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Winter constellations - Winter constellations - The Moon sets on the horizon to the west this 28 April 2006 in Maryland. In the sky on the left, the constellation of Orion, in the center the Taurus with the clusters of the Hyades and Pleiades, on the right the constellation of Persee, above to the center the Coach with the bright star Capella, on its left, the Gemels with the planet Mars. The crescent Moon with Earthshine sets in the twilight in the west with the Winter constellations of Orion, Gemini, Auriga, Taurus and Perseus

Winter constellations - Winter constellations - The Moon sets on the horizon to the west this 28 April 2006 in Maryland. In the sky on the left, the constellation of Orion, in the center the Taurus with the clusters of the Hyades and Pleiades, on the right the constellation of Persee, above to the center the Coach with the bright star Capella, on its left, the Gemels with the planet Mars. The crescent Moon with Earthshine sets in the twilight in the west with the Winter constellations of Orion, Gemini, Auriga, Taurus and Perseus

Jerry Lodriguss

PIX4594072

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Miller, Ron (b.1947)

PIX4607909

Exoplanete Gliese 849 b: Artist's view of the extrasolar planet Gliese 849 b, an exoplanet whose mass is less than that of Jupiter, discovered in 2006 and located 29 light years from Earth in the constellation Aquarius. Gliese 849 b is an extrasolar planet approximately 29 light years away in the constellation of Aquarius. It is the first long-period Jupiter-like planet discovered around a red dwarf

Exoplanete Gliese 849 b: Artist's view of the extrasolar planet Gliese 849 b, an exoplanet whose mass is less than that of Jupiter, discovered in 2006 and located 29 light years from Earth in the constellation Aquarius. Gliese 849 b is an extrasolar planet approximately 29 light years away in the constellation of Aquarius. It is the first long-period Jupiter-like planet discovered around a red dwarf

Miller, Ron (b.1947)

PIX4607959

Untitled (acrylic)

premium — Untitled (acrylic)

Untitled (acrylic)

JUN214579

Winter constellations - Winter constellations - The Moon sets on the horizon to the west this 28 April 2006 in Maryland. In the sky on the left, the constellation of Orion, in the center the Taurus with the clusters of the Hyades and Pleiades, on the right the constellation of Persee, above to the center the Coach with the bright star Capella, on its left, the Gemels with the planet Mars. The crescent Moon with Earthshine sets in the twilight in the west with the Winter constellations of Orion, Gemini, Auriga, Taurus and Perseus

Winter constellations - Winter constellations - The Moon sets on the horizon to the west this 28 April 2006 in Maryland. In the sky on the left, the constellation of Orion, in the center the Taurus with the clusters of the Hyades and Pleiades, on the right the constellation of Persee, above to the center the Coach with the bright star Capella, on its left, the Gemels with the planet Mars. The crescent Moon with Earthshine sets in the twilight in the west with the Winter constellations of Orion, Gemini, Auriga, Taurus and Perseus

Jerry Lodriguss

PIX4594068

This observation shows a fresh, approximately 7.5 kilometer diameter crater that resides in a larger crater in the Southern hemisphere. MRO.

This observation shows a fresh, approximately 7.5 kilometer diameter crater that resides in a larger crater in the Southern hemisphere. MRO.

UIG866559

Detection of an exoplanet by radial velocity - Detection of an exoplanet: Radial velocity or Doppler method - This detection method is based on the study of the light spectrum of the star. A planet orbiting around a star periodically influences the movement of that star. By Doppler effect (the star's light wave shifts to blue when it approaches and decals to red when it moves away), we can measure the radial velocity of the star and know the position of the planet's orbit. An exoplanet orbiting a larger star could produce changes in position and velocity of the star as they orbit their common center of mass. Those variations in the radial velocity are known in studying the spectral lines of the star due to the Doppler effect (blue shift when the star is approaching, redshift when it is receding)

Detection of an exoplanet by radial velocity - Detection of an exoplanet: Radial velocity or Doppler method - This detection method is based on the study of the light spectrum of the star. A planet orbiting around a star periodically influences the movement of that star. By Doppler effect (the star's light wave shifts to blue when it approaches and decals to red when it moves away), we can measure the radial velocity of the star and know the position of the planet's orbit. An exoplanet orbiting a larger star could produce changes in position and velocity of the star as they orbit their common center of mass. Those variations in the radial velocity are known in studying the spectral lines of the star due to the Doppler effect (blue shift when the star is approaching, redshift when it is receding)

PIX4573959

Detailed view of the ring system that the planet Saturn, the second largest planet in our solar system, surrounds photographed from 8.9 million kilometers (photo)

Detailed view of the ring system that the planet Saturn, the second largest planet in our solar system, surrounds photographed from 8.9 million kilometers (photo)

SZT3043088

Along the Red River in North Dakota, floodwaters are moving northward into Canada. April 17, 2011.

