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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

Earth 200 million years ago - Artist's view - Early Jurassic Earth - Earth seen at the beginning of the Jurassic, about 200 million years ago. The western hemisphere is representative, the north is up. The Pangee has just split, forming Laurasia to the north and Gondwana to the south. This is how the western hemisphere of the Earth may have appeared 200 million years ago during the Early Jurassic period. North is at the top. During this period continental drift, driven by the massive forces of plate tectonics, had just begun to break the supercontinent of Pangea into Laurasia in the north and Gondwana in the south. In this image the nascent North American continent has just broken away from North Africa while South America and the rest of Africa remain joined as Gondwana. To the west in the global Panthalassa ocean are strips of land corresponding to the Wrangellia Terrane which later merged with western North America

Earth 200 million years ago - Artist's view - Early Jurassic Earth - Earth seen at the beginning of the Jurassic, about 200 million years ago. The western hemisphere is representative, the north is up. The Pangee has just split, forming Laurasia to the north and Gondwana to the south. This is how the western hemisphere of the Earth may have appeared 200 million years ago during the Early Jurassic period. North is at the top. During this period continental drift, driven by the massive forces of plate tectonics, had just begun to break the supercontinent of Pangea into Laurasia in the north and Gondwana in the south. In this image the nascent North American continent has just broken away from North Africa while South America and the rest of Africa remain joined as Gondwana. To the west in the global Panthalassa ocean are strips of land corresponding to the Wrangellia Terrane which later merged with western North America

Walter B Myers

PIX4633329

Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003

Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003

Sebastian Voltmer

PIX4626631

The planet Saturn observed with the Hubble space telescope in October 1997. Saturn is 120,000 km in diameter -: The planet Saturn seen by the Hubble space telescope in 1997 - Saturn seen from the Hubble space telescope in october 1997

The planet Saturn observed with the Hubble space telescope in October 1997. Saturn is 120,000 km in diameter -: The planet Saturn seen by the Hubble space telescope in 1997 - Saturn seen from the Hubble space telescope in october 1997

PIX4624811

Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. Nasa's Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however - when intense enough - they can disturb the atmosphere in the layer where GPS and communications signals travel

Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. Nasa's Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however - when intense enough - they can disturb the atmosphere in the layer where GPS and communications signals travel

PIX4627273

La terre vue par Apollo 17 - Earth seen by Apollo 17 - La terre vue par Apollo 17 le 7 décembre 1972. View of the Earth as seen by the Apollo 17 crew traveling towards the moon. December 7 1972

La terre vue par Apollo 17 - Earth seen by Apollo 17 - La terre vue par Apollo 17 le 7 décembre 1972. View of the Earth as seen by the Apollo 17 crew traveling towards the moon. December 7 1972

PIX4632131

Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Astronomical Union (IAU) at Cambridge, Massachusetts, USA, which acts as a central clearing house for asteroid and comet observations. The measurements collected there are retrieved by the European Small Bodies Data Centre; orbits and miss distances are computed. In case of high-risk impact predictions, the data will be cross-checked with NASA's SENTRY system, operated by the Jet Propulsion Laboratory (JPL), California, before issuing alerts — Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Ast

Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Ast

P. Carril

PIX4583884

Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune. Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites — Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete

Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete

Walter B Myers

PIX4633164

Titan - Illustration - Saturn's satellite Titan - Artist's view of Titan, Saturn's largest satellite. Titan is Saturn's largest satellite and the second - largest satellite in the Solar System (just slightly smaller than Jupiter's Ganymede). Although Titan orbits Saturn, it is still larger than the planet Mercury and has the most substantial atmosphere of any satellite in the Solar System

Titan - Illustration - Saturn's satellite Titan - Artist's view of Titan, Saturn's largest satellite. Titan is Saturn's largest satellite and the second - largest satellite in the Solar System (just slightly smaller than Jupiter's Ganymede). Although Titan orbits Saturn, it is still larger than the planet Mercury and has the most substantial atmosphere of any satellite in the Solar System

Walter B Myers

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Le Soleil en maximum solaire - The Sun seen by SDO - Composite - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) from February 11, 2013 to February 11, 2014. Image composed of 25 different images, illustrating the sun in high activity. This image is a composite of 25 separate images spanning the period of February 11, 2013 to February 11, 2014. It uses the SDO AIA wavelength of 304 Angstroms and reveals the zones on the sun where active regions and associated eruptions most commonly occur during Solar Maximum

