Redshift
英音[ ˈredʃɪft ] 美音[ ˈredʃɪft ]

红移

常用释义

词性释义

n.

[天] 红移;红向移动
例句
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  • 红移
AndrewBenson说,“从多方面看,这都是一种开创,因为对具有高红移的星系做这种详细的研究是非常困难的。”
这个现象被称为红移,并简单的解释为由于空间膨胀光波被拉伸。
他们发现的红移量,似乎是由引力所引起,其数量恰好与广义相对论的预测相符合。
The film has obvious redshift phenomenon and its euphotic rate reduces with the increases of the number of coating layer.
镀膜层数增加,薄膜有明显红移现象并且透光率会降低。
这种称做重力红移的效应,并不是黑洞所特有。
The distant redshift, if confirmed, would also give valuable information about galaxy surroundings at the end of the universe's dark age.
这个年轻星系如果能被证实,那么经由这份观测,就可以获得宇宙位于处在暗黑年代末期的一些重要信息。
Redshift refers to what happens when light seen coming from an object is proportionally shifted to appear more red.
红移是指当一个天体发出的光线看起来成比例地更偏向红色。
The redshift periodicity is evidence for past oscillations in the expansion rate of the universe. . .
该红移的周期性是过去宇宙膨胀速率变化的证据…
"The apparent orientation is biased because we measure orientation not with a compass or with a ruler but with redshift, " Marinoni says.
“因为我们测量方向并不是用指南针或者尺子而是用红移,所以呈现的方向会有畸变,”马里诺尼说。
引力红移效应对不同的引力参量的依赖性使它各具特点。
毕竟只有在正确的将红移变换为位置的参数下,重建结果才会是一个球形。
这理论可以完满解释水星环绕太阳的奇异轨道,与及预测恒星被本身重力所造成的红移现象。
引力红移的发现是在1959年,当时的研究者在地球上的实验室里所发射出的γ射线那里,测量到了引力红移。
并且红移取决于宇宙如何膨胀。
The power of this massive cluster telescope has allowed astronomers to detect a galaxy at the distant redshift of 5. 58.
这巨大质量星系团望远镜的强力使天文学家探测到了一个红移5.58的遥远星系。
时空必须要有某种颗粒性来驯服暧昧的无限红移。
为了在这些观点之间做出区分,就需要精确测量哈勃常数作为红移的函数。
Could GPS ever be used to measure effects besides the gravitational redshift and Doppler effect?
GPS除了用来量度重力红移与多普勒效应外,它还能测度其他效应吗?
The infinite redshift is an avatar of the unphysical assumption of infinitely small atoms.
无限红移只是无限小的原子这个非物理假设的化身。
Redshift of absorption peak and molar absorbance coefficient of complexes increased in UV spectra.
紫外光谱中配合物的吸收峰红移和摩尔吸收系数增大。
in high - redshift galaxies , however , the rate of star formation is 10 times as great.
但是,在高红移的星系中,恒星形成率是这个数目的10倍之多。
这些天体的视亮度可以得到距离,它们的红移可以得出速度。
A decreased frequency is equivalent to a longer, or redder, wavelength. This is gravitational redshift.
较低了的频率,相当于较长或较红的波长,这就是红移。
给出了一种新的类星体光谱的红移测量方法。
the greater the amount of redshift , the more rapid the movement.
红移的量越多,移动的速度越快。
Such a high redshift indicates the galaxy is 9. 3 billion light years away, so we see it just 4. 4 billion years after the Big Bang.
这样的一个高红移量表明这个星系距离我们93亿光年,所以我们现在看到的它是宇宙大爆炸44亿年之后的它。
The universe as it appears today is redshift 0. Redshift 1 refers to when the universe was half its present age.
当宇宙为目前一半的年龄时的红移值为1。
The animation below schematically shows what a redshift and blueshift might look like, again using a car as an example.
下面的动画显示了红移或蓝移看上去的可能样子。
为了探测引力红移的证据,物理学家已经花了43年的时间。
There's another survey which is very similar to this, called the Two-degree Field of View Galaxy Redshift Survey.
还有一个和这个相近的调查叫做2度視場星系紅移巡天
1·General relativity predicts that the wavelength of this light will be shifted by a small amount due to the galaxies' mass, in an effect called gravitational redshift.
广义相对论预言这种光的波长会因这些星系的质量而有少量的偏移,这种效应称为引力红移。
2·A decreased frequency is equivalent to a longer, or redder, wavelength. This is gravitational redshift.
较低了的频率,相当于较长或较红的波长,这就是红移。
3·And redshift depends on just how the universe is expanding.
并且红移取决于宇宙如何膨胀。
4·As light from the most distant explosions travels toward Earth, it is stretched by the universe's expansion so that it appears red, a phenomenon known as redshift.
最遥远的爆炸光飞向地球时,被宇宙的膨胀拉长而呈红色——一种被称作红移的现象。
5·On the histograms of their redshift, optical luminosity and average optical X-ray spectral index, it is found that X-ray selected quasars are distributed at the low ends of plots of these parameters.
发现在它们的红移、光学光度以及平均光学- X射线谱指数的直方分布图上,X射线选择类星体统计上都分布在这些参数图的低端。