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Bilder zu 'J Round' gefunden, 4,712

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Oslo, 19480919. Football match Norway - Sweden (3-5) ..., 1948 (photo)

Oslo, 19480919. Football match Norway - Sweden (3-5) ..., 1948 (photo)

Aktuell

NTB8600638

Oslo 19480919. Football match Norway - Sweden (3-5). Enthusiasm at Ullevål Stadium when the …, 1948 (photo)

Oslo 19480919. Football match Norway - Sweden (3-5). Enthusiasm at Ullevål Stadium when the …, 1948 (photo)

Aktuell

NTB8909793

Crete vue de l'espace - Crete seen from space - La Crete vue from the International Space Station (ISS) on 22 July 2011. Crete is the largest and most heavily populated island of Greece (or the Hellenic Republic). The island stretches approximately 260 kilometers (161 miles) from west to east, and it is roughly 60 kilometers (37 miles) across at its widest point. The rugged terrain of Crete includes mountains, plateaus, and several deep gorges. The largest city on the island, Heraklion, sits on the northern coastline. Several smaller islands ring Crete. Two of the largest of these, Dia and Gavdos, are sparsely populated year - round, although Gavdos hosts numerous summer visitors. The western and central parts of Crete appear surrounded by quicksilver in this astronaut photograph taken from the International Space Station. This phenomenon is known as sunglint, caused by light reflecting off of the sea surface directly towards the observer. The point of maximum reflectance is visible as

Crete vue de l'espace - Crete seen from space - La Crete vue from the International Space Station (ISS) on 22 July 2011. Crete is the largest and most heavily populated island of Greece (or the Hellenic Republic). The island stretches approximately 260 kilometers (161 miles) from west to east, and it is roughly 60 kilometers (37 miles) across at its widest point. The rugged terrain of Crete includes mountains, plateaus, and several deep gorges. The largest city on the island, Heraklion, sits on the northern coastline. Several smaller islands ring Crete. Two of the largest of these, Dia and Gavdos, are sparsely populated year - round, although Gavdos hosts numerous summer visitors. The western and central parts of Crete appear surrounded by quicksilver in this astronaut photograph taken from the International Space Station. This phenomenon is known as sunglint, caused by light reflecting off of the sea surface directly towards the observer. The point of maximum reflectance is visible as

PIX4665986

Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Fi

Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Fi

Laurent Laveder

PIX4578916

Sunrise - 22 June 2005. - Full moon rising - June 22, 2005 - Moonrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevat

Sunrise - 22 June 2005. - Full moon rising - June 22, 2005 - Moonrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevat

Laurent Laveder

PIX4578903

Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Fi

Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Fi

Laurent Laveder

PIX4578927

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

PIX4583529

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 hal

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 hal

PIX4613739

Oslo 19480919. Football match Norway - Sweden (3-5). Enthusiasm at Ullevål Stadium when the …, 1948 (photo)

Oslo 19480919. Football match Norway - Sweden (3-5). Enthusiasm at Ullevål Stadium when the …, 1948 (photo)

Aktuell

NTB8913020

Colt 1911 A1 pistol. The stock has chequered walnut grips. The butt incorporates the magazine and there is a magazine release catch on the underside of the butt. The detachable box magazine takes seven rounds. The frame incorporates the trigger guard. The cocking slide takes up the whole of the top of the weapon. Semi-automatic, with recoil action. Rounds are thrust up into the breech by the magazine spring when the action is to the rear. After cocking for the first round, the weapon is automatically reloaded. The action is semi-automatic as the trigger has to be squeezed for each seperate shot. The barrel is rifled, for the most part enclosed within the slide. The barrel has a blade foresight and a notch rear sight. The calibre is 0.45in. Supplies of these pistols were shipped to Britain during 1915/16. Serial numbers special to this contract were prefixed by the letter W. ©National Maritime Museum, Greenwich/Leemage

Colt 1911 A1 pistol. The stock has chequered walnut grips. The butt incorporates the magazine and there is a magazine release catch on the underside of the butt. The detachable box magazine takes seven rounds. The frame incorporates the trigger guard. The cocking slide takes up the whole of the top of the weapon. Semi-automatic, with recoil action. Rounds are thrust up into the breech by the magazine spring when the action is to the rear. After cocking for the first round, the weapon is automatically reloaded. The action is semi-automatic as the trigger has to be squeezed for each seperate shot. The barrel is rifled, for the most part enclosed within the slide. The barrel has a blade foresight and a notch rear sight. The calibre is 0.45in. Supplies of these pistols were shipped to Britain during 1915/16. Serial numbers special to this contract were prefixed by the letter W. ©National Maritime Museum, Greenwich/Leemage

