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Artist's view of the Exoplanet HD 189733b - Exoplanet HD 189733b - Artist's view of the transit of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. Using the Hubble space telescope, astronomers have detected carbon dioxide and monoxide in the atmosphere of this planet. Previously, methane and water vapour had already been detected in his atmosphere. But with a surface temperature of over 900 degrees, this planet remains too hot to shelter life. This is an artist's impression of the Jupiter - size extrasolar planet, HD 189733b, being eclipsed by its parent star. Astronomers using the Hubble Space Telescope have measured carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a “” hot Jupiter,””” which is so close to its star that it completes an orbit in only 2.2 days. The planet is too hot for life as we know it. But under the right conditions,

Artist's view of the Exoplanet HD 189733b - Exoplanet HD 189733b - Artist's view of the transit of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. Using the Hubble space telescope, astronomers have detected carbon dioxide and monoxide in the atmosphere of this planet. Previously, methane and water vapour had already been detected in his atmosphere. But with a surface temperature of over 900 degrees, this planet remains too hot to shelter life. This is an artist's impression of the Jupiter - size extrasolar planet, HD 189733b, being eclipsed by its parent star. Astronomers using the Hubble Space Telescope have measured carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a “” hot Jupiter,””” which is so close to its star that it completes an orbit in only 2.2 days. The planet is too hot for life as we know it. But under the right conditions,

PIX4573420

Detection of an exoplanet by microlens effect - Detection of an exoplanet: Gravitational microlensing - On the left, the observation of a distant star whose light is diluted. On the right, the light of this star is amplified by gravitational lens effect. The gravitational lens effect occurs when the gravitational field of a star acts as a magnifying glass by amplifying the light emitted by a farther star. This amplification is measurable, and when the foreground star is accompanied by a planet, a second peak of intensity in the life rays appears more weakly. Illustration showing at left the observation of faint light emitted by a distant star, at right, the light of the same star magnified by a gravitational lens. Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. Possible planets orbiting the foreground star can cause detectable anomalies in the lensing event light curve

Detection of an exoplanet by microlens effect - Detection of an exoplanet: Gravitational microlensing - On the left, the observation of a distant star whose light is diluted. On the right, the light of this star is amplified by gravitational lens effect. The gravitational lens effect occurs when the gravitational field of a star acts as a magnifying glass by amplifying the light emitted by a farther star. This amplification is measurable, and when the foreground star is accompanied by a planet, a second peak of intensity in the life rays appears more weakly. Illustration showing at left the observation of faint light emitted by a distant star, at right, the light of the same star magnified by a gravitational lens. Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. Possible planets orbiting the foreground star can cause detectable anomalies in the lensing event light curve

PIX4573970

Prode Juno and Jupiter - Artist view - Juno Over Jupiter's South Pole -Illustration:

Prode Juno and Jupiter - Artist view - Juno Over Jupiter's South Pole -Illustration:

PIX4605936

Saturn seen from his satellite Japet - Saturn as seen from Iapetus

Saturn seen from his satellite Japet - Saturn as seen from Iapetus

Miller, Ron (b.1947)

PIX4974169

Artist's view of an ocean planet - Ocean planet - Artist's view of an exoplanet covered with water on its surface

Artist's view of an ocean planet - Ocean planet - Artist's view of an exoplanet covered with water on its surface

Miller, Ron (b.1947)

PIX4945162

Mission to Phobos - Phobos mission ready for departure - A spaceship assemblies in Earth orbit is ready to depart to Phobos, one of Mars's satellites. This ship consists of several fuel tanks and an Orion-type space capsule with three astronauts on board. No landing gear is required because the mass of Phobos is so low that this satellite can be approached by astronauts in extravehicular exit. A complete rocket system for delivering a crew of three to Mars' moon Phobos and returning them to the Earth. The vast bulk of the rocket is propellant divided into stages that are each released in turn as the mission progresses. On the far right are the crew accomodations and an attached Orion class command module. No dedicated lander is required as Phobos' mass is so low that it could be easily approached by the command module and explored by suited astrogeologists in Manned Maneuvering Units (MMUS)

Mission to Phobos - Phobos mission ready for departure - A spaceship assemblies in Earth orbit is ready to depart to Phobos, one of Mars's satellites. This ship consists of several fuel tanks and an Orion-type space capsule with three astronauts on board. No landing gear is required because the mass of Phobos is so low that this satellite can be approached by astronauts in extravehicular exit. A complete rocket system for delivering a crew of three to Mars' moon Phobos and returning them to the Earth. The vast bulk of the rocket is propellant divided into stages that are each released in turn as the mission progresses. On the far right are the crew accomodations and an attached Orion class command module. No dedicated lander is required as Phobos' mass is so low that it could be easily approached by the command module and explored by suited astrogeologists in Manned Maneuvering Units (MMUS)

