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Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

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

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

Miller, Ron (b.1947)

PIX4624110

Saturn and satellites shepherds - Artist view - Saturn and Shepherd Moons - Artist view - Artist view of Saturn's F ring accompanies small satellites shepherds Promethee and Pandora. The weirdly braided F - ring of Saturn is confined by two tiny “” shepherd”” moons, named Prometheus and Pandora, which orbit just on either side of it

Saturn and satellites shepherds - Artist view - Saturn and Shepherd Moons - Artist view - Artist view of Saturn's F ring accompanies small satellites shepherds Promethee and Pandora. The weirdly braided F - ring of Saturn is confined by two tiny “” shepherd”” moons, named Prometheus and Pandora, which orbit just on either side of it

PIX4626404

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

PIX4606652

Conjunction Venus Jupiter - Jupiter-Venus conjunction - Venus (the brightest) and Jupiter seen above the horizon. Riviere Odet, Brittany. 25/11/2008 Venus (the brightest) with Jupiter seen above the horizon. Odet river, Brittany. November 25, 2008

Conjunction Venus Jupiter - Jupiter-Venus conjunction - Venus (the brightest) and Jupiter seen above the horizon. Riviere Odet, Brittany. 25/11/2008 Venus (the brightest) with Jupiter seen above the horizon. Odet river, Brittany. November 25, 2008

Laurent Laveder

PIX4587464

Venus and Mercury - Venus and Mercury planets seen at dusk. Long pose. 12 January 2015. Venus and Mercury seen in twilight. January 12 2015

Venus and Mercury - Venus and Mercury planets seen at dusk. Long pose. 12 January 2015. Venus and Mercury seen in twilight. January 12 2015

Sebastian Voltmer

PIX4587519

Sedimentary depots on Mars seen by Curiosity 02/2013 - Martian surface seen from the rover Curiosity 02/2013 - Sedimentary depots in the crater Gale sur Mars. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on February 14, 2013. This mosaic of images from the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west - northwest. Mastcam took the images for this mosaic during the 188th Martian day, or sol, of Curiosity's work on Mars (Feb. 14, 2013). The image has been white - balanced to show what the rocks would look like if ther were on Earth

Sedimentary depots on Mars seen by Curiosity 02/2013 - Martian surface seen from the rover Curiosity 02/2013 - Sedimentary depots in the crater Gale sur Mars. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on February 14, 2013. This mosaic of images from the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west - northwest. Mastcam took the images for this mosaic during the 188th Martian day, or sol, of Curiosity's work on Mars (Feb. 14, 2013). The image has been white - balanced to show what the rocks would look like if ther were on Earth

PIX4616681

Dust disc around Beta Pictoris - Disk around Beta Pictoris. Artwork: Beta Pictoris is a young star aged 12 million years old located about 63 light years ago in the southern constellation of the Painter. It is surrounded by a dust disc (protoplanetary disc). Only 12 million years old, the 'baby star' Beta Pictoris is located about 63 light-years away towards the constellation Pictor (the Painter)

Dust disc around Beta Pictoris - Disk around Beta Pictoris. Artwork: Beta Pictoris is a young star aged 12 million years old located about 63 light years ago in the southern constellation of the Painter. It is surrounded by a dust disc (protoplanetary disc). Only 12 million years old, the 'baby star' Beta Pictoris is located about 63 light-years away towards the constellation Pictor (the Painter)

Miller, Ron (b.1947)

PIX4608433

A spaceship explores an extrasolar planet - A spaceship over an alien plane

A spaceship explores an extrasolar planet - A spaceship over an alien plane

Dixon, Don (b.1951)

