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Lonar Meteor Impact Crater, India, True Colour Satellite Image. True colour satellite image of Lonar impact structure, India (diameter : 1,83 km). Image taken on 4 November 1992 using LANDSAT data ©Planet Observer/UIG/Leemage

Lonar Meteor Impact Crater, India, True Colour Satellite Image. True colour satellite image of Lonar impact structure, India (diameter : 1,83 km). Image taken on 4 November 1992 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421399

Impact Crater Roter Kamm, Namibia - Roter Kamm impact crater, Namibia - The impact crater of Roter Kamm would have been formed 3.7 million years ago and has a diameter of 2.5 km. False colour image obtained by Landsat-7 satellite. Roter Kamm is a 2,5 km meteorite impact crater with an age estimated to be 3,7 million years. False color image taken by Landsat - 7 satellite

Impact Crater Roter Kamm, Namibia - Roter Kamm impact crater, Namibia - The impact crater of Roter Kamm would have been formed 3.7 million years ago and has a diameter of 2.5 km. False colour image obtained by Landsat-7 satellite. Roter Kamm is a 2,5 km meteorite impact crater with an age estimated to be 3,7 million years. False color image taken by Landsat - 7 satellite

PIX4630666

Apollo 14: the LEM - Apollo 14 Lunar Module on the Moon. Feb 05 1971 - The lunar module of Apollo 14 (“Antares”) on the Moon. 05/02/1971. A front view of the Apollo 14 Lunar Module “” Antares””, which reflects a circular flare caused by the brilliant sun. The unusual ball of light was said by the astronauts to have a jewel - like appearance. At extreme left, the lower slope of Cone Crater can be seen

Apollo 14: the LEM - Apollo 14 Lunar Module on the Moon. Feb 05 1971 - The lunar module of Apollo 14 (“Antares”) on the Moon. 05/02/1971. A front view of the Apollo 14 Lunar Module “” Antares””, which reflects a circular flare caused by the brilliant sun. The unusual ball of light was said by the astronauts to have a jewel - like appearance. At extreme left, the lower slope of Cone Crater can be seen

PIX4597116

Tookoonooka Meteor Impact Crater, Queensland, Australia, True Colour Satellite Image. True colour satellite image of Tookoonooka impact structure, Queensland, Australia (diameter : 55 km). Image taken on 18 July 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

Tookoonooka Meteor Impact Crater, Queensland, Australia, True Colour Satellite Image. True colour satellite image of Tookoonooka impact structure, Queensland, Australia (diameter : 55 km). Image taken on 18 July 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421392

Vredefort Meteor Impact Crater, South Africa, True Colour Satellite Image. True colour satellite image of Vredefort impact structure, South Africa (diameter : 140 km). Composite image of LANDSAT data taken on 7 April 1991 and 30 April 1991 ©Planet Observer/UIG/Leemage

Vredefort Meteor Impact Crater, South Africa, True Colour Satellite Image. True colour satellite image of Vredefort impact structure, South Africa (diameter : 140 km). Composite image of LANDSAT data taken on 7 April 1991 and 30 April 1991 ©Planet Observer/UIG/Leemage

UIG5421400

Impact Crater Roter Kamm, Namibia - Roter Kamm impact crater, Namibia - The impact crater of Roter Kamm would have been formed 3.7 million years ago and has a diameter of 2.5 km. Image obtained from the International Space Station (ISS) on 5 October 2007. Roter Kamm is a 2,5 km meteorite impact crater with an age estimated to be 3,7 million years. Image taken from the International space station (ISS) on October 5, 2007

Impact Crater Roter Kamm, Namibia - Roter Kamm impact crater, Namibia - The impact crater of Roter Kamm would have been formed 3.7 million years ago and has a diameter of 2.5 km. Image obtained from the International Space Station (ISS) on 5 October 2007. Roter Kamm is a 2,5 km meteorite impact crater with an age estimated to be 3,7 million years. Image taken from the International space station (ISS) on October 5, 2007

