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Images of 'Moon Dust' found, 84

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)
Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays
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 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 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 title of cosmic dust. The experiment measures particle speed, radiant direction, particle momentum, and particle kinetic energy. The particle detectors of the instrument were multi - layered arrays that were capable of measuring the velocity and energy of incident particles. It consisted of 3 sensors - East, West, and Up. It stood on 4 legs and was connected to the ALSEP central station by a cable. 11 Dec 1972
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 who first spotted the orange soil. 12 Dec 1972
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
Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Each telescope's contribution is presented in a different color: - Yellow represents the near-infrared observations of Hubble. These observations outline the energetic regions where stars are being born as well as reveal hundreds of thousands of stars. - Red represents the infrared observations of Spitzer. The radiation and winds from stars create glowing dust clouds that exhibit complex structures from compact, spherical globules to long, stringy filaments. - Blue and violet represent the X-ray observations of Chandra. X-rays are emitted by gas heated to millions of degrees by stellar explosions and by outflows from the supermassive black hole in the galaxy's center. The bright blue blob on the left side is emission from a double star system containing either a neutron star or a black hole. When these views are brought together, this composite image provides one of the most detailed
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 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 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 15: lunar ground and footprints - Apollo 15: lunar footprint
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 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 14: laser reflector - moon - Apollo 14: View of the Laser Ranging Reflector. Feb 05 1971 - The Laser Ranging Reflector LR-3 which calculates the distance from Earth to Moon. 05/02/1971. A close - up view of the laser ranging retro reflector (LR3) which the Apollo 14 astronauts deployed on the moon during their lunar surface extravehicular activity (EVA). While astronauts Alan B. Shepard Jr., commander, and Edgar D. Mitchell, lunar module pilot, descended in the Lunar Module (LM) to explore the moon, astronaut Stuart A. Roosa, command module pilot, remained with the Command and Service Modules (CSM) in lunar orbit
Apollo 15: D. Scott on the Moon - Apollo 15: David Scott gives salute beside US flag - David Scott greets the American flag. 01/08/1971. Astronaut David R. Scott, commander, gives a military salute while standing beside the deployed United States flag during the Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site. The flag was deployed towards the end of EVA-2. The Lunar Module (LM), “” Falcon,””” is partially visible on the right. Hadley Delta in the background rises approximately 4,000 meters (about 13,124 feet) above the plain. The base of the mountain is approximately 5 kilometers (about three statue miles) away. This photograph was taken by astronaut James B. Irwin, lunar module pilot. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained in lunar orbit in the Command and Service Modules (CSM). August 1st 1971
Apollo 16: C. Duke on the Moon - Apollo 16: Charles Duke near Lunar Roving Vehicle (LRV) - Charles Duke near the lunar jeep. 22/04/1972. Astronaut Charles M. Duke Jr., lunar module pilot of the Apollo 16 lunar landing mission, stands near the Lunar Roving Vehicle at Station no. 4, near Stone Mountain, during the second Apollo 16 extravehicular activity (EVA - 2) at the Descartes landing site. Light rays from South Ray crater can be seen at upper left. The gnomon, which is used as a photographic reference to establish local vertical Sun angle, scale, and lunar color, is deployed in the center foreground. Note angularity of rocks in the area
Apollo 15: J. Irwin on the Moon - James Irwin gives salute beside US flag - James Irwin greets the American flag. 01/08/1971. Astronaut James B. Irwin, lunar module pilot, gives a military salute while standing beside the deployed United States flag during the Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site. The flag was deployed towards the end of EVA-2. The Lunar Module (LM) “” Falcon”” is in the center. On the right is the Lunar Roving Vehicle (LRV). This view is looking almost due south. Hadley Delta in the background rises approximately 4,000 meters (about 13,124 feet) above the plain. The base of the mountain is approximately 5 kilometers (about 3 statute miles) away. This photograph was taken by astronaut David R. Scott, Apollo 15 commander. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar orbit. 1 Aug 1971
Apollo 15: D. Scott on the Moon - David R. Scott on the Rover during Apollo 15 EVA - 1 - David R. Scott flying the Lunar Roving Vehicle. 31/07/1971. Astronaut David R. Scott, commander, is seated in the Lunar Roving Vehicle (LRV) during the first Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site (31 July 1971). This photograph was taken by astronaut James B. Irwin, lunar module pilot. While astronauts Scott and Irwin descended in the Lunar Module (LM) “” Falcon”” to explore the Hadley - Apennine area of the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar orbit
Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon) is largely empty. Located in the constellation Fornax, the region is so empty that only a handful of stars within the Milky Way galaxy can be seen in the image. In this image, blue and green correspond to colors that can be seen by the human eye, such as hot, young, blue stars and the glow of Sun - like stars in the disks of galaxies. Red represents near - infrared light, which is invisible to the human eye, such as the red glow of dust - enshrouded galaxies.The image required 800 exposures taken over the course of 400 Hubble orbits around Earth. The total amount of exposure time was 11.3 days, taken between Sept. 24, 2003 and Jan. 16, 2004
On the October Trail. (A Navajo family.), 1907 (oil on canvas)
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Faerie flower, 1986 (acrylic on board)
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United States, 1960s: Astronauts on moon
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Dancing to Restore an Eclipsed Moon - Qágyuhl, 1914 (photogravure)
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Apollo 11 Mission Eagle Has Landed
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Ice Volcano on Triton - Illustration - Ice volcano on Triton - Cryovolcanoes and geysers of nitrogen and methane have been observed on the surface of the Triton satellite. There is evidence that the south pole of Neptune's satellite Triton is host to dozens of ice volcanoes, or geysers. One such eruption was observed to shoot a towering jet of material to a height of five miles, while the tenuous nitrogen atmosphere carried the smoky plume over 80 miles “” downwind.” The eruptive material is believed to be a combination of liquid nitrogen, dust, and methane compounds driven by seasonal heating from the Sun
Mars: Olympus Mons - Illustration - Artist's view of the volcano Olympus Mons on Mars. Above, in the sky, the Deimos and Phobos satellites are represented. The northwest side of Olympus Mons' 20,000 foot scarps cast long shadows into the water mist and dust - filled atmosphere over the plains of the Tharsis Bulge. In the sky immediately above Olympus Mons' caldera are, left to right, Mars' satellites Deimos and Phobos. Nearly as large as the state of Arizona and three times the height of Mount Everest, Olympus Mons is the largest volcano - - and mountain - - in the Solar System. It is thought to be very old, though its last eruption may have been as (geologically) recent as 40 million years ago. Olympus Mons may yet still be an active volcano
Mars: Phobos breaks apart - Illustration - Phobos breaking up to form ring - Illustration - Artist's view of Phobos, the largest of Mars's two satellites, which due to its proximity to the planet Mars will break in 20 to 50 million years. The larger pieces will crush on Mars, forming new crateres, but the smaller ones and the dust should remain in suspension, in orbit and leave all around Mars to form a ring. Phobos, one of Mars' moons, is getting closer to the planet and in several million years Phobos will break apart upon reaching the Roche limit, and become a set of rings
Moon, planets and zodiacal light - Paranal observatory - Paranal observatory, Moon, planets and zodiacal light - Near the horizon, the Moon with Venus planets (the brightest at the bottom right of the Moon), Mercury (on the right of the Moon) and Mars (on the top right of the Moon); above, the zodiacal light. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plan of the Solar System. September 1, 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction near the horizon. Above is zodiacal light. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. Paranal Observatory, Chile. Sep 1st 2008
DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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Spaceship Tug and Space Station - Artist's View - Trans-Lunar space tug and the International Space Station - A towing spaceship joins the International Space Station (ISS) to bring material to the Moon. A trans-lunar space tug departs the International Space Station (ISS)* in preparation for retrieving a lunar lander currently in Earth orbit. What might be mistaken for wings are in fact solar voltaic panels for converting sunlight into electricity, just like those that adorn the ISS. Over two hundred miles below is the Atlantic Ocean, the Canary Islands, and the west coast of Saharan Africa. Long clouds of dust can be seen blowing westward off Morocco. If advances in astronautical engineering continue and lunar exploration becomes a regular activity it may become cost-effective to place a dedicated space tug into permanent orbit. Such a craft could serve the same purpose as the Apollo Command Modules did in the 1970s - ferrying astronauts and lunar landers between Earth orbit and lunar orbit - with the exception that this space tug could make the trip multiple times. suggestion only
DEU, Germany, Dortmund: A delegation of scientists from the USSR visited …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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DEU, Germany, Dortmund: A delegation of scientists from the USSR …, 1973 (photo)
