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单词 Tidal force
释义

Tidal force

原声例句
Crash Course 天文篇

Tidal forces rapidly synchronized the Moon's spin and orbital period, so that one face always pointed toward Earth.

引潮力迅速同步了月球的自转与公转,因此月球总是以同一面指向地球。

VOA慢速英语_科技

The planet might have been torn apart by its star's " tidal forces" .

这颗行星可能已经被其母恒星的" 潮汐力" 撕裂了。

美国历史频道纪录片《宇宙》

And we believe that these patterns are due to tidal forces that crack it.

我们认为那种现象是潮汐的力量在破碎。

Crash Course 天文篇

And this is where tidal forces become very important.

这也是为什么引潮力很重要的原因。

假如有如果

The gravitational tidal forces of that star affect the planet unevenly, stretching it at the equator.

这颗恒星的引力,潮汐力对行星的影响不均匀,从赤道处将行星拉长。

Crash Course 天文篇

The farther away the affected object is, the lower the tidal force will be.

距离越远,引潮力就越弱。

Crash Course 天文篇

The overall effect of the tidal force is to stretch an object.

引潮力的总体效果是拉伸物体。

Crash Course 天文篇

Tides depend on gravity, and if gravity is weaker, so is the tidal force.

潮汐取决于引力,如果引力较弱,潮汐力也就较弱。

地球实验室

And now locked in the giant planet's deadly embrace, tidal forces begin to tear the comet apart.

现在,彗星被锁在这颗巨行星致命的怀抱中,潮汐力开始撕裂这颗彗星。

Crash Course 天文篇

The Moon's tidal force aligns with the Sun's, reinforcing it.

月球的引潮力与太阳方向一致,叠加在了一起。

传说之境

Of course without the moon, the tidal forces on the world's oceans and lakes would drop dramatically as well.

当然,没有了月亮,世界上海洋和湖泊的潮汐力也会大幅下降。

Crash Course 天文篇

When you have a massive object affecting another object with its gravity, its tidal force depends on several factors.

当一个巨大的物体通过引力影响另一个物体时,它的引潮力取决于几个因素。

Crash Course 天文篇

This change in the force of gravity over distance is what astronomers call the tidal force.

这种由于距离造成的引力改变被天文学家成为引潮力。

Crash Course 天文篇

This is probably the weirdest thing about tidal forces.

这恐怕就是引潮力最奇怪的地方了。

Crash Course 天文篇

This process is aided by collisions with gas clouds and the tidal forces of the collected stars in the galaxy itself.

这一过程是由气体云的碰撞和星系中收集的恒星的潮汐力所辅助的。

VOA慢速英语_科技

When a smaller body passes near a much bigger one, tidal forces created by the larger body can destroy the smaller one.

当一个较小的物体经过一个大得多的物体附近时,较大的物体产生的潮汐力可以摧毁较小的物体。

Crash Course 天文篇

The tidal force stretches the solid Earth by about 30 centimeters.

引潮力会拉伸地球的固态部分大约30厘米。

Crash Course 天文篇

The water bulges up where the tidal force is strongest, on opposite sides of the Earth.

在引潮力最强的地方,也就是在地球的两侧,水会形成凸起。

Crash Course 天文篇

The wider it is, the more the force of gravity from the first object changes across it, and the bigger the tidal force.

它越宽,来自第一个物体作用在它上面引力的变化就越大,引潮力也就越大。

Crash Course 天文篇

The way the Sun's tidal force and the Moon's tidal force interact on Earth depends on their geometry, which changes as the Moon orbits us.

具体太阳和月球的引潮力如何相互作用取决于它们的几何位置,而这个位置随着月球公转而不断变化。

中文百科

潮汐力

潮汐力引潮力是万有引力的效果,它使得潮汐发生。它源于在一个星体的直径上各点的引力场不相等。

当一个天体甲受到天体乙的引力的影响,力场在甲面对乙跟背向乙的表面的作用,有很大差异。这使得甲出现很大应变,甚至会化成碎片(参见洛希极限)。除非引力场完全相等,否则这些应变还是会出现。

潮汐力会改变天体的形状而不改变其体积。地球的每部分都受到月球的引力影响而加速,在地球的观察者因此看到海洋内的水不断重新分布。

当天体受潮汐力而自转,内部摩擦力会令其旋转动能化为内能,内能继而转成热。若天体相当接近系统内质量最大的天体,自转的天体便会以同一面朝质量最大的天体公转,即潮汐锁定,例如月球和地球。

英语百科

Tidal force 潮汐力

Figure 1: Comet Shoemaker-Levy 9 in 1994 after breaking up under the influence of Jupiter's tidal forces during a previous pass in 1992.
Figure 2: The Moon's gravity differential field at the surface of the Earth is known (along with another and weaker differential effect due to the Sun) as the Tide Generating Force. This is the primary mechanism driving tidal action, explaining two tidal equipotential bulges, and accounting for two high tides per day. In this figure, the Earth is the central blue circle while the Moon is far off to the right. The outward direction of the arrows on the right and left indicates that where the Moon is overhead (or at the nadir) its perturbing force opposes that between the earth and ocean.
Figure 3: Saturn's rings are inside the orbits of its principal moons. Tidal forces oppose gravitational coalescence of the material in the rings to form moons.[5]
Tidal force is responsible for the merge of galactic pair MRK 1034.[9]

The tidal force is a secondary effect of the force of gravity and is responsible for the tides. It arises because the gravitational force exerted by one body on another is not constant across it; the nearest side is attracted more strongly than the farthest side. Thus, the tidal force is differential. Consider the gravitational attraction of the moon on the oceans nearest to the moon, the solid Earth and the oceans farthest from the moon. There is a mutual attraction between the moon and the solid earth which can be considered to act on its centre of mass. However, the near oceans are more strongly attracted and, since they are fluid, they approach the moon slightly, causing a high tide. The far oceans are attracted less. The attraction on the far-side oceans could be expected to cause a low tide but since the solid earth is attracted (accelerated) more strongly towards the moon, there is a relative acceleration of those waters in the outwards direction. Viewing the Earth as a whole, we see that all its mass experiences a mutual attraction with that of the moon but the near oceans more so than the far oceans, leading to a separation of the two.

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更新时间:2025/6/22 17:13:53