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・ NGC 151
・ NGC 1512
・ NGC 1514
・ NGC 1528
・ NGC 1531
・ NGC 1532
・ NGC 1533
・ NGC 1535
・ NGC 1545
・ NGC 1553
・ NGC 1554
・ NGC 1555
・ NGC 1559
・ NGC 1560
・ NGC 1566
NGC 1569
・ NGC 157
・ NGC 1579
・ NGC 1592
・ NGC 16
・ NGC 1637
・ NGC 1647
・ NGC 1664
・ NGC 1672
・ NGC 1705
・ NGC 1721
・ NGC 1723
・ NGC 1725
・ NGC 1728
・ NGC 1746


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NGC 1569 : ウィキペディア英語版
NGC 1569

NGC 1569 is a dwarf irregular galaxy in Camelopardalis. While this faint galaxy is not a popular amateur astronomy target, it is well studied by professional astronomers, who are interested in the history of star formation within the galaxy. The galaxy is relatively nearby. Consequently, the Hubble Space Telescope can easily resolve the stars within the galaxy. The distance to the galaxy was previously believed to be only 2.4 Mpc (7.8 Mly). However, in 2008 scientists studying images from Hubble calculated the galaxy's distance at nearly 11 million light-years away, about 4 million light-years farther than previous thought and making it a member of the IC 342 group of galaxies.〔
== Physical characteristics ==

NGC 1569 is smaller than the Small Magellanic Cloud, but brighter than the latter or the Large Magellanic Cloud

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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