwarf Planet Ceres seen by the Dawn probe - Dwarf Planet Ceres: Image reconstructed in very high resolution from observations made by the Dawn probe, showing the dwarf planet Ceres with the occator crater in the center. This orthographic projection shows dwarf planet Ceres as seen by Nasa's Dawn spacecraft. The projection is centered on Occator Crater, home to the brightest area on Ceres. Occator is centered at 20 degrees north latitude, 239 degrees east longitude. This image was made from views Dawn took during its low-altitude mapping orbit, at about 240 miles (385 kilometers) above the surface. The image resolution is about 120 feet (35 meters) per pixel

PIX4583550

Pluto and Charon - Artist view - Pluto and Charon - Artist view - Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Pluto and Charon - Artist view - Pluto and Charon - Artist view - Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Miller, Ron (b.1947)

PIX4624499

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view - Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view - Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Miller, Ron (b.1947)

PIX4624464

Asteroide Ceres seen by the space telescope Hubble - Asteroid Ceres - Photos obtained in visible and ultraviolet of the asteroid Ceres from December 2003 to January 2004. Since August 2006, Ceres is considered a dwarf planet. Hubble Space Telescope color image of Ceres, the largest object in the asteroid belt. The observations were made in visible and ultraviolet light between December 2003 and January 2004

Asteroide Ceres seen by the space telescope Hubble - Asteroid Ceres - Photos obtained in visible and ultraviolet of the asteroid Ceres from December 2003 to January 2004. Since August 2006, Ceres is considered a dwarf planet. Hubble Space Telescope color image of Ceres, the largest object in the asteroid belt. The observations were made in visible and ultraviolet light between December 2003 and January 2004

PIX4583523

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Miller, Ron (b.1947)

PIX4624501

Geysers sur Pluto - Artist view - Hot springs and Geysers on Pluto - Artist view

Geysers sur Pluto - Artist view - Hot springs and Geysers on Pluto - Artist view

Miller, Ron (b.1947)

PIX4624513

Pluto Mountains - Artist's view: Norgay Montes are mountains of ice that peak 3400m above the surface of Pluto - The Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Pluto Mountains - Artist's view: Norgay Montes are mountains of ice that peak 3400m above the surface of Pluto - The Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Miller, Ron (b.1947)

PIX4624719

Pluto and Charon - View d'artiste - Pluto seen from above Charon - Artist view: Pluto seen above his satellite Charon

Pluto and Charon - View d'artiste - Pluto seen from above Charon - Artist view: Pluto seen above his satellite Charon

Miller, Ron (b.1947)

PIX4624552

Pluto surface - Artist view - Pluto surface- Artist view: From liquid neon could circulate to the surface of Pluto - Pools of liquid neon on Pluto

Pluto surface - Artist view - Pluto surface- Artist view: From liquid neon could circulate to the surface of Pluto - Pools of liquid neon on Pluto

Miller, Ron (b.1947)

PIX4624570

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

PIX4583529

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

PIX4582252

Pluto and Charon - Vue d'artiste - Pluto and Charon - Artist view - Vue d'artiste de Pluto et de son satellite Charon. Pluto and its moon Charon

Pluto and Charon - Vue d'artiste - Pluto and Charon - Artist view - Vue d'artiste de Pluto et de son satellite Charon. Pluto and its moon Charon

PIX4624438

The Dawn probe orbiting around Ceres - Artist's view - Dawn in orbit around Ceres - Artist's view of the Dawn probe orbiting around the dwarf planet Ceres. In march 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn is entering orbit around Ceres. In late November 2015 Dawn will descend to its closest orbit around Ceres at a distance of about 230 miles. While no close - up observations of yet been made of Ceres itself, here it is rendered as appearing similar to a much smaller version of the Earth's Moon, heavily cratered with the addition of surface water ice and hypothesized plumes of ice crystals from water g

The Dawn probe orbiting around Ceres - Artist's view - Dawn in orbit around Ceres - Artist's view of the Dawn probe orbiting around the dwarf planet Ceres. In march 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn is entering orbit around Ceres. In late November 2015 Dawn will descend to its closest orbit around Ceres at a distance of about 230 miles. While no close - up observations of yet been made of Ceres itself, here it is rendered as appearing similar to a much smaller version of the Earth's Moon, heavily cratered with the addition of surface water ice and hypothesized plumes of ice crystals from water g