Along the Red River in North Dakota, floodwaters are moving northward into Canada. April 17, 2011.

UIG866871

As the summer 2012 drought continued to afflict the U.S. Midwest, water levels of the Mississippi River approached historic lows Aug. 24, 2012.

As the summer 2012 drought continued to afflict the U.S. Midwest, water levels of the Mississippi River approached historic lows Aug. 24, 2012.

UIG867005

Galaxy in the Sky of an Exoplanet - Red Galaxy Sunset - Exotic flora on an orphan planet draw sustinance from the energetic core of a distant galaxy

Galaxy in the Sky of an Exoplanet - Red Galaxy Sunset - Exotic flora on an orphan planet draw sustinance from the energetic core of a distant galaxy

Walter B Myers

PIX4573515

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

PIX4574126

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Miller, Ron (b.1947)

PIX4608105

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this dis

Miller, Ron (b.1947)

PIX4608153

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Artist's view of the exoplanet OGLE-2005-BLG-390L b: Artist's view of the exoplanet OGLE-05-390L b, the first extrasolar planet of earth type discovered. Located in the constellation of Scorpio, this planet, made of rock and ice, is outside the habitable area of its star, a red dwarf star. This is the first terrestrial type of exoplanet discovered

Miller, Ron (b.1947)

PIX4607920

Exoplanete OGLE-2013-BLG-0341L Bb - Artist's view: OGLE-2013-BLG-0341L Bb is an exoplanet about twice the mass of the Earth gravitating around the red dwarf OGLE-2013-BLG-0341L B, a secondary component of the binary star OGLE-2013-BLG-0341L located in the constellation. OGLE-2013-BLG-0341LBB, is located in the constellation Sagittarius, about 3,000 light-years away. It is twice the mass of Earth, and orbits one of the stars in the binary system at almost exactly the same distance from which Earth orbits the Sun. But its star is 400 times dimmer than our Sun, so the exoplanet is very cold - around minus 213 degrees Celsius

Exoplanete OGLE-2013-BLG-0341L Bb - Artist's view: OGLE-2013-BLG-0341L Bb is an exoplanet about twice the mass of the Earth gravitating around the red dwarf OGLE-2013-BLG-0341L B, a secondary component of the binary star OGLE-2013-BLG-0341L located in the constellation. OGLE-2013-BLG-0341LBB, is located in the constellation Sagittarius, about 3,000 light-years away. It is twice the mass of Earth, and orbits one of the stars in the binary system at almost exactly the same distance from which Earth orbits the Sun. But its star is 400 times dimmer than our Sun, so the exoplanet is very cold - around minus 213 degrees Celsius

Miller, Ron (b.1947)

PIX4608038

Artist's view of a hot Jupiter - Exoplanet - Hot Jupiter - Artist's view of a gas giant exoplanet very close to its star. Many of the extra - solar planets which have been discovered in recent years are large, massive, and orbit surprisingly close to their parent stars. These are believed to be gas giant planets similar to Jupiter. Since they're so close to their sun, they're hot. Thus the common term for them has become “” hot Jupiter””. This one is hot enough to glow a dull red even on its night side. The existence of these planets has proven that the arrangement of other solar systems need not closely resemble our own

Artist's view of a hot Jupiter - Exoplanet - Hot Jupiter - Artist's view of a gas giant exoplanet very close to its star. Many of the extra - solar planets which have been discovered in recent years are large, massive, and orbit surprisingly close to their parent stars. These are believed to be gas giant planets similar to Jupiter. Since they're so close to their sun, they're hot. Thus the common term for them has become “” hot Jupiter””. This one is hot enough to glow a dull red even on its night side. The existence of these planets has proven that the arrangement of other solar systems need not closely resemble our own

PIX4574132

Artist view of the Exoplanete Gliese 581c - Artwork of exoplanet Gliese 581c - Artist view of the Exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” This image of a rocky and variegated Gliese 581 c with an atmosphere and clouds is purely speculative

Artist view of the Exoplanete Gliese 581c - Artwork of exoplanet Gliese 581c - Artist view of the Exoplanete Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” This image of a rocky and variegated Gliese 581 c with an atmosphere and clouds is purely speculative

