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Quaoar illustration
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Quaoars orbit illustration
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Interacting galaxies
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Andromeda Galaxy True-colour optical image from the Palomar Observatory Sky Survey of the Great Andromeda Galaxy (M31; NGC 224) It is 22 million li
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Spiral galaxy NGC 300 composite image
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Crab nebula and Zeta Tauri star
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Emission nebulae IC 1848 and IC 1805
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W3 starbirth region Chandra image
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Alnilam nebula NGC 1990
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Los Angeles California 1949Part of he interior of the Mt Palomar Observatory to Underwood Archives The Image Works
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Palomar Mountain California 1941The smaller observatory at the right houses the 18 refracting telescope The Image Works
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Emission nebula IC 1848
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Emission nebula NGC 2174
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Emission nebula IC 1805 This is a huge cloud of gas and dust that glows red as the hydrogen gas it contains is ionised by radiation from hot young st
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California nebula (NGC 1499)
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Bubble nebula and surrounding nebulae
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Eris and Dysnomia
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Eris dwarf planet
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Eris dwarf planet
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Orbit or Eris Computer graphic of the orbit (large oval) of the dwarf planet Eris The orbits of the other eight planets and Pluto are also shown Ea
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George Ellery Hale (1868-1938) American astronomer Director of Yerkes (1895-1905) and Mount Wilson (1904-1923) observatories Research on sunspots H
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George Ellery Hale American astronomer George Ellery Hale (1868-1938) working in his Mount Wilson observatory near Los Angeles USA Hale is using an
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Palomar Observatory dome Road approach to the dome that houses the Hale telescope at Palomar Observatory in California USA This reflector telescope
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Palomar Observatory dome USA
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Hale telescope Palomar Observatory USA
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Palomar Testbed Interferometer (PTI) The PTI is used to measure the diameters of stars the size of the emissions surrounding young stars and binary
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Palomar Hale Telescope dome
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Hale telescope View of the dome of the 5 metre (200-inch) Hale telescope at Mount Palomar California USA When this reflecting mirror telescope was
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View of 200in Hale telescope observation cage from the viewing gallery
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Saturn
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Supernova remnant Composite image showing the remains of supernova W49B This highly distorted supernova remnant lies around 26000 light years from
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W H Walter Baade Portrait of Wilhelm Heinrich Walter Baade American astronomer (1893-1960) Born in Germany he worked at the Hamburg observatory be
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200-inch Hale telescope at Palomar Observatory shown at night Built in 1948 and named for George Ellery Hale (1868-1938) Courtesy of Mount Wilson and
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Mount Palomar telescope
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Mount Palomar telescope eyepiece
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Mount Palomar Observatory This dome completed in 1948 houses the Hale Telescope named after the astronomer George Ellery Hale This mirror telescop
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Mount Palomar Observatory This dome completed in 1948 houses the Hale Telescope named after the astronomer George Ellery Hale This mirror telescop
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Carina Nebula (NGC 3372) and the star Eta Carinae (upper centre) composite image Eta Carinae is a variable hypergiant star This region is 10000 li
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Palomar Hale Telescope dome
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Hale Telescope and dome at Palomar Mountain Observatory cutaway computer artwork The Hale Telescope is an optical telescope that spans about five me
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Butterfly nebula (IC 1318) Composite optical image of the emission cloud IC 1318 a giant HII region (a region of ionised interstellar atomic hydroge
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The Christmas Tree Cluster also known as NGC 2264 is a well-known region in the Monoceros (the Unicorn) constellation The Christmas Tree Cluster t
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George Ellery Hale (1868-1938) American astronomer Director of Yerkes (1895-1905) and Mount Wilson (1904-1923) observatories Research on sunspots H
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Palomar Observatory San Diego County California c1941 From San Diego California Herz California
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Deneb and the North America Nebula
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The Andromeda Galaxy
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The Horse Head and Flame Nebulae in Orion
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The Horse Head and Flame Nebulae in Orion
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Star Betelgeuse
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Part of the Taurus Molecular Cloud in the constellation of Taurus (The Bull); the cloud lies about 450 light-years from Earth Its relative closeness
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Star 51 Pegasi
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Wide field view of the Antennae Galaxies
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Polaris designated Alpha Ursae Minoris (abbreviated Alpha UMi) commonly the North Star or Pole Star is the brightest star in the constellation of U
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200-inch Hale telescope at Palomar Observatory shown at night Built in 1948 and named for George Ellery Hale (1868-1938) Courtesy of Mount Wilson and
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Andromeda Galaxy True-colour optical image from the Palomar Observatory Sky Survey of the Great Andromeda Galaxy (M31; NGC 224) It is 22 million li
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NGC281 the Pacman Nebula
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Mizar and Alcor Star System Close-up View
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Mizar and Alcor are two stars forming a double-stars system easily visible at the naked eye in the constellation of Ursa Major Mizar is the second st
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The Hercules Globular Cluster (M13 or NGC 6205) is a globular cluster of several hundred thousand stars in the constellation of Hercules M13 is abo
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The Elephants Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constella
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Gamma Cygni Region
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The Elephants Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constella
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Cygnus Constellation
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The Cocoon Nebula
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The 5m mirror for the telescope on Mt Palomar California on its grinding and polishing machine The image was taken in 1934 when the casting of 65 t
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The Cocoon Nebula
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Cederblad 214 is one of the largest molecular cloud complexes in our Galaxy Together with NGC 7822 it forms a large region of glowing hydrogen gas
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CTB-1 is a large supernova remnant located in Cassiopeia constellation It is also catalogued as Abell 85 and LBN576 It was originally believed by Ge
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Barnard 163 is a dark nebula of dust and gas so thick that visible light cant shine through it It is observable because it obscures light from other
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Algol designated Beta Persei and known as the Demon Star is a bright multiple star in Perseus constellation located 93 light-years from Earth It i
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Albireo is the proper name of double star Beta Cygni in the Cygnus constellation It is easily visible to the naked eye as a single star but even an
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