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Khusrau listening to Barbad playing the lute. (Inscription: over pavilion 'May this festive assembly be as rain to the garden and may the light of the countenance of the Shah be bright. From the dome of the heavens, as long as the sun and the moon exist, may the assembly be adorned with the person of the Shah'. Round the carpet: 'With the furnishing of your two eyes you make a bridal chamber of that dwelling. In every place you travel you wish to make the dust into a road there. How pleasant . . . with one another'). (Mirza 'Ali)
Lunar Vehicle Prototype - Crew Mobility Chassis Prototype - Crew Mobility Chassis Prototype as part of the constellation program that is expected to take men to the Moon around 2020. The Crew Mobility Chassis Prototype is Nasa's new concept for a lunar truck. Researchers are trying it out at Moses Lake, Wash., as part of a series of tests of lunar surface concepts. One feature is its high mobility. Each set of wheels can pivot individually in any direction, giving the vehicle the ability to drive sideways, forward, backward and any direction in between - important if the truck becomes mired in lunar dust, needs to zigzag down a steep crater wall or parallel park at its docking station. NASA currently is building the spacecraft and systems to return to the moon by 2020
Astronauts explore Callisto - Illustration: Astronauts explore the erodes peaks of Callisto - Astronauts among eroded peaks of its moon Callisto - Several square miles of the surface is dominated by towering spires of ice, 260 to 330 feet (80 to 100 m) tall. While composed mostly of ice, the spires also contain some darker dust, which absorbs heat from the Sun. As the ice erodes, the dark material apparently slides down and collects in low-lying areas. As the ice continues to vaporize, the dark material accumulates and the erosion process accelerates
Milky way all around the horizon and Gegenschein - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up in the sky. When all these conditions are met, being very close to what the “” darkest””” sky could be, the very faint Gegenschein becomes visible. Like the zodiacal light, the gegenschein is sunlight reflected by interplanetary dust. Most of this dust is orbiting the sun in about the ecliptic plane. The Gegenschein is clearly visible covering most of the right side of the picture. The Large (LMC) and Small (SMC) Magellanic clouds are visible to the left, Orion constellation with Barnard loop to the top, California Nebula and 'tiny' Andromeda galaxy to the right while the Milky Way is visible all around the image on the horizon line. Bright jupiter is visible near the center of the image and bright red Eta Carina Nebula is rising on the horizon line at the very left
Nebula of the Rosette in the Unicorn - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Rosetta Nebula in the constellation Monoceros (the Unicorn) is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Issue - line image presented here in false color
Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the central region of the galaxy where a huge mass of stars is orbiting around the nucleus. This picture covers almost half a degree of sky (about the size of the full moon), but wide angle telescopes show the galaxy to be over three degrees long at its widest. Here we see only the central part of M31, the huge mass of stars that are in orbit around its nucleus. Silhouetted against this starry background are tangled sheets and curtains of dust, very reminiscent of dust clouds we see in our own galaxy. This picture was made from three black and white glass negatives. Some care has been taken to ensure that the colours seen here are realistic
Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
A Jordanian vendor prepares his produce for brisk selling ahead of Ramadan in an Amman market Decemb.., 1999 (photo)
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A Jordanian vendor prepares his produce for brisk selling ahead of Ramadan in an Amman market Decemb.., 1999-12-08 (photo)
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JORDANIAN VEGETABLE VENDOR PREPARES FOR RAMADAM, 1999-12-08 (photo)
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JORDANIANS PREPARE FOR RAMADAM, 1999-12-08 (photo)
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Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m telescope on Kitt Peak with the Mosaic camera, and is presented here in false color (hydrogen alpha, OIII oxygen, and SII sulfur red respectively, green and blue, using five ten - minute exposures each). The Rosette is a prominent star formation region, glowing due to ultraviolet light from the young, hot, blue stars whose winds also cleared the central hole. It is enormously large on the sky, covering more than six times the area of the full moon
The Rosette nebula in Monoceros - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas situated about 5500 years from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This composite mosaic (Hybrid Image) was assembled from multiple frames taken at different focal lengths with different instruments. The image data included approximately 9 hours of hydrogen alpha filtered data and was acquired using an AP155 (F7), FSQ 106 (F5), STL11000. The composite was assembled using Adobe Photoshop 6.
