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Apollo 12: Lunar sample - View of Apollo 12 lunar sample - Lunar soil sample collected during the Apollo 12 mission. A close - up view of Apollo 12 lunar sample no. 12025, called Core Sample 1, and collected on the lunar surface, about 225 meters below the point where the Apollo 12 Lunar Module touched down. This core sample and others collected on the Apollo 12 mission differ from those collected by the Apollo 11 crewmen in the Sea of Tranquility in that the Apollo 12 core samples have easily recognizable stratigraphy and two coherent crust - like layers. This sample has dominantly fine - grained texture

Apollo 12: Lunar sample - View of Apollo 12 lunar sample - Lunar soil sample collected during the Apollo 12 mission. A close - up view of Apollo 12 lunar sample no. 12025, called Core Sample 1, and collected on the lunar surface, about 225 meters below the point where the Apollo 12 Lunar Module touched down. This core sample and others collected on the Apollo 12 mission differ from those collected by the Apollo 11 crewmen in the Sea of Tranquility in that the Apollo 12 core samples have easily recognizable stratigraphy and two coherent crust - like layers. This sample has dominantly fine - grained texture

PIX4596644

Martian Landscape - Illustration - Martian landscape - Illustration: Landscape on Mars with “dust devils” - Mars with dust devils

Martian Landscape - Illustration - Martian landscape - Illustration: Landscape on Mars with “dust devils” - Mars with dust devils

Miller, Ron (b.1947)

PIX4617016

Pust Tempete sur Mars - Illustration - Channel and dust storm on Mars: Landscape on Mars with dust devils - Mars with dust devils

Pust Tempete sur Mars - Illustration - Channel and dust storm on Mars: Landscape on Mars with dust devils - Mars with dust devils

Miller, Ron (b.1947)

PIX4617018

Apollo 15: Lunar soil sample - Apollo 15: lunar soil - Container filled with lunar soil brought back by the crew of the Apollo 15 mission. A close - up view of a container full of green - colored lunar soil in the Non - Sterile Nitrogen Processing Line (NNPL) in the Lunar Receiving Laboratory (LRL) at the Manned Spacecraft Center (MSC). This sample, broken down into six separate samples after this photo was made, was made up of comprehensive fines from near Spur Crater on the Apennine Front. The numbers assigned to the sample include numbers 15300 through 15305. Astronauts David R. Scott and James B. Irwin took the sample during their second extravehicular activity (EVA) at a ground elapsed time (GET) of 146:05 to 146:06

Apollo 15: Lunar soil sample - Apollo 15: lunar soil - Container filled with lunar soil brought back by the crew of the Apollo 15 mission. A close - up view of a container full of green - colored lunar soil in the Non - Sterile Nitrogen Processing Line (NNPL) in the Lunar Receiving Laboratory (LRL) at the Manned Spacecraft Center (MSC). This sample, broken down into six separate samples after this photo was made, was made up of comprehensive fines from near Spur Crater on the Apennine Front. The numbers assigned to the sample include numbers 15300 through 15305. Astronauts David R. Scott and James B. Irwin took the sample during their second extravehicular activity (EVA) at a ground elapsed time (GET) of 146:05 to 146:06

PIX4597407

Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

PIX4597805

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut robs the soil of March as a dust storm comes up. Artist's view. Astronaut walking on Mars soil with a dust storm approaching

Astronaut on Mars - Illustration - Astronaut on Mars - Illustration - An astronaut robs the soil of March as a dust storm comes up. Artist's view. Astronaut walking on Mars soil with a dust storm approaching

PIX4639949

Photograph of Garden City after a dust storm has settled

Photograph of Garden City after a dust storm has settled

UIG3524675

Dust Tempete in Afghanistan - Afghanistan Dust Front - Dust Tempete in northern Afghanistan. Image obtained from Space Shuttle Atlantis in September 2000. Winds in the upper Amu Darya valley, along the northern border of Afghanistan lofted thick, light brown dust into the air (top half of the view). In this desert environment land surfaces are not protected by vegetation from the effect of blowing wind. The central Asian deserts experience the greatest number of dust storm days on the planet each year. The sharp dust front shows that the dust has not traveled far, but has been raised from the surfaces in the view. Image taken from the space shuttle Atlantis in september 2000