PIX4640457

Earth Globe Showing European and African Continents

Earth Globe Showing European and African Continents

UIG675252

Ocean of Hydrogen on Jupiter - Jupiter's hydrogen sea - Under the clouds of Jupiter could exist an ocean of hydrogen. The pressure here is much higher than the bottom of the Earth's oceans. Liquid hydrogen is responsible for the intense magnetic field of the planet. Miles beneath Jupiter's brown clouds of ammonia, hydrogen and helium lies mysterious realm where the weight of the atmosphere above far exceeds the pressures found in Earth's deepest oceans. It is believed that in this realm, somewhere between Jupiter's cloud tops and the jovian core, the atmosphere gives way to a planet - wide ocean of liquid hydrogen. This image suggests that there is a clear demarcation between atmosphere and the hydrogen sea - - a dark, extremely dense world where giant bolts of lightning erupt from the ever - changing electrical potential between liquid and gas. Too deep for sunlight to penetrate, the only light here is from the glow of this ubiquitous lightning. Further down toward Jupiter's core the

Ocean of Hydrogen on Jupiter - Jupiter's hydrogen sea - Under the clouds of Jupiter could exist an ocean of hydrogen. The pressure here is much higher than the bottom of the Earth's oceans. Liquid hydrogen is responsible for the intense magnetic field of the planet. Miles beneath Jupiter's brown clouds of ammonia, hydrogen and helium lies mysterious realm where the weight of the atmosphere above far exceeds the pressures found in Earth's deepest oceans. It is believed that in this realm, somewhere between Jupiter's cloud tops and the jovian core, the atmosphere gives way to a planet - wide ocean of liquid hydrogen. This image suggests that there is a clear demarcation between atmosphere and the hydrogen sea - - a dark, extremely dense world where giant bolts of lightning erupt from the ever - changing electrical potential between liquid and gas. Too deep for sunlight to penetrate, the only light here is from the glow of this ubiquitous lightning. Further down toward Jupiter's core the

Walter B Myers

PIX4575024

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

PIX4616545

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

PIX4616735

Mars: Phobos breaks apart - Illustration - Phobos breaking up to form ring - Illustration - Artist's view of Phobos, the largest of Mars's two satellites, which due to its proximity to the planet Mars will break in 20 to 50 million years. The larger pieces will crush on Mars, forming new crateres, but the smaller ones and the dust should remain in suspension, in orbit and leave all around Mars to form a ring. Phobos, one of Mars' moons, is getting closer to the planet and in several million years Phobos will break apart upon reaching the Roche limit, and become a set of rings

Mars: Phobos breaks apart - Illustration - Phobos breaking up to form ring - Illustration - Artist's view of Phobos, the largest of Mars's two satellites, which due to its proximity to the planet Mars will break in 20 to 50 million years. The larger pieces will crush on Mars, forming new crateres, but the smaller ones and the dust should remain in suspension, in orbit and leave all around Mars to form a ring. Phobos, one of Mars' moons, is getting closer to the planet and in several million years Phobos will break apart upon reaching the Roche limit, and become a set of rings

Miller, Ron (b.1947)

PIX4617115

Venus, Mars and Mercury - Venus, Mars and Mercury - Planet Mars near the brilliant Venus on the right. On the left, the planet Mercury. 13 September 2008. March close to the bright planet Venus. At left, planet Mercury. September 13 2008

Venus, Mars and Mercury - Venus, Mars and Mercury - Planet Mars near the brilliant Venus on the right. On the left, the planet Mercury. 13 September 2008. March close to the bright planet Venus. At left, planet Mercury. September 13 2008

Sebastian Voltmer

PIX4587767

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

PIX4588448

Transit of Venus in front of the Sun. 06/06/2012 - Venus Transit. 06/06/2012 - End of the transit of Venus in front of the Sun seen by the SDO satellite, June 6, 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

Transit of Venus in front of the Sun. 06/06/2012 - Venus Transit. 06/06/2012 - End of the transit of Venus in front of the Sun seen by the SDO satellite, June 6, 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

PIX4588462

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

PIX4624813

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the Mercury Surface and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter (MMO) orbiting Mercury.

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the Mercury Surface and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter (MMO) orbiting Mercury.

PIX4643594

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter (MMO) orbiting Mercury.

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter (MMO) orbiting Mercury.