PIX4630665

Talemzane Meteor Impact Crater, Algeria, True Colour Satellite Image. True colour satellite image of Talemzane impact structure, Algeria (age : 3 million years ; diameter : 1,75 km). Image taken on 3 March 1987 using LANDSAT data ©Planet Observer/UIG/Leemage

Talemzane Meteor Impact Crater, Algeria, True Colour Satellite Image. True colour satellite image of Talemzane impact structure, Algeria (age : 3 million years ; diameter : 1,75 km). Image taken on 3 March 1987 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421404

Wanapitei Lake Meteor Impact Crater, Manitoba, Canada, True Colour Satellite Image. True colour satellite image of Wanapitei Lake impact structure, Ontario, Canada (diameter : 7,5 km). Image taken on 12 May 1987 using LANDSAT data ©Planet Observer/UIG/Leemage

Wanapitei Lake Meteor Impact Crater, Manitoba, Canada, True Colour Satellite Image. True colour satellite image of Wanapitei Lake impact structure, Ontario, Canada (diameter : 7,5 km). Image taken on 12 May 1987 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421411

La Moinerie Lake Meteor Impact Crater, Canada, True Colour Satellite Image. True colour satellite image of La Moinerie Lake impact structure, Canada (diameter : 8 km). Image taken on 24 August 1988 using LANDSAT data ©Planet Observer/UIG/Leemage

La Moinerie Lake Meteor Impact Crater, Canada, True Colour Satellite Image. True colour satellite image of La Moinerie Lake impact structure, Canada (diameter : 8 km). Image taken on 24 August 1988 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421387

Apollo 16: crater Plum and LRV - Apollo 16: view of Plum crater with LRV - View of the crater Plum (40 km in diameter) and the lunar jeep. 21/04/1972. A view of Plum Crater, which was visited by the two Moon - exploring crew members of the Apollo 16 lunar landing mission, on their first extravehicular activity (EVA - 1) traverse. The Lunar Roving Vehicle (LRV) is parked on the far side of the crater, which measures approximately 40 meters in diameter

Apollo 16: crater Plum and LRV - Apollo 16: view of Plum crater with LRV - View of the crater Plum (40 km in diameter) and the lunar jeep. 21/04/1972. A view of Plum Crater, which was visited by the two Moon - exploring crew members of the Apollo 16 lunar landing mission, on their first extravehicular activity (EVA - 1) traverse. The Lunar Roving Vehicle (LRV) is parked on the far side of the crater, which measures approximately 40 meters in diameter

PIX4597515

Wolf Creek Meteor Impact Crater, Australia, True Colour Satellite Image. True colour satellite image of Wolf Creek impact structure, Australia (age : 300 000 years ; diameter : 875 m). Image taken on 27 April 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

Wolf Creek Meteor Impact Crater, Australia, True Colour Satellite Image. True colour satellite image of Wolf Creek impact structure, Australia (age : 300 000 years ; diameter : 875 m). Image taken on 27 April 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421412

Mars: dunes in the crater Endurance - Mars: Endurance crater dunes - Image obtained by the rover Opportunity in August 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This approximate true - color panoramic camera image highlights the reddish - colored dust present in Endurance crater floor. Sinuous tendrils of sand less than 1 meter (3.3 feet) high extend from the main dune field towards the rover. Image made by the martian rover Opportunity in August 2004

Mars: dunes in the crater Endurance - Mars: Endurance crater dunes - Image obtained by the rover Opportunity in August 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This approximate true - color panoramic camera image highlights the reddish - colored dust present in Endurance crater floor. Sinuous tendrils of sand less than 1 meter (3.3 feet) high extend from the main dune field towards the rover. Image made by the martian rover Opportunity in August 2004

