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Artist's view of the volcano Ganesa Macula on Titan - This formation with a diameter of 180 km, seems to be a cryovolcano, an ice volcano. The surface temperature of Titan is about - 180* C, so the “lava” (a mixture of methane, ammonia and water) flows from it is icy.
Artist's view of the volcano Ganesa Macula on Titan - This formation with a diameter of 180 km, seems to be a cryovolcano, an ice volcano. The surface temperature of Titan is about - 180* C, so the “lava” (a mixture of methane, ammonia and water) flows from it is icy.

PIX4625925: Artist's view of the volcano Ganesa Macula on Titan - This formation with a diameter of 180 km, seems to be a cryovolcano, an ice volcano. The surface temperature of Titan is about - 180* C, so the “lava” (a mixture of methane, ammonia and water) flows from it is icy. / Bridgeman Images

Surface of Titan seen by Huygens - Illustration - Titan Emerges - Artist's view of the surface of Titan as it appeared at the European probe Huygens on January 14, 2005 when it descended, about 20 km from the ground. This is how the surface of Titan may have appeared to the European Space Agency's Huygens probe when it emerged from the satellite's ubiquitous hydrocarbon haze about 12 miles above Titan's surface. Huygens made its historic decent on 14 January 2005, making it the first man - made object to reach the surface of the satellite of another planet
Surface of Titan seen by Huygens - Illustration - Titan Emerges - Artist's view of the surface of Titan as it appeared at the European probe Huygens on January 14, 2005 when it descended, about 20 km from the ground. This is how the surface of Titan may have appeared to the European Space Agency's Huygens probe when it emerged from the satellite's ubiquitous hydrocarbon haze about 12 miles above Titan's surface. Huygens made its historic decent on 14 January 2005, making it the first man - made object to reach the surface of the satellite of another planet

PIX4626018: Surface of Titan seen by Huygens - Illustration - Titan Emerges - Artist's view of the surface of Titan as it appeared at the European probe Huygens on January 14, 2005 when it descended, about 20 km from the ground. This is how the surface of Titan may have appeared to the European Space Agency's Huygens probe when it emerged from the satellite's ubiquitous hydrocarbon haze about 12 miles above Titan's surface. Huygens made its historic decent on 14 January 2005, making it the first man - made object to reach the surface of the satellite of another planet / Bridgeman Images

The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996
The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996

PIX4624800: The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996 / Bridgeman Images

Saturn seen by the Hubble Space Telescope in different wavelengths 03/2003 - The Saturn Planet observed with the Hubble Space Telescope on March 7, 2003 at the time of the maximum opening of the rings. This happens every 30 years and offers observers a degagee view of the southern pole of the planet. Here the planet is photographed in different wavelengths: ultraviolet top, visible middle, infrared bottom
Saturn seen by the Hubble Space Telescope in different wavelengths 03/2003 - The Saturn Planet observed with the Hubble Space Telescope on March 7, 2003 at the time of the maximum opening of the rings. This happens every 30 years and offers observers a degagee view of the southern pole of the planet. Here the planet is photographed in different wavelengths: ultraviolet top, visible middle, infrared bottom

PIX4624824: Saturn seen by the Hubble Space Telescope in different wavelengths 03/2003 - The Saturn Planet observed with the Hubble Space Telescope on March 7, 2003 at the time of the maximum opening of the rings. This happens every 30 years and offers observers a degagee view of the southern pole of the planet. Here the planet is photographed in different wavelengths: ultraviolet top, visible middle, infrared bottom / Bridgeman Images

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter
Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

PIX4624826: Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter / Bridgeman Images

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of the planet Saturn is projected on its rings. Image obtained by the Voyager 1 probe on November 14, 1980. The shadow of Saturn casted on the rings was photographed by Voyager 1 on November 14, 1980
Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of the planet Saturn is projected on its rings. Image obtained by the Voyager 1 probe on November 14, 1980. The shadow of Saturn casted on the rings was photographed by Voyager 1 on November 14, 1980

PIX4624898: Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of the planet Saturn is projected on its rings. Image obtained by the Voyager 1 probe on November 14, 1980. The shadow of Saturn casted on the rings was photographed by Voyager 1 on November 14, 1980 / Bridgeman Images

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The planet Saturn seen through its rings. Image obtained by the Voyager 1 probe on November 14, 1980. Saturn's limb seen through the veil of its rings by Voyager 1 on November 14, 1980
Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The planet Saturn seen through its rings. Image obtained by the Voyager 1 probe on November 14, 1980. Saturn's limb seen through the veil of its rings by Voyager 1 on November 14, 1980