PIX4643616

Comparison between the sizes of Earth, Pluto, Charon and the Moon

Comparison between the sizes of Earth, Pluto, Charon and the Moon

Walter B Myers

PIX4629992

Saturn's B ring - Artist view - Mountains of Saturns rings: Artist view of the shadows projected by ice mountains in Saturn's B ring - Vertical structures, among the tallest seen in Saturn's main rings, rise abruptly from the edge of Saturn's B ring to cast long shadows on the ring

Saturn's B ring - Artist view - Mountains of Saturns rings: Artist view of the shadows projected by ice mountains in Saturn's B ring - Vertical structures, among the tallest seen in Saturn's main rings, rise abruptly from the edge of Saturn's B ring to cast long shadows on the ring

Miller, Ron (b.1947)

PIX4625773

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view: Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn - Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view: Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn - Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole

Miller, Ron (b.1947)

PIX4625876

Cross-section view of the Earth - Earth cutaway - Internal structure of the Earth. On the surface, the crust forms a bark of about 7 km under the oceans and 30 to 40 km under the continents. Below is the mantle, a 2900 km thick rock belt. The outer core is composed of liquid metal, mainly iron and nickel. The inner core, or seed, is composed of the same alloy but is solid. Art cutaway of Earth showing interior structure. The surface is a crust, a thin layer of solid rock about 7 km thick under the oceans and 30 to 40 km thick where there are continents. Below is the mantle, 2900 km thick layer of molten rock. The outer core consists of liquid metal, mostly iron and nickel. The inner core has a similar composition but is solid

Cross-section view of the Earth - Earth cutaway - Internal structure of the Earth. On the surface, the crust forms a bark of about 7 km under the oceans and 30 to 40 km under the continents. Below is the mantle, a 2900 km thick rock belt. The outer core is composed of liquid metal, mainly iron and nickel. The inner core, or seed, is composed of the same alloy but is solid. Art cutaway of Earth showing interior structure. The surface is a crust, a thin layer of solid rock about 7 km thick under the oceans and 30 to 40 km thick where there are continents. Below is the mantle, 2900 km thick layer of molten rock. The outer core consists of liquid metal, mostly iron and nickel. The inner core has a similar composition but is solid

PIX4633327

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Walter B Myers

PIX4639664

An automatic cargo ship en route to Mars - Unmanned cargo capsule departs Mars cycler - An automatic cargo ship separates from the Mars Cycler to bring equipment to Mars. 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. With small bursts from its reaction control thrusters, an automated cargo capsule begins its one-way journey from a Mars cycler to 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 la

An automatic cargo ship en route to Mars - Unmanned cargo capsule departs Mars cycler - An automatic cargo ship separates from the Mars Cycler to bring equipment to Mars. 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. With small bursts from its reaction control thrusters, an automated cargo capsule begins its one-way journey from a Mars cycler to 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 la

Walter B Myers

PIX4639566

A Day on Io - 6/6 - Illustration - A Day on Io - 6/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-6. At the end of the day, the Sun is just below the horizon to the left. He's about to get up and disappear again behind Jupiter. Io takes about 42 hours to go around Jupiter - Io keeps the same face toward Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 6. Near the end of the day and the sun is just below the left horizon. It will be rising soon only to disappear again behind Jupiter

A Day on Io - 6/6 - Illustration - A Day on Io - 6/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-6. At the end of the day, the Sun is just below the horizon to the left. He's about to get up and disappear again behind Jupiter. Io takes about 42 hours to go around Jupiter - Io keeps the same face toward Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 6. Near the end of the day and the sun is just below the left horizon. It will be rising soon only to disappear again behind Jupiter

Miller, Ron (b.1947)

PIX4614157

March: Volcano Olympus Mons - False colors - Mars: volcano Olympus Mons - Altimetric data obtained by the Mars Express probe. The Olympus Mons volcano is 600 km in diameter and 26 km above the plains. This is a mosaic of Olympus Mons, the highest volcano on Mars, which towers 26 km above the surrounding plains. The image covers an area of approximately 600,000 sq km and is color - coded according to height