Dust Tempete in Afghanistan - Afghanistan Dust Front - Dust Tempete in northern Afghanistan. Image obtained from Space Shuttle Atlantis in September 2000. Winds in the upper Amu Darya valley, along the northern border of Afghanistan lofted thick, light brown dust into the air (top half of the view). In this desert environment land surfaces are not protected by vegetation from the effect of blowing wind. The central Asian deserts experience the greatest number of dust storm days on the planet each year. The sharp dust front shows that the dust has not traveled far, but has been raised from the surfaces in the view. Image taken from the space shuttle Atlantis in september 2000

PIX4659665

Apollo 17: E. Cernan in the LEM - Apollo 17: E. Cernan in the lunar module - Eugene Cernan in the LEM after his third extravehicular exit

Apollo 17: E. Cernan in the LEM - Apollo 17: E. Cernan in the lunar module - Eugene Cernan in the LEM after his third extravehicular exit

PIX4598232

Back to the Moon - Program constellation - Astronauts in a Lunar vehicle - Constellation program - View of an artist of astronauts exploring the surface of the Moon in a pressurized vehicle (Lunar Electric Rover), as part of the Nasa constellation program that is expected to take men to the Moon around 2020. A Lunar Electric Rover (LER), with crewmembers inside, performs work on the lunar surface in this art work depicting return to the moon activities

Back to the Moon - Program constellation - Astronauts in a Lunar vehicle - Constellation program - View of an artist of astronauts exploring the surface of the Moon in a pressurized vehicle (Lunar Electric Rover), as part of the Nasa constellation program that is expected to take men to the Moon around 2020. A Lunar Electric Rover (LER), with crewmembers inside, performs work on the lunar surface in this art work depicting return to the moon activities

PIX4639303

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit

PIX4598221

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

PIX4597546

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt collecting samples. 12/12/1972. Harrison Schmitt uses scoop to retrieve lunar samples. Dec 12 1972

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt collecting samples. 12/12/1972. Harrison Schmitt uses scoop to retrieve lunar samples. Dec 12 1972

PIX4598051

Apollo 17: H. Schmitt sur la Lune - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt preleve des samantillons lunaires à la station 1. 11/12/1972. 11 December 1972: Scientist - Astronaut Harrison H. Schmitt collects lunar rake samples at Station 1 during the first Apollo 17 extravehicular activity (EVA - 1) at the Taurus Littrow landing site. This picture was taken by Astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. The Lunar Rake, an Apollo Lunar Geology Hand Tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 cm) to one inch (2.5 cm)

Apollo 17: H. Schmitt sur la Lune - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt preleve des samantillons lunaires à la station 1. 11/12/1972. 11 December 1972: Scientist - Astronaut Harrison H. Schmitt collects lunar rake samples at Station 1 during the first Apollo 17 extravehicular activity (EVA - 1) at the Taurus Littrow landing site. This picture was taken by Astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. The Lunar Rake, an Apollo Lunar Geology Hand Tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 cm) to one inch (2.5 cm)

PIX4598119

Back to the Moon - Program constellation - Astronauts in a Lunar vehicle - Constellation program - View of an artist of astronauts exploring the surface of the Moon in a pressurized vehicle (Lunar Electric Rover), as part of the Nasa constellation program that is expected to take men to the Moon around 2020. A Lunar Electric Rover (LER), with crewmembers inside, performs work on the lunar surface in this art work depicting return to the moon activities

Back to the Moon - Program constellation - Astronauts in a Lunar vehicle - Constellation program - View of an artist of astronauts exploring the surface of the Moon in a pressurized vehicle (Lunar Electric Rover), as part of the Nasa constellation program that is expected to take men to the Moon around 2020. A Lunar Electric Rover (LER), with crewmembers inside, performs work on the lunar surface in this art work depicting return to the moon activities