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Apollo 17: Lunar Jeep on the Moon - Apollo 17: Lunar Roving Vehicle on the Moon - Lunar Jeep (LRV) parking near a big rock. 13/12/1972. This view shows the Lunar Roving Vehicle (LRV) parked by an outcrop of rocks by astronauts Eugene A. Cernan and Harrison H. (Jack) Schmitt during their visit to extravehicular activity Station 6 (Henry Crater). Dec 13 197

Apollo 17: Lunar Jeep on the Moon - Apollo 17: Lunar Roving Vehicle on the Moon - Lunar Jeep (LRV) parking near a big rock. 13/12/1972. This view shows the Lunar Roving Vehicle (LRV) parked by an outcrop of rocks by astronauts Eugene A. Cernan and Harrison H. (Jack) Schmitt during their visit to extravehicular activity Station 6 (Henry Crater). Dec 13 197

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Tin Bider Meteor Impact Crater, Algeria, True Colour Satellite Image. True colour satellite image of Tin Bider impact structure, Algeria (age : 70 million years ; diameter : 6 km). Image taken on 19 February 1988 using LANDSAT data ©Planet Observer/UIG/Leemage

Tin Bider Meteor Impact Crater, Algeria, True Colour Satellite Image. True colour satellite image of Tin Bider impact structure, Algeria (age : 70 million years ; diameter : 6 km). Image taken on 19 February 1988 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421405

Apollo 17: Lunar Jeep on the Moon - Apollo 17: Lunar Roving Vehicle on the Moon - Lunar Jeep (LRV) parking near a big rock. 13/12/1972. This view shows the Lunar Roving Vehicle (LRV) parked by an outcrop of rocks by astronauts Eugene A. Cernan and Harrison H. (Jack) Schmitt during their visit to extravehicular activity Station 6 (Henry Crater). Dec 13 197

Apollo 17: Lunar Jeep on the Moon - Apollo 17: Lunar Roving Vehicle on the Moon - Lunar Jeep (LRV) parking near a big rock. 13/12/1972. This view shows the Lunar Roving Vehicle (LRV) parked by an outcrop of rocks by astronauts Eugene A. Cernan and Harrison H. (Jack) Schmitt during their visit to extravehicular activity Station 6 (Henry Crater). Dec 13 197

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Cratere Manicouagan -Québec- Manicouagan impact crater seen from the space station: Cratere d'impact Manicouagan, Quebec, vu depuis la station spatiale internationale (ISS) on 15/04/2016. This 100 km-diameter crater formed 212 million years ago, following the fall of an asteroid on Earth. - Manicouagan Impact Crater, Quebec, Canada is a 212 million year old impact crater, roughly 100 km in diameter. This is one of the most photographed impact craters from ISS because it is often visible at the top of the orbit. April 15 2016

Cratere Manicouagan -Québec- Manicouagan impact crater seen from the space station: Cratere d'impact Manicouagan, Quebec, vu depuis la station spatiale internationale (ISS) on 15/04/2016. This 100 km-diameter crater formed 212 million years ago, following the fall of an asteroid on Earth. - Manicouagan Impact Crater, Quebec, Canada is a 212 million year old impact crater, roughly 100 km in diameter. This is one of the most photographed impact craters from ISS because it is often visible at the top of the orbit. April 15 2016

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Clearwater Meteor Impact Crater, Canada, True Colour Satellite Image. True colour satellite image of Clearwater Lakes impact structures (age : 270 to 310 million years ; diameters of both craters : 32 km and 22 km). Image taken on 18 September 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

Clearwater Meteor Impact Crater, Canada, True Colour Satellite Image. True colour satellite image of Clearwater Lakes impact structures (age : 270 to 310 million years ; diameters of both craters : 32 km and 22 km). Image taken on 18 September 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

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March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

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Heat shield impact site of Mars Exploration Rover 'Opportunity', 2004

