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Sedna (minor-planet designation: 90377 Sedna) is a dwarf planet in the outermost reaches of the Solar System, orbiting the Sun beyond the orbit of Neptune. Discovered in 2003, the planetoid's surface is one of the reddest known among Solar System bodies.
Sedna's presence suggests that the previously speculated inner disk on the ecliptic does exist. Date: March 15, 2004 (original image), August 2006 (SVG conversion) Source: SVG version of Image:Oort cloud Sedna orbit.jpg, which lists the following sources: Splitzer Space Telescope Released Images about Sedna: Author
90377 Sedna; Usage on fr.wikipedia.org (90377) Sedna; Usage on ga.wikipedia.org 90377 Sedna; Usage on gl.wikipedia.org Sedna; Usage on hi.wikipedia.org ९०३७७ सेडना; Usage on hr.wikipedia.org Jan Hendrik Oort; Usage on id.wikipedia.org 90377 Sedna; Usage on it.wikipedia.org Oggetti del sistema solare più lontani dal Sole
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The Oschin Telescope was responsible for the discovery of 90377 Sedna on 2003-11-14 and Eris, the "10th Planet" on 2005-01-05 from images taken 2003-10-21. The peculiar Type Ia supernova SN 2002cx was discovered with the Oschin telescope on 2002-05-12, 21 UT. [ 7 ]
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90377 Sedna, a large trans-Neptunian object, had the provisional designation 2003 VB 12, meaning it was identified in the first half of November 2003 (as indicated by the letter "V"), and that it was the 302nd object identified during that time, as 12 cycles of 25 letters give 300, and the letter "B" is the second position in the current cycle.
This was the telescope that produced the images leading to the discovery of 50000 Quaoar in 2002, and 90377 Sedna in 2003 (published 2004) and the dwarf planet Eris. In addition to discovering thousands of asteroids , NEAT was also credited with the co-discovery (recovery) of periodic comet 54P/de Vico-Swift-NEAT and of the high proper motion ...