March: Volcano Olympus Mons - False colors - Mars: volcano Olympus Mons - Altimetric data obtained by the Mars Express probe. The Olympus Mons volcano is 600 km in diameter and 26 km above the plains. This is a mosaic of Olympus Mons, the highest volcano on Mars, which towers 26 km above the surrounding plains. The image covers an area of approximately 600,000 sq km and is color - coded according to height

PIX4615892

Europe and Jupiter - Illustration - Jupiter and Europa - Illustration - Jupiter and its satellite Europe. Artist's view. Planet Jupiter with Europa

Europe and Jupiter - Illustration - Jupiter and Europa - Illustration - Jupiter and its satellite Europe. Artist's view. Planet Jupiter with Europa

PIX4575154

Phases of the Moon - Phases of the Moon - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660 - 1661. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660 - 1661

Phases of the Moon - Phases of the Moon - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660 - 1661. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660 - 1661

Sebastien Beaucourt

PIX4576012

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on June 5 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events: the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117

PIX4588485

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

PIX4580075

World map centred on Pacific ocean

World map centred on Pacific ocean

UIG674416

World map

World map

UIG674420

Earth Globe Showing Antarctica

Earth Globe Showing Antarctica

UIG675273

Diagram of seismic tomography

Diagram of seismic tomography

DGA572716

Whole Earth At Night With Cloud Coverage, True Colour Satellite Image

Whole Earth At Night With Cloud Coverage, True Colour Satellite Image

UIG520921

Whole Earth, True Colour Satellite Image

Whole Earth, True Colour Satellite Image

UIG520912

Whole Earth With Bump Effect, True Colour Satellite Image

Whole Earth With Bump Effect, True Colour Satellite Image

UIG520911

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

UIG521125

Whole Earth At Night Centred On Pacific Ocean, True Colour Satellite Image

Whole Earth At Night Centred On Pacific Ocean, True Colour Satellite Image

UIG521130

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

UIG521120

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

UIG521121

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

Whole Earth Centred On Pacific Ocean, True Colour Satellite Image

UIG521124

Earth Globe Showing European and African Continents With Country Borders

Earth Globe Showing European and African Continents With Country Borders

UIG675254

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

PIX4616532

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Walter B Myers

PIX4616961

The Cassini probe and the Enceladus geysers - Cassini spacecraft with Enceladus Geysers: Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. His mission ended on 15 September 2017. Cassini spacecraft is diving through the plume of Saturn's moon Enceladus

The Cassini probe and the Enceladus geysers - Cassini spacecraft with Enceladus Geysers: Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. His mission ended on 15 September 2017. Cassini spacecraft is diving through the plume of Saturn's moon Enceladus

PIX4606103

Mars and Zodiacal Light - The Zodiacal Light with Mars - In the middle up, the bright spot is the planet Mars, in the constellation Gemeaux. Below, the zodiac light. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plan of the Solar System. September 20, 2009. The Zodiacal light is visible here as a large diffuse triangular - shaped cone of light rising along the ecliptic, which is tilted a bit to the right. Its base stretches from Leo on the left to the head of Hydra on the right. It goes up through Cancer and into Gemini where it crosses the Milky Way. The planet Mars was also located in Gemini when this photo was taken. The Zodiacal light is composed of fine particles of dust in orbit around the Sun. It is visible because of sunlight scattered by the particles. These particles have sizes between a couple of micrometers and a few millimeters. From the mid - northern latitudes, the Zodiacal light is most easily visible

Mars and Zodiacal Light - The Zodiacal Light with Mars - In the middle up, the bright spot is the planet Mars, in the constellation Gemeaux. Below, the zodiac light. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plan of the Solar System. September 20, 2009. The Zodiacal light is visible here as a large diffuse triangular - shaped cone of light rising along the ecliptic, which is tilted a bit to the right. Its base stretches from Leo on the left to the head of Hydra on the right. It goes up through Cancer and into Gemini where it crosses the Milky Way. The planet Mars was also located in Gemini when this photo was taken. The Zodiacal light is composed of fine particles of dust in orbit around the Sun. It is visible because of sunlight scattered by the particles. These particles have sizes between a couple of micrometers and a few millimeters. From the mid - northern latitudes, the Zodiacal light is most easily visible