Walter B Myers

PIX4573773

Futuristic advertising poster for tourism on Trappist-1e - Illustration - Futuristic Advert for tourism on Trappist-1e - Illustration: Advertising promoting tourism on Trappist-1e. This exoplanet is orbiting in the habitable zone of the star system TRAPPIST-1, a red dwarf star located at a distance of about 40 light years from the Sun in the constellation Aquarius. At least seven exoplanets the size of the Earth orbit this star. Some 40 light-years from Earth, a planet called Trappist-1e offers a heart-stopping view: brilliant objects in a red sky, looming like larger and smaller versions of our own moon. But these are no moons. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle around their small, dim, red star, like a family around a campfire. Any of them could harbor liquid water, but the planet shown here, fourth from the TRAPPIST-1 star, is in the habitable zone, the area around the star where liquid water is most likely

Futuristic advertising poster for tourism on Trappist-1e - Illustration - Futuristic Advert for tourism on Trappist-1e - Illustration: Advertising promoting tourism on Trappist-1e. This exoplanet is orbiting in the habitable zone of the star system TRAPPIST-1, a red dwarf star located at a distance of about 40 light years from the Sun in the constellation Aquarius. At least seven exoplanets the size of the Earth orbit this star. Some 40 light-years from Earth, a planet called Trappist-1e offers a heart-stopping view: brilliant objects in a red sky, looming like larger and smaller versions of our own moon. But these are no moons. They are Earth-sized planets in a spectacular planetary system outside our own. These seven rocky worlds huddle around their small, dim, red star, like a family around a campfire. Any of them could harbor liquid water, but the planet shown here, fourth from the TRAPPIST-1 star, is in the habitable zone, the area around the star where liquid water is most likely

PIX4608509

In Jupiter's Red Spot - Illustration - Jupiter's Red Spot - Illustration - Artist's view of Jupiter's huge permanent tempete. Giant lights are seen between the clouds. Artwork showing the large storm in Jupiter's clouds. Lightning bolts passes between cloud layers

In Jupiter's Red Spot - Illustration - Jupiter's Red Spot - Illustration - Artist's view of Jupiter's huge permanent tempete. Giant lights are seen between the clouds. Artwork showing the large storm in Jupiter's clouds. Lightning bolts passes between cloud layers

Miller, Ron (b.1947)

PIX4575366

Jupiter and its satellite Io - Illustration - Io and the Great Red Spot - Illustration - The Io satellite in front of Jupiter's Great Red Spot. In the center of the picture, the small satellite Amalthee. This painting shows Io superimposed in front of the Great Red Spot of Jupiter. It represents the spot's appearance during the 1970s. The small central object is the tiny moon Amalthea

Jupiter and its satellite Io - Illustration - Io and the Great Red Spot - Illustration - The Io satellite in front of Jupiter's Great Red Spot. In the center of the picture, the small satellite Amalthee. This painting shows Io superimposed in front of the Great Red Spot of Jupiter. It represents the spot's appearance during the 1970s. The small central object is the tiny moon Amalthea

PIX4575236

Artist's impression of sunset on the super - Earth world Gliese 667 Cc - This artist's view represents a sunset seen from Super Earth Gliese 667Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B also appear right in the sky. Gliese 667 Cc is an exoplanet orbiting the star Gliese 667 C, located about 23 years from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. This artist's impression shows a sunset seen from the super - Earth Gliese 667 Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B appear in the sky also to the right. On 19 October 2009, the team who built the High Accuracy Radial Velocity Planet Searcher, better known as HARPS, the spectrograph for ESO's 3.6 - metre te

Artist's impression of sunset on the super - Earth world Gliese 667 Cc - This artist's view represents a sunset seen from Super Earth Gliese 667Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B also appear right in the sky. Gliese 667 Cc is an exoplanet orbiting the star Gliese 667 C, located about 23 years from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. This artist's impression shows a sunset seen from the super - Earth Gliese 667 Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B appear in the sky also to the right. On 19 October 2009, the team who built the High Accuracy Radial Velocity Planet Searcher, better known as HARPS, the spectrograph for ESO's 3.6 - metre te

PIX4573998

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Walter B Myers

PIX4624042

Saturn seen by the Cassini probe - Saturn seen by Cassini spacecraft: Saturn seen by the Cassini probe on 28 October 2016. Images taken on Oct. 28, 2016 with the wide angle camera using red, green and blue spectral filters were combined to create this color view. This view looks toward the sunlit side of the rings from about 25 degrees above the ringplane. The view was acquired at a distance of approximately 870,000 miles (1.4 million kilometers) from Saturn. Image scale is 50 miles (80 kilometers) per pixel