PIX4639346

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. E. Cernan inside the LM after EVA-

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. E. Cernan inside the LM after EVA-

PIX4598216

Apollo 17: orange soil on the Moon - Apollo 17: the orange soil - View of orange soil, rich in zinc, probably of volcanic origin. Station 4, near the Shorty Crater. 12/12/1972. A view of the area at Station 4 (Shorty Crater) showing the now highly - publicized orange soil which the Apollo 17 crew members found on the moon during the second Apollo 17 extravehicular activity (EVA) at the Taurus - Littrow landing site. The tripod - like object is the gnomon and photometric chart assembly which is used as a photographic reference to establish local vertical sun angle, scale and lunar color. The gnomon is one of the Apollo lunar geology hand tools. While astronauts Eugene A. Cernan, commander, and Harrison H. Schmitt, lunar module pilot, descended in the Lunar Module (LM) “” Challenger”” to explore the Taurus - Littrow region of the moon, astronaut Ronald E. Evans, command module pilot, remained with the Command and Service Modules (CSM) “” America”” in lunar orbit. Schmitt was the crew man

Apollo 17: orange soil on the Moon - Apollo 17: the orange soil - View of orange soil, rich in zinc, probably of volcanic origin. Station 4, near the Shorty Crater. 12/12/1972. A view of the area at Station 4 (Shorty Crater) showing the now highly - publicized orange soil which the Apollo 17 crew members found on the moon during the second Apollo 17 extravehicular activity (EVA) at the Taurus - Littrow landing site. The tripod - like object is the gnomon and photometric chart assembly which is used as a photographic reference to establish local vertical sun angle, scale and lunar color. The gnomon is one of the Apollo lunar geology hand tools. While astronauts Eugene A. Cernan, commander, and Harrison H. Schmitt, lunar module pilot, descended in the Lunar Module (LM) “” Challenger”” to explore the Taurus - Littrow region of the moon, astronaut Ronald E. Evans, command module pilot, remained with the Command and Service Modules (CSM) “” America”” in lunar orbit. Schmitt was the crew man

PIX4598153

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

PIX4597551

Apollo 14: E. Mitchell on the Moon - Apollo 14: E. Mitchell moonwalk - Extravehicular release of Edgar Mitchell with a map. 05/02/1971. Astronaut Edgar D. Mitchell, lunar module pilot, moves across the lunar surface as he looks over a traverse map during an extravehicular activity (EVA). Lunar dust can be seen clinging to the boots and legs of the space suit. Astronauts Alan B. Shepard Jr., commander, and Mitchell explored the lunar surface while astronaut Stuart A. Roosa, command module pilot, orbited the moon in the Command and Service Modules (CSM)

Apollo 14: E. Mitchell on the Moon - Apollo 14: E. Mitchell moonwalk - Extravehicular release of Edgar Mitchell with a map. 05/02/1971. Astronaut Edgar D. Mitchell, lunar module pilot, moves across the lunar surface as he looks over a traverse map during an extravehicular activity (EVA). Lunar dust can be seen clinging to the boots and legs of the space suit. Astronauts Alan B. Shepard Jr., commander, and Mitchell explored the lunar surface while astronaut Stuart A. Roosa, command module pilot, orbited the moon in the Command and Service Modules (CSM)

PIX4597125

Apollo 17: H. Schmitt sur la Lune - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt preleve des samantillons lunaires à la station 1. 11/12/1972. 11 December 1972: Scientist - Astronaut Harrison H. Schmitt collects lunar rake samples at Station 1 during the first Apollo 17 extravehicular activity (EVA - 1) at the Taurus Littrow landing site. This picture was taken by Astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. The Lunar Rake, an Apollo Lunar Geology Hand Tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 cm) to one inch (2.5 cm)