Walter B Myers

PIX4639606

Phobos mission approaching Phobos - The control module in approach to the Phobos satellite. The command module, now free of the larger Phobos mission rocket, begins a close approach to Phobos. With an average diameter of less than 12 miles, irregularly shaped Phobos has a very weak gravitational field making it relatively easy for the command module to come very close without being drawn all the way to its surface. The goal is to come close enough to permit space-suited astrogeologists equipped with personal manned maneuvering units (MMUS) to act as mini-spaceships themselves and descend to the surface. On the surface of Mars to the right can be seen Elysium Planitia and the volcano Albor Tholus

Phobos mission approaching Phobos - The control module in approach to the Phobos satellite. The command module, now free of the larger Phobos mission rocket, begins a close approach to Phobos. With an average diameter of less than 12 miles, irregularly shaped Phobos has a very weak gravitational field making it relatively easy for the command module to come very close without being drawn all the way to its surface. The goal is to come close enough to permit space-suited astrogeologists equipped with personal manned maneuvering units (MMUS) to act as mini-spaceships themselves and descend to the surface. On the surface of Mars to the right can be seen Elysium Planitia and the volcano Albor Tholus

Walter B Myers

PIX4639650

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

Exploration of Mars-Illustration - Man on Mars - An astronaut comes out of his pressurized vehicle to make a trip to Martian soil. An explorer steps out of the airlock and on to the porch of a martian motor home to begin several hours of extravehicular activity. The explorer's specialized suit is revealing of the extreme inhospitably of the martian environment to human life. Without the suit, not only would a human immediately suffer from Mars' lack of breathable oxygen and extreme cold, but the very thin atmosphere would result in all the fluids in the explorer's body quickly coming to a boil - at room temperature. That alone would cause immediate and catastrophic organ failure, unconsciousness, and imminent death. Thereafter the flesh would quickly desiccate and any liquids that had not boiled away would solidify, leaving a freeze-dried corpse far more impervious to decay than any Earth-bound mumm

Exploration of Mars-Illustration - Man on Mars - An astronaut comes out of his pressurized vehicle to make a trip to Martian soil. An explorer steps out of the airlock and on to the porch of a martian motor home to begin several hours of extravehicular activity. The explorer's specialized suit is revealing of the extreme inhospitably of the martian environment to human life. Without the suit, not only would a human immediately suffer from Mars' lack of breathable oxygen and extreme cold, but the very thin atmosphere would result in all the fluids in the explorer's body quickly coming to a boil - at room temperature. That alone would cause immediate and catastrophic organ failure, unconsciousness, and imminent death. Thereafter the flesh would quickly desiccate and any liquids that had not boiled away would solidify, leaving a freeze-dried corpse far more impervious to decay than any Earth-bound mumm

Walter B Myers

PIX4639843

Saturn

Saturn

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The formation of Saturn's rings - Artist's view - Saturn moon break up - A satellite of Saturn breaks giving birth to the rings of Saturn and has small satellites

The formation of Saturn's rings - Artist's view - Saturn moon break up - A satellite of Saturn breaks giving birth to the rings of Saturn and has small satellites

Miller, Ron (b.1947)

PIX4945569

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

PIX4616646

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

PIX4616696

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

Mars and its satellites - Mars and its moons - Photomontage showing the planet Mars surrounded by its two satellites, Phobos (middle) and Deimos (right)

Mars and its satellites - Mars and its moons - Photomontage showing the planet Mars surrounded by its two satellites, Phobos (middle) and Deimos (right)

PIX4616910

A Day on Io - 1/6 - Illustration - A Day on Io - 1/6 - 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 - Here, the Sun has just appeared behind Jupiter and the atmosphere of the giant planet illuminates - Io keeps the same face towards 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 - 1. The sun has just come out from behind Jupiter while the thick atmosphere of the planet is illuminated in a glowing ring

A Day on Io - 1/6 - Illustration - A Day on Io - 1/6 - 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 - Here, the Sun has just appeared behind Jupiter and the atmosphere of the giant planet illuminates - Io keeps the same face towards 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 - 1. The sun has just come out from behind Jupiter while the thick atmosphere of the planet is illuminated in a glowing ring

Miller, Ron (b.1947)

