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・ NGC 5838
・ NGC 584
・ NGC 5866
・ NGC 5866 Group
・ NGC 5879
・ NGC 5882
・ NGC 5886
・ NGC 5890
・ NGC 59
・ NGC 5907
・ NGC 5921
・ NGC 5925
・ NGC 5929
・ NGC 5930
・ NGC 595
NGC 5962
・ NGC 5964
・ NGC 5970
・ NGC 5985
・ NGC 5986
・ NGC 5999
・ NGC 60
・ NGC 6000
・ NGC 6005
・ NGC 602
・ NGC 6025
・ NGC 6027
・ NGC 6027a
・ NGC 6027b
・ NGC 6027c


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NGC 5962 : ウィキペディア英語版
NGC 5962

NGC 5962 is a spiral galaxy in the constellation Serpens Caput and is the brightest member of the Serpens galaxy cluster. Along with a populated nucleus, it has a relatively large core, but a small central bulge, in which spiral arms begin to unfurl. It appears to have three smaller, orange-hued, dwarf galaxy satellites.
About six solar masses of material form into stars every year in NGC 5962. It is an 11.3 magnitude object that appears 2.5' × 1.5' in the night sky at 90 million light years away, but is still associated with the Virgo supercluster. It has a right ascension of 15h 36.5m and a declination of 16°36'.
==Discovery==
NGC 5962 was discovered by British astronomer Sir. William Herschel in 1784 using his Newtonian reflector, the largest telescope in the world at that time.

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 5962」の詳細全文を読む



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