cluster of galaxies造句
例句與造句
- Galaxies are held together by gravity to form clusters of galaxies
星系團是由星系因引力結(jié)集而成。 - Membership of cluster of galaxies
星系團成員 - Open cluster of galaxies
疏散星系團 - Proto - cluster of galaxies
原星系團 - Clusters of galaxies , in turn , are grouped in larger structures called superclusters
星系群再往上組成更大的結(jié)構(gòu)稱為超星系群。 - It's difficult to find cluster of galaxies in a sentence. 用cluster of galaxies造句挺難的
- But we see mostly one large intervening cluster of galaxies , called the virgo cluster
但是我們只看到一團相互作用的星系，成為室女座星系團。 - For the mass of a typical cluster of galaxies , it happens at a few million light - years from the center
對于典型的星系團質(zhì)量而言，轉(zhuǎn)變處則離中心約數(shù)百萬光年。 - On larger scales , analogous halos are thought to keep clusters of galaxies bound together
在更大的尺度上，有人相信，由于存在著類似的暈體，星系團才凝聚在一起。 - Im believed that the four heros are probably part of the same cluster of galaxies to which 53w002 belongs
Im相信，這四個hero可能與那個射電星系是在同一個星系團中。 - Some clusters of galaxies contain thousands of galaxies , and there are roughly 100 billion galaxies in the universe
星系一些群包含數(shù)以萬計星系,并且有大致100十億星系在宇宙。 - Typically , a cluster of galaxies contains 1000 galaxies within a million parsecs . in a larger scale , clusters group together to form
一個典型的星系團大小約一百萬秒差距，包含大約1000個星系。 - Scientists compare and combine the wmap data with the other diverse cosmic measurements , including clusters of galaxies , lyman - a cloud clustering and supernovae
科學(xué)家在仔細(xì)比較和結(jié)合wmap與其他測量方法包括星系團賴曼 - We and the rest of our gaggle are flocking en masse at 600 kilometers per second , lured by the virgo cluster of galaxies and other outside masses
由于室女座星系團和其他外部物質(zhì)的吸引，我們和其他星系以每秒600公里的速度群聚在一塊兒。 - But now , by observing a massive collision between two large clusters of galaxies , astronomers have detected what they say could only be the signature of dark matter
不過現(xiàn)在，通過觀測兩個巨大星系云團的碰撞，天文學(xué)家們可以測量出暗物質(zhì)。 - From hubble s law , we know that measurement of recession rate of celestial objects mostly clusters of galaxies and distances are the pre - requisites for the search of h
，先要測量出天體主要是星系團的退行速度和距離。哈勃本人在1929年給出第一個數(shù)值： h
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