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发表于 2022-12-8 11:07:53
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弹钢琴 发表于 2022-12-8 10:22
1 K( y% v, _ {" Q' }; O但在英文版中,这个“环”用了复数。& i1 { S2 j# S6 i- }2 @' A
m& B5 Z \# d) m6 C6 R: N"For a while, the two ripped-apart pieces were still connected ...
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了解下“洛希极限”/ e# }% H6 V' u- e+ R) P9 O3 P
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https://en.m.wikipedia.org/wiki/Roche_limit
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In celestial mechanics, the Roche limit, also called Roche radius, is the distance from a celestial body within which a second celestial body, held together only by its own force of gravity, will disintegrate because the first body's tidal forces exceed the second body's gravitational self-attraction.[1] Inside the Roche limit, orbiting material disperses and forms rings, whereas outside the limit, material tends to coalesce.
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Far from the Roche limit (white line), the mass is practically spherical.
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3 v4 ~' K2 y4 G+ A+ sCloser to the Roche limit, the body is deformed by tidal forces.2 L& _; g) u( _3 Z
5 F8 l8 p- _; R5 I- H. |7 W2 vWithin the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.& T! P2 v( G. {: V/ I) O0 _
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Particles closer to the primary move more quickly than particles farther away, as represented by the red arrows.
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5 e8 ^( q( U$ |" JThe varying orbital speed of the material eventually causes it to form a ring. |
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