Unverified50% confidenceFactExact time
Any celestial body (such as Earth or the Moon) exerts tidal forces on objects near it, and their magnitude depends on the degree of non-uniformity of the gravitational field.
1
Sources
50%
Confidence
Long-term
Relevance
10/28/2026
First Seen
Sources
Related Entities
Related Claims
UnverifiedThe Moon is tidally locked, and the lunar geostationary orbit calculated in isolation is approximately 87,000 kilometers above the lunar surface, but it is strongly perturbed by Earth, whose mass is 81 times that of the Moon.63% similarUnverifiedThe radial velocity method more easily finds massive, short-period planets, while the transit method has strict requirements on orbital inclination.57% similarUnverifiedThe communication link between the Moon and Earth may be completely interrupted on the lunar far side or during solar activity interference.55% similarUnverifiedFor stellar-mass black holes, the region where tidal forces are strong enough to tear objects apart lies far outside the event horizon; for supermassive black holes, tidal forces near the event horizon are instead relatively small, so an astronaut might safely cross the horizon first and then be torn apart near the singularity.55% similarUnverified轨道力学中，阻力消耗卫星轨道能量时使轨道高度降低，卫星在更低轨道上以更快速度运行，但总能量持续减少55% similar
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