Le Soleil en maximum solaire - The Sun seen by SDO - Composite - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) from February 11, 2013 to February 11, 2014. Image composed of 25 different images, illustrating the sun in high activity. This image is a composite of 25 separate images spanning the period of February 11, 2013 to February 11, 2014. It uses the SDO AIA wavelength of 304 Angstroms and reveals the zones on the sun where active regions and associated eruptions most commonly occur during Solar Maximum

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Jupiter seen by the Hubble Space Telescope

Jupiter seen by the Hubble Space Telescope

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

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

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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

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Earth and Sun - artist view - Earth and Sun - Artwor

Earth and Sun - artist view - Earth and Sun - Artwor

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

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

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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

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Mars - Illustration - Artist's view of Mars Planet. This detailed artist's view of the planet Mars, based on high-resolution spacecraft imaging, reveals some of the many craters that cover much of its surface

Mars - Illustration - Artist's view of Mars Planet. This detailed artist's view of the planet Mars, based on high-resolution spacecraft imaging, reveals some of the many craters that cover much of its surface

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Global view of Mars

Global view of Mars

UIG533595

The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (both resulting in global sun - reflecting ash clouds), or variance's in the Earth's orbit — The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (bot

The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (bot

Walter B Myers

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

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

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A geocroiser asteroid passes Jupiter's orbit, 2016 (photo)

A geocroiser asteroid passes Jupiter's orbit, 2016 (photo)

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

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

Jerry Lodriguss

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Uranus photographed by Voyager 2 in January 1986.

Uranus photographed by Voyager 2 in January 1986.

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Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Walter B Myers

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Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

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Neptune et Triton- Illustration - Neptune with its moon Triton Artwork

Neptune et Triton- Illustration - Neptune with its moon Triton Artwork

S. Numazawa

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

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

Sebastian Voltmer

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International Space Station (ISS) 10/2018 (photo)

International Space Station (ISS) 10/2018 (photo)

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Mars - Phobos Satellite - Martian moon Phobos - View of the Phobos satellite obtained by the Mars Express probe in March 2010. The north pole is indicated. Mars Express took this image of the surface of the moon Phobos in March 2010. The resolution is about 9 m/pixel

Mars - Phobos Satellite - Martian moon Phobos - View of the Phobos satellite obtained by the Mars Express probe in March 2010. The north pole is indicated. Mars Express took this image of the surface of the moon Phobos in March 2010. The resolution is about 9 m/pixel

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Opposition de Mars en 2005 - Mars opposition in 2005 - Different views of Mars obtained during its opposition in 2005. Planet Mars images taken during its opposition in 2005

Opposition de Mars en 2005 - Mars opposition in 2005 - Different views of Mars obtained during its opposition in 2005. Planet Mars images taken during its opposition in 2005

Sebastian Voltmer

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

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

Walter B Myers

PIX4630011

Uranus - Illustration - The planet Uranus and its system of rings. This image suggests how Uranus might look from a position in space several hundred thousand miles above its south pole. Like Saturn and Jupiter, Uranus is a Gas Giant, composed primarily of hydrogen and helium gases surrounding a relatively small, dense core of molten rock and metal. Its bluish color is due to the presence of methane in its upper atmosphere. Also like Saturn and Jupiter, Uranus has rings. However Uranus' rings are over three orders of magnitude dimmer than Saturn's; where Saturn's rings are almost white, Uranus' rings are more like the color of charcoal. Uranus 'rings are so dim that they went undetected from 1781, when the English astronomer William Herschel first observed Uranus through a telescope, until 1977 when astronomers watched as a star passing behind Uranus appeared to blink several times, caused by the ten rings surrounding the planet. One bizarre aspect of Uranus is that its axis of rotation is tipped beyond 90 degrees in relation to the plane of its orbit around the Sun. This puts Uranus' north and south poles, relative to the Sun, where the other planets have their equators — Uranus - Illustration - The planet Uranus and its system of rings. This image suggests how Uranus might look from a position in space several hundred thousand miles above its south pole. Like Saturn and Jupiter, Uranus is a Gas Giant, composed primarily of hydrogen and helium gases surrounding a relatively small, dense core of molten rock and metal. Its bluish color is due to the presence of methane in its upper atmosphere. Also like Saturn and Jupiter, Uranus has rings. However Uranus' rings are over three orders of magnitude dimmer than Saturn's; where Saturn's rings are almost white, Uranus' rings are more like the color of charcoal. Uranus 'rings are so dim that they went undetected from 1781, when the English astronomer William Herschel first observed Uranus through a telescope, until 1977 when astronomers watched as a star passing behind Uranus appeared to blink several times, caused by the ten rings surrounding the planet. One bizarre aspect of Uranus is that its axis of rotatio

