Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

Olber's Paradox: Why is the Sky Dark at Night?

奥伯定律:为什么夜空是黑暗的?

If the universe were infinite and filled with stars in a uniform distribution, then every line of sight would terminate on the surface of a star and should be bright. To be sure, those further away would be fainter, but there would be more of them. Careful analysis suggests that the sky should be as bright as the surface of an average star.

如果宇宙是无限的,并且充满了均匀分布的恒星,那么每条视线都会终止在一颗恒星的表面,天空应当是明亮的。当然,远处的恒星会更暗,但它们的数量也会更多。仔细分析表明,天空的亮度应与一颗普通恒星的表面亮度相当。

Noting that the night sky is obviously not that bright, there are two lines of explanation. First, the universe appears to be of finite age and that light from stars at an infinite distance would not have reached us in the age of the universe. Second, we observe that the universe is expanding and that stars further away from us are receding at a faster rate. The result of this expansion is that the light from more distant stars is Doppler shifted more toward the red and beyond a certain distance would not contribute significantly in the visible region of the electromagnetic spectrum.

注意到夜空显然并不那么明亮,有两条解释。首先,宇宙似乎有有限的年龄,而来自无限远处的星体的光在宇宙年龄内未能到达我们这里。其次,我们观察到宇宙在膨胀,距离我们越远的星体退行速度越快。这种膨胀的结果是,来自更远星体的光红移得更明显,超过一定距离后,这些光在电磁波谱的可见区域将不再有显著贡献。
Index

Star concepts

Reference
Shu
Ch 16
索引星概念参考Shu Ch 16
 
HyperPhysics***** Astrophysics
HyperPhysics ***** 天体物理学
R Nave
Go Back
返回