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

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

PIX4643593

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury, and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. On his 7-year journey, the probe will pass twice near Venus.

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled for October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury, and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. On his 7-year journey, the probe will pass twice near Venus.

PIX4643590

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

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

PIX4643601

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

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

PIX4643577

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

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

PIX4643569

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

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

PIX4643632

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

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

PIX4643574

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

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

PIX4643573

Montage of images relating to the space shuttle (gouache on paper)

Montage of images relating to the space shuttle (gouache on paper)

Hardy, Wilf (Wilfred) (20th century)

LAL724436

Solar Orbiter (photo)

Solar Orbiter (photo)

PIX6039538

Enhanced-color image of Phobos from the Mars

Enhanced-color image of Phobos from the Mars

UIG3519930

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

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

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

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

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

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

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

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Martian dune erosion - Mars: Disappearing and Shrinking Dome Dunes - Dune sur Mars photographed by the HIRISE camera of the Mars Reconnaissance probe orbiting on January 30, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This false - color image from the HIRISE (High Resolution Imaging Science Experiment) camera on Mars Recognition Orbiter was taken on January 30, 2008

Martian dune erosion - Mars: Disappearing and Shrinking Dome Dunes - Dune sur Mars photographed by the HIRISE camera of the Mars Reconnaissance probe orbiting on January 30, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This false - color image from the HIRISE (High Resolution Imaging Science Experiment) camera on Mars Recognition Orbiter was taken on January 30, 2008

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

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

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Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

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LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

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Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

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LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

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The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

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Full Moon - Full Moon

Full Moon - Full Moon

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Martian dunes at the end of winter - March: Late Winter view of Dunes: Detail on dunes in the southern hemisphere of Mars. With the end of winter, the Sun melts the carbon dioxide ice present all winter. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on March 21, 2016. HIRISE is a 50 cm telescope that observes visible and near infrared. Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. It is now late winter here in the Southern hemisphere, and these dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide. Spots form where pressurized carbon dioxide gas escapes to the surface

Martian dunes at the end of winter - March: Late Winter view of Dunes: Detail on dunes in the southern hemisphere of Mars. With the end of winter, the Sun melts the carbon dioxide ice present all winter. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on March 21, 2016. HIRISE is a 50 cm telescope that observes visible and near infrared. Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. It is now late winter here in the Southern hemisphere, and these dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide. Spots form where pressurized carbon dioxide gas escapes to the surface

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Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

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Sunrise on the crater Tycho - Tycho Crater Sunrise - Sunrise on the central peak of the crater Tycho on the Moon. This crater is about 82 km in diameter and its central peak rises at 2 km above sea level. Image obtained on June 10, 2011 by the LRO (Lunar Reconnaissance Orbiter) probe. On 10 June 2011 the LRO spacecraft slewed 65* to the west, allowing the LROC NACs to capture this dramatic sunrise view of Tycho crater. A very popular target with amateur astronomers, Tycho is located at 43.37* S, 348.68* E, and is ~ 82 km (51 miles) in diameter. The summit of the central peak is 2 km (6562 ft) above the crater floor, and the crater floor is about 4700 m (15,420 ft) below the rim. Many “” clasts”” ranging in size from 10 meters to 100s of meters are exposed in the central peak slopes

Sunrise on the crater Tycho - Tycho Crater Sunrise - Sunrise on the central peak of the crater Tycho on the Moon. This crater is about 82 km in diameter and its central peak rises at 2 km above sea level. Image obtained on June 10, 2011 by the LRO (Lunar Reconnaissance Orbiter) probe. On 10 June 2011 the LRO spacecraft slewed 65* to the west, allowing the LROC NACs to capture this dramatic sunrise view of Tycho crater. A very popular target with amateur astronomers, Tycho is located at 43.37* S, 348.68* E, and is ~ 82 km (51 miles) in diameter. The summit of the central peak is 2 km (6562 ft) above the crater floor, and the crater floor is about 4700 m (15,420 ft) below the rim. Many “” clasts”” ranging in size from 10 meters to 100s of meters are exposed in the central peak slopes

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

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

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The large galaxy in Andromeda, Messier 31. The Andromeda galaxy is the most massive in the local group of galaxies that includes our Milky Way. Andromeda is the nearest large galaxy to our own. GALEX Orbiter.