PIX4624899: Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The planet Saturn seen through its rings. Image obtained by the Voyager 1 probe on November 14, 1980. Saturn's limb seen through the veil of its rings by Voyager 1 on November 14, 1980 / Bridgeman Images

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4624901: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003. / Bridgeman Images

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of Saturn's rings is projected on the planet. Image obtained by the Voyager 1 probe on November 12, 1980. Ring's shadow casted on Saturn photographed by Voyager 1 on November 12, 1980
Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of Saturn's rings is projected on the planet. Image obtained by the Voyager 1 probe on November 12, 1980. Ring's shadow casted on Saturn photographed by Voyager 1 on November 12, 1980

PIX4624910: Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of Saturn's rings is projected on the planet. Image obtained by the Voyager 1 probe on November 12, 1980. Ring's shadow casted on Saturn photographed by Voyager 1 on November 12, 1980 / Bridgeman Images

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4624917: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003. / Bridgeman Images

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4624926: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003. / Bridgeman Images

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4624951: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003. / Bridgeman Images

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova Kepler in Ophiuchus - Kepler's supernova remnant
Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova Kepler in Ophiuchus - Kepler's supernova remnant

PIX4626476: Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova Kepler in Ophiuchus - Kepler's supernova remnant / Bridgeman Images

Sunspots are cooler areas on the sun's surface, the photosphere, associated with strong local magnetic activity. The spots, which are about 4,500 degrees K, only look dark because of the contrast with the surrounding surface, which is about 6,000 degrees K -: Sun and Sunspots - Sun with sunspots
Sunspots are cooler areas on the sun's surface, the photosphere, associated with strong local magnetic activity. The spots, which are about 4,500 degrees K, only look dark because of the contrast with the surrounding surface, which is about 6,000 degrees K -: Sun and Sunspots - Sun with sunspots

PIX4626532: Sunspots are cooler areas on the sun's surface, the photosphere, associated with strong local magnetic activity. The spots, which are about 4,500 degrees K, only look dark because of the contrast with the surrounding surface, which is about 6,000 degrees K -: Sun and Sunspots - Sun with sunspots / Bridgeman Images

The Abstract-Creation room of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937 Artist: Robert Delaunay (1885-1941) Photography 29/10/10
The Abstract-Creation room of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937 Artist: Robert Delaunay (1885-1941) Photography 29/10/10

ITR4626538: The Abstract-Creation room of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937 Artist: Robert Delaunay (1885-1941) Photography 29/10/10 / Bridgeman Images

Soleil et taches solaires le 11/08/2000 - Sun with sunspots - Le Soleil vu le 11 august 2000. Sunspots are visible. Sunspots are visible in this color image taken on August 11, 2000
Soleil et taches solaires le 11/08/2000 - Sun with sunspots - Le Soleil vu le 11 august 2000. Sunspots are visible. Sunspots are visible in this color image taken on August 11, 2000

PIX4626622: Soleil et taches solaires le 11/08/2000 - Sun with sunspots - Le Soleil vu le 11 august 2000. Sunspots are visible. Sunspots are visible in this color image taken on August 11, 2000 / Bridgeman Images

Housing building, Paris 16th.
Housing building, Paris 16th.

TEC4624104: Housing building, Paris 16th. / Bridgeman Images

Square du Palais Galliera in Paris 16th.
Square du Palais Galliera in Paris 16th.

TEC4624131: Square du Palais Galliera in Paris 16th. / Bridgeman Images

Hall of a residential building, Paris 16th.
Hall of a residential building, Paris 16th.

TEC4624133: Hall of a residential building, Paris 16th. / Bridgeman Images

Housing real estate, Paris 16th.
Housing real estate, Paris 16th.

