When light loses energy its wavelength gets longer — that's what cosmological redshift is.
当光失去能量,它的波长会变长,这就是宇宙学的红移。
单词 | Cosmological redshift |
释义 |
Cosmological redshift
原声例句
Crash Course 天文篇 When light loses energy its wavelength gets longer — that's what cosmological redshift is. 当光失去能量,它的波长会变长,这就是宇宙学的红移。 Crash Course Physics 速成课物理 And this trend of distant galaxies moving away from us, and from one another, is called cosmological redshift. 这种遥远星系 远离我们、彼此远离的趋势被称为 宇宙学红移。
中文百科
哈柏定律 Hubble's law(重定向自Cosmological redshift)
![]() 在物理宇宙学里,哈伯定律(Hubble's law)表明,来自遥远星系光线的红移与它们的距离成正比。这条定律是因证实者哈伯而命名。它被认为是空间尺度扩展(metric expansion of space)的第一个观察依据,和今天经常被援引作为支持大爆炸的一个重要证据。 在宇宙学研究中,哈伯定律成为宇宙膨胀理论的基础,以方程序表示 其中, 2012年12月20日,美国国家航空暨太空总署的威尔金森微波各向异性探测器实验团队宣布,哈伯常数为69.32 ± 0.80 (km/s)/Mpc。
英语百科
Hubble's law 哈柏定律(重定向自Cosmological redshift)
![]() ![]() Hubble's law is the name for the observation in physical cosmology that: Hubble's law is considered the first observational basis for the expansion of the universe and today serves as one of the pieces of evidence most often cited in support of the Big Bang model. The motion of astronomical objects due solely to this expansion is known as the Hubble flow. |
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