
Mice Galaxies - Wikipedia
NGC 4676, or the Mice Galaxies, are two spiral galaxies in the constellation Coma Berenices. About 290 million light-years distant, [ 2 ] they have begun the process of colliding and …
雙鼠星系 - 维基百科,自由的百科全书
雙鼠星系 (也稱為 NGC 4676)是在 后髮座 的兩個 螺旋星系,距離我們大約2億9千萬光年遠 [2],它們目前正在碰撞和合併的過程中,名稱則是來自 潮汐作用 -有別於地心引力,是星系 …
Mice Galaxies (NGC 4676): Colliding Galaxies in Coma Cluster ...
2021年5月13日 · The Mice Galaxies (NGC 4676) are a pair of colliding galaxies located 290 million light years away in the constellation Coma Berenices. They are known for the long tidal …
The Mice (NGC 4676): Colliding Galaxies With Tails of Stars and Gas
2002年4月30日 · Located 300 million light-years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed "The Mice" because of the long tails of stars and gas …
NGC4676: 老鼠星系 | NASA中文
2021年10月8日 · NGC 4676 lies about 300 million light-years away toward the constellation of Bernice’s Hair (Coma Berenices) and are likely members of the Coma Cluster of Galaxies. …
双鼠星系 - 百度百科
双鼠星系(英语:Mice Galaxies;NGC 4676) [1] 是位于 后发座 的两个正在相互碰撞的 螺旋星系,距离 地球 大约290,000,000 光年 [2]。 双鼠星系它们正在碰撞和合并的过程中,名称则是来 …
The Mice/NGC 4676 (ACS Full Field Image) - ESA/Hubble
Located 300 million light-years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed "The Mice" because of the long tails of stars and gas emanating from …
“The Mice” (NGC 4676): Colliding Galaxies Stream Stars and Gas
2002年4月30日 · The Mice (NGC 4676): Colliding Galaxies With Tails of Stars and Gas The Advanced Camera for Surveys (ACS), the newest camera on NASA's Hubble Space …
NGC 4676:双鼠星系 | NASA中文
NGC 4676 lies about 300 million light-years away toward the constellation of Bernice’s Hair (Coma Berenices) and are likely members of the Coma Cluster of Galaxies. Not often imaged …
NGC 4676 from Hubble - The Astronomy Enthusiast
2021年10月4日 · NGC 4676 lies about 300 million light-years away toward the constellation of Coma Berenices and are likely members of the Coma Cluster of Galaxies. The above picture …