Saturn seen by the Cassini probe - Saturn seen by Cassini spacecraft: Saturn seen by the Cassini probe on 28 October 2016. Images taken on Oct. 28, 2016 with the wide angle camera using red, green and blue spectral filters were combined to create this color view. This view looks toward the sunlit side of the rings from about 25 degrees above the ringplane. The view was acquired at a distance of approximately 870,000 miles (1.4 million kilometers) from Saturn. Image scale is 50 miles (80 kilometers) per pixel

PIX4582280

Artist's view of a supernova explosion threatening spacecraft - Starships threatened by a supernova explosion - Artist's view of the explosion of a supernova threatening spacecraft. Cover illustration of Michael McCollum's novel “Antares Dawn”. Antares Dawn - cover for novel by Michael McCollum, a starship hovers against the backdrop of the exploding red giant Antares

Artist's view of a supernova explosion threatening spacecraft - Starships threatened by a supernova explosion - Artist's view of the explosion of a supernova threatening spacecraft. Cover illustration of Michael McCollum's novel “Antares Dawn”. Antares Dawn - cover for novel by Michael McCollum, a starship hovers against the backdrop of the exploding red giant Antares

Dixon, Don (b.1951)

PIX4640469

On Oct. 4, 2010, a million cubic meters (35 million cubic feet) of red sludge spilled from a reservoir at an alumina plant in Ajka in western Hungary. Four people were killed and about 100 injured. The sludge entered the Marcal River and has reached the Danube. Aquatic life in the Marcal was severely harmed; the mud also caused significant damage in nearby villages and towns, as well as adjacent farmland. On Oct. 11. Satellite image.

On Oct. 4, 2010, a million cubic meters (35 million cubic feet) of red sludge spilled from a reservoir at an alumina plant in Ajka in western Hungary. Four people were killed and about 100 injured. The sludge entered the Marcal River and has reached the Danube. Aquatic life in the Marcal was severely harmed; the mud also caused significant damage in nearby villages and towns, as well as adjacent farmland. On Oct. 11. Satellite image.

UIG866672

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. Close-up of a large impact crater measuring 20 km in diameter. The image was obtained by the Mars Express probe on December 28, 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The image shows a large impact crater measuring 20 km in diameter. It shows a blanket of ejecta with flow forms surrounding the rim

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. Close-up of a large impact crater measuring 20 km in diameter. The image was obtained by the Mars Express probe on December 28, 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The image shows a large impact crater measuring 20 km in diameter. It shows a blanket of ejecta with flow forms surrounding the rim

PIX4616168

Artist view of a spaceship near an exoplanet - Spacecraft over an exoplanet - Artist view - Artist view of a spaceship approaching an extrasolar planet of Earth type orbiting Nemesis, the hypothetical star companion of the Sun. Artist's view for Isaac Asimov's novel, Nemesis. A starship orbits a world of Barnard's star Nemesis, the hypothetical red dwarf brown dwarf star orbiting the Sun. Cover illustration for the novel of Isaac Asimov “” Nemesis””

Artist view of a spaceship near an exoplanet - Spacecraft over an exoplanet - Artist view - Artist view of a spaceship approaching an extrasolar planet of Earth type orbiting Nemesis, the hypothetical star companion of the Sun. Artist's view for Isaac Asimov's novel, Nemesis. A starship orbits a world of Barnard's star Nemesis, the hypothetical red dwarf brown dwarf star orbiting the Sun. Cover illustration for the novel of Isaac Asimov “” Nemesis””

Dixon, Don (b.1951)

PIX4640403

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

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

Miller, Ron (b.1947)

PIX4607996

March - Arabia Terra - Mars Express probe on June 17, 2019.

March - Arabia Terra - Mars Express probe on June 17, 2019.

PIX5940214

Mars: crateres and canals in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. This image covering an area of approximately 150 km exhibits a large impact crater measuring 20 kilometers in diameter. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region

Mars: crateres and canals in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. This image covering an area of approximately 150 km exhibits a large impact crater measuring 20 kilometers in diameter. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region

PIX4616155

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left of the image measures 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. The left side of the image shows a large impact crater measuri

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left of the image measures 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. The left side of the image shows a large impact crater measuri

PIX4616156

Mars Exploration - Mars Exploration - Illustration: Astronauts drill the surface of Mars to find water. Astronauts drill for water on the Red Planet.