Jerry Lodriguss

PIX4581551

Venus and the Moon in broad daylight 18/06/2007 - Venus and Moon in daylight June 18 2007 - Photograph of Venus near the Moon obtained in broad daylight on June 18, 2007 before its occultation by our satellite. Venus, the bright spot near the top of the cloud, is going to disappear hidden by the moon. Daylight image taken on June 18, 2007

Venus and the Moon in broad daylight 18/06/2007 - Venus and Moon in daylight June 18 2007 - Photograph of Venus near the Moon obtained in broad daylight on June 18, 2007 before its occultation by our satellite. Venus, the bright spot near the top of the cloud, is going to disappear hidden by the moon. Daylight image taken on June 18, 2007

Laurent Laveder

PIX4586764

Conjunction Venus Jupiter of July 1, 2015 - Venus and Jupiter on july 1st 2015 - Arrival of Venus, below, and Jupiter (lower above) seen in France at the beginning of the night. The two planets Venus (bottom) and Jupiter (fainter above)

Conjunction Venus Jupiter of July 1, 2015 - Venus and Jupiter on july 1st 2015 - Arrival of Venus, below, and Jupiter (lower above) seen in France at the beginning of the night. The two planets Venus (bottom) and Jupiter (fainter above)

Sebastian Voltmer

PIX4587217

Mars in the open cluster M44 - Planet Mars in the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. May 23, 2008. Bright Mars among M44 stars; this cluster is located about 600 light year away in Cancer. May 23, 2008

Mars in the open cluster M44 - Planet Mars in the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. May 23, 2008. Bright Mars among M44 stars; this cluster is located about 600 light year away in Cancer. May 23, 2008

PIX4588238

Earth Globe Showing Asia and Australia

Earth Globe Showing Asia and Australia

UIG675240

Earth - artist's view - Earth. Artwork - The Earth centered on Africa. Earth with Europe and Africa

Earth - artist's view - Earth. Artwork - The Earth centered on Africa. Earth with Europe and Africa

Walter B Myers

PIX4633160

Giant planets of our solar system - From top to bottom the planets Jupiter, Neptune and Saturn. Illustration. Illustration showing from top to bottom planets Jupiter, Neptune and Saturn

Giant planets of our solar system - From top to bottom the planets Jupiter, Neptune and Saturn. Illustration. Illustration showing from top to bottom planets Jupiter, Neptune and Saturn

D. Ducros

PIX4629732

Size comparison: Uranus and Earth - Uranus and Earth compared - The planet Uranus compares to Earth. Uranus' diameter is four times that of the Earth's. It has 15 times the mass. If you weigh 180 pounds on Earth, you would weigh only 160 pounds at Uranus' cloud tops. Uranus is 19 times further from the Sun than the Earth

Size comparison: Uranus and Earth - Uranus and Earth compared - The planet Uranus compares to Earth. Uranus' diameter is four times that of the Earth's. It has 15 times the mass. If you weigh 180 pounds on Earth, you would weigh only 160 pounds at Uranus' cloud tops. Uranus is 19 times further from the Sun than the Earth

Walter B Myers

PIX4629918

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

PIX4625303

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

PIX4606029

Spaceship - Artist View - Huge Spaceship - Artist view - Artist view of a gigantic spaceship to escape from a cosmic catastrophe. Cover illustration for John Brunner novel about a civilization's struggle to survive cosmic catastrophes

Spaceship - Artist View - Huge Spaceship - Artist view - Artist view of a gigantic spaceship to escape from a cosmic catastrophe. Cover illustration for John Brunner novel about a civilization's struggle to survive cosmic catastrophes

Dixon, Don (b.1951)

PIX4640436

Earth Globe Showing Pacific Ocean

Earth Globe Showing Pacific Ocean

UIG675266

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