Heat shield impact site of Mars Exploration Rover 'Opportunity', 2004

UIS5104248

Moon: Moscow Sea and crateres - Moon: Mare Moscoviense and craters - Part of the hidden face of the Moon with the Moscow Sea on the right. Image obtained during the Apollo 13 mission, April 1970. This oblique view of the lunar farside was photographed from the Apollo 13 spacecraft as it passed around the moon on its hazardous journey home. The large conspicuous mare area is Mare Moscoviense which is located at 146 degrees east longitude and 25 degrees north latitude. The large crater at the horizon is International Astronomical Union Crater No. 221. This view is looking northeast from the spacecraft

Moon: Moscow Sea and crateres - Moon: Mare Moscoviense and craters - Part of the hidden face of the Moon with the Moscow Sea on the right. Image obtained during the Apollo 13 mission, April 1970. This oblique view of the lunar farside was photographed from the Apollo 13 spacecraft as it passed around the moon on its hazardous journey home. The large conspicuous mare area is Mare Moscoviense which is located at 146 degrees east longitude and 25 degrees north latitude. The large crater at the horizon is International Astronomical Union Crater No. 221. This view is looking northeast from the spacecraft

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Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

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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

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Cratere Manicouagan - Quebec - March 2001 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station in March 2001. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 200

Cratere Manicouagan - Quebec - March 2001 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station in March 2001. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 200

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Crater Bacolor on Mars - Bacolor Crater on planet Mars - View of the impact crater Bacolor obtained by the Mars Odyssey probe. It's an impact crater about 20 km in diameter. Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide. The lines on the ejecta blanket surrounding the crater rim come from a surge of superheated gas and debris flying outward in the wake of the meteorite impact that made the crater. This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on Nasa's Mars Odyssey orbiter. The pictured location on Mars is 33 degrees north latitude, 118.6 degrees east longitude

Crater Bacolor on Mars - Bacolor Crater on planet Mars - View of the impact crater Bacolor obtained by the Mars Odyssey probe. It's an impact crater about 20 km in diameter. Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide. The lines on the ejecta blanket surrounding the crater rim come from a surge of superheated gas and debris flying outward in the wake of the meteorite impact that made the crater. This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on Nasa's Mars Odyssey orbiter. The pictured location on Mars is 33 degrees north latitude, 118.6 degrees east longitude

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Apollo 16: J. Young on the Moon - Apollo 16: J. Young moonwalk - John Young collecting samples during the third and last extravehicular release. 23/04/1972. Astronaut John W. Young, Apollo 16 commander, with a sample bag in his left hand, moves towards the bottom part of the gnomon (center) while collecting samples at the North Ray Crater geological site. Note how soiled Young's Extravehicular Mobility Unit (EMU) is during this the third and final Apollo 16 extravehicular activity (EVA - 3, 23 April 1972). The Lunar Roving Vehicle (LRV) is parked at upper left

Apollo 16: J. Young on the Moon - Apollo 16: J. Young moonwalk - John Young collecting samples during the third and last extravehicular release. 23/04/1972. Astronaut John W. Young, Apollo 16 commander, with a sample bag in his left hand, moves towards the bottom part of the gnomon (center) while collecting samples at the North Ray Crater geological site. Note how soiled Young's Extravehicular Mobility Unit (EMU) is during this the third and final Apollo 16 extravehicular activity (EVA - 3, 23 April 1972). The Lunar Roving Vehicle (LRV) is parked at upper left

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Surface of the Moon - Apollo 14 - Lunar surface - Apollo 14 - Close-up of a large rock on the surface of the Moon, Apollo 14 mission, February 1971. A close - up view of a large boulder in a field of boulders near the rim of Cone Crater, which was photographed by the Apollo 14 moon - explorers during the mission's second extravehicular activity (EVA). Astronauts Alan B. Shepard Jr., commander, and Edgar D. Mitchell, lunar module pilot, descended in the Apollo 14 Lunar Module (LM) to explore the lunar surface while astronaut Stuart A. Roosa, command module pilot, remained with the Command and Service Modules (CSM) in lunar orbit. 6 Feb. 1971