Walter B Myers

PIX4607275

The dwarf planet Eris - Illustration - Dwarf planet Eris. Artwork - Artist's view of the dwarf planet Eris. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 at the lonely outer fringes of our solar system. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

The dwarf planet Eris - Illustration - Dwarf planet Eris. Artwork - Artist's view of the dwarf planet Eris. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 at the lonely outer fringes of our solar system. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

PIX4629580

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de la glace à la surface de Charon. Pluto is visible in the sky - Ice on Charon surface

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de la glace à la surface de Charon. Pluto is visible in the sky - Ice on Charon surface

Miller, Ron (b.1947)

PIX4624674

Pluto vue de Charon - View d'artiste - Pluto seen from Charon - Artist view: View d'artiste de la surface de Charon. Pluto is visible in the sky. Charon surface.

Pluto vue de Charon - View d'artiste - Pluto seen from Charon - Artist view: View d'artiste de la surface de Charon. Pluto is visible in the sky. Charon surface.

Miller, Ron (b.1947)

PIX4624692

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

Walter B Myers

PIX4630042

The dwarf planet Eris - Illustration - Dwarf planet Eris - Artwork - Artist's view of the dwarf planet Eris and its satellite Dysnomia. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 with its moon Dysnomia. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

The dwarf planet Eris - Illustration - Dwarf planet Eris - Artwork - Artist's view of the dwarf planet Eris and its satellite Dysnomia. Eris is about three times more distant from the Sun than Pluto. The dwarf planet, formerly known as 2003 UB313 (or Xena), is now called Eris, after the Greek goddess of discord and strife. This artist's concept shows the planet catalogued as 2003 UB313 with its moon Dysnomia. Our Sun can be seen in the distance. The new planet, which is yet to be formally named, is at least as big as Pluto and about three times farther away from the Sun than Pluto. It is very cold and dark. The planet was discovered by the Samuel Oschin Telescope at the Palomar Observatory near San Diego, Calif., on Jan. 8, 2005

PIX4629642

Pluto seen by the New Horizons probe: Pluto seen in false colors by the New Horizons probe. Composite image created from images obtained on July 14, 2015 - Nasa's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds. Many landforms have their own distinct colors, telling a complex geological and climatological story that scientists have only just begun to decode. The image resolves details and colors on scales as small as 0.8 miles (1.3 kilometers).

Pluto seen by the New Horizons probe: Pluto seen in false colors by the New Horizons probe. Composite image created from images obtained on July 14, 2015 - Nasa's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds. Many landforms have their own distinct colors, telling a complex geological and climatological story that scientists have only just begun to decode. The image resolves details and colors on scales as small as 0.8 miles (1.3 kilometers).

PIX4624474

Pluto and Charon - Artist view: Pluto, in the foreground, and its satellite Charon - Foreground is Pluto

Pluto and Charon - Artist view: Pluto, in the foreground, and its satellite Charon - Foreground is Pluto

Miller, Ron (b.1947)

PIX4624553

Pluto and Charon satellite seen by the New Horizons probe on July 14, 2015 at 250,000 km from the dwarf planet

Pluto and Charon satellite seen by the New Horizons probe on July 14, 2015 at 250,000 km from the dwarf planet

PIX4624378

Pluto and its five satellites - Artist's view - Pluto and its five moons: In Pluto's sky, its satellites Charon, Hydre, Nix, Kerberos and Styx

Pluto and its five satellites - Artist's view - Pluto and its five moons: In Pluto's sky, its satellites Charon, Hydre, Nix, Kerberos and Styx

Miller, Ron (b.1947)

PIX4624593

Pluto and Charon - Vue d'artiste - Pluto and Charon - Artist view - Vue d'artiste de Pluto et de son satellite Charon. Pluto and its moon Charon

Pluto and Charon - Vue d'artiste - Pluto and Charon - Artist view - Vue d'artiste de Pluto et de son satellite Charon. Pluto and its moon Charon

Miller, Ron (b.1947)

PIX4624445

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

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

PIX4607290

In the foothills of Pluto's mountains: Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

In the foothills of Pluto's mountains: Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Miller, Ron (b.1947)

