NGC 147 和 NGC 185
NGC 147 and NGC 185

來源:Chuck Ayoub|發表日期:2026-02-13
在這張深空望遠鏡拍攝的肖像中,矮星系NGC 147 (左)與NGC 185 並肩而立。 這兩座罕見成像的衛星星系隸屬於M 31 ——即距地球約 250 萬光年的仙女座大螺旋星系。它們在天球上的相距不足一度(位於仙后座方向的廣闊視野中),按仙女座星系的距離換算僅約 3 . 5 萬光年,但仙女座本體遠超此畫面範圍。 仙女座更明亮著名的衛星星系M 32 和M 110 則緊鄰主星系盤。NGC 147 與NGC 185 已被確認為雙星系,構成引力穩定的雙星系統。而新近發現的暗淡矮星系仙后座II 似乎也隸屬該系統,共同構成了仙女座眾多小型衛星星系中引力束縛的特殊星系群。
原文:Dwarf galaxies NGC 147 (left) and NGC 185 stand side by side in this deep telescopic portrait. The two are not-often-imaged satellite galaxies of M31, the great spiral Andromeda Galaxy, some 2.5 million light-years away. Their separation on the sky, less than one degree across a pretty field of view toward the constellation Cassiopeia, translates to only about 35 thousand light-years at Andromeda's distance, but Andromeda itself is found well outside this frame. Brighter and more famous satellite galaxies of Andromeda, M32 and M110, are seen much closer to the great spiral. NGC 147 and NGC 185 have been identified as binary galaxies, forming a gravitationally stable binary system. But recently discovered faint dwarf galaxy Cassiopeia II also seems to be part of their system, forming a gravitationally bound group within Andromeda's intriguing population of small satellite galaxies.
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