Surface of the Moon - Apollo 14 - Lunar surface - Apollo 14 - Close-up of a large rock on the surface of the Moon, Apollo 14 mission, February 1971. A close - up view of a large boulder in a field of boulders near the rim of Cone Crater, which was photographed by the Apollo 14 moon - explorers during the mission's second extravehicular activity (EVA). Astronauts Alan B. Shepard Jr., commander, and Edgar D. Mitchell, lunar module pilot, descended in the Apollo 14 Lunar Module (LM) to explore the lunar surface while astronaut Stuart A. Roosa, command module pilot, remained with the Command and Service Modules (CSM) in lunar orbit. 6 Feb. 1971

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Switzerland World War II Samedan Bombing, 1943 (b/w photo)

Switzerland World War II Samedan Bombing, 1943 (b/w photo)

Milou Steiner

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Switzerland World War II Samedan Bombing, 1943 (b/w photo)

Switzerland World War II Samedan Bombing, 1943 (b/w photo)

Milou Steiner

KES6234213

Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

Occator Crater on Ceres - Occator Crater on Ceres: View of Occator crater in the northern hemisphere of the dwarf planet Ceres. Occator is 92 km wide and 4 km deep. Bright spots are visible, probably salt deposits. Mosaic of images taken by the Dawn probe. Occator Crater, home of Ceres' intriguing brightest areas, is 57 miles (92 kilometers) wide and 2.5 miles (4 kilometers) deep. Occator displays evidence of recent geologic activity. The latest research suggests that the bright material in this crater is comprised of salts left behind after a briny liquid emerged from below, froze and then sublimated, meaning it turned from ice into vapor. Mosaic of images taken by Dawn spacecraft

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Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt near Shorty crater - Harrison H. Schmitt working near the lunar jeep at Station 4 (Shorty Crater) during the second extravehicular exit Apollo 17 (EVA - 2). 12/12/1972. A view of the lunarscape at Station 4 (Shorty Crater) showing scientist - astronaut Harrison H. Schmitt working at the lunar roving vehicle (LRV) during the second Apollo 17 extravehicular activity (EVA - 2) at the Taurus - Littrow landing site. This is the area where Schmitt first spotted the orange soil. Orange soil is clearly visible on either side of the rover in this picture. Shorty Crater is to the right. The peak in the center background is Family Mountain. Portion of South Massif is on the horizon at the left edge. 12/12/1972

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt near Shorty crater - Harrison H. Schmitt working near the lunar jeep at Station 4 (Shorty Crater) during the second extravehicular exit Apollo 17 (EVA - 2). 12/12/1972. A view of the lunarscape at Station 4 (Shorty Crater) showing scientist - astronaut Harrison H. Schmitt working at the lunar roving vehicle (LRV) during the second Apollo 17 extravehicular activity (EVA - 2) at the Taurus - Littrow landing site. This is the area where Schmitt first spotted the orange soil. Orange soil is clearly visible on either side of the rover in this picture. Shorty Crater is to the right. The peak in the center background is Family Mountain. Portion of South Massif is on the horizon at the left edge. 12/12/1972

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Surface of the Moon - Apollo 15 - Lunar surface - Apollo 15 - Crack on the Moon named Hadley Rille, Apollo 15 mission. 31 July 1971. A view of Hadley Rille, looking northwest, as photographed from near Station No. 2 (St. George Crater) during the first Apollo 15 lunar surface extravehicular activity (EVA). This picture shows layering in the rille wall and blocks on the floor of the rille. The feature referred to as the “” Terrace”” is visible on the right (east) side of the rille. While astronauts David R. Scott, commander, and James B. Irwin, lunar module pilot, descended in the Lunar Module (LM) “” Falcon”” to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Model's (CSM) in lunar orbit. 31 July 1971