The large galaxy in Andromeda, Messier 31. The Andromeda galaxy is the most massive in the local group of galaxies that includes our Milky Way. Andromeda is the nearest large galaxy to our own. GALEX Orbiter.

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The spiral galaxy known as Messier 81, or M81. GALEX Orbiter,Hubble Space Telescope,Spitzer Space Telescope.

The spiral galaxy known as Messier 81, or M81. GALEX Orbiter,Hubble Space Telescope,Spitzer Space Telescope.

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Jupiter's south polar region, 2017

Jupiter's south polar region, 2017

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LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

LRO Probe - Artist View - LRO - Artist view - Lunar Reconnaissance Orbiter (LRO) is a space probe of NASA that will be put into orbit around the Moon in order to map it and identify potential landing sites for sending a human crew around 2020. LRO is expected to be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite). Lunar Reconnaissance Orbiter (LRO) in Moon orbit. LRO objectives are to find safe landing sites, locate potential resources, characterize the radiation environment, and demonstrate new technology to prepare future human exploration of the Moon. It should be launched in June 2009 with LCROSS (Lunar Crater Observation and Sensing Satellite) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida

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Nili Patera; one of the most active dune fields on Mars, 2014

Nili Patera; one of the most active dune fields on Mars, 2014

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Premier quartier de Lune - Moon first quarter - First district of Moon seen by the LRO probe. Moon first quarter seen by LRO spacecraft

Premier quartier de Lune - Moon first quarter - First district of Moon seen by the LRO probe. Moon first quarter seen by LRO spacecraft

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Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

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Liftoff Of Space Shuttle Discovery 51A. 11/84.

Liftoff Of Space Shuttle Discovery 51A. 11/84.

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

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

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Mosaic of the visible face of the Moon by the probe LRO - High resolution mosaic of the lunar nearside by LRO - Spectacular mosaic of 1300 images obtained during two weeks mid-December 2010 by the probe LRO. The resolution is 145 meters per pixel. For two weeks in mid - December 2010, the LRO spacecraft remained nadir looking (straight down) so that the LROC Wide Angle Camera (WAC) could acquire about 1300 images, allowing the LROC team to construct this spectacular mosaic

Mosaic of the visible face of the Moon by the probe LRO - High resolution mosaic of the lunar nearside by LRO - Spectacular mosaic of 1300 images obtained during two weeks mid-December 2010 by the probe LRO. The resolution is 145 meters per pixel. For two weeks in mid - December 2010, the LRO spacecraft remained nadir looking (straight down) so that the LROC Wide Angle Camera (WAC) could acquire about 1300 images, allowing the LROC team to construct this spectacular mosaic

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Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

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The unusual stone mesas of the Cydonia region on Mars are quite striking in appearance. This mesa, when lit from just the right sun angle, can appear similar to a human face and became famous as the Face on Mars in 1976 Viking orbiter images.

The unusual stone mesas of the Cydonia region on Mars are quite striking in appearance. This mesa, when lit from just the right sun angle, can appear similar to a human face and became famous as the Face on Mars in 1976 Viking orbiter images.

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The spiral galaxy known as Messier 81, or M81. GALEX Orbiter,Hubble Space Telescope,Spitzer Space Telescope.

The spiral galaxy known as Messier 81, or M81. GALEX Orbiter,Hubble Space Telescope,Spitzer Space Telescope.