Uranus - Illustration - The planet Uranus and its system of rings. This image suggests how Uranus might look from a position in space several hundred thousand miles above its south pole. Like Saturn and Jupiter, Uranus is a Gas Giant, composed primarily of hydrogen and helium gases surrounding a relatively small, dense core of molten rock and metal. Its bluish color is due to the presence of methane in its upper atmosphere. Also like Saturn and Jupiter, Uranus has rings. However Uranus' rings are over three orders of magnitude dimmer than Saturn's; where Saturn's rings are almost white, Uranus' rings are more like the color of charcoal. Uranus 'rings are so dim that they went undetected from 1781, when the English astronomer William Herschel first observed Uranus through a telescope, until 1977 when astronomers watched as a star passing behind Uranus appeared to blink several times, caused by the ten rings surrounding the planet. One bizarre aspect of Uranus is that its axis of rotatio

Walter B Myers

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Earth Moon and the Sun - Earth Moon and Sun - Artist's view

Earth Moon and the Sun - Earth Moon and Sun - Artist's view

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Arctic ice has its minimum, September 2018 (photo)

Arctic ice has its minimum, September 2018 (photo)

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Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973

Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973

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Earth and Sun - artist view - Earth and Sun - Artwor

Earth and Sun - artist view - Earth and Sun - Artwor

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Mars - Illustration - Artist's view of Mars Planet Mars with starry sky. Artwork

Mars - Illustration - Artist's view of Mars Planet Mars with starry sky. Artwork

D. Ducros

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Transit of Mercury in front of the Sun, May 9, 2016 (photo)

Transit of Mercury in front of the Sun, May 9, 2016 (photo)

Sebastian Voltmer

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The Earth 600 million years ago - Artist's view - Ediacaran Earth - The Earth seen about 600 million years ago after an important period of glaciation. This is how the Earth may have appeared 600 million years ago following the Cryogenian “” Snowball Earth”” period. The worldwide glaciers have melted and the ocean is largely liquid again. During this, the Ediacaran period, it is hypothesized that all of the Earth's landmasses had merged into a single supercontinent known as Pannotia, also known as the Vendian supercontinent. Surrounding this massive landmass is the vast Panthalassic Ocean, also known as Panthalassa. While the ocean was home to a variety of evolving multicellular life forms including the ubiquitous Dickinsonia costata, it is not believed that life had moved to dry land with possible exception of bacteria and other microbial colonies

The Earth 600 million years ago - Artist's view - Ediacaran Earth - The Earth seen about 600 million years ago after an important period of glaciation. This is how the Earth may have appeared 600 million years ago following the Cryogenian “” Snowball Earth”” period. The worldwide glaciers have melted and the ocean is largely liquid again. During this, the Ediacaran period, it is hypothesized that all of the Earth's landmasses had merged into a single supercontinent known as Pannotia, also known as the Vendian supercontinent. Surrounding this massive landmass is the vast Panthalassic Ocean, also known as Panthalassa. While the ocean was home to a variety of evolving multicellular life forms including the ubiquitous Dickinsonia costata, it is not believed that life had moved to dry land with possible exception of bacteria and other microbial colonies

Walter B Myers

PIX4633308

International Space Station (ISS) 10/2018 (photo)

International Space Station (ISS) 10/2018 (photo)

PIX5973650

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

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

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Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Sinus Sabaeous and Sinus Meridiani along the equator; and the small southern polar cap — Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

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Le Soleil vu par SDO - The Sun seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (20:44:57 UT). Image taken on March 29, 2011 (20:44:57 UT) by Solar Dynamics Observatory (SDO)

Le Soleil vu par SDO - The Sun seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (20:44:57 UT). Image taken on March 29, 2011 (20:44:57 UT) by Solar Dynamics Observatory (SDO)

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The Sun seen by SDO on October 26, 2014 - The Sun seen by SDO - October 26, 2014 - Solar eruption (bright spot below right) seen by SDO (Solar Dynamics Observatory) on October 26, 2014. The bright light in the lower right of the sun shows an X-class solar flare on Oct. 26, 2014, as captured by NASA's SDO. This was the third X-class flare in 48 hours, which erupted from the largest active region seen on the sun in 24 years. This flare was classified as an X2.0-class flare and it peaked at 6:56 a.m. EDT.

