cepheid variable中文什么意思

造父变星

• cepheid:    (variable) 【天文学】造父 ...
• variable:    adj. 1.易变的，变化无常的，无 ...
• beat cepheid:    拍合造父变星

例句与用法

更多例句：  上一页  

1. Cepheid variables are dimmer than the type i supernova . as a result , the supernova allows us to measure the distances of galaxies further away , but it happens much less often
   I型超新星比造父变星光亮，所以能够量度更遥远星系的距离，唯一缺点是不经常有i型超新星爆发。
2. Astronomers made observations of cepheid variable stars [ pictured above ] ? pulsating stars used to measure vast distances ? in the virgo and other clusters to establish the expansion rate and the universe ' s age
   天文学家用哈勃观测到仙女星座和其它星群中的造父变星(如图) ，以确定宇宙的膨胀速度和宇宙的年龄。
3. The longer the period , the brighter the star is . thus , by measuring the period of a cepheid variable , we know its absolute magnitude , hence , we can tell how far it is away by comparing with its apparent magnitude
   所以，只要知道某一造父变星的周期，我们便可得知它的绝对星等，只要和它的视星等作比较，便可以求得它和我们的距离。
4. We have to use some other methods to measure the luminosity or equivalently the absolute magnitude of the cepheid variable . since we can readily measure the apparent magnitude of a cepheid variable , to measure the luminosity means measuring the distance . we use some distance measurement methods , for example , parallax , to determine the relation
   要弄清这个关系，我们要知道不同造父变星的光度和光变周期数据，量度光变周期当然不是问题，但要得知一颗恒星的光度，我们首先要得知它的距离，这时便须借助好像视差法等其他量度天体距离的方法。
5. Except those celestial objects of several hundred light years , astronomers rely primarily on cepheid variables for measuring distances of celestial objects . using ground telescopes to gauge cepheid variables enable us to directly measure celestial objects within 20 to 30 millions light years . for more distant stars , other methods have to be used
   除了几百光年内的星体外，天文学家很主要倚靠测量造父变星来计算天体的距离，利用地面望远镜测量造父变星，可直接给出约二三千万光年内星体的距离，而对于更遥远的星体，天文学家便要借助其他方法，但这些方法还是需要利用造父变星来作校正。

百科释义

A Cepheid ( or ) is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.