Apollo 17: H. Schmitt sur la Lune - Apollo 17: H. Schmitt retrieving lunar samples - H. Schmitt preleve des samantillons lunaires à la station 1. 11/12/1972. 11 December 1972: Scientist - Astronaut Harrison H. Schmitt collects lunar rake samples at Station 1 during the first Apollo 17 extravehicular activity (EVA - 1) at the Taurus Littrow landing site. This picture was taken by Astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. The Lunar Rake, an Apollo Lunar Geology Hand Tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 cm) to one inch (2.5 cm)

PIX4598106

Apollo 17: Lunar Jeep - Apollo 17: Lunar Rover Vehicle - Mudguard at the rear of the jeep. 12/12/1972. A close - up view of the lunar roving vehicle (LRV) at the Taurus - Littrow landing site photographed during Apollo 17 lunar surface extravehicular activity. Note the makeshift repair arrangement on the right rear fender of the LRV. During EVA - 1 a hammer got underneath the fender and a part of it was knocked off. Astronauts Eugene A. Cernan and Harrison H. Schmitt were reporting a problem with lunar dust because of the damage fender. Following a suggestion from astronaut John W. Young in the Mission Control Center at Houston the crewmen repaired the fender early in EVA - 2 using lunar maps and clamps from the optical alignment telescope lamp. Schmitt is seated in the rover. Cernan took this picture. 12 Dec 1972

Apollo 17: Lunar Jeep - Apollo 17: Lunar Rover Vehicle - Mudguard at the rear of the jeep. 12/12/1972. A close - up view of the lunar roving vehicle (LRV) at the Taurus - Littrow landing site photographed during Apollo 17 lunar surface extravehicular activity. Note the makeshift repair arrangement on the right rear fender of the LRV. During EVA - 1 a hammer got underneath the fender and a part of it was knocked off. Astronauts Eugene A. Cernan and Harrison H. Schmitt were reporting a problem with lunar dust because of the damage fender. Following a suggestion from astronaut John W. Young in the Mission Control Center at Houston the crewmen repaired the fender early in EVA - 2 using lunar maps and clamps from the optical alignment telescope lamp. Schmitt is seated in the rover. Cernan took this picture. 12 Dec 1972

PIX4598144

Apollo 12: A. Bean and lunar soil samples - Apollo 12: A.Bean and lunar soil sample - Alan Bean holding a container filled with lunar dust. Reflecting on his visor, Conrad taking the picture. 19/11/1969. Astronaut Alan L. Bean, lunar module pilot for the Apollo 12 lunar landing mission, holds a Special Environmental Sample Container filled with lunar soil collected during the extravehicular activity (EVA) in which astronauts Charles Conrad Jr., commander, and Bean participated. Connrad, who took this picture, is reflected in the helmet visor of the lunar module pilot

Apollo 12: A. Bean and lunar soil samples - Apollo 12: A.Bean and lunar soil sample - Alan Bean holding a container filled with lunar dust. Reflecting on his visor, Conrad taking the picture. 19/11/1969. Astronaut Alan L. Bean, lunar module pilot for the Apollo 12 lunar landing mission, holds a Special Environmental Sample Container filled with lunar soil collected during the extravehicular activity (EVA) in which astronauts Charles Conrad Jr., commander, and Bean participated. Connrad, who took this picture, is reflected in the helmet visor of the lunar module pilot

PIX4596625

Zodiacal light - Zodiacal light - Zodiacal light. May 2004, Namibia. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plane of the Solar System. Zodiacal light, Namibia, May 2004. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system

Zodiacal light - Zodiacal light - Zodiacal light. May 2004, Namibia. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plane of the Solar System. Zodiacal light, Namibia, May 2004. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system

Sebastian Voltmer

PIX4581492

Wells Fargo agent buying gold

Wells Fargo agent buying gold

McBride, Angus (1931-2007)

LAL337253

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - Harrison Schmitt collecting samples. 11/12/1972. Panorama. Scientist - astronaut Harrison H. Schmitt, lunar module pilot, collects lunar rake samples at Station 1 during the first Apollo 17 Extrahicular Activity (EVA - 1) at the Taurus - Littrow landing site. This panorama was taken by astronaut Eugene Cernan, commander. The lunar rake, an Apollo lunar geology hand tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 centimeter) to one inch (2.5 centimeter). 11 December 1972