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Mars Recognition Orbiter and the Comet, Artist view (photo)

Mars Recognition Orbiter and the Comet, Artist view (photo)

Steven Hobbs

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North pole of the Moon seen by the LRO - North pole of the Moon - Mosaic probe of 281 images obtained in 2010 by the LRO probe. LROC collected 281 WAC images during a lunar northern summer month to provide this complete picture of the polar region

North pole of the Moon seen by the LRO - North pole of the Moon - Mosaic probe of 281 images obtained in 2010 by the LRO probe. LROC collected 281 WAC images during a lunar northern summer month to provide this complete picture of the polar region

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Spider-shaped features in the south polar region of Mars are carved by vaporizing dry ice in a dynamic seasonal process. Mars Reconnaissance Orbiter.

Spider-shaped features in the south polar region of Mars are carved by vaporizing dry ice in a dynamic seasonal process. Mars Reconnaissance Orbiter.

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Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

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Earthrise and Moon seen since LRO. 10/2015 - Earthrise and Moon as seen from LRO. 10/2015 - Earthrise above the Moon seen from Lunar Reconnaissance Orbiter (LRO). Composite of images obtained on October 12, 2015. Nasa's Lunar Reconnaissance Orbiter (LRO) captured a unique view of Earth from the spacecraft's vantage point in orbit around the moon. In this composite image we see Earth appear to rise over the lunar horizon from the viewpoint of the spacecraft, with the center of the Earth just off the coast of Liberia (at 4.04 degrees North, 12.44 degrees West). The large tan area in the upper right is the Sahara Desert, and just beyond is Saudi Arabia. The Atlantic and Pacific coasts of South America are visible to the left. On the moon, we get a glimpse of the crater Compton, which is located just beyond the eastern limb of the moon, on the lunar farside. LRO was launched on June 18, 2009, and has collected a treasure trove of data with its seven powerful instruments, making an invaluab

Earthrise and Moon seen since LRO. 10/2015 - Earthrise and Moon as seen from LRO. 10/2015 - Earthrise above the Moon seen from Lunar Reconnaissance Orbiter (LRO). Composite of images obtained on October 12, 2015. Nasa's Lunar Reconnaissance Orbiter (LRO) captured a unique view of Earth from the spacecraft's vantage point in orbit around the moon. In this composite image we see Earth appear to rise over the lunar horizon from the viewpoint of the spacecraft, with the center of the Earth just off the coast of Liberia (at 4.04 degrees North, 12.44 degrees West). The large tan area in the upper right is the Sahara Desert, and just beyond is Saudi Arabia. The Atlantic and Pacific coasts of South America are visible to the left. On the moon, we get a glimpse of the crater Compton, which is located just beyond the eastern limb of the moon, on the lunar farside. LRO was launched on June 18, 2009, and has collected a treasure trove of data with its seven powerful instruments, making an invaluab

PIX4577425

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

PIX4616482

This canyon system, Valles Marineris, was named in honor of its discoverer, Mariner 9. Melas Chasma is shown in the image.

This canyon system, Valles Marineris, was named in honor of its discoverer, Mariner 9. Melas Chasma is shown in the image.

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This image from NASA's Mars Reconnaissance Orbiter shows channels to the southeast of Hale crater on southern Mars.

This image from NASA's Mars Reconnaissance Orbiter shows channels to the southeast of Hale crater on southern Mars.

UIG866536

This stereo view shows fractured mounds on the southern edge of Elysium Planitia on Mars. Mars Reconnaissance Orbiter.

This stereo view shows fractured mounds on the southern edge of Elysium Planitia on Mars. Mars Reconnaissance Orbiter.

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It is northern summer on Mars and clouds are very common over the famous Tharsis volcanoes during the afternoon. Mars Global Surveyor Orbiter.

It is northern summer on Mars and clouds are very common over the famous Tharsis volcanoes during the afternoon. Mars Global Surveyor Orbiter.

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This image is of an eroded mesa made famous by its similarity to a human face. Mars Reconnaissance Orbiter spacecraft.

This image is of an eroded mesa made famous by its similarity to a human face. Mars Reconnaissance Orbiter spacecraft.