The Sun seen by SDO on October 26, 2014 - The Sun seen by SDO - October 26, 2014 - Solar eruption (bright spot below right) seen by SDO (Solar Dynamics Observatory) on October 26, 2014. The bright light in the lower right of the sun shows an X-class solar flare on Oct. 26, 2014, as captured by NASA's SDO. This was the third X-class flare in 48 hours, which erupted from the largest active region seen on the sun in 24 years. This flare was classified as an X2.0-class flare and it peaked at 6:56 a.m. EDT.

PIX4627305

Earth and Moon - Artist view - Earth and Moon. Artwork - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km

Earth and Moon - Artist view - Earth and Moon. Artwork - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km

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Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

D. Ducros

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

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

PIX4624339

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

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

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Jupiter seen by Hubble Space Telescope - Jupiter seen by HST - Image obtained on April 3, 2017 by Hubble Space Telescope. On April 3, 2017, as Jupiter made its nearest approach to Earth in a year, Nasa's Hubble Space Telescope viewed the solar system's largest planet in all of its up-close glory. At a distance of 415 million miles (668 million kilometers) from Earth, Jupiter offered spectacular views of its colorful, roiling atmosphere, the legendary Great Red Spot, and its smaller companion at farther southern latitudes dubbed “” Red Spot Jr.””

Jupiter seen by Hubble Space Telescope - Jupiter seen by HST - Image obtained on April 3, 2017 by Hubble Space Telescope. On April 3, 2017, as Jupiter made its nearest approach to Earth in a year, Nasa's Hubble Space Telescope viewed the solar system's largest planet in all of its up-close glory. At a distance of 415 million miles (668 million kilometers) from Earth, Jupiter offered spectacular views of its colorful, roiling atmosphere, the legendary Great Red Spot, and its smaller companion at farther southern latitudes dubbed “” Red Spot Jr.””

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March -Satellite Phobos - Martian moon Phobos: View of the Phobos satellite obtained by the ExoMars probe on November 26, 2016, at a distance of 7700 km from the satellite. Colour composite of Phobos taken with the ExoMars orbiter's Colour and Stereo Surface Imaging System (Cassis) on 26 November 2016. The observation was made at a distance of 7700 km and yields a resolution of 87 m/pixel

March -Satellite Phobos - Martian moon Phobos: View of the Phobos satellite obtained by the ExoMars probe on November 26, 2016, at a distance of 7700 km from the satellite. Colour composite of Phobos taken with the ExoMars orbiter's Colour and Stereo Surface Imaging System (Cassis) on 26 November 2016. The observation was made at a distance of 7700 km and yields a resolution of 87 m/pixel

PIX4616732

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the highest possible detail when Nasa's New Horizons probe flies by Pluto in 2015. The Hubble images are a few pixels wide. But through a technique called dithering, multiple, slightly offset pictures can be combined through computer - image processing to synthesize a higher - resolution view than could be seen in a single exposure. This series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish — Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

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

PIX4624317

Uranus and its satellite Puck - Illustration - Uranus from Puck orbit - Illustration - The planet Uranus seen from the orbit of its small satellite Puck. This is how Uranus and its tiny satellite Puck might look from a position in orbit around Puck. Puck in turn orbits Uranus at a height of 37 thousand miles above Uranus' cloud tops, completing one orbit in about 18 hours. Due to the fact that Puck's orbit is on the same plane as Uranus' rings, they would appear as little more than a thin line from this vantage punin

Uranus and its satellite Puck - Illustration - Uranus from Puck orbit - Illustration - The planet Uranus seen from the orbit of its small satellite Puck. This is how Uranus and its tiny satellite Puck might look from a position in orbit around Puck. Puck in turn orbits Uranus at a height of 37 thousand miles above Uranus' cloud tops, completing one orbit in about 18 hours. Due to the fact that Puck's orbit is on the same plane as Uranus' rings, they would appear as little more than a thin line from this vantage punin