Apollo 17: H. Schmitt on the Moon - Apollo 17: H. Schmitt retrieving lunar samples - Harrison Schmitt collecting samples. 11/12/1972. Panorama. Scientist - astronaut Harrison H. Schmitt, lunar module pilot, collects lunar rake samples at Station 1 during the first Apollo 17 Extrahicular Activity (EVA - 1) at the Taurus - Littrow landing site. This panorama was taken by astronaut Eugene Cernan, commander. The lunar rake, an Apollo lunar geology hand tool, is used to collect discrete samples of rocks and rock chips ranging in size from one - half inch (1.3 centimeter) to one inch (2.5 centimeter). 11 December 1972

PIX4598086

A London Dust-Yard (engraving)

A London Dust-Yard (engraving)

Buckman, Edwin (1841-1930)

LIP1105210

Sand pillars in the desert (engraving)

Sand pillars in the desert (engraving)

German School, (19th century)

FEH328998

The clouds of dust behind US Air Force C-17 Globemaster III at Fort Irwin

The clouds of dust behind US Air Force C-17 Globemaster III at Fort Irwin

UIG2911462

Funeral service for Virginia Hill, 1966 (b/w photo)

Funeral service for Virginia Hill, 1966 (b/w photo)

Alfred Strobel

SZT6314446

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

R. Gendler

PIX4612037

Tornado striking town, United States, 1930s

Tornado striking town, United States, 1930s

UIG2603727

Probe Mars 3 - Mars 3 spacecraft - The landing gear of the Mars-3 probe was the first aircraft to land intact on Mars soil on December 2, 1971. Unfortunately, due to a heavy dust storm, it only operated for 20 seconds. The Soviet Mars 3 lander separates from its mother craft above Mars. The timing is unfortunate as the planet is experiencing a global dust storm. March - 3 was launched to Mars on May 28, 1971. On December 2, 1971 it's descent capsule made a soft landing on the surface of Mars. This mission was not successful, because of a dust storm on the Mars surface

Probe Mars 3 - Mars 3 spacecraft - The landing gear of the Mars-3 probe was the first aircraft to land intact on Mars soil on December 2, 1971. Unfortunately, due to a heavy dust storm, it only operated for 20 seconds. The Soviet Mars 3 lander separates from its mother craft above Mars. The timing is unfortunate as the planet is experiencing a global dust storm. March - 3 was launched to Mars on May 28, 1971. On December 2, 1971 it's descent capsule made a soft landing on the surface of Mars. This mission was not successful, because of a dust storm on the Mars surface

Steven Hobbs

PIX4606351

Apollo 15: lunar ground and footprints - Apollo 15: lunar footprint

Apollo 15: lunar ground and footprints - Apollo 15: lunar footprint

PIX4597294

Zodiacal light - Zodiacal light - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 1 November 2006, Monts d'Arree (Finistere - France) The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. November 1st 2006, Monts d'Arree (Finistere - France)

Zodiacal light - Zodiacal light - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 1 November 2006, Monts d'Arree (Finistere - France) The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. November 1st 2006, Monts d'Arree (Finistere - France)

Laurent Laveder

PIX4581449

Dust buried farm during the height of the Dust Bowl years, Great Plains, USA

Dust buried farm during the height of the Dust Bowl years, Great Plains, USA

UIG3519942

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

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

Miller, Ron (b.1947)

PIX4608433

Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

R. Gendler

PIX4612036

Scenario of a star formation - In a cloud of gas and interstellar dust, a blood cell contracts and heats. The blood cell flattens in a disc around the young star. The star starts to shine. In a cloud of gaz and interstellar dust a dark globule will contract to create a rotating disk flattening; at the center of this disk, the stars ingnites