Mars Exploration - Mars Exploration - Illustration: Astronauts drill the surface of Mars to find water. Astronauts drill for water on the Red Planet.

PIX4639956

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

PIX4615036

Venus Surface - Artist View - Venus from ground level - Artist view - A visit to Venus 'surface would reveal a wasteland of vast proportions. While Venus is nearly as large as the Earth, it has over three times the land mass (most of the Earth's surface is under water). The conditions are so dry and hostile to life as we know it the surface of Venus is likely as sterile as an autoclave. Venus' surface is actually hotter than Mercury's, despite being nearly twice as far from the Sun. It is so hot that the stony venusian ground itself may be slightly plastic and emit a red glow at night. The closest the Earth comes to matching this combination of extreme pressure and temperature is in the realm of deep undersea volcanic vents

Venus Surface - Artist View - Venus from ground level - Artist view - A visit to Venus 'surface would reveal a wasteland of vast proportions. While Venus is nearly as large as the Earth, it has over three times the land mass (most of the Earth's surface is under water). The conditions are so dry and hostile to life as we know it the surface of Venus is likely as sterile as an autoclave. Venus' surface is actually hotter than Mercury's, despite being nearly twice as far from the Sun. It is so hot that the stony venusian ground itself may be slightly plastic and emit a red glow at night. The closest the Earth comes to matching this combination of extreme pressure and temperature is in the realm of deep undersea volcanic vents

Walter B Myers

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Saturn and satellites seen by the Cassini probe on 30/01/2008 - Saturn and satellites seen by Cassini spacecraft Jan. 30 2008 - Saturn seen by the Cassini probe on 30 January 2008 at a distance of 1.3 million km from the planet. The Tethys satellite is visible under Saturn's rings and the Titan satellite appears at the top of the picture. Titan emerges from behind Saturn, while Tethys streaks into view, in this colorful scene. Saturn's shadow darkens the far arm of the rings near the planet's limb. Titan is 5,150 kilometers (3,200 miles) wide; Tethys is 1,071 kilometers (665 miles) wide. This view looks toward the unilluminated side of the rings from about 3 degrees above the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Jan. 30, 2008 at a distance of approximately 1.3 million kilometers (800,000 miles) from Saturn. Image scale is 77 kilomete

Saturn and satellites seen by the Cassini probe on 30/01/2008 - Saturn and satellites seen by Cassini spacecraft Jan. 30 2008 - Saturn seen by the Cassini probe on 30 January 2008 at a distance of 1.3 million km from the planet. The Tethys satellite is visible under Saturn's rings and the Titan satellite appears at the top of the picture. Titan emerges from behind Saturn, while Tethys streaks into view, in this colorful scene. Saturn's shadow darkens the far arm of the rings near the planet's limb. Titan is 5,150 kilometers (3,200 miles) wide; Tethys is 1,071 kilometers (665 miles) wide. This view looks toward the unilluminated side of the rings from about 3 degrees above the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Jan. 30, 2008 at a distance of approximately 1.3 million kilometers (800,000 miles) from Saturn. Image scale is 77 kilomete

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Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

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Saturn seen by the Cassini probe - Saturn seen by Cassini - Saturn seen by the Cassini probe on 22 August 2008 at a distance of 1.2 million km from the planet. The Cassini spacecraft looks toward the sunlit face of Saturn's rings, whose shadows continue to slide southward on the planet toward their temporary disappearance during equinox in August 2009. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Aug. 22, 2008 at a distance of approximately 1.2 million kilometers (728,000 miles) from Saturn. Image scale is 66 kilometers (41 miles) per pixel

Saturn seen by the Cassini probe - Saturn seen by Cassini - Saturn seen by the Cassini probe on 22 August 2008 at a distance of 1.2 million km from the planet. The Cassini spacecraft looks toward the sunlit face of Saturn's rings, whose shadows continue to slide southward on the planet toward their temporary disappearance during equinox in August 2009. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Aug. 22, 2008 at a distance of approximately 1.2 million kilometers (728,000 miles) from Saturn. Image scale is 66 kilometers (41 miles) per pixel

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Permanent station between Mars and Earth - Artist view - Mars lander departs cycler - Artist view - A landing ship (top left) leaves the Mars Cycler to land on the red planet. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. A manned Mars lander/return vehicle, upper left, disembarks from a Mars cycler for the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a large and well-equipped Mars cycler would off