Walter B Myers

PIX4634804

Variation of solar activity - Solar activity - The Sun in minimum activity on the left (March 18, 2009), without any solar spot, and near its solar maximum on the right (July 19, 2000) where many sunspots are present on its surface. Images obtained by the SOHO satellite. A comparison of the Sun near the minimum of its activity with none sunspot (left, on March 18, 2009) and near its maximum at right on July 19, 2000. Images taken by SOHO spacecraft

Variation of solar activity - Solar activity - The Sun in minimum activity on the left (March 18, 2009), without any solar spot, and near its solar maximum on the right (July 19, 2000) where many sunspots are present on its surface. Images obtained by the SOHO satellite. A comparison of the Sun near the minimum of its activity with none sunspot (left, on March 18, 2009) and near its maximum at right on July 19, 2000. Images taken by SOHO spacecraft

PIX4627025

Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the highest possible detail when Nasa's New Horizons probe flies by Pluto in 2015. The Hubble images are a few pixels wide. But through a technique called dithering, multiple, slightly offset pictures can be combined through computer - image processing to synthesize a higher - resolution view than could be seen in a single exposure. This series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish — Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will b

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

PIX4624313

Le Soleil vu by SDO on September 19, 2010 - The Sun seen by SDO. September 19, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on September 19, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on September 19, 2010

Le Soleil vu by SDO on September 19, 2010 - The Sun seen by SDO. September 19, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on September 19, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on September 19, 2010

PIX4627212

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 in order of their discovery rather than their position around Saturn.) The rings also cast a shadow on Saturn at the limb of the planet in the lower right quadrant — 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

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Transit of Venus in front of the Sun seen by the SDO satellite, 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 - Transit of Venus in front of the Sun seen by the SDO satellite, 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

PIX4588480

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Transit of Venus in front of the Sun seen by the SDO satellite, 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 - Transit of Venus in front of the Sun seen by the SDO satellite, 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

PIX4588459

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color mosaic. This image was acquired on Feb. 24, 2007, while the spacecraft was 1.58 million kilometers (1 million miles) from the planet and 34.6 degrees above the ring plane. The solar phase angle was 69.5 degrees. In this view, Cassini was looking down on the northern, unlit side of the rings, which are rendered visible by sunlight filtering through from the sunlit, southern face. On the night side (right side of image), with no sunlight, Saturn's own thermal radiation lights things up. This light at 5.1 microns wavelength (some seven times the longest wavelength visible to the human eye) is generated deep within Saturn, and works its way upward, eventually escaping into space. Thick clouds deep in the atmosphere block that light. An amazing array of dark streaks, spots, and globe - encircling bands is visible instead. Saturn's strong thermal glow at 5.1 microns even allows these deep clouds to be seen on portions of the dayside (left side), especially where overlying h — Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

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

PIX4624969

Le Soleil en H - Alpha - 21/06/2004 - The Sun - June 21, 2004 - Le Soleil vu le 21 juin 2004. The image shows sunspots, protuberances and a very active region near the center of the image (AR 10652). The Sun on June 21, 2004. The image shows sunspots, filaments, prominences and a very active region (AR 10652) near the center of the sun

Le Soleil en H - Alpha - 21/06/2004 - The Sun - June 21, 2004 - Le Soleil vu le 21 juin 2004. The image shows sunspots, protuberances and a very active region near the center of the image (AR 10652). The Sun on June 21, 2004. The image shows sunspots, filaments, prominences and a very active region (AR 10652) near the center of the sun

Stefan Seip

PIX4626697

The stages of Earth formation - Artist view - Earth formation - Artist view - The Earth was formed 4.5 billion years ago from a gigantic cloud of gas and dust. From microscopic grains, planetesimal form, clash and agglomerate to form our planet; it was then subjected to a large bombardment of meteorites bringing a significant share of the water to Earth. Earth formed 4.54 billion years ago from a large protoplanetary disk accreting. The proto earth was bombarded by planetoids heating the newly formed planet