Scenario of a star formation - In a cloud of gas and interstellar dust, a blood cell contracts and heats. The blood cell flattens in a disc around the young star. The star starts to shine. In a cloud of gaz and interstellar dust a dark globule will contract to create a rotating disk flattening; at the center of this disk, the stars ingnites

S. Numazawa

PIX4572925

Spiral galaxy NGC 4402 - Spiral galaxy NGC 4402 - NGC 4402 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Image obtained by the Hubble Space Telescope. Close - up of the disc of gas and dust of the spiral galaxy NGC 4402 in the Virgo cluster. Image taken by the Hubble Space Telescope

Spiral galaxy NGC 4402 - Spiral galaxy NGC 4402 - NGC 4402 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Image obtained by the Hubble Space Telescope. Close - up of the disc of gas and dust of the spiral galaxy NGC 4402 in the Virgo cluster. Image taken by the Hubble Space Telescope

PIX4611327

Spiral galaxy NGC 5775 - NGC 5775 is located about 85 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. This NASA/ESA Hubble Space Telescope image shows the edge - on profile of the slender spiral galaxy NGC 5775. NGC 5775 is a member of the Virgo Cluster and lies at a distance of about 85 million light - years. This colour picture was created from images taken using the Wide Field Channel of Hubble's Advanced Camera for Surveys

Spiral galaxy NGC 5775 - NGC 5775 is located about 85 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. This NASA/ESA Hubble Space Telescope image shows the edge - on profile of the slender spiral galaxy NGC 5775. NGC 5775 is a member of the Virgo Cluster and lies at a distance of about 85 million light - years. This colour picture was created from images taken using the Wide Field Channel of Hubble's Advanced Camera for Surveys

PIX4612800

Spiral Galaxy NGC 4452 - Galaxy Spiral NGC 4452 - NGC 4452 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope has imaged a striking galaxy called NGC 4452, which appears to lie exactly edge - on as seen from Earth. The bright nucleus can be seen at the centre, along with the very thin disc that looks like a straight line from our unusual viewing position. To complete the picture, a hazy halo of stars on the periphery of the galaxy makes it seem to glow. NGC 4452 was first seen by William Herschel in 1784 with his 47 cm telescope in England. He described the object as a bright nebula, small and very much elongated. The new Hubble image shows just how elongated this unusual object really is. NGC 4452 is part of the Virgo Cluster, so - called because many

Spiral Galaxy NGC 4452 - Galaxy Spiral NGC 4452 - NGC 4452 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Seen from the Earth, this spiral galaxy is presented by the slice, leaving only the thickness of its disc visible. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope has imaged a striking galaxy called NGC 4452, which appears to lie exactly edge - on as seen from Earth. The bright nucleus can be seen at the centre, along with the very thin disc that looks like a straight line from our unusual viewing position. To complete the picture, a hazy halo of stars on the periphery of the galaxy makes it seem to glow. NGC 4452 was first seen by William Herschel in 1784 with his 47 cm telescope in England. He described the object as a bright nebula, small and very much elongated. The new Hubble image shows just how elongated this unusual object really is. NGC 4452 is part of the Virgo Cluster, so - called because many

PIX4611380

Star formation in the heart of a dark nebula - Protostellar nebula

Star formation in the heart of a dark nebula - Protostellar nebula

Miller, Ron (b.1947)

PIX4572934

Zodiacal light - Zodiacal light - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 1 November 2006, Monts d'Arree (Finistere - France) The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. November 1st 2006, Monts d'Arree (Finistere - France)

Zodiacal light - Zodiacal light - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 1 November 2006, Monts d'Arree (Finistere - France) The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. November 1st 2006, Monts d'Arree (Finistere - France)

Laurent Laveder

PIX4581489

Artist's view of a planetary system in formation - Planetary system formation. Artwork - Artist's view of an exoplanet and his young star still surrounded by dust. Artwork showing an exoplanet with its young star and dust

Artist's view of a planetary system in formation - Planetary system formation. Artwork - Artist's view of an exoplanet and his young star still surrounded by dust. Artwork showing an exoplanet with its young star and dust

