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The Palomar Distant Solar System Survey (P … The Palomar Distant Solar System Survey (PDSSS) was a wide-field survey aimed at finding distant trans-Neptunian objects that used the robotic 1.2 m Samuel Oschin Telescope at Palomar Observatory and the QUEST large-area CCD camera.The survey was specifically designed to identify putative members of a Sedna-like population with perihelia greater than 45 AU. The limiting magnitude of this study was 21.3 in the R-band, it was sensitive out to distances of 1000 AU, and 12,000 square degrees of sky were searched. This observing program was responsible for the discovery of 25 minor planets including trans-Neptunian objects and centaurs. (309239) 2007 RW10 and Gǃkúnǁʼhòmdímà ((229762) 2007 UK126) were among the objects discovered by this survey. It redetected Sedna but no other objects in Sedna-like orbits were identified.ects in Sedna-like orbits were identified.
, O Palomar Distant Solar System Survey (PDS … O Palomar Distant Solar System Survey (PDSSS) foi um amplo campo de pesquisa que visava encontrar objetos transnetunianos distantes usando o telescópio robótico Samuel Oschin de 1,2 metro do Observatório Palomar e a QUEST large-area câmera CCD. O PDSSS foi projetado especificamente para identificar possíveis membros de uma população Sedna com periélios superiores a 45 UA. A limitação de magnitude deste estudo foi de 21,3 na banda R, era sensível para distâncias de 1,000 AU, e 12.000 graus quadrados do céu foram revistados. Este programa de observação foi o responsável pela descoberta de 25 corpos menores, incluindo objetos transnetunianos e centauros. (309239) 2007 RW10 e (229762) 2007 UK126 estavam entre os objetos descobertos pelo projeto. Ele foi capaz de detectar Sedna, mas não consegui identificar outros objetos em órbitas como Sedna.icar outros objetos em órbitas como Sedna.
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1981
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March 2015
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rdfs:comment |
The Palomar Distant Solar System Survey (P … The Palomar Distant Solar System Survey (PDSSS) was a wide-field survey aimed at finding distant trans-Neptunian objects that used the robotic 1.2 m Samuel Oschin Telescope at Palomar Observatory and the QUEST large-area CCD camera.The survey was specifically designed to identify putative members of a Sedna-like population with perihelia greater than 45 AU. The limiting magnitude of this study was 21.3 in the R-band, it was sensitive out to distances of 1000 AU, and 12,000 square degrees of sky were searched. This observing program was responsible for the discovery of 25 minor planets including trans-Neptunian objects and centaurs. (309239) 2007 RW10 and Gǃkúnǁʼhòmdímà ((229762) 2007 UK126) were among the objects discovered by this survey. It redetected Sedna but no other objects in Sedna-ected Sedna but no other objects in Sedna-
, O Palomar Distant Solar System Survey (PDS … O Palomar Distant Solar System Survey (PDSSS) foi um amplo campo de pesquisa que visava encontrar objetos transnetunianos distantes usando o telescópio robótico Samuel Oschin de 1,2 metro do Observatório Palomar e a QUEST large-area câmera CCD. O PDSSS foi projetado especificamente para identificar possíveis membros de uma população Sedna com periélios superiores a 45 UA. A limitação de magnitude deste estudo foi de 21,3 na banda R, era sensível para distâncias de 1,000 AU, e 12.000 graus quadrados do céu foram revistados. Este programa de observação foi o responsável pela descoberta de 25 corpos menores, incluindo objetos transnetunianos e centauros. (309239) 2007 RW10 e (229762) 2007 UK126 estavam entre os objetos descobertos pelo projeto. Ele foi capaz de detectar Sedna, mas não consegui capaz de detectar Sedna, mas não consegu
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rdfs:label |
Palomar Distant Solar System Survey
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