Permanent station between Mars and Earth - Artist view - Mars lander departs cycler - Artist view - A landing ship (top left) leaves the Mars Cycler to land on the red planet. Mars Cycler is a space station placed in orbit between Mars and Earth whose trajectory would alternate between Mars and Earth. Once positioned in orbit, this gravitational assistance vessel would use very little fuel. This project would make a permanent link between the two planets. A manned Mars lander/return vehicle, upper left, disembarks from a Mars cycler for the surface of Mars. A Mars cycler is a permanently orbiting vehicle with a path that alternately brings it near Earth and Mars. Once a cycler has been accelerated into orbit it continues on its own momentum, going back and forth between the two planets, only requiring propellant for occasional course adjustments. A one-way trip between Earth and Mars involves six to eight months of space travel, therefore a large and well-equipped Mars cycler would off

Walter B Myers

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Saturn en jour seen by Cassini - Backlit Saturn seen by Cassini - Image obtained by the Cassini probe on October 17, 2012 at a distance of 800,000 km from the planet. At the bottom left of the image, the two brilliant dots are the Enceladus and Tethys satellites. Nasa's Cassini spacecraft has delivered a glorious view of Saturn, taken while the spacecraft was in Saturn's shadow. The cameras were turned toward Saturn and the sun so that the planet and rings are backlit. (The sun is behind the planet, which is shielding the cameras from direct sunlight.) In addition to the visual splendor, this special, very - high - phase viewing geometry lets scientists study ring and atmosphere phenomena not easily seen at a lower phase. Also captured in this image are two of Saturn's moons: Enceladus and Tethys. Both appear on the left side of the planet, below the rings. Enceladus is closer to the rings; Tethys is below and to the left. This view looks toward the non - illuminated side of the rings

Saturn en jour seen by Cassini - Backlit Saturn seen by Cassini - Image obtained by the Cassini probe on October 17, 2012 at a distance of 800,000 km from the planet. At the bottom left of the image, the two brilliant dots are the Enceladus and Tethys satellites. Nasa's Cassini spacecraft has delivered a glorious view of Saturn, taken while the spacecraft was in Saturn's shadow. The cameras were turned toward Saturn and the sun so that the planet and rings are backlit. (The sun is behind the planet, which is shielding the cameras from direct sunlight.) In addition to the visual splendor, this special, very - high - phase viewing geometry lets scientists study ring and atmosphere phenomena not easily seen at a lower phase. Also captured in this image are two of Saturn's moons: Enceladus and Tethys. Both appear on the left side of the planet, below the rings. Enceladus is closer to the rings; Tethys is below and to the left. This view looks toward the non - illuminated side of the rings

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Titan, Saturn satellite seen by Cassini - Titan near Saturn seen by Cassini spacecraft - Natural color image of Titan near Saturn blade taken by the Cassini probe on 29 January 2008 at a distance of about 2.3 million km from the satellite. Swathed in its thick blanket of atmosphere, frigid Titan approaches the brilliant limb of Saturn. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Jan. 29, 2008 at a distance of approximately 2.3 million kilometers (1.4 million miles) from Titan. Image scale is 14 kilometers (8 miles) per pixel

Titan, Saturn satellite seen by Cassini - Titan near Saturn seen by Cassini spacecraft - Natural color image of Titan near Saturn blade taken by the Cassini probe on 29 January 2008 at a distance of about 2.3 million km from the satellite. Swathed in its thick blanket of atmosphere, frigid Titan approaches the brilliant limb of Saturn. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Jan. 29, 2008 at a distance of approximately 2.3 million kilometers (1.4 million miles) from Titan. Image scale is 14 kilometers (8 miles) per pixel

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Cyclones encircle Jupiter's North Pole (photo)

Cyclones encircle Jupiter's North Pole (photo)

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Arctic ice has its minimum, September 2018 (photo)

Arctic ice has its minimum, September 2018 (photo)

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Appearance of life on Mars - Artist's view - Mars thermal crater - Artwork: Four billion years ago, the impacts of meteorites on Mars could create hot springs where life would have developed - A bombardment of the Red Planet 4 billion years ago could have created hot springs that allowed life to flourish

Appearance of life on Mars - Artist's view - Mars thermal crater - Artwork: Four billion years ago, the impacts of meteorites on Mars could create hot springs where life would have developed - A bombardment of the Red Planet 4 billion years ago could have created hot springs that allowed life to flourish

Miller, Ron (b.1947)

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Saturn seen by the Cassini probe - Saturn northern hemisphere seen by Cassini spacecraft: Saturn seen by the Cassini probe on 25 April 2016. Cassini scanned across the planet and its rings on April 25, 2016, capturing three sets of red, green and blue images to cover this entire scene showing the planet and the main rings. The images were obtained using Cassini's wide-angle camera at a distance of approximately 1.9 million miles (3 million kilometers) from Saturn and at an elevation of about 30 degrees above the ring plane. The view looks toward the sunlit side of the rings from a Sun-saturn-spacecraft angle, or phase angle, of 55 degrees.