Surface of the Moon - Apollo 15 - Lunar surface - Apollo 15 - Crack on the Moon named Hadley Rille, Apollo 15 mission. 31 July 1971. A view of Hadley Rille, looking northwest, as photographed from near Station No. 2 (St. George Crater) during the first Apollo 15 lunar surface extravehicular activity (EVA). This picture shows layering in the rille wall and blocks on the floor of the rille. The feature referred to as the “” Terrace”” is visible on the right (east) side of the rille. While astronauts David R. Scott, commander, and James B. Irwin, lunar module pilot, descended in the Lunar Module (LM) “” Falcon”” to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Model's (CSM) in lunar orbit. 31 July 1971

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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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Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

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Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

Constellations de la Compsole, la Machine Pneumatica et les Voiles - Constellations Antlia, Pyxis and Vela - Constellations de l'hemisphere sud Antlia (originally Antlia Pneumatica, the Air Pump) is an unremarkable constellation invented by the Abbe Nicolas de Lacaille in the 1750s. It is hemmed in by the meandering body of Hydra to the north and the sparkling constellations of the Milky Way to the south. It contains a fine planetary nebula, NGC 3132 and a beautiful spiral galaxy, NGC 2997. Pyxis (Pyxis Nautica, the Mariner's Compasse) is the least interesting fragment of the great vessel Argo Navis, dismantled by Lacaille. The other parts are Puppis (the stern), Carina, (the keel) and Vela. Vela (the sails) is best known for the supernova remnant seen on large telescope pictures and the Gum nebula, visible as faint red nebulosity towards the right (west) of the constellation. Best seen in the early evening in March - April Other constellations in the image: Carina, Centaurus, Corvus,

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March: Victoria crater. - March: Victoria Crater at Meridiani Planum - View of the Victoria crater obtained by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This crater is 800 meters in diameter. The opportunity rover reached this crater on September 27, 2006. After exploring about a quarter of the crater's edges, the rover descended almost a year later to begin an exploration of the crater's interior. Victoria Crater, about 800 meters (one - half mile) in diameter, has been home ground for Nasa's Mars Exploration Rover Opportunity for more 14 of the rover's first 46 months on Mars. Opportunity first reached the crater's rim on Sept. 27, 2006, during the 951st Martian day, or sol, of the rover's work in the Meridian Planum region of Mars. The rover then explored clockwise about one - fourth of the way around the rim before returning to a point close to its first overlook. On the mission's 1,293rd sol (Sept. 13, 2007), Opportunity began a sustained exploration of the

March: Victoria crater. - March: Victoria Crater at Meridiani Planum - View of the Victoria crater obtained by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This crater is 800 meters in diameter. The opportunity rover reached this crater on September 27, 2006. After exploring about a quarter of the crater's edges, the rover descended almost a year later to begin an exploration of the crater's interior. Victoria Crater, about 800 meters (one - half mile) in diameter, has been home ground for Nasa's Mars Exploration Rover Opportunity for more 14 of the rover's first 46 months on Mars. Opportunity first reached the crater's rim on Sept. 27, 2006, during the 951st Martian day, or sol, of the rover's work in the Meridian Planum region of Mars. The rover then explored clockwise about one - fourth of the way around the rim before returning to a point close to its first overlook. On the mission's 1,293rd sol (Sept. 13, 2007), Opportunity began a sustained exploration of the

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Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

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March: impact crater Maunder - Mars: Maunder crater - Perspective view of an impact crater located between Argyre Planitia and Hellas Planitia. The Maunder crater is 90 km in diameter and 900 m deep. The dark areas at the bottom of the crater are dunes. Image obtained by the Mars Express probe in 2005. On 29 November and 14 December 2005 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 15 meters per pixel. The data were acquired in the region of Noachis Terra at approximately 50* southern latitude and 2* eastern longitude. The Maunder Crater, located halfway between Argyre Planitia and Hellas Planitia on the southern Highlands of Mars, has a diameter of 90 kilometers and a current depth of barely 900 meters. In the east, the crater floor is bounded by an approximately 700 meters deep trough. It may be associated with the landslide on the western edge of the crater. Some gullies formed on th

