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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
4 w) B' q* Z! e' W6 u但在英文版中,这个“环”用了复数。
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! m) C4 R: r5 q/ D1 `. ^"For a while, the two ripped-apart pieces were still connected ...
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了解下“洛希极限”
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5 s8 u" m/ V; ~- Q7 Fhttps://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.0 n+ m1 s: {, i. h; T2 \# a
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Far from the Roche limit (white line), the mass is practically spherical.2 s" S5 S7 X- o! v, J* O
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Closer to the Roche limit, the body is deformed by tidal forces.
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7 k5 y; u r7 o+ iWithin the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.9 V: }+ `$ Y" h5 p) z8 L
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Particles closer to the primary move more quickly than particles farther away, as represented by the red arrows.! E2 F& T' f% u; d: X+ j) u* v
D) B* M1 Z1 ~. m T% H% wThe varying orbital speed of the material eventually causes it to form a ring. |
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