Poyasnenie: Zvezdy chasto sobirayutsya v gruppy. Sredi bolee 200 sharovyh zvezdnyh skoplenii, obrashayushihsya vokrug centra nashei Galaktiki Mlechnyi Put', 47 Tukana - vtoroe po yarkosti, ustupaya tol'ko skopleniyu Omega Centavra. Izvestnoe takzhe kak 47 Tuc ili NGC 104, ono vidno tol'ko v Yuzhnom polusharii Zemli. Neudivitel'no, chto ono posluzhilo podhodyashim ob'ektom dlya pervyh nablyudenii na novom gigantskom 10-metrovom Bol'shom Yuzhno-Afrikanskom teleskope (Southern African Large Telescope - SALT) na proshloi nedele. Zdes' pokazano poluchennoe izobrazhenie. Svet ot 47 Tuc idet do nas okolo 20 tysyach let. Skoplenie mozhno uvidet' ryadom s Malym Magellanovym Oblakom v sozvezdii Tukana. Dinamika zvezd okolo centra 47 Tuc ne vpolne ponyatna, v osobennosti to, chto tam ochen' malo dvoinyh sistem.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: globular cluster - 47 Tuc - 47 Tukana - Sharovoe skoplenie Publikacii so slovami: globular cluster - 47 Tuc - 47 Tukana - Sharovoe skoplenie
Sm. takzhe: Milliony zvezd v ω Centavra Sharovoe zvezdnoe skoplenie 47 Tukana Ogromnoe sharovoe skoplenie v Gerkulese M15: plotnoe sharovoe zvezdnoe skoplenie NGC 2419: mezhgalakticheskii strannik NGC 4372 i tumannost' Temnaya shtuchka NGC 1850: v Mlechnom Puti takih net Vse publikacii na tu zhe temu >>