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11/11/2012. C.Barbieri Astronomia AA 2006/07. 2. La Parallasse. Il fenomeno della parallasse ? dovuto alla distanza finita dell\'astro dall\'osservatore. Osservatori situati in diverse localit?, o lo stesso osservatore che si muova a causa della rotazione diurna o della rivoluzione annua, vedranno l\'

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