The stages of Earth formation - Artist view - Earth formation - Artist view - The Earth was formed 4.5 billion years ago from a gigantic cloud of gas and dust. From microscopic grains, planetesimal form, clash and agglomerate to form our planet; it was then subjected to a large bombardment of meteorites bringing a significant share of the water to Earth. Earth formed 4.54 billion years ago from a large protoplanetary disk accreting. The proto earth was bombarded by planetoids heating the newly formed planet

PIX4633396

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. In red, the coldest regions, in blue and green, the warmer regions. SDO (Solar Dynamics Observatory) First Light Image. A full - disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F)

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. In red, the coldest regions, in blue and green, the warmer regions. SDO (Solar Dynamics Observatory) First Light Image. A full - disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F)

PIX4627139

Le Soleil vu en ultraviolet by SOHO on 18/11/2009 - The Sun seen in ultraviolet by Soho. November 18, 2009 - A protuberance, a plasma cloud, escapes from the Sun. White areas are the hottest and most active areas. Prominences are cooler clouds of gases suspended above the Sun by magnetic forces

Le Soleil vu en ultraviolet by SOHO on 18/11/2009 - The Sun seen in ultraviolet by Soho. November 18, 2009 - A protuberance, a plasma cloud, escapes from the Sun. White areas are the hottest and most active areas. Prominences are cooler clouds of gases suspended above the Sun by magnetic forces

PIX4627010

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

PIX4627209

Transit from Venus in front of the Sun. 08/06/2004 - Venus Transit. 08/06/2004 - Seen with H-Alpha filter. Venus seen in front of Sun with a H-alpha filter

Transit from Venus in front of the Sun. 08/06/2004 - Venus Transit. 08/06/2004 - Seen with H-Alpha filter. Venus seen in front of Sun with a H-alpha filter

Stefan Seip

PIX4588390

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

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

PIX4583550

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

Earth - The geoid - Earth's geoid - The Earth's geoid, an image of the inegalites of the Earth's gravitation field. Image centred on Indonesia. Image obtained by the GOCE satellite in 2011. ESA's GOCE mission has delivered the most accurate model of the 'geoid' ever produced, which will be used to further our understanding of how Earth works. A precise model of Earth's geoid is crucial for deriving accurate measurements of ocean circulation, sea - level change and terrestrial ice dynamics. The geoid is also used as a reference surface from which to map the topographical features on the planet. In addition, a better understanding of variations in the gravity field will lead to a deeper understanding of Earth's interior, such as the physics and dynamics associated with volcanic activity and earthquakes

Earth - The geoid - Earth's geoid - The Earth's geoid, an image of the inegalites of the Earth's gravitation field. Image centred on Indonesia. Image obtained by the GOCE satellite in 2011. ESA's GOCE mission has delivered the most accurate model of the 'geoid' ever produced, which will be used to further our understanding of how Earth works. A precise model of Earth's geoid is crucial for deriving accurate measurements of ocean circulation, sea - level change and terrestrial ice dynamics. The geoid is also used as a reference surface from which to map the topographical features on the planet. In addition, a better understanding of variations in the gravity field will lead to a deeper understanding of Earth's interior, such as the physics and dynamics associated with volcanic activity and earthquakes

