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单词 Tidal bulge
释义

Tidal bulge

原声例句
宇宙的奇迹

Eventually, the tidal bulge became aligned with the Earth, locking the speed of the moon's rotation.

最终,月球的突起正对地球,锁定了月球的转速。

Crash Course 天文篇

Just like Earth, there are two tidal bulges on the Moon: one facing the Earth and one facing away.

就像地球一样,月球上也有两个凸起:一个面向地球,另一个背向地球。

SciSHow 快问快答小科普

The way things are now, the Moon’s gravity tugs on the Earth, creating tidal bulges.

现在的情况是, 月球的引力拉动地球, 造成潮汐隆起。

Crash Course 天文篇

The Moon's tidal bulges didn't align with the Earth, and the Earth's gravity tugged on them, slowing the Moon's spin and moving it farther away.

月球由于引潮力而产生的凸起也不完全在地球月球的连线上,地球的引力拉着它,减慢了月球的自转速度,并使它移得更远。

宇宙的奇迹

Now, the size of that tidal bulge facing the Earth is something like seven metres in rock and then, as the moon rotates, that bulge sweeps across the lunar surface.

面向地球的那部分会增加 7 米的高度,当月球自转时这个突起会穿过月球表面。

SciSHow 快问快答小科普

At that point, the Earth’s tidal bulges would always be directly in line with the Moon, so it would finally stop getting farther away.

到那时, 地球的潮汐隆起将始终与月球成一直线,因此它最终不会远离月球。

假如有如果

And lucky for us, our Moon's orbit and gravitational pull tilt the Earth 23.4 degrees, creating tidal bulges that help slow the rotation of our planet just enough for life to safely exist, or so we think.

幸运的是,月球的轨道运行和引力作用使地球倾斜 23.4 度,产生的潮汐使地球自转速度减慢到恰好能让生命幸存下来,或者这只是我们的假想。

中文百科

潮汐力 Tidal force

(重定向自Tidal bulge)

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

(重定向自Tidal bulge)
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:2025/6/21 9:10:09