D. Ducros

PIX4574193

Artist's view of a planetary system in formation - Planetary system formation. Artwork: Artist's view of a young star surrounded by a protoplanetary disc. Artwork showing exoplanets in fusion with their young star and dust

Artist's view of a planetary system in formation - Planetary system formation. Artwork: Artist's view of a young star surrounded by a protoplanetary disc. Artwork showing exoplanets in fusion with their young star and dust

Miller, Ron (b.1947)

PIX4574220

Beta Pictoris b - Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbiting the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three - thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light - years away towards the constellation of Pictor (the Painter) and is one of the best - known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell - tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth - Sun separation -

Beta Pictoris b - Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbiting the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three - thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light - years away towards the constellation of Pictor (the Painter) and is one of the best - known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell - tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth - Sun separation -

PIX4574181

Artist's view of the double star Epsilon Aurigae (Almaaz) - Binary star Epsilon Aurigae. Artwork - Almaaz is a binary star with a strange eclipse; it is eclipsed by a gigantic companion for two years. It is believed that this companion could be composed of one or two stars surrounded by a large disc of dust. The visible companion is a yellow supergiant type F, one of the brightest stars in the sky. Epsilon Aurigae (Almaaz) is an eclipsing binary star

Artist's view of the double star Epsilon Aurigae (Almaaz) - Binary star Epsilon Aurigae. Artwork - Almaaz is a binary star with a strange eclipse; it is eclipsed by a gigantic companion for two years. It is believed that this companion could be composed of one or two stars surrounded by a large disc of dust. The visible companion is a yellow supergiant type F, one of the brightest stars in the sky. Epsilon Aurigae (Almaaz) is an eclipsing binary star

S. Numazawa

PIX4572671

Galaxy NGC 660 in Pisces - Galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image of the central part of the galaxy obtained by the Hubble Space Telescope (HST). NGC 660 is described as being a “” polar ring””” galaxy. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million light years away. Image taken with the Hubble space telescope (HST)

Galaxy NGC 660 in Pisces - Galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image of the central part of the galaxy obtained by the Hubble Space Telescope (HST). NGC 660 is described as being a “” polar ring””” galaxy. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million light years away. Image taken with the Hubble space telescope (HST)

R. Gendler

PIX4609420

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This image was obtained by Siding Spring's 3.9m telescope. This is one of many peculiar galaxies that populate the large southern constellation of Centaurus. This remarkable spiral galaxy seen almost edge - on, and the spiral structure is chaotic and difficult to discern. In part this is because the galaxy is itself extremely dusty, and it is seen through dust in the Milky Way. These effects together account for its yellowish hue, though patches of bluish stars can be seen. The dust in NGC 4945 absorbs most of the visible light, especially the blue light from the numerous bright stars known present within the galaxy. This energy is re - radiated at infrared wavelengths, which penetrate dust more readily, which is why the galaxy is found to be unusually bright in the infrared

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This image was obtained by Siding Spring's 3.9m telescope. This is one of many peculiar galaxies that populate the large southern constellation of Centaurus. This remarkable spiral galaxy seen almost edge - on, and the spiral structure is chaotic and difficult to discern. In part this is because the galaxy is itself extremely dusty, and it is seen through dust in the Milky Way. These effects together account for its yellowish hue, though patches of bluish stars can be seen. The dust in NGC 4945 absorbs most of the visible light, especially the blue light from the numerous bright stars known present within the galaxy. This energy is re - radiated at infrared wavelengths, which penetrate dust more readily, which is why the galaxy is found to be unusually bright in the infrared

PIX4612044

Artist's view of a birth of stars - Birth of stars. Artwork - Stars in formation in the heart of a dark nebula

Artist's view of a birth of stars - Birth of stars. Artwork - Stars in formation in the heart of a dark nebula

S. Numazawa

PIX4572906

Exoplanets around the star HR 8799 - Planets orbiting star HR 8799 - Artist's view of the extrasolar planet HR 8799e, a planet located 129 light years from the Sun, in the constellation of Pegase. The HR 8799 star is located in the center of a system that forms a debris disc and at least four massive exoplanets. Foreground is the exoplanet HR 8799 e