March: impact crater Maunder - Mars: Maunder crater - Perspective view of an impact crater located between Argyre Planitia and Hellas Planitia. The Maunder crater is 90 km in diameter and 900 m deep. The dark areas at the bottom of the crater are dunes. Image obtained by the Mars Express probe in 2005. On 29 November and 14 December 2005 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 15 meters per pixel. The data were acquired in the region of Noachis Terra at approximately 50* southern latitude and 2* eastern longitude. The Maunder Crater, located halfway between Argyre Planitia and Hellas Planitia on the southern Highlands of Mars, has a diameter of 90 kilometers and a current depth of barely 900 meters. In the east, the crater floor is bounded by an approximately 700 meters deep trough. It may be associated with the landslide on the western edge of the crater. Some gullies formed on th

PIX4615975

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of a dozen images taken by the robot on October 6, 2015. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the “” Big Sky”” site, where its drill collected the mission's fifth taste of Mount Sharp. The scene combines dozens of images taken during the 1,126th Martian day, or sol, of Curiosity's work on Mars (Oct. 6, 2015, PDT), by the Mars Hand Lens Imager (MAHLI) camera at the end of the rover's robotic arm. The rock drilled at this site is sandstone in the Stimson geological unit inside Gale Crater. The view is centered toward the west-northwest. It does not include the rover's robotic arm, though the shadow of the arm is visible on the ground. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot

Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of a dozen images taken by the robot on October 6, 2015. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the “” Big Sky”” site, where its drill collected the mission's fifth taste of Mount Sharp. The scene combines dozens of images taken during the 1,126th Martian day, or sol, of Curiosity's work on Mars (Oct. 6, 2015, PDT), by the Mars Hand Lens Imager (MAHLI) camera at the end of the rover's robotic arm. The rock drilled at this site is sandstone in the Stimson geological unit inside Gale Crater. The view is centered toward the west-northwest. It does not include the rover's robotic arm, though the shadow of the arm is visible on the ground. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot

PIX4643642

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

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

Steven Hobbs

PIX4615030

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

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

PIX4616168

Constellations of the Cup and the Raven - Constellations of Crater and Corvus - On the left, the bright star is Spica, in the Virgin. Corvus (the Raven or Crow) is a southern constellation of rather faint stars. It occupies about 184 square degrees, which makes it the 70th largest constellation (out of 88 recognised today). However, it is ancient, and is associated with Crater (the Cup) and Hydrus, the water snake, on whose back Corvus sits. The grouping was recognised by Ptolemy almost 2000 years ago. Crater (Latin for cup) was also recognised by Ptolemy and covering 282 square degrees is larger than Corvus but is no more distinguished

Constellations of the Cup and the Raven - Constellations of Crater and Corvus - On the left, the bright star is Spica, in the Virgin. Corvus (the Raven or Crow) is a southern constellation of rather faint stars. It occupies about 184 square degrees, which makes it the 70th largest constellation (out of 88 recognised today). However, it is ancient, and is associated with Crater (the Cup) and Hydrus, the water snake, on whose back Corvus sits. The grouping was recognised by Ptolemy almost 2000 years ago. Crater (Latin for cup) was also recognised by Ptolemy and covering 282 square degrees is larger than Corvus but is no more distinguished

PIX4590096

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

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

PIX4616176

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

PIX4625616

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

PIX4574821

Mars - Artist's View - Mars - Artwork - A view from north of Mars' equato

Mars - Artist's View - Mars - Artwork - A view from north of Mars' equato

Steven Hobbs

PIX4616817

Moon: Tsiolkovsky crater on the hidden face - Moon: crater Tsiolkovsky on lunar farside - Image obtained during the Apollo 15 mission, August 1971. Image taken during Apollo 15 mission

Moon: Tsiolkovsky crater on the hidden face - Moon: crater Tsiolkovsky on lunar farside - Image obtained during the Apollo 15 mission, August 1971. Image taken during Apollo 15 mission