PIX4624653

The dwarf planet Makemake - Illustration -The dwarf planet Makemake: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Solar system seen from Makemake. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

The dwarf planet Makemake - Illustration -The dwarf planet Makemake: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Solar system seen from Makemake. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

PIX4584252

Ice volcano on Ceres - Ceres ice volcano

Ice volcano on Ceres - Ceres ice volcano

Miller, Ron (b.1947)

PIX4584165

Pluto and Charon seen by the New Horizons probe - Pluto and Charon seen by New Horizons: Pluto and Charon satellite (in the background) seen by the New Horizons probe on 14 July 2015

Pluto and Charon seen by the New Horizons probe - Pluto and Charon seen by New Horizons: Pluto and Charon satellite (in the background) seen by the New Horizons probe on 14 July 2015

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L'ombre de Charon sur Pluto - View d'artiste - Charon's shadow on Pluto - Artist view - View d'artiste de l'ombre du satellite Charon projected on Pluto. Pluto seen from its moon Charon with Charon's shadow projected on Pluto

L'ombre de Charon sur Pluto - View d'artiste - Charon's shadow on Pluto - Artist view - View d'artiste de l'ombre du satellite Charon projected on Pluto. Pluto seen from its moon Charon with Charon's shadow projected on Pluto

Miller, Ron (b.1947)

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Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and the satellite Charon

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and the satellite Charon

Miller, Ron (b.1947)

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Pluto - Tombaugh Regio - Ice Plains of Pluto's - Artist view: Artist view of the Ice Plains of Tombaugh Regio (the Heart). In the sky, satellite Charon - The ice plains of Tombaugh Regio - Pluto's -heart

Pluto - Tombaugh Regio - Ice Plains of Pluto's - Artist view: Artist view of the Ice Plains of Tombaugh Regio (the Heart). In the sky, satellite Charon - The ice plains of Tombaugh Regio - Pluto's -heart

Miller, Ron (b.1947)

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Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

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The dwarf planet Makemake - Illustration - Dwarf planet Makemake - Artwork: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km - Solar system seen from Makemake - Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

The dwarf planet Makemake - Illustration - Dwarf planet Makemake - Artwork: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km - Solar system seen from Makemake - Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

Miller, Ron (b.1947)

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Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and satellites Charon, Hydra, and Nix

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and satellites Charon, Hydra, and Nix

Miller, Ron (b.1947)

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Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet -: The Sun seen from Pluto - Illustration - Sun seen from Pluto. Artwork

Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet -: The Sun seen from Pluto - Illustration - Sun seen from Pluto. Artwork

S. Numazawa

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The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays pr

The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays pr

Walter B Myers

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Comparison between the Earth, Ceres and the Moon - Ceres, Earth, & Earth's Moon compared - Comparison at the scale of the size of the Earth, the dwarf planet Ceres and the Moon. Ceres, the most massive object in the asteroid belt, is only 950 km in diameter. While Ceres is the most massive single object in the asteroid belt, it is yet quite small when compared with the Earth and moon

Comparison between the Earth, Ceres and the Moon - Ceres, Earth, & Earth's Moon compared - Comparison at the scale of the size of the Earth, the dwarf planet Ceres and the Moon. Ceres, the most massive object in the asteroid belt, is only 950 km in diameter. While Ceres is the most massive single object in the asteroid belt, it is yet quite small when compared with the Earth and moon

Walter B Myers

PIX4630008

Dawn and Vesta and Ceres - Artist's concept of the Dawn spacecraft with Vesta and Ceres - Artist's view of the Dawn probe near the Vesta asteroid and the dwarf planet Ceres Artist's concept of the Dawn spacecraft with Vesta and Ceres. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta and the dwarf planet Ceres. The two bodies have very different properties from each other. By observing them both with the same set of instruments, Dawn will probe the early solar system and specify the properties of each body

Dawn and Vesta and Ceres - Artist's concept of the Dawn spacecraft with Vesta and Ceres - Artist's view of the Dawn probe near the Vesta asteroid and the dwarf planet Ceres Artist's concept of the Dawn spacecraft with Vesta and Ceres. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta and the dwarf planet Ceres. The two bodies have very different properties from each other. By observing them both with the same set of instruments, Dawn will probe the early solar system and specify the properties of each body

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