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・ NGC 3550
・ NGC 3552
・ NGC 3553
・ NGC 3554
・ NGC 3561
・ NGC 3576
・ NGC 358
・ NGC 3593
・ NGC 3596
・ NGC 36
・ NGC 3603
・ NGC 3603-A1
・ NGC 3603-B
・ NGC 3603-C
・ NGC 3607
NGC 362
・ NGC 3621
・ NGC 3626
・ NGC 3628
・ NGC 3669
・ NGC 37
・ NGC 371
・ NGC 3718
・ NGC 3738
・ NGC 3766
・ NGC 3783
・ NGC 38
・ NGC 3808A
・ NGC 3808B
・ NGC 381


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NGC 362 : ウィキペディア英語版
NGC 362

NGC 362 (Caldwell 104) is a globular cluster located in the constellation Tucana in the Southern Hemisphere, slightly north of the Small Magellanic Cloud. It was discovered on August 1, 1826 by James Dunlop.〔(【引用サイトリンク】url=http://spider.seds.org/spider/MWGC/n0362.html )〕 It is visible to the naked eye in dark skies, and is an impressive sight in a telescope, although it is somewhat overshadowed by its larger and brighter neighbour 47 Tucanae.
The stars of NGC 362 have an average metallicity higher than the stars in most globulars. This implies that NGC 362 is a relatively young globular cluster.〔 It also has an overabundance of binary stars, and an exceptionally tight core 13 light-years in diameter.〔 The orbit of NGC 362 is highly eccentric, taking it to within 3,260 light-years of the galactic center.〔
==See also==

* List of globular clusters

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「NGC 362」の詳細全文を読む



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