MMM5471608

Walther PPK presentation pistol. The stock consists of hard composite grips, the rest of the pistol is steel decorated with oak leaves.The butt incorporates the eight round magazine. The barrel is hidden by the cocking slide which takes up the whole of the top of the weapon. Semi-automatic, blowback action. The barrel is rifled. The pistol is fitted with a rear notch sight and a small blade foresight. The calibre is 7.65mm. It is in a box with a magazine, a cleaning rod and three rounds of ammuntion. Inscribed on the pistol is the serial number '293578K' and the maker's mark, 'Waffenfabrik Walther Zelia-Mehlis (Thur)' along with an eagle over 'M'. A compact and easily concealed weapon, this pistol was originally designed for detectives - PPK stands for Polizei Pistole Kriminal. It was later adopted by the Luftwaffe and German Staff Officers. This engraved example was a naval presentation piece to a German Naval Officer. ©National Maritime Museum, Greenwich/Leemage

Walther PPK presentation pistol. The stock consists of hard composite grips, the rest of the pistol is steel decorated with oak leaves.The butt incorporates the eight round magazine. The barrel is hidden by the cocking slide which takes up the whole of the top of the weapon. Semi-automatic, blowback action. The barrel is rifled. The pistol is fitted with a rear notch sight and a small blade foresight. The calibre is 7.65mm. It is in a box with a magazine, a cleaning rod and three rounds of ammuntion. Inscribed on the pistol is the serial number '293578K' and the maker's mark, 'Waffenfabrik Walther Zelia-Mehlis (Thur)' along with an eagle over 'M'. A compact and easily concealed weapon, this pistol was originally designed for detectives - PPK stands for Polizei Pistole Kriminal. It was later adopted by the Luftwaffe and German Staff Officers. This engraved example was a naval presentation piece to a German Naval Officer. ©National Maritime Museum, Greenwich/Leemage

MMM5471781

Mugby Junction Galop, c1880 (chromolithograph on paper)

Mugby Junction Galop, c1880 (chromolithograph on paper)

Lee, Thomas Wales (1833-1910)

IGM8836222

Grinding Corn (litho)

Grinding Corn (litho)

Kingman, Eduardo (1913-1997)

DMA1067009

Remington rolling block pistol. The pistol is half-stocked with a flared butt (no cap) secured by steel strips back and front. The lock is a Remington rolling block in two parts. The hammer has a knurled spur with half and fully cocked positions. The block is lightly spring-loaded and contains a striker, with a knurled protrusion on its right side and a notch for a rear sight on top. It is moved to the rear to permit the loading of a single round and then pushed forward to close, but not to lock the breech. It can only be moved when the hammer is at full cock. The breech is locked shut when the hammer has moved forward to engage the rear of the striker in the block. The entire lock is enclosed within a case-hardened steel box, the trigger within an oval trigger guard. The barrel is of circular section with large blade foresight and rifled. The Calibre is 0.5in. ©National Maritime Museum, Greenwich/Leemage

Remington rolling block pistol. The pistol is half-stocked with a flared butt (no cap) secured by steel strips back and front. The lock is a Remington rolling block in two parts. The hammer has a knurled spur with half and fully cocked positions. The block is lightly spring-loaded and contains a striker, with a knurled protrusion on its right side and a notch for a rear sight on top. It is moved to the rear to permit the loading of a single round and then pushed forward to close, but not to lock the breech. It can only be moved when the hammer is at full cock. The breech is locked shut when the hammer has moved forward to engage the rear of the striker in the block. The entire lock is enclosed within a case-hardened steel box, the trigger within an oval trigger guard. The barrel is of circular section with large blade foresight and rifled. The Calibre is 0.5in. ©National Maritime Museum, Greenwich/Leemage

MMM5471617

Grinding Sugar Cane, 1946 (litho)

Grinding Sugar Cane, 1946 (litho)

Beltrán, Alberto (1923-2002)

DMA1066976

Peasants of Tláhuac, 1946 (litho)

Peasants of Tláhuac, 1946 (litho)

Bustos, Arturo Garcia (b.1926)

DMA1066982

Ritual of the Huichol Indian Tribe, 1946 (litho)

Ritual of the Huichol Indian Tribe, 1946 (litho)

Bracho, Ángel (1911-2005)

DMA1066983

Pottery Maker, 1946 (litho)

Pottery Maker, 1946 (litho)

Ocampo, Isadoro (b.1910)

DMA1066979

Fighting Cocks (litho)

Fighting Cocks (litho)

Chavez, Edward (b.1917)

DMA1066998

Woman in the Coal Line-Up, 1947 (litho)

Woman in the Coal Line-Up, 1947 (litho)

Aguirre, Ignacio (1900-90)

DMA1066975

Silver Mine Worker, 1946 (litho)

Silver Mine Worker, 1946 (litho)

Mora, Francisco (1922-2002)

DMA1066980

Fishwives, 1940 (litho)

Fishwives, 1940 (litho)

Dosamantes, Francisco (b.1911)

DMA1067008

Working with Ixtle, 1946 (litho)

