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16 médias trouvés pour 'Parallaxe'

Friedrich Wilhelm Bessel
Double star 61 Cygni - Binary star 61 Cygni - 61 Cygni is a binary system of two stars comparable to the Sun. Located 11.4 years - light from the Earth, 61 Cygni is the first star (after the Sun) whose distance was measured thanks to its parallax. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. 61 Cygni is a binary star system in the Constellation Cygnus at approximately 11.4 light - years distance from Earth. Composite image obtained by the Oschin telescope refractor at the Palomar Observatory, USA
Diagram of planetary parallax
Frontispiece to 'Theoria motuum planetarium et cometarum', 1744 (litho)
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Brabham Strealine (photo)
Zenith sector telescope, 1727 (iron, tin)
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Oxford heliometer, 1840-48
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Giovanni Domenico Cassini, late 17th century
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View of the 'Oxford heliometer' , 1849
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Observatory building for seven inch heliometer, Cape, 1909
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Seven inch heliometer, Cape Town, South Africa, 1909
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Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 450 years - light from Earth. Image obtained by a 50 cm telescope, 42 poses of 15 minutes accumulated. Located in the constellation of Aquarius, the Helix is our closest planetary nebula at only 450 light years distance. It is so close that it can be telescopically seen shifting one side to the other in front of the more distant background stars as the earth moves around the sun - a phenomenon called parallax. Parallax measurements are used to trigonometrically deduce distance between an object in space and the earth. A planetary nebula results when a red giant star, near the ends of it's productive life, sheds its outer layers into space and creates a breathtaking shell of surrounding gas that early visual astronomers likened to the disks of planets. This planetary spans approximately 1.5 light years and is still expanding. The name associated with the Helix is derived from the cork - screw appearance that resulted from the spin induced by the nebula's central star as its outer layers were thrown off into the surrounding vacuum of space. This image of the Helix Nebula, photographed by R. Jay GabAny was the result of combining forty two, fifteen minute digital exposures taken during the month of September 2005, through a remotely controlled twenty inch Ritchey - Chretien telescope with an eleven mega - pixel camera at f/8. The remote observatory is located in Cloudcroft, New Mexico City, 7,000 feet above sea level in the Sacramento Mountains