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Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft - Comparison of the two hemispheres of Japet, a satellite of Saturn of 1471 kilometres in diameter. Its main feature is the color difference between the two hemispheres. On the left, the dark region called Cassini Regio with to the east the largest crater of Japet, named Turgis (580 km in diameter). On the right, the bright side of the satellite with Roncevaux Terra (north) and Saragossa Terra (south) housing the large impact crater Engelier (504 km in diameter). Both images were obtained by the Cassini probe on 10 September 2007 (right) and 27 December 2004 (left). These two global images of Iapetus show the extreme brightness dichotomy on the surface of this peculiar Saturnian moon. The left - hand panel shows the moon's leading hemisphere and the right - hand panel shows the moon's trailing side. While low and mid latitudes of the leading side exhibit a surface almost as dark as charcoal, broad tracts of the trailing side are almost as bright as snow. The dark terrain covers about 40 percent of the surface and is named Cassini Regio. The names of the bright terrain are Roncesvaux Terra (north) and Saragossa Terra (south). On both hemispheres, the dominant landforms are impact craters. The largest known well - preserved basin on Iapetus, called Turgis, has a diameter of about 580 kilometers (360 miles). It lies at 17 degrees north latitude, 28 degrees west longitude at the eastern edge of the dark Cassini Regio and is visible on the right side of the left - hand panel. The prominent basin on the southern trailing side (at the lower left of the right - hand panel) is Engelier. Engelier is located at 41 degrees south latitude, 265 degrees west longitude, and has a diameter of about 504 kilometers (313 miles). Its formation destroyed about half of Gerin, another large basin on Iapetus. Gerin is located at 46 degrees south latitude, 233 degrees — Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft - Comparison of the two hemispheres of Japet, a satellite of Saturn of 1471 kilometres in diameter. Its main feature is the color difference between the two hemispheres. On the left, the dark region called Cassini Regio with to the east the largest crater of Japet, named Turgis (580 km in diameter). On the right, the bright side of the satellite with Roncevaux Terra (north) and Saragossa Terra (south) housing the large impact crater Engelier (504 km in diameter). Both images were obtained by the Cassini probe on 10 September 2007 (right) and 27 December 2004 (left). These two global images of Iapetus show the extreme brightness dichotomy on the surface of this peculiar Saturnian moon. The left - hand panel shows the moon's leading hemisphere and the right - hand panel shows the moon's trailing side. While low and mid latitudes of the leading side exhibit a surface almost as dark as charcoal,

Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft - Comparison of the two hemispheres of Japet, a satellite of Saturn of 1471 kilometres in diameter. Its main feature is the color difference between the two hemispheres. On the left, the dark region called Cassini Regio with to the east the largest crater of Japet, named Turgis (580 km in diameter). On the right, the bright side of the satellite with Roncevaux Terra (north) and Saragossa Terra (south) housing the large impact crater Engelier (504 km in diameter). Both images were obtained by the Cassini probe on 10 September 2007 (right) and 27 December 2004 (left). These two global images of Iapetus show the extreme brightness dichotomy on the surface of this peculiar Saturnian moon. The left - hand panel shows the moon's leading hemisphere and the right - hand panel shows the moon's trailing side. While low and mid latitudes of the leading side exhibit a surface almost as dark as charcoal,

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Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

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Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

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Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) caught the action in dramatic detail in extreme ultraviolet light of Helium. It had been almost a million km long ((about half a solar radius) and a prominent feature on the Sun visible over two weeks ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) caught the action in dramatic detail in extreme ultraviolet light of Helium. It had been almost a million km long ((about half a solar radius) and a prominent feature on the Sun visible over two weeks ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

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Le Soleil vu par SDO le 2 mars 2012 - The Sun seen by SDO - March 2012 - Solar eruption seen in ultraviolet by SDO (Solar Dynamics Observatory) on 2 mars 2012. On March 2, 2012, a giant eruption of solar material exploded up off the surface of the right side of the sun, as captured in this image from Nasa's Solar Dynamics Observatory. Known as a prominence eruption, most of the material usually falls right back down on to the sun

Le Soleil vu par SDO le 2 mars 2012 - The Sun seen by SDO - March 2012 - Solar eruption seen in ultraviolet by SDO (Solar Dynamics Observatory) on 2 mars 2012. On March 2, 2012, a giant eruption of solar material exploded up off the surface of the right side of the sun, as captured in this image from Nasa's Solar Dynamics Observatory. Known as a prominence eruption, most of the material usually falls right back down on to the sun

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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

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Full Moon - Full Moon

Full Moon - Full Moon

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Solar eruption - The Sun seen by SDO: Coronal rain (right) during an eruption on the surface of the Sun, ultraviolet view by SDO (Solar Dynamics Observatory) on July 19, 2012. On July 19, 2012, an eruption occurred on the sun that produced a moderately powerful solar flare and a dazzling magnetic display known as coronal rain. Hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, and outlining the fields as it slowly falls back to the solar surface

Solar eruption - The Sun seen by SDO: Coronal rain (right) during an eruption on the surface of the Sun, ultraviolet view by SDO (Solar Dynamics Observatory) on July 19, 2012. On July 19, 2012, an eruption occurred on the sun that produced a moderately powerful solar flare and a dazzling magnetic display known as coronal rain. Hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, and outlining the fields as it slowly falls back to the solar surface

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

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

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Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 19, 1986. On the left, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the same image seen in false colors.The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two images of Uranus are shown here to reveal the pole rotation of the planet, as photographed by Voyager 2. The left is seen as the human eye would see, and the right isfalse color to reveal more intricate details