Saturn seen by the Cassini probe - Saturn northern hemisphere seen by Cassini spacecraft: Saturn seen by the Cassini probe on 25 April 2016. Cassini scanned across the planet and its rings on April 25, 2016, capturing three sets of red, green and blue images to cover this entire scene showing the planet and the main rings. The images were obtained using Cassini's wide-angle camera at a distance of approximately 1.9 million miles (3 million kilometers) from Saturn and at an elevation of about 30 degrees above the ring plane. The view looks toward the sunlit side of the rings from a Sun-saturn-spacecraft angle, or phase angle, of 55 degrees.

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Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

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Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. In this artist's view, Curiosity analyses the chemical composition of a Martian rock using the ChECAM instrument. This artist's concept depicts the rover Curiosity, of Nasa's Mars Science Laboratory mission, as it uses its Chemistry and Camera (ChemCam) instrument to investigate the composition of a rock surface. ChemCam fires laser pulses at a target and views the resulting spark with a telescope and spectrometers to identify chemical elements. The laser is actually in an invisible infrared wavelength, but is shown here as visible red light for purposes of illustration

Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. In this artist's view, Curiosity analyses the chemical composition of a Martian rock using the ChECAM instrument. This artist's concept depicts the rover Curiosity, of Nasa's Mars Science Laboratory mission, as it uses its Chemistry and Camera (ChemCam) instrument to investigate the composition of a rock surface. ChemCam fires laser pulses at a target and views the resulting spark with a telescope and spectrometers to identify chemical elements. The laser is actually in an invisible infrared wavelength, but is shown here as visible red light for purposes of illustration

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Saturn and Mimas seen by the Cassini probe on 04/09/2007 - Saturn and Mimas seen by Cassini spacecraft Sept. 4 2007 - Saturn seen by the Cassini probe on 4/09/2007 at a distance of 2.7 million km from the planet. The Mimas ice satellite is visible under Saturn's rings. The Cassini spacecraft looks beyond Saturn's limb towards the icy face of Mimas, the innermost of the planet's major moons. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Mimas is 396 kilometers (246 miles) across. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Sept. 4, 2007 at a distance of approximately 2.7 million kilometers (1.7 million miles) from Saturn and 2.8 million kilometers (1.8 million miles) from Mimas. Image scale is 16 kilometers (10 miles) per pixel on Saturn and 17 kilometers (11 miles) per pixel on Mimas

Saturn and Mimas seen by the Cassini probe on 04/09/2007 - Saturn and Mimas seen by Cassini spacecraft Sept. 4 2007 - Saturn seen by the Cassini probe on 4/09/2007 at a distance of 2.7 million km from the planet. The Mimas ice satellite is visible under Saturn's rings. The Cassini spacecraft looks beyond Saturn's limb towards the icy face of Mimas, the innermost of the planet's major moons. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Mimas is 396 kilometers (246 miles) across. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Sept. 4, 2007 at a distance of approximately 2.7 million kilometers (1.7 million miles) from Saturn and 2.8 million kilometers (1.8 million miles) from Mimas. Image scale is 16 kilometers (10 miles) per pixel on Saturn and 17 kilometers (11 miles) per pixel on Mimas

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Size Comparison: Earth and Jupiter - Jupiter and Earth compared - Comparison of the sizes of the Earth and Jupiter, the largest planet in the solar system. Diameter of Earth: 12 756.28 km Diametre of Jupiter: 142,984 km Jupiter's diameter is over ten times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh 426 pounds at Jupiter's cloud tops. Jupiter is five times further from the Sun than the Earth. Jupiter is so large that its famous Great Red Spot (actually a giant, hurricane-like storm that's at least 400 years old) would easily swallow the Earth. Jupiter spins so fast on its axis that it bulges noticeably at its equator (a day on Jupiter is about ten hours long)