Oslo, 19700406 The Geological Museum exhibits its material from the lunar fashion Apollo 12 ..., 1970 (photo)
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Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. This colorful image is a large - scale composite mosaic assembled from data collected at a variety of different wavelengths. Views at visible wavelengths appear blue, near - infrared light is depicted as green, and mid - infrared data is portrayed as red. The result is a contrast between structures seen in visible light (blue) and those observed in the infrared (yellow and red). The image covers an area about two times that of a full moon. The red filaments stretching across the Spitzer image denote the presence of polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by surrounding i
Center of the particular galaxy Arp 220 in the Serpent - Heart of the galaxy Arp 220 - The galaxy Arp 220 (IC 4553) is about 250 million years away - light from Earth. Designee in the 1960s as a particular galaxy, today it is defined as an ultra-aluminous infrared galaxy. The Hubble space telescope photographed its heart in April 1997 in infrared light and discovered that its nucleus had two spiral galaxies colliding. The two nuclei (the two light points in the center) are 1200 light years apart and orbit around each other. This collision caused a tremendous flare of new stars. The Hubble Space Telescope's Near Infrared Camera and Multi - Object Spectrometer (NICMOS) has uncovered a collision between two spiral galaxies in the heart of the peculiar galaxy called Arp 220. The collision has provided the spark for a burst of star formation. The bright, crescent moon - shaped object is a remnant core of one of the colliding galaxies. The core is a cluster of 1 billion stars. The core's half - moon shape suggests that its bottom half is obscured by a disk of dust about 300 light - years across. This disk is embedded in the core and may be swirling around a black hole. The core of the other colliding galaxy is the bright round object to the left of the crescent moon - shaped object. Both cores are about 1,200 light - years apart and are orbiting each other. Arp 220, located 250 million light - years away in the constellation Serpens, is the 220th object in Halton Arp's Atlas of Peculiar Galaxies. The image was taken April 5, 1997
The comet NEOWISE (C/2020 F3) at dawn from Mount Aigoual, Cévennes, France, Sunday 12th of July 2020 (photo)
Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. The image is a large - scale mosaic assembled from individual photographs obtained with the Infraared Array Camera (IRAC) aboard Spitzer. The image covers an area about two times that of a full moon. The mosaic is a composite of images obtained at mid - infrared wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). The brightest infrared cloud near the top center corresponds to DR21, which presumably contains a cluster of newly forming stars at a distance of 10,000 light - years. Protruding out from DR21 toward the bottom left of the image is a gaseous outflow (green), containing both carbon monoxide and molecular hydrogen. Data from the Spitzer spectrograph, which breaks light into its constitutes
Total lunar eclipse, 3 March 2007
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Total lunar eclipse, 3 March 2007
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Total lunar eclipse, 3 March 2007
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Total lunar eclipse, 3 March 2007
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Total lunar eclipse, 3 March 2007
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COMPILATION OF MOONSHOTS TAKEN FROM EARTH AND HUBBLE TELESCOPES, 1999-04-16 (photo)
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Detail in the nebula Omega (M17) - Part of M17 nebula - Detail in the nebula Omega (M17), a region of star formation. Image obtained from the 3.5-metre NTT telescope of the European Observatory of La Silla in Chile. The Omega Nebula (M17) is one of the youngest and most massive star - forming regions in the Milky Way. Active star - birth started a few million years ago and continues through today. The brightly shining gas shown in this picture is just a blister erupting from the side of a much larger dark cloud of molecular gas. The dust that is so prominent in this picture comes from the remains of massive hot stars that have ended their brief lives and ejected material back into space, as well as the cosmic detritus from which future suns form. Three - colour composite image of the Omega Nebula (Messier 17), based on images obtained with the EMMI instrument on the ESO 3.58 - metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the image. It spans an angle equal to about one third the diameter of the Full Moon, corresponding to about 15 light - years at the distance of the Omega Nebula
Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - called “” T Tauri””” class, a type that is quite common in star - forming regions. T Tauri stars are in the early stages of stellar evolution and display various observable characteristics of this phase, e.g. emission at visible and infrared wavelengths due to the accretion of matter left over from their formation, as well as X - ray emission. The nebulosity seen in this picture is mostly due to reflection of the stellar light by small dust particles. The stars in the R Coronae Australis complex do not emit sufficient ultraviolet light to ionize a substantial fraction of the surrounding hydrogen, and thus cause this gas to glow. Also visible are so - called Herbig - Haro objects, i.e., dense clumps of gas ejected from the immediate vicinity of newly formed stars with velocities of about 200 km/sec. The observations were obtained on the night of 30 August 2000
Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking for star - forming regions like these. He catalogued 85 new such regions, named Gum 1 to85 (Gum Crater on the moon was also named in his honor). Going counter - clockwise from Gum 22, the other catalogued nebulae in the image are Gum 23 (part of same cloud as 22), IRAS 09002 - 4732 (orange cloud near center), Bran 226 (upper cloud of the two at lower left), and finally Gum 25 at far lower left. There are also several smaller and/or more distant regions scattered throughout the image that have yet to be catalogued. Most of the regions are thought to be part of our local Orion spiral arm spur in the Milky Way galaxy. Their distances range from about 4,000 to 10,000 light - years away. Notice the very bright green star near the lower right portion of the image. You can tell it's a star because it appears to have 'spikes' sticking out of it (diffraction spikes like these are an optical effect caused by the structure of the te