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 19, 1986. On the left, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the same image seen in false colors.The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two images of Uranus are shown here to reveal the pole rotation of the planet, as photographed by Voyager 2. The left is seen as the human eye would see, and the right isfalse color to reveal more intricate details

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

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

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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

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The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

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Data obtained by the Mars Global Surveyor probe in 2000 - High resolution topographic shaded relief map of Mars made from Mars Global Surveyor observations: Altimetric map of Mars - Mars shaded relief map

Data obtained by the Mars Global Surveyor probe in 2000 - High resolution topographic shaded relief map of Mars made from Mars Global Surveyor observations: Altimetric map of Mars - Mars shaded relief map

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Uranus and its satellite Puck - Illustration - Uranus and Puck - Illustration - Planet Uranus with its Puck satellite in the foreground. On the right, closer to the planet, is the Belinda satellite. Even closer to Uranus, on the left, the Portia satellite. On Uranus, a giant storm is represented. This is how Uranus and its tiny satellite Puck might look from a position in space about a thousand miles above and beyond Puck itself. With a diameter of about 100 miles, Puck is the largest and outermost of the ten known “” inner”” satellites that orbit Uranus within a radius of 51 thousand miles. Further in toward Uranus on the right is Belinda, a satellite that is about 40 miles in diameter. Even closer to Uranus on the far left is the 60 - mile - diameter satellite Portia. On Uranus itself can be seen a giant, cyclonic storm that's almost as big as the Earth

Uranus and its satellite Puck - Illustration - Uranus and Puck - Illustration - Planet Uranus with its Puck satellite in the foreground. On the right, closer to the planet, is the Belinda satellite. Even closer to Uranus, on the left, the Portia satellite. On Uranus, a giant storm is represented. This is how Uranus and its tiny satellite Puck might look from a position in space about a thousand miles above and beyond Puck itself. With a diameter of about 100 miles, Puck is the largest and outermost of the ten known “” inner”” satellites that orbit Uranus within a radius of 51 thousand miles. Further in toward Uranus on the right is Belinda, a satellite that is about 40 miles in diameter. Even closer to Uranus on the far left is the 60 - mile - diameter satellite Portia. On Uranus itself can be seen a giant, cyclonic storm that's almost as big as the Earth

Walter B Myers

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Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

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Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The bright clouds immediately to the south and east of this oval are seen to substantially change their appearances in periods as short as four hours. The second dark spot, at 54 degrees south latitude near the terminator (lower right edge), Neptune circuits every 16.1 hours. This image has been processed to enchance the visibility of small features, at some sacrifice of color fidelity — Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

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

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

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Mercury Transit in front of the Sun. May 9, 2016 - Mercury Transit. May 9, 2016: The planet Mercury (black dot on the left) passes in front of the Sun. May 9, 2016 - Mercury is located at left as a small, dark, round spot

Mercury Transit in front of the Sun. May 9, 2016 - Mercury Transit. May 9, 2016: The planet Mercury (black dot on the left) passes in front of the Sun. May 9, 2016 - Mercury is located at left as a small, dark, round spot

Sebastian Voltmer

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Solar eruption seen by Skylab - Solar prominence seen by Skylab - Ultraviolet view of the Sun obtained from Skylab Station in December 1973. Ultraviolet image of a giant loop prominence on the Sun, recorded by the Skylab space station on December 19, 197

Solar eruption seen by Skylab - Solar prominence seen by Skylab - Ultraviolet view of the Sun obtained from Skylab Station in December 1973. Ultraviolet image of a giant loop prominence on the Sun, recorded by the Skylab space station on December 19, 197

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Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) caught the action in dramatic detail in extreme ultraviolet light of Helium. It had been almost a million km long ((about half a solar radius) and a prominent feature on the Sun visible over two weeks ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) caught the action in dramatic detail in extreme ultraviolet light of Helium. It had been almost a million km long ((about half a solar radius) and a prominent feature on the Sun visible over two weeks ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

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Planet Formation - Artist View - Planet Birth - Artist view - Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A new born planet in a star's dusty, planet - forming disc

Planet Formation - Artist View - Planet Birth - Artist view - Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A new born planet in a star's dusty, planet - forming disc

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