Size Comparison: Earth and Jupiter - Jupiter and Earth compared - Comparison of the sizes of the Earth and Jupiter, the largest planet in the solar system. Diameter of Earth: 12 756.28 km Diametre of Jupiter: 142,984 km Jupiter's diameter is over ten times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh 426 pounds at Jupiter's cloud tops. Jupiter is five times further from the Sun than the Earth. Jupiter is so large that its famous Great Red Spot (actually a giant, hurricane-like storm that's at least 400 years old) would easily swallow the Earth. Jupiter spins so fast on its axis that it bulges noticeably at its equator (a day on Jupiter is about ten hours long)

Walter B Myers

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Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

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The hidden face of the Moon and the Earth seen from DSCOVR. 07/2015 - Far side of the Moon with Earth seen from DSCOVR. 07/2015 - This image obtained on July 16, 2015 by the Deep Space Climate Observatory (DSCOVR) satellite shows the passage of the Moon and its face hidden from the Earth. The distance between DSCOVR and Earth is about 1.5 million kilometres. The Moon was approximately 400,000 kilometres from Earth, so it was closer to DSCOVR and therefore appears larger than it is in relation to Earth. This image shows the far side of the moon, illuminated by the sun, as it crosses between the Deep Space Climate Observatory (DSCOVR) spacecraft's Earth Polychromatic Imaging Camera (EPIC) camera and telescope, and the Earth - one million miles away. Because the moon has moved in relation to the Earth between the time the first (red) and last (green) exposures were made, a thin green offset appears on the right side of the moon when the three exposures are combined. July 16 2015

The hidden face of the Moon and the Earth seen from DSCOVR. 07/2015 - Far side of the Moon with Earth seen from DSCOVR. 07/2015 - This image obtained on July 16, 2015 by the Deep Space Climate Observatory (DSCOVR) satellite shows the passage of the Moon and its face hidden from the Earth. The distance between DSCOVR and Earth is about 1.5 million kilometres. The Moon was approximately 400,000 kilometres from Earth, so it was closer to DSCOVR and therefore appears larger than it is in relation to Earth. This image shows the far side of the moon, illuminated by the sun, as it crosses between the Deep Space Climate Observatory (DSCOVR) spacecraft's Earth Polychromatic Imaging Camera (EPIC) camera and telescope, and the Earth - one million miles away. Because the moon has moved in relation to the Earth between the time the first (red) and last (green) exposures were made, a thin green offset appears on the right side of the moon when the three exposures are combined. July 16 2015

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Arrival of a colony on Mars-Illustration - Red Mars ship - Artist view - A gigantic spaceship orbiting Mars Detail of colony ship from cover of Red Mars

Arrival of a colony on Mars-Illustration - Red Mars ship - Artist view - A gigantic spaceship orbiting Mars Detail of colony ship from cover of Red Mars

Dixon, Don (b.1951)

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Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

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Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

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November 2007 Temperature Map - Land surface temperatures in november 2007 - Map of average temperatures observed on Earth's surface by the Terra satellite between November 1 and December 1, 2007. The coldest regions appear in blue and white, the warmest in yellow and red. Moderate Resolution Imaging Spectroradiometer (MODIS) flying on NASA's Terra satellite between November 1 and December 1, 2007. It shows how the indirectness of sunlight at high latitudes affects temperature. The coldest areas, colored blue and white, are in the north, while the warmest areas, yellow and red, are near the Equator. These are also the planet's most snow - covered areas

November 2007 Temperature Map - Land surface temperatures in november 2007 - Map of average temperatures observed on Earth's surface by the Terra satellite between November 1 and December 1, 2007. The coldest regions appear in blue and white, the warmest in yellow and red. Moderate Resolution Imaging Spectroradiometer (MODIS) flying on NASA's Terra satellite between November 1 and December 1, 2007. It shows how the indirectness of sunlight at high latitudes affects temperature. The coldest areas, colored blue and white, are in the north, while the warmest areas, yellow and red, are near the Equator. These are also the planet's most snow - covered areas

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Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

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Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

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Conjunction Venus Jupiter from 14/03/2012 - Photographer, Venus and Jupiter - The photographer with a red headlamp, observes the rapprochement of Venus, on the right, and Jupiter (weaker on the left). March 14, 2012

Conjunction Venus Jupiter from 14/03/2012 - Photographer, Venus and Jupiter - The photographer with a red headlamp, observes the rapprochement of Venus, on the right, and Jupiter (weaker on the left). March 14, 2012

PIX4587172

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

PIX4573107

This photo of Jupiter was taken by Voyager 1 on March 1, 1979. The region shown is just to the southeast of the Great Red Spot.

This photo of Jupiter was taken by Voyager 1 on March 1, 1979. The region shown is just to the southeast of the Great Red Spot.

UIG867449

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