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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 10:222 r; j$ @4 s6 B4 N8 K) r8 L: i
但在英文版中,这个“环”用了复数。
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"For a while, the two ripped-apart pieces were still connected ...
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& p2 X, O: e! E) g了解下“洛希极限”. c8 g5 j9 e' N% H7 z5 c
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https://en.m.wikipedia.org/wiki/Roche_limit5 v) P+ v! z3 V4 c/ y
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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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' V0 z; t6 ~8 \4 t7 wFar from the Roche limit (white line), the mass is practically spherical.4 ]7 L# ~4 t' x$ ]8 G% J7 f
, h) S8 Z: V" k' L; W( JCloser to the Roche limit, the body is deformed by tidal forces.0 z7 P$ q7 z1 t P* f$ N5 g
' l# l! e) [9 y5 BWithin the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.$ n. A" I9 J% t& d. Y
6 O9 {7 E3 I) U- |! wParticles closer to the primary move more quickly than particles farther away, as represented by the red arrows.
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! B7 S- v m) N2 qThe varying orbital speed of the material eventually causes it to form a ring. |
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