UIG866499

This Mars Global Surveyor Mars Orbiter Camera view of the red planet shows the region that includes Ares Vallis and the Chryse Plains upon which both Mars Pathfinder and the Viking 1 landed in 1997 and 1976, respectively.

This Mars Global Surveyor Mars Orbiter Camera view of the red planet shows the region that includes Ares Vallis and the Chryse Plains upon which both Mars Pathfinder and the Viking 1 landed in 1997 and 1976, respectively.

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Twelve orbits a day provide the Mars Global Surveyor MOC wide angle cameras a global "snapshot" of weather patterns across the planet.

Twelve orbits a day provide the Mars Global Surveyor MOC wide angle cameras a global "snapshot" of weather patterns across the planet.

UIG866507

This image covers the northern edge of the largest volcano in the solar system, Olympus Mons on Mars. Mars Reconnaissance Orbiter.

This image covers the northern edge of the largest volcano in the solar system, Olympus Mons on Mars. Mars Reconnaissance Orbiter.

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Mosaic of the face of the Moon by the probe LRO - High resolution mosaic of the lunar farside by LRO - Spectacular mosaic of 15000 images obtained between November 2009 and February 2011 by the probe LRO. The resolution is 100 meters per pixel. This spectacular mosaic of the lunar farside is a composite of over 15,000 Wide Angle Camera (WAC) images acquired between November 2009 and February 2011 by the LRO spacecraft

Mosaic of the face of the Moon by the probe LRO - High resolution mosaic of the lunar farside by LRO - Spectacular mosaic of 15000 images obtained between November 2009 and February 2011 by the probe LRO. The resolution is 100 meters per pixel. This spectacular mosaic of the lunar farside is a composite of over 15,000 Wide Angle Camera (WAC) images acquired between November 2009 and February 2011 by the LRO spacecraft

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South pole of the Moon seen by the LRO - South pole of the Moon - Mosaic probe of 288 images obtained in 2010 by the LRO probe. As LRO passes over the pole every two hours, the LROC WAC snaps an image, and over a month, images covering the entire polar region are captured (80* S to 90* S). This mosaic contains 288 images taken in one month; you can see where the month began and ended at about 90* E longitude (note how the lighting changed). The rim of Shackleton crater seems to be disjointed. However, if you look closely, you can see that the Sun came from opposite sides for portions of the mosaic, resulting in opposite sides of the crater's wall being illuminated in some images. As the mission progresses, the WAC captures the pole across the full range of seasons

South pole of the Moon seen by the LRO - South pole of the Moon - Mosaic probe of 288 images obtained in 2010 by the LRO probe. As LRO passes over the pole every two hours, the LROC WAC snaps an image, and over a month, images covering the entire polar region are captured (80* S to 90* S). This mosaic contains 288 images taken in one month; you can see where the month began and ended at about 90* E longitude (note how the lighting changed). The rim of Shackleton crater seems to be disjointed. However, if you look closely, you can see that the Sun came from opposite sides for portions of the mosaic, resulting in opposite sides of the crater's wall being illuminated in some images. As the mission progresses, the WAC captures the pole across the full range of seasons

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Mars Global Surveyor Mars Orbiter Camera (MOC) passed over the Apollinaris Patera volcano and captured a patch of bright clouds hanging over its summit.

Mars Global Surveyor Mars Orbiter Camera (MOC) passed over the Apollinaris Patera volcano and captured a patch of bright clouds hanging over its summit.

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View of Earth from an orbit around the moon, 2009

View of Earth from an orbit around the moon, 2009

UIG3585507

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Steven Hobbs

PIX4606683

The main phases of the Moon - Main Lunar phases - Photomontage showing the Moon in first crescent, first quarter, growing gibbeuse, full moon, decrowing gibbeuse, last quarter and last crescent. Composite image of lunar phases

The main phases of the Moon - Main Lunar phases - Photomontage showing the Moon in first crescent, first quarter, growing gibbeuse, full moon, decrowing gibbeuse, last quarter and last crescent. Composite image of lunar phases

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