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Mounting a 15 millimeter cannon, 1916 (w/c)
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding material to collapse into dense clumps that are the birthplaces of new stars. The region, called RCW120, is about 4200 light years from Earth, towards the constellation of Scorpius. A hot, massive star in its centre is emitting huge amounts of ultraviolet radiation, which ionises the surrounding gas, stripping the electrons from hydrogen atoms and producing the characteristic red glow of so - called H - alpha emission. Here, the submillimetre emission is shown as the blue clouds surrounding the reddish glow of the ionised gas (shown with data from the SuperCosmoS H - alpha survey). The image also contains data from the Second Generation Digitized Sky Survey (I - band shown in blue, R - band shown in red). As this ionised region expands into space, the associated shock wave sweeps up a layer of the surrounding cold interstellar gas and cosmic dust. This layer b
Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to discover. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, launched in 2009, studies the formation of galaxies, stars and planetary systems in the infrared. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) studies the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory is bigger and better than any of its predecessors. Moreover, it observes at wavelengths never covered before. It is located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Observatory will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope
Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Observatory will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope
Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to discover. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Satellite Herschel - Illustration - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Satellite Herschel - Illustration - Ariane 5 stage with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched on May 14 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Observatory will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope
Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This composite image reveals the lobes and jets that escape from the center of this active galaxy, or replaces a black hole. To produce this image, three instruments observing in different wavelengths were used; in orange, the data obtained by the APEX submillimetre telescope, in blue the X-ray image obtained by the Chandra space telescope, in visible, the image obtained by the 2,2m MPG telescope of La Silla in Chile. Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy's central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870 - micron submillimetre data, from LABOCA on APEX, are shown in orange. X - ray data from the Chandra X - ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the background stars and the galaxy's characteristic dust lane in close to “” true colour””
Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Launched on May 14 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Mirror of the Herschel satellite - Herschel spacecraft's mirror - Inspection of the mirror of the European Herschel satellite. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. The gigantic telescope of ESA's space - based infrared observatory, Herschel, is being prepared to be assembled with its spacecraft. Herschel's telescope, which will carry the largest mirror ever flown in space, has been delivered to ESA's European Space Research and Technology Centre, ESTEC, where engineers and scientists are busy with the final steps that will prepare the infrared observatory for launch in 2009. ESA's Herschel Space Observatory will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope
Herschel satellite - Herschel spacecraft being prepared for acoustic tests - The European satellite Herschel prepares for acoustic tests in June 2008. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. A picture of the Herschel spacecraft being prepared for acoustic tests. On 5 and 6 June 2008, the Herschel spacecraft successfully passed its acoustic tests. During the tests, the spacecraft was subjected to acoustic noise, generated to simulate the noise levels during launch, at the European Space Research and Technology Centre's Large European Acoustic Facility (LEAF). ESA's Herschel Space Observatory will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory will be bigger and better than any of its predecessors. Moreover, it will observe at wavelengths never covered before. It will be located 1.5 million kilometers away from Earth, farther than any previous space telescope. Due for launch in 2009, Herschel is one the Cornerstone missions ESA's Horizons 2000 programme. Herschel is a key project space astronomy in the next millennium
Galactic Center Region - Center of our galaxy (photo)
Mauna Kea Observatory - SMA Radiotelescope - Mauna Kea Observatory - SMA Radiotelescope - The new sub-millimeter array of the Mauna Kea Observatory
Mauna Kea Observatory - SMA Radiotelescope - photographer - The new sub-millimetric SMA (Sub Millimeter Array) network of the Mauna Kea Observatory
Mauna Kea Observatory. Radiotelescopes - Radiotelescopes at Mauna Kea Observatory - View of the Mauna Kea Observatory located 4200 metres above sea level in Hawaii, USA. Here, the radiotelescopes with in the foreground the CSO (Caltech Submillimeter Observatory), then the JCMT (James Clerk Maxwell Telescope) and the SMA antenna network (Sub - Millimeter Array). Foreground is CSO (Caltech Submillimeter Observatory), then, JCMT (James Clerk Maxwell Telescope) and background is the antennas network SMA (Sub - Millimeter Array)
Senator Burton Wheeler speaks at peace rally. Washington, D.C. June 8, 1940. Isolationist Democrat Wheeler criticized proposals to sell rifles, 75 millimeter guns and ammunition 'officially described as obsolete' to Britain
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British army officer looks at a destroyed German dual purpose 88 millimeter gun. It was put out of action by British Artillery near El Gubbi. c. 1940-42 during World War 2
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Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. Its construction is due to be completed in 2010. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Apollo 11: lunar rock - Apollo 11: lunar rock - Microscope photo of the 10022 lunar rock sample brought by astronauts from the Apollo 11 mission. September 1969. This is a photo micrograph of lunar sample 10022. Magnification one inch equals one - tenth millimeter. The light blue and white mineral is plagioclase. The black is ilmenite, and the blue and/or green and/or orange and/or yellow and/or red mineral is pyroxene. The large pyroxene is a phenocryst that had been partially resorbed. The lunar samples collected by astronauts Neil A. Armstrong and Edwin E. Aldrin Jr. during the Apollo 11 lunar landing mission have been subjected to extensive tests and examinations at the Manned Spacecraft Center's Lunar Receiving Laboratory. September 1969
