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单词 Gravitational Lensing
释义

Gravitational Lensing

原声例句
Veritasium真理元素

Gravitational lensing tends to magnify distant sources and increase their apparent brightness, as rays of light become concentrated.

引力透镜往往会聚焦光束,放大远处的光源并且增加其视亮度。

Crash Course 天文篇

So we call this effect “gravitational lensing.”

所以我们称这种效应为“引力透镜效应”。

VOA Special 2023年6月合集

The researchers said an observation method called gravitational lensing also helped them.

研究人员表示,一种名为引力透镜效应的观测方法也对他们有所帮助。

Veritasium真理元素

In gravitational lensing, there are three essential components -- the source, the lens, and the telescope.

在引力透镜中,有三个基本组成部分-光源,透镜和观测点。

VOA慢速英语_科技

In both cases, astronomers were able to see the light from the star because of an effect known as gravitational lensing.

在这两种情况下,天文学家都能看到恒星发出的光,因为一种叫做引力透镜的效应。

学科图谱 天文篇

This  phenomenon is known as gravitational lensing.

这种现象被称为引力透镜。

VOA Special 2023年6月合集

Vieira said that the combined abilities of James Webb and gravitational lensing made it possible for the researchers to observe through the dust to identify the PAHs.

维埃拉说,詹姆斯·韦伯太空望远镜和引力透镜效应的结合能使研究人员有可能透过尘埃观察到多环芳香烃。

TED-Ed(视频版)

Similarly, light that passes close enough to an event horizon will be deflected in a phenomenon known as gravitational lensing.

类似地,通过足够靠近事件视界的光将在称为引力透镜的现象中发生偏转。

VOA慢速英语_科技

While gravitational lensing is one way to measure amounts of dark matter, the method is more difficult when trying to observe the material in the most distant parts of the universe.

虽然引力透镜是测量暗物质数量的一种方法,但试图观察宇宙最遥远部分的物质时,这种方法仍旧面临困难。

学科图谱 天文篇

Finally, the incredible gravity around a  black hole leads to interesting gravitational lensing effects on the accretion disk  resulting in this familiar image.

最后,黑洞周围令人难以置信的引力导致了吸积盘上有趣的引力透镜效应,从而产生了这张熟悉的图像。

中文百科

引力透镜 Gravitational lens

(重定向自Gravitational Lensing)
星系引力透镜效应
重力透镜效应模拟
引力透镜效应
重力透镜效应造成的爱因斯坦十字爱因斯坦十字原理

引力透镜效应gravitational lensing),根据广义相对论,就是当背景光源发出的光在引力场(比如星系、星系团及黑洞)附近经过时,光线会像通过透镜一样发生弯曲。光线弯曲的程度主要取决于引力场的强弱。分析背景光源的扭曲,可以帮助研究中间作为“透镜”的引力场的性质。根据尺度与效果的不同,引力透镜效应可以分为强引力透镜效应和弱引力透镜效应。

一般从数学上来讲,面质量密度(\kappa)大于1的为强引力透镜区域,小于1的为弱引力透镜区域。在强透镜区域一般可以形成多个背景源的像,甚至圆弧(又称“爱因斯坦环”,Einstein Ring),而弱透镜区域则只产生比较小的扭曲。强透镜方法通过对爱因斯坦环的曲率和多个像的位置的分析,可以估计测量透镜天体质量。弱透镜方法通过对大量背景源像的统计分析,可以估算大尺度范围天体质量分布,并被认为是现在宇宙学中最好的测量暗物质的方法。

英语百科

Gravitational lens 引力透镜

(重定向自Gravitational Lensing)
Gravitational lensing - intervening galaxy modifies appearance of a galaxy far behind it (video; artist's concept).
This schematic image shows how light from a distant galaxy is distorted by the gravitational effects of a foreground galaxy, which acts like a lens and makes the distant source appear distorted, but magnified, forming characteristic rings of light, known as Einstein rings.
An analysis of the distortion of SDP.81 caused by this effect has revealed star-forming clumps of matter.

A gravitational lens refers to a distribution of matter (such as a cluster of galaxies) between a distant source and an observer, that is capable of bending the light from the source, as it travels towards the observer. This effect is known as gravitational lensing and the amount of bending is one of the predictions of Albert Einstein's general theory of relativity. (Classical physics also predicts bending of light, but only half that of general relativity's.)

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更新时间:2025/6/23 20:06:27