PIX4614123

Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole

Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole

PIX4615388

Mars - View of the north pole - Mars north pole - Image based on altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It's about 1100 km long. The ice - rich north polar cap (the quasi - circular white area at center) is approximately 1,000 kilometers (621 miles) across. The white cap is riven with dark, spiral - shaped bands. These are deep troughs that are in shadow. They do not reflect sunlight as well or have more internal layers exposed. To the right of center, a large canyon, Chasma Boreale, almost bisects the ice cap. Chasma Boreale is about the length of the United States' famous Grand Canyon and up to 2 kilometers (1.2 miles) deep. The image synthesizes topographic data from Mars Orbiter Laser Altimeter (MOLA) and images from the Mars Orbiter Camera (MOC)

Mars - View of the north pole - Mars north pole - Image based on altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It's about 1100 km long. The ice - rich north polar cap (the quasi - circular white area at center) is approximately 1,000 kilometers (621 miles) across. The white cap is riven with dark, spiral - shaped bands. These are deep troughs that are in shadow. They do not reflect sunlight as well or have more internal layers exposed. To the right of center, a large canyon, Chasma Boreale, almost bisects the ice cap. Chasma Boreale is about the length of the United States' famous Grand Canyon and up to 2 kilometers (1.2 miles) deep. The image synthesizes topographic data from Mars Orbiter Laser Altimeter (MOLA) and images from the Mars Orbiter Camera (MOC)

PIX4615389

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

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Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

D. Ducros

PIX4606058

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

D. Ducros

PIX4606645

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

D. Ducros

PIX4606649

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter. This illustration presents a purely speculative view of what such a “” hot Jupiter”” might look like. It could have a powerful magnetic field that traps charged particles from the star. These particles create glowing auroral rings around the planet's magnetic poles

Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter. This illustration presents a purely speculative view of what such a “” hot Jupiter”” might look like. It could have a powerful magnetic field that traps charged particles from the star. These particles create glowing auroral rings around the planet's magnetic poles

PIX4608319

Galaxy in the sky of an exoplanet - Galaxy seen from a rogue planet: Artist's view of a galaxy in the sky of an isolated exoplanet

Galaxy in the sky of an exoplanet - Galaxy seen from a rogue planet: Artist's view of a galaxy in the sky of an isolated exoplanet

Miller, Ron (b.1947)

PIX4573513

Exoplanetes glacees - Three worlds of ice and snow - Artist's view of extrasolar planets composed of ice. Far beyond our own solar system there are a likely billions of other planets orbiting stars like and unlike our own sun. Our sun, our Earth and moon, our solar system, represent only one of an unimaginable number of possibilities

Exoplanetes glacees - Three worlds of ice and snow - Artist's view of extrasolar planets composed of ice. Far beyond our own solar system there are a likely billions of other planets orbiting stars like and unlike our own sun. Our sun, our Earth and moon, our solar system, represent only one of an unimaginable number of possibilities

Walter B Myers

PIX4573229

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

PIX4573350

Uranus view from Cordelia - Illustration - Uranus as seen from Cordelia - Illustration: Illustration of Uranus seen from the Cordelia bergere Moon. Uranus as seen from shepherd moon Cordelia

Uranus view from Cordelia - Illustration - Uranus as seen from Cordelia - Illustration: Illustration of Uranus seen from the Cordelia bergere Moon. Uranus as seen from shepherd moon Cordelia

Miller, Ron (b.1947)

PIX4584311

Occultation of Saturn by the Moon - Saturn occultation by the moon Artwork - Artist view

Occultation of Saturn by the Moon - Saturn occultation by the moon Artwork - Artist view

S. Numazawa

PIX4588586

The Moon and Saturn - Moon with Saturn. November 3 2001 - The Moon and Planet Saturn. End of the blackout on 3 November 2001. Moon with Saturn. End of the occultation of november 3rd 2001

The Moon and Saturn - Moon with Saturn. November 3 2001 - The Moon and Planet Saturn. End of the blackout on 3 November 2001. Moon with Saturn. End of the occultation of november 3rd 2001

Sebastian Voltmer

PIX4588258

Mercury Transit in front of the Sun. May 9, 2016 - Mercury Transit. May 9, 2016: Mercury is located at the bottom center as a small, dark, round spot

Mercury Transit in front of the Sun. May 9, 2016 - Mercury Transit. May 9, 2016: Mercury is located at the bottom center as a small, dark, round spot

Sebastian Voltmer

PIX4588338

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

PIX4606810

Exoplanete Kepler-36 c: Kepler-36 c view from the surface of Kepler-36 b. These two planets have close orbits and revolve around the star Kepler-36 in the constellation Swan. Kepler-36c is a gas giant that orbits very close to Kepler-36b, a rocky world, in the Kepler-36 system

