星际分子、星际微波激射、太阳引力弯曲的检验都与射电干涉仪紧密联系。
The test of interstellar molecules, interstellar maser and solar gravitational deflection are closely related to radio interferometer.
这个光谱中的光线，向四面八方离开太阳，由于地球引力弯曲导致本该从地球旁边经过的光线弯向地球的中心。
Light in this spectrum, leaving the Sun in all directions, is bent by the gravity of Earth so that what would normally pass on either side of the Earth is bent back toward the center of the Earth.
然而，当木卫二绕其行星运行时，由于姊妹卫星和木星之间的引力拉锯战，它会弯曲。
As Europa orbits its planet, however, it flexes due to the gravitational tug-of-war between it, its sister moons, and Jupiter.
这一方法指的是将目光集中在恒星上，当行星从恒星前经过时产生的引力将会使光线弯曲，这时就会得到关于详细情况的报告。
The idea would be to stare at a distant star and report instances when its light had been bent by the gravity of a planet passing in front of it.
作为例子，这个球面代表了恒星或其他质量附近的空间是怎样弯曲的-光通过这个扭曲空间所引起的弯曲称为引力透镜效应。
The sphere, for instance, represents how space is bent around a star or other mass - light passing through this warped space bends in an effect called gravitational lensing.
在天体物理学中，引力作用量描述了在被物质和能量弯曲的时空中如何形成引力的机理。
In astrophysics, a gravitational action is the mechanism that describes how gravity can emerge from space-time being curved by matter and energy.
最初，该理论能够用来说明水星独特运行轨道[译者注]和太阳光的弯曲，这两种情况是牛顿引力理论所无法解释的。
Originally, the theory was able to account for peculiarities in the orbit of Mercury and the bending of light by the Sun, both unexplained in Isaac Newton's theory of gravity.
引力透镜现象就是光被巨大质量物体弯曲的现象。
A gravitational lens is formed when light is bent by a massive object.
这一现象是指光线在时空中传播的过程中由于大质量物质的引力而发生弯曲，这也是爱因斯坦的广义相对论所预言的。
This phenomenon, predicted by Einstein's theory of general relativity, causes light to curve as it flies through space-time that has been dented by the gravity of large bodies of mass.
广义相对论并不将引力视为“力”，而是将它看作是时空弯曲的结果。
General relativity views gravity not as a force but as a consequence of the curved geometry of space and time.
实验有助于形象化地显示光在被引力所弯曲空间内的传播情况。
The experiments help visualise how light travels in space warped by gravity.
光环的直径不仅取决于产生它的星系的远近还与引力透镜的质量有关——质量越大光就弯曲的越厉害。
The diameter of the rings depends not only on the distance to the galaxies that caused them but also on the masses of those galaxies. The more massive they are, the more the light is bent.
例如，当恒星发出的光经过一个星系附近，其路径会弯曲，改变恒星出现在天空中的位置——这就是所谓的引力透镜效应。
When light from a star passes near a galaxy, for example, its path bends, changing where the star appears in the sky-the so-called gravitational lensing effect.
引力透镜利用这样的一个现象：巨大的天体会扭曲它附近的时空组成物。比如，当光线经过恒星或行星附近时会发生弯曲。
Gravitational lensing takes advantage of the fact that large celestial objects such as stars or planets warp the fabric of space-time such that light rays passing nearby are bent.
使时空弯曲的波纹被称为引力波，引力波能使任何穿过它的物体暂时扭曲变形。
These waves of curvature in space-time are known as gravitational waves and will temporarily distort any object they pass through.
得益于它们的重量，MACS星系就像一个巨大的宇宙镜头，能放大，变形和弯曲经过它们的任何光，和引力透镜的效果一样。
Because of their heft, the clusters act like giant cosmic lenses, magnifying, distorting and bending any light that passes through them - an effect known as gravitational lensing.
我们解释过这是由于红色光谱更容易弯曲，所以当其他光线还没怎么样时，红光首先由于地球的引力而沿着地球的曲线弯曲。
We have explained this being due to light in the red spectrum bending readily, so red light is bent first over the horizon by the gravity of Earth where light in the other spectrums is not so bend.
极光，正如我们所说，跟磁场没有一点关系而是由于引力而弯曲的光线。
The Auroras, as we have stated, are not magnetic at all but light rays bent by gravity.
暗物质构成了大部分的总质量，并主宰了集群的引力透镜，或从光线弯曲的背景星系因引力。
The dark matter makes up most of the total mass, and dominates the gravitational lensing of the cluster, or the bending of light from background galaxies due to gravity.
太阳的引力使光束弯曲。
在下一次合适的日食到来，也就是1919年，科学家就能测出挨着太阳的星光是如何被太阳的引力所弯曲。
At the next appropriate eclipse, in 1919, scientists could measure how starlight passing close to the sun was bent by its gravity.
预期会更加弯曲想地球的引力中心，不仅太阳会显得比平时大，所有的行星物体的大小都将被扭曲。
Additional bending toward the Earth's center of gravity can be expected, with more than the Sun appearing extra large at sunrise and sunset. All planetary objects may have their size skewed.
时间和空间是相对论研究的重要物理问题，在物质的空间中，存在引力场，而由于引力场的存在，则会导致时间的变化，空间的弯曲，光线轨迹的改变等。
Time and space are important for relativity study in physics. In matter space exists a gravitational field, owning to which time is varied, space is bent, and light trace is changed.
介绍两辊式和三辊式机械弯曲除锈原理，给出关键参数如辊子直径、牵引力等的设计计算方法。
Design and calculation method of the key parameter such as the diameter of roller and pulling force are given.
一目了然引力可以弯曲光线。
It is a known fparticipate that gravity can benjamind light rays.
高耐磨人字形外底与区域弯曲凹槽，提供出色的牵引力和灵活性。
High abrasion herringbone outsole with regional flex grooves provides superior traction and flexibility.
或许在一个时空弯曲不再是必须条件的情况下，能够成功的将引力量子化。
Without space-time curvature, there is no meaning to general relativity, ie. , classical gravity… without classical gravity, what is the meaning of quantizing it?
或许在一个时空弯曲不再是必须条件的情况下，能够成功的将引力量子化。
Without space-time curvature, there is no meaning to general relativity, ie. , classical gravity… without classical gravity, what is the meaning of quantizing it?
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