240-mm steel gun used to defend coasts, engraving, c. 1867
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120-mm gun used during siege, engraving, c. 1867
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Weapons of the Cambodian Civil War 1967 1975-Cambodia
Weapons of the Cambodian Civil War 1967 1975-Cambodia
155-mm gun used for sieges, engraving, c. 1867
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220-33 mortar used during sieges, engraving, c. 1867
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Weapons of the Cambodian Civil War 1967 1975-Cambodia
Weapons of the Cambodian Civil War 1967 1975-Cambodia
Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded buttes in the distance contain sulfate minerals, perhaps indicating a change in the availability of water when they formed. Some of the layering patterns on higher levels of Mount Sharp in the background are tilted at different angles than others, evidence of complicated relationships still to be deciphered. The scene spans from southeastward at left to southwestward at right. The component images were taken on April 10 and 11, 2015, the 952nd and 953rd Martian days (or sols) since the rover's landing on Mars on Aug. 6, 2012, UTC (Aug. 5, PDT). Images in the central part of the panorama are from Mastcam's right - eye camera, which is equipped with a 100 - millimeter - focal - length telephoto lens. Images used in outer portions, including the most remote portions of the mountain in the scene, were taken with Mastcam's left - eye camera, using a wider - angle, 34 - millimeter lens
II. WK, armament industry, 1942 (photo)
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Eastman Kodak Company's new 3700 (L) and 3100 Advantix cameras utilizing the Advanced Photo System, .., 1996-02-01 (photo)
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NEW ZEALAND DAVID BOLSPAD RAISES HIS AXE AFTER BECOMING WORLD CHAMPION WOODCHOPPER IN SYDNEY, 2000-04-24 (photo)
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East African Mobile Artillery (b/w photo)
Arc de fog - Fogbow - Arc de brume observed in Brittany on February 23, 2008. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on Feb 23, 2008. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
A ROMANIAN OFFICER CHECKS A SUB-MACHINE GUN AT EXHIBITION IN BUCHAREST, 1999-10-26 (photo)
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Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Arc de fog - Fogbow - Arc de brume observed in Brittany on February 23, 2008. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on Feb 23, 2008. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Arc de fog - Fogbow - Arc de brume observed in Brittany on 16 December 2008. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on December 16, 2008. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Vietnam War
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Indy Car driver Emerson Fittipaldi works out under the guidance of Occupational Therapist Elisa Pris.., 1996-09-19 (photo)
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Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
MEDICAL EXAMINERS EMPLOYEES REMOVE A BODY FROM MESA ARIZONA HOME, 2002-12-10 (photo)
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ARIZONA MASS MURDER SUSPECT CROWLEY IS PHOTOGRAPHED IN JAIL IN PHOENIX, 2002-12-10 (photo)
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Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Spitzer were found in four dark cores, or stellar “” incubators,””” where stars are born. Astronomers using data from the Institute of Radioastronomy millimeter telescope in Spain had previously identified these cores but thought they were not quite ripe for stars. Spitzer's highly sensitive infrared eyes were able to penetrate all four cores to reveal rapidly growing embryos. Astronomers can actually count the individual embryos tucked inside the cores by looking closely at the Spitzer image taken by its infrared array camera (top right). This instrument has the highest spatial resolution of Spitzer's imaging cameras. The Spitzer image from the multiband imaging photometer (bottom right), on the other hand, specializes in detecting cooler materials. Its view highlights the relatively cool core material falling onto the Trifidi's growing embryos. The middle panel is a combination of Spitzer data from both of these instruments. The embryos are thought to have been triggered by a massiv
Dresden, historical, places, roads, districts, Residential areas Schiller …, 1987 (photo)
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Torrents of spring, 1989 (film still)
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US Army artillery crew firing a 105 millimetre howitzer
Torrents of spring, 1989 (film still)
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Notebook set to 2 millimeters, models to be reproduced, c.1890 (printing)
Notebook set to 4 millimeters. Precepts and maxims, c.1890 (print)
Notebook set to 2 millimeters, models to be reproduced, c.1890 (printing)
Notebook set to 4 millimeters, models to be reproduced, c.1890 (printing)
Notebook set to 2 millimeters. Precepts and maxims, c.1890 (print)
The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist
The atom and science: the size of atoms. A point in front of Mont Blanc represented by a millimetre. 1925 (print)
Second World War Italy 1944-Anzio
240 mm trench mortar transported by railway wagon, World War I, Italy, 20th century
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240 mm Italian trench mortar, Trench Mortars School in Susegana, World War I, Italy, 20th century
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320 mm Maggiora trench mortar, triggered by acetylene gas, Trench Mortars School in Susegana, World War I, Italy, 20th century
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240 mm trench mortar with assistants involved in carrying 67 kg bomb, to right dismantled 240 C trench mortar, Trench Mortars School in Susegana, World War I, Italy, 20th century
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Fog arc - Fogbow - Fog arc observed in La Palma, Canary Islands. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, diffraction in fog droplets is preponderant, which has the effect of refracting colors at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Fogbow in La Palma, Canary Islands
Fog arc - Fogbow - Fog arc observed in La Palma, Canary Islands. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, diffraction in fog droplets is preponderant, which has the effect of refracting colors at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Fogbow in La Palma, Canary Islands