Exoplanete Kepler-36 c: Kepler-36 c view from the surface of Kepler-36 b. These two planets have close orbits and revolve around the star Kepler-36 in the constellation Swan. Kepler-36c is a gas giant that orbits very close to Kepler-36b, a rocky world, in the Kepler-36 system

Miller, Ron (b.1947)

PIX4608186

Exoplanete in formation - LKCA 15 b - Exoplanet forming - LKCA 15 b: Artist's view showing the exoplanet LKCA 15 b, an exoplanet in formation by accretion. LKCA 15 b or Lick-Calcium 15b is a candidate protoplanetary object in orbit around LKCA 15, a star in the Taurus-Auriga Star Forming Region. It was discovered by direct imaging techniques using the Keck II telescope in 2011. A 2015 study of observations from the Magellan Telescopes and the Large Binocular Telescope argued that the planet is forming though accretion. It is the first observed exoplanet seen in the process of active accretion.

Exoplanete in formation - LKCA 15 b - Exoplanet forming - LKCA 15 b: Artist's view showing the exoplanet LKCA 15 b, an exoplanet in formation by accretion. LKCA 15 b or Lick-Calcium 15b is a candidate protoplanetary object in orbit around LKCA 15, a star in the Taurus-Auriga Star Forming Region. It was discovered by direct imaging techniques using the Keck II telescope in 2011. A 2015 study of observations from the Magellan Telescopes and the Large Binocular Telescope argued that the planet is forming though accretion. It is the first observed exoplanet seen in the process of active accretion.

Miller, Ron (b.1947)

PIX4608448

Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003

Spitzer space telescope - Artist's view - Artwork of Spitzer space telescope - Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003

PIX4645627

From Earth to Moon, then March -Illustration - Aurora program - Illustration - Aurora Programme is part of Europe's strategy for space, endorsed by the European Union Council of Research and the ESA Council in 2001. The objective of the Aurora is first to formulate and then to implement a European long-term plan for the robotic and human exploration of solar system, with Mars, the Moon and the asteroids as the most likely targets

From Earth to Moon, then March -Illustration - Aurora program - Illustration - Aurora Programme is part of Europe's strategy for space, endorsed by the European Union Council of Research and the ESA Council in 2001. The objective of the Aurora is first to formulate and then to implement a European long-term plan for the robotic and human exploration of solar system, with Mars, the Moon and the asteroids as the most likely targets

P. Carril

PIX4639717

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut crowds the soil of March. Artist's view. In some distant future, astronauts amble about on Mars. The hardware designs are based on the Lunar spacecraft being imagined by NASA

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut crowds the soil of March. Artist's view. In some distant future, astronauts amble about on Mars. The hardware designs are based on the Lunar spacecraft being imagined by NASA

PIX4639858

Depart to the Moon - Artist view - Tug and lunar lander leaving Earth - Artist view - A spaceship leaves Earth orbit for a three-day journey to the Moon. Following a powerful burst from its primary thruster, a trans-moon space tug accelerates itself and the attached lunar lander into a much larger Earth orbit that will intercept the moon in about three days

Depart to the Moon - Artist view - Tug and lunar lander leaving Earth - Artist view - A spaceship leaves Earth orbit for a three-day journey to the Moon. Following a powerful burst from its primary thruster, a trans-moon space tug accelerates itself and the attached lunar lander into a much larger Earth orbit that will intercept the moon in about three days

Walter B Myers

PIX4638880

Trajectory of the Ulysses probe, launched by Europeans to study the Sun.: The Ulysses probe - Ulysses spacecraft trajectory- Artwork

Trajectory of the Ulysses probe, launched by Europeans to study the Sun.: The Ulysses probe - Ulysses spacecraft trajectory- Artwork

L. Bret

PIX4643812

A pair of Saturn's moons accompany the planet and its rings. Dione is in top left and Tethys is below. Cassini.

A pair of Saturn's moons accompany the planet and its rings. Dione is in top left and Tethys is below. Cassini.

UIG866377

Io and its shadow (photo)

Io and its shadow (photo)

Sebastian Voltmer

PIX6333925

Total Eclipse of Moon and March, 27 July 2018.

Total Eclipse of Moon and March, 27 July 2018.

Alex Conu

PIX5940210

The Cassini spacecraft captured this natural color view of Saturn almost a month after the planet's August 2009 equinox. The shadow cast on the planet by the rings remains narrow.

The Cassini spacecraft captured this natural color view of Saturn almost a month after the planet's August 2009 equinox. The shadow cast on the planet by the rings remains narrow.