TEC4624167: Housing real estate, Paris 16th. / Bridgeman Images

Lactee route from the Pic du Midi observatory - Milky way from Pic du Midi observatory
Lactee route from the Pic du Midi observatory - Milky way from Pic du Midi observatory

PIX4624190: Lactee route from the Pic du Midi observatory - Milky way from Pic du Midi observatory / Bridgeman Images

La Palma Observatory: Gamma-ray Telescope MAGIC - La Palma Observatory: The MAGIC Gamma-ray telescope: The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC-I is a telescope of 17 meters in diameter. MAGIC-II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). View of night sky reflected in the multi-mirrored surface of one of a pair of MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes at the Roque de Los Muchachos Observatory, La Palma, Canary Islands. This observatory is situated 2,400 metres above sea level and is home to some of the world's leading research telescopes. The MAGIC telescope is intended to indirectly observe gamma rays by detecting brief flashes of optical light, called Cherenkov light
La Palma Observatory: Gamma-ray Telescope MAGIC - La Palma Observatory: The MAGIC Gamma-ray telescope: The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC-I is a telescope of 17 meters in diameter. MAGIC-II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). View of night sky reflected in the multi-mirrored surface of one of a pair of MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes at the Roque de Los Muchachos Observatory, La Palma, Canary Islands. This observatory is situated 2,400 metres above sea level and is home to some of the world's leading research telescopes. The MAGIC telescope is intended to indirectly observe gamma rays by detecting brief flashes of optical light, called Cherenkov light

PIX4624214: La Palma Observatory: Gamma-ray Telescope MAGIC - La Palma Observatory: The MAGIC Gamma-ray telescope: The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC-I is a telescope of 17 meters in diameter. MAGIC-II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). View of night sky reflected in the multi-mirrored surface of one of a pair of MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes at the Roque de Los Muchachos Observatory, La Palma, Canary Islands. This observatory is situated 2,400 metres above sea level and is home to some of the world's leading research telescopes. The MAGIC telescope is intended to indirectly observe gamma rays by detecting brief flashes of optical light, called Cherenkov light / Bridgeman Images

Tenerife Observatory - Teide observatory
Tenerife Observatory - Teide observatory

PIX4624219: Tenerife Observatory - Teide observatory / Bridgeman Images

Tenerife Observatory under the Stars - Starry sky above Teide observatory: The Moon and the Star Sky seen above the dome of the European Space Agency OGS in Tenerife, Canary Islands. Night sky seen above Tenerife observatory in Canary islands. OGS telescope was originally built by ESA for tests with laser link and for space debris observations. For the remainder of the available observing time the OGS is currently used by the IAC for astronomy observations. It is a one-meter telescope with a focal length of 13.3 m
Tenerife Observatory under the Stars - Starry sky above Teide observatory: The Moon and the Star Sky seen above the dome of the European Space Agency OGS in Tenerife, Canary Islands. Night sky seen above Tenerife observatory in Canary islands. OGS telescope was originally built by ESA for tests with laser link and for space debris observations. For the remainder of the available observing time the OGS is currently used by the IAC for astronomy observations. It is a one-meter telescope with a focal length of 13.3 m

PIX4624229: Tenerife Observatory under the Stars - Starry sky above Teide observatory: The Moon and the Star Sky seen above the dome of the European Space Agency OGS in Tenerife, Canary Islands. Night sky seen above Tenerife observatory in Canary islands. OGS telescope was originally built by ESA for tests with laser link and for space debris observations. For the remainder of the available observing time the OGS is currently used by the IAC for astronomy observations. It is a one-meter telescope with a focal length of 13.3 m / Bridgeman Images

La Muette metro station in Paris.
La Muette metro station in Paris.

TEC4624252: La Muette metro station in Paris. / Bridgeman Images

Star Sky on Old Faithful - Airglow in Yellowstone National Park - View of the star sky above the eruption Old Faithful geyser. Yellowstone National Park, Wyoming, USA. A panorama of the night sky from Ursa Major to Aquarius showing colorful airglow. Old Faithful geyser erupts to the right
Star Sky on Old Faithful - Airglow in Yellowstone National Park - View of the star sky above the eruption Old Faithful geyser. Yellowstone National Park, Wyoming, USA. A panorama of the night sky from Ursa Major to Aquarius showing colorful airglow. Old Faithful geyser erupts to the right

PIX4624256: Star Sky on Old Faithful - Airglow in Yellowstone National Park - View of the star sky above the eruption Old Faithful geyser. Yellowstone National Park, Wyoming, USA. A panorama of the night sky from Ursa Major to Aquarius showing colorful airglow. Old Faithful geyser erupts to the right / Bridgeman Images

La Muette in Paris. Photography 09/08/07.
La Muette in Paris. Photography 09/08/07.

TEC4624282: La Muette in Paris. Photography 09/08/07. / Bridgeman Images

Avenue Mozart in Paris. Photography 09/08/07.
Avenue Mozart in Paris. Photography 09/08/07.