Exoplanets around the star HR 8799 - Planets orbiting star HR 8799 - Artist's view of the extrasolar planet HR 8799e, a planet located 129 light years from the Sun, in the constellation of Pegase. The HR 8799 star is located in the center of a system that forms a debris disc and at least four massive exoplanets. Foreground is the exoplanet HR 8799 e

Miller, Ron (b.1947)

PIX4607693

Black hole - Artist view - Black Hole and Red Giant - Artist view - A giant red star orbiting a black hole. A black hole doing some damage to a passing red giant star

Black hole - Artist view - Black Hole and Red Giant - Artist view - A giant red star orbiting a black hole. A black hole doing some damage to a passing red giant star

PIX4584704

The dust devil tracks in this VIS image are located in Utopia Planitia.

The dust devil tracks in this VIS image are located in Utopia Planitia.

UIG866621

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell-tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 1

Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell-tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 1

Miller, Ron (b.1947)

PIX4608449

Artist's view of a planetary system in formation - Planetary system formation. Artwork - Artist's view of an exoplanet and his young star still surrounded by dust. Artwork showing an exoplanet with its young star and dust

Artist's view of a planetary system in formation - Planetary system formation. Artwork - Artist's view of an exoplanet and his young star still surrounded by dust. Artwork showing an exoplanet with its young star and dust

D. Ducros

PIX4574204

Page of catalogue for the Ironmongery and Hardware Trades, c 1895 (litho)

Page of catalogue for the Ironmongery and Hardware Trades, c 1895 (litho)

English School, (19th century)

LLR6034163

Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites

Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites

P. Carril

PIX4572917

Sand tempete on the islands of Cape Verde - Dust storm over the Cape Verde islands - Sand tempete on the islands of Cape Verde observed on 22 June 2009 by the Terra satellite. The borders are added. Two dust plumes blow toward the southwest, one plume stretching possibly 150 kilometers (95 miles) off the coast, and the other plume forming an arc that reaches all the way to Cape Verde. Although this image shows dust immediately off the coast of West Africa, a layer of dust from storms such as this often travels virtually intact to the other side of the Atlantic. This layer of dry, hot, dusty air is called the Saharan Air Layer. Terra satellite took this natural - color picture on June 22, 2009. Borders have been added

Sand tempete on the islands of Cape Verde - Dust storm over the Cape Verde islands - Sand tempete on the islands of Cape Verde observed on 22 June 2009 by the Terra satellite. The borders are added. Two dust plumes blow toward the southwest, one plume stretching possibly 150 kilometers (95 miles) off the coast, and the other plume forming an arc that reaches all the way to Cape Verde. Although this image shows dust immediately off the coast of West Africa, a layer of dust from storms such as this often travels virtually intact to the other side of the Atlantic. This layer of dry, hot, dusty air is called the Saharan Air Layer. Terra satellite took this natural - color picture on June 22, 2009. Borders have been added

PIX4659178

Apollo 17: equipment in the LEM - Apollo 17: space suits and helmets - Helmets and suits in the tight space of the LEM. 13/12/1972. LM Interior after the completion of EVA-3. Helmets and suits on the engine cover

Apollo 17: equipment in the LEM - Apollo 17: space suits and helmets - Helmets and suits in the tight space of the LEM. 13/12/1972. LM Interior after the completion of EVA-3. Helmets and suits on the engine cover

PIX4598251

Zodiacal light - Star Trainee - Zodiacal light - Star trails - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 9 March 2007 at sunset, Treguennec (Finistere - France). The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. 6 minutes exposure, March 9 2007, sunset, Treguennec (Finistere - France)

Zodiacal light - Star Trainee - Zodiacal light - Star trails - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 9 March 2007 at sunset, Treguennec (Finistere - France). The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. 6 minutes exposure, March 9 2007, sunset, Treguennec (Finistere - France)

Laurent Laveder

PIX4581475

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