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Diagram of Meteoric falls near Earth

Diagram of Meteoric falls near Earth

DGA572737

Earth Globe Showing Asia and Australia With Country Borders

Earth Globe Showing Asia and Australia With Country Borders

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Earth Globe Showing Asia and Australia With Country Borders

Earth Globe Showing Asia and Australia With Country Borders

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Earth Globe Showing Asia and Australia

Earth Globe Showing Asia and Australia

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

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

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

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

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Whole Earth At Night With Country Borders, True Colour Satellite Image

Whole Earth At Night With Country Borders, True Colour Satellite Image

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Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

PIX4605637

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

PIX4605645

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of the ice jets on the surface of the Enceladus satellite observed by the Cassini probe. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Enceladus 'ice geysers - Saturn is in background. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of the ice jets on the surface of the Enceladus satellite observed by the Cassini probe. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Enceladus 'ice geysers - Saturn is in background. Artist view

M. Carroll

PIX4625793

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Walter B Myers

PIX4625835

Saturn and Titan - Illustration - Saturn from Titan orbit - The planet Saturn seen from the orbit of its Titan satellite. This is how Saturn and Titan might look from a position in orbit around Titan. While in reality Saturn is vastly larger than Titan, it appears smaller here because Titan's orbit puts Saturn at a distance of about 700 thousand miles. Sunlight filtering through Titan's upper atmospheric haze - - extending over 300 miles above the surface - - gives a bluish cast to its limb

Saturn and Titan - Illustration - Saturn from Titan orbit - The planet Saturn seen from the orbit of its Titan satellite. This is how Saturn and Titan might look from a position in orbit around Titan. While in reality Saturn is vastly larger than Titan, it appears smaller here because Titan's orbit puts Saturn at a distance of about 700 thousand miles. Sunlight filtering through Titan's upper atmospheric haze - - extending over 300 miles above the surface - - gives a bluish cast to its limb

Walter B Myers

PIX4626066

Mars surface seen by the probe Mariner 7 - Mariner 7 view of martian craters - Martian crateres near the southern pole seen by the probe Mariner 7 in August 1969. Recolorized image. Mars craters near south pole seen by Mariner 7 in august 1969. Recolorized picture

Mars surface seen by the probe Mariner 7 - Mariner 7 view of martian craters - Martian crateres near the southern pole seen by the probe Mariner 7 in August 1969. Recolorized image. Mars craters near south pole seen by Mariner 7 in august 1969. Recolorized picture

Steven Hobbs

PIX4615030

March: chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles and Sacra Fossae. To the north, the large impact crater is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The image shows an old 35 km - diameter impact crater in the north. The crater's southwestern rim is eroded strongly, mostly by flowing water. The source of the water was located in Etus Chasma, which lies about 850 km to the southwest. The crater floor and the northwestern part are remarkably flat, formed by sediments and basaltic lava fl

March: chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles and Sacra Fossae. To the north, the large impact crater is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The image shows an old 35 km - diameter impact crater in the north. The crater's southwestern rim is eroded strongly, mostly by flowing water. The source of the water was located in Etus Chasma, which lies about 850 km to the southwest. The crater floor and the northwestern part are remarkably flat, formed by sediments and basaltic lava fl

PIX4616176

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

Volcanic eruption on Io - Illustration - Volcano on Io - Artwork

Volcanic eruption on Io - Illustration - Volcano on Io - Artwork

Miller, Ron (b.1947)

PIX4614202

Jupiter seen from the satellite Europe - Illustration - Jupiter from Europa - Illustration: Jupiter seen from the icy surface of the satellite Europe. Artist View

Jupiter seen from the satellite Europe - Illustration - Jupiter from Europa - Illustration: Jupiter seen from the icy surface of the satellite Europe. Artist View

Miller, Ron (b.1947)

PIX4614357

The hidden face of the Moon and the Earth seen from DSCOVR. 07/2016 - Far side of the Moon with Earth seen from DSCOVR. 07/2016: This image obtained on July 5, 2016, the moon again passed between DSCOVR and the Earth. EPIC snapped these images over a period of about 4 hours. In this set, the far side of the moon, which is never seen from Earth, passes by. In the backdrop, Earth rotates, starting with the Australia and Pacific and gradually revealing Asia and Africa

The hidden face of the Moon and the Earth seen from DSCOVR. 07/2016 - Far side of the Moon with Earth seen from DSCOVR. 07/2016: This image obtained on July 5, 2016, the moon again passed between DSCOVR and the Earth. EPIC snapped these images over a period of about 4 hours. In this set, the far side of the moon, which is never seen from Earth, passes by. In the backdrop, Earth rotates, starting with the Australia and Pacific and gradually revealing Asia and Africa

PIX4614527

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