TEC4624290: Avenue Mozart in Paris. Photography 09/08/07. / Bridgeman Images

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 highest possible detail when Nasa's New Horizons probe flies by Pluto in 2015. The Hubble images are a few pixels wide. But through a technique called dithering, multiple, slightly offset pictures can be combined through computer - image processing to synthesize a higher - resolution view than could be seen in a single exposure. This series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish
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 highest possible detail when Nasa's New Horizons probe flies by Pluto in 2015. The Hubble images are a few pixels wide. But through a technique called dithering, multiple, slightly offset pictures can be combined through computer - image processing to synthesize a higher - resolution view than could be seen in a single exposure. This series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish

PIX4624317: 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 highest possible detail when Nasa's New Horizons probe flies by Pluto in 2015. The Hubble images are a few pixels wide. But through a technique called dithering, multiple, slightly offset pictures can be combined through computer - image processing to synthesize a higher - resolution view than could be seen in a single exposure. This series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish / Bridgeman Images

La rue de l'Annonciation in Paris 16th.
La rue de l'Annonciation in Paris 16th.

TEC4624344: La rue de l'Annonciation in Paris 16th. / Bridgeman Images

La rue de la Tour in Paris 16th.
La rue de la Tour in Paris 16th.

TEC4624352: La rue de la Tour in Paris 16th. / Bridgeman Images

La rue de Passy in Paris 16th.
La rue de Passy in Paris 16th.

TEC4624397: La rue de Passy in Paris 16th. / Bridgeman Images

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

PIX4624427: 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 / Bridgeman Images

Le Lycee Janson, Rue de la Pompe in Paris 16th.
Le Lycee Janson, Rue de la Pompe in Paris 16th.

TEC4624440: Le Lycee Janson, Rue de la Pompe in Paris 16th. / Bridgeman Images

Villa prives rue de la Pompe in Paris 16th. Photo 090/08/07.
Villa prives rue de la Pompe in Paris 16th. Photo 090/08/07.

TEC4624475: Villa prives rue de la Pompe in Paris 16th. Photo 090/08/07. / Bridgeman Images

Summer on Pluto - Illustration - Summer on Pluto - Artist view - Artist view of Pluto's surface when the planet is closer to the Sun and sees its weak atmosphere reforming. Despite its small size and extreme distance from the Sun, Pluto does have an atmosphere. The atmosphere arises because there are periods when Pluto is closer to the Sun than Neptune, making it the 8th planet from the Sun for roughly 20 years at a time (on 11 February 1999, Pluto crossed Neptune's orbit and once again became farther from the Sun Neptune and will remain so until the year 2231). During this plutonian “” summer”” the ices on Pluto's surface sublimate and form a methane and nitrogen atmosphere. This atmosphere is continually produced and lost again while Pluto is inside Neptune's orbit; during this time the density of Pluto's atmosphere may rival that of Mars
Summer on Pluto - Illustration - Summer on Pluto - Artist view - Artist view of Pluto's surface when the planet is closer to the Sun and sees its weak atmosphere reforming. Despite its small size and extreme distance from the Sun, Pluto does have an atmosphere. The atmosphere arises because there are periods when Pluto is closer to the Sun than Neptune, making it the 8th planet from the Sun for roughly 20 years at a time (on 11 February 1999, Pluto crossed Neptune's orbit and once again became farther from the Sun Neptune and will remain so until the year 2231). During this plutonian “” summer”” the ices on Pluto's surface sublimate and form a methane and nitrogen atmosphere. This atmosphere is continually produced and lost again while Pluto is inside Neptune's orbit; during this time the density of Pluto's atmosphere may rival that of Mars

PIX4624480: Summer on Pluto - Illustration - Summer on Pluto - Artist view - Artist view of Pluto's surface when the planet is closer to the Sun and sees its weak atmosphere reforming. Despite its small size and extreme distance from the Sun, Pluto does have an atmosphere. The atmosphere arises because there are periods when Pluto is closer to the Sun than Neptune, making it the 8th planet from the Sun for roughly 20 years at a time (on 11 February 1999, Pluto crossed Neptune's orbit and once again became farther from the Sun Neptune and will remain so until the year 2231). During this plutonian “” summer”” the ices on Pluto's surface sublimate and form a methane and nitrogen atmosphere. This atmosphere is continually produced and lost again while Pluto is inside Neptune's orbit; during this time the density of Pluto's atmosphere may rival that of Mars / Bridgeman Images


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