Working with Ixtle, 1946 (litho)

Castro-Pacheco, Fernando (b.1918)

DMA1066984

Henequen Plant, 1946 (litho)

Henequen Plant, 1946 (litho)

Zalce, Alfredo (1908-2003)

DMA1066981

High Pressure Steamboat Mayflower, 1855 (colour litho)

High Pressure Steamboat Mayflower, 1855 (colour litho)

Currier, Nathaniel (1813-88)

XDM1067002

Lumber Workers, 1946 (colour litho)

Lumber Workers, 1946 (colour litho)

Zalce, Alfredo (1908-2003)

DMA1066977

The Market, 1946 (colour litho)

The Market, 1946 (colour litho)

O'Higgins, Pablo (1904-1983)

DMA1066978

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

PIX4623194

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

PIX4623200

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

PIX4665079

Automatic pistol. The stock consists of blue steel with chequered rubber grips. The butt incorporates the magazine and there is a magazine release latch on the underside of the butt. A lanyard ring is fitted to the heel of the butt. The back of the slide is vertically fluted to afford a grip when cocking. The magazine contains seven rounds. The lock is automatic. The barrel is round with a foresight. The calibre is 0.455in. The pistol is inscribed on the barrel 'WEBLEY ; SCOTT LTD/PISTOL SELF-LOADING 455 MARK I 1913'. There are proof marks on the trigger and back of action. The pistol is in a brown leather case lined with red baize containing a cleaning rod. The outside of the case is inscribed 'G.R.T', the inside lid of the case 'W W GREENER/Gun and Ammunition Maker/WINNER AT ALL THE GREAT LONDON GUN TRIALS/Prize Works St Mary's Square, Birmingham AND 29 PALL MALL LONDON S W'. The Webley & Scott Mark I pistol was approved for Government service on May 19 1913 and adopted by the Royal

Automatic pistol. The stock consists of blue steel with chequered rubber grips. The butt incorporates the magazine and there is a magazine release latch on the underside of the butt. A lanyard ring is fitted to the heel of the butt. The back of the slide is vertically fluted to afford a grip when cocking. The magazine contains seven rounds. The lock is automatic. The barrel is round with a foresight. The calibre is 0.455in. The pistol is inscribed on the barrel 'WEBLEY ; SCOTT LTD/PISTOL SELF-LOADING 455 MARK I 1913'. There are proof marks on the trigger and back of action. The pistol is in a brown leather case lined with red baize containing a cleaning rod. The outside of the case is inscribed 'G.R.T', the inside lid of the case 'W W GREENER/Gun and Ammunition Maker/WINNER AT ALL THE GREAT LONDON GUN TRIALS/Prize Works St Mary's Square, Birmingham AND 29 PALL MALL LONDON S W'. The Webley & Scott Mark I pistol was approved for Government service on May 19 1913 and adopted by the Royal

MMM5471597

Automatic pistol. The stock consists of blue steel with chequered rubber grips. The butt incorporates the magazine and there is a magazine release latch on the underside of the butt. A lanyard ring is fitted to the heel of the butt. The back of the slide is vertically fluted to afford a grip when cocking. The magazine contains seven rounds. The lock is automatic. The barrel is round with a foresight. The calibre is 0.455in. The pistol is inscribed on the barrel 'WEBLEY ; SCOTT LTD/PISTOL SELF-LOADING 455 MARK I 1913'. There are proof marks on the trigger and back of action. The pistol is in a brown leather case lined with red baize containing a cleaning rod. The outside of the case is inscribed 'G.R.T', the inside lid of the case 'W W GREENER/Gun and Ammunition Maker/WINNER AT ALL THE GREAT LONDON GUN TRIALS/Prize Works St Mary's Square, Birmingham AND 29 PALL MALL LONDON S W'. The Webley & Scott Mark I pistol was approved for Government service on May 19 1913 and adopted by the Royal

Automatic pistol. The stock consists of blue steel with chequered rubber grips. The butt incorporates the magazine and there is a magazine release latch on the underside of the butt. A lanyard ring is fitted to the heel of the butt. The back of the slide is vertically fluted to afford a grip when cocking. The magazine contains seven rounds. The lock is automatic. The barrel is round with a foresight. The calibre is 0.455in. The pistol is inscribed on the barrel 'WEBLEY ; SCOTT LTD/PISTOL SELF-LOADING 455 MARK I 1913'. There are proof marks on the trigger and back of action. The pistol is in a brown leather case lined with red baize containing a cleaning rod. The outside of the case is inscribed 'G.R.T', the inside lid of the case 'W W GREENER/Gun and Ammunition Maker/WINNER AT ALL THE GREAT LONDON GUN TRIALS/Prize Works St Mary's Square, Birmingham AND 29 PALL MALL LONDON S W'. The Webley & Scott Mark I pistol was approved for Government service on May 19 1913 and adopted by the Royal

MMM5471602

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