PIX4576932

Mars surface seen by the probe Mariner 6 - Mariner 6 closeup view of Martian craters - Martian crateres in Sinus Meridiani seen by the probe Mariner 6 in July 1969. Recolorized image. Mars craters in Sinus Meridiani seen by Mariner 6 in july 1969. Recolorized picture

Mars surface seen by the probe Mariner 6 - Mariner 6 closeup view of Martian craters - Martian crateres in Sinus Meridiani seen by the probe Mariner 6 in July 1969. Recolorized image. Mars craters in Sinus Meridiani seen by Mariner 6 in july 1969. Recolorized picture

Steven Hobbs

PIX4615020

Moon: Cratere Clavius - Moon: Clavius Crater: Image obtained on August 24, 2016, a day before the last quarter of the moon

Moon: Cratere Clavius - Moon: Clavius Crater: Image obtained on August 24, 2016, a day before the last quarter of the moon

Sebastian Voltmer

PIX4614521

Surface of Ceres - Ceres' surface - Surface of the dwarf planet Ceres. Artist's view. What is known about Ceres' surface is that it has an albedo (surface brightness) about the same as the Earth's Moon and never gets warmer than minus 30o F. In this image the artist is suggesting a lunar-like terrain modified by the presence of water ice

Surface of Ceres - Ceres' surface - Surface of the dwarf planet Ceres. Artist's view. What is known about Ceres' surface is that it has an albedo (surface brightness) about the same as the Earth's Moon and never gets warmer than minus 30o F. In this image the artist is suggesting a lunar-like terrain modified by the presence of water ice

Walter B Myers

PIX4584135

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

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

PIX4616151

Moon: grooves and mountain, April 1972 (photo)

Moon: grooves and mountain, April 1972 (photo)

PIX4576961

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

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

PIX4616156

Moon: Aristarchus crater - Moon: Aristarchus crater - Apollo 15 - The Aristarchus crater and the Schroeter valley. Image obtained from the Apollo 15 control module. An oblique view of Schroeter's Valley and the crater Aristarchus, as photographed by the Apollo 15 Command and Service Module (CSM) in lunar orbit. The large, bright - appearing crater to the left of the head of meandering Schroeter's Valley is Aristarchus, the center of which is located at 48 degrees west longitude and 214 degrees north latitude. The crater Aristarchus approximately 35 kilometers (about 21.75 statute miles) in diameter. The head of Schroeter's Valley, a sinuous rille in the Aristarchus Plateau in the Ocean of Storms, is called Cobra Head. Herodotus the crater just above and to the right of Cobra Head in upper center

Moon: Aristarchus crater - Moon: Aristarchus crater - Apollo 15 - The Aristarchus crater and the Schroeter valley. Image obtained from the Apollo 15 control module. An oblique view of Schroeter's Valley and the crater Aristarchus, as photographed by the Apollo 15 Command and Service Module (CSM) in lunar orbit. The large, bright - appearing crater to the left of the head of meandering Schroeter's Valley is Aristarchus, the center of which is located at 48 degrees west longitude and 214 degrees north latitude. The crater Aristarchus approximately 35 kilometers (about 21.75 statute miles) in diameter. The head of Schroeter's Valley, a sinuous rille in the Aristarchus Plateau in the Ocean of Storms, is called Cobra Head. Herodotus the crater just above and to the right of Cobra Head in upper center

PIX4576885

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

PIX4594435

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

PIX4625563

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

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

PIX4616155

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

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

PIX4616171

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

PIX4625625

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

PIX4616154

Moon: Cratere Eratosthene - Moon: Eratosthenes crater - Cratere Eratosthene seen from the control module of Apollo 12. View of Eratosthenes crater, on the lunar nearside, as photographed from the Apollo 12 spacecraft

Moon: Cratere Eratosthene - Moon: Eratosthenes crater - Cratere Eratosthene seen from the control module of Apollo 12. View of Eratosthenes crater, on the lunar nearside, as photographed from the Apollo 12 spacecraft

PIX4576824

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