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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
! L! a: E: }& z a# I- a( y$ Y但在英文版中,这个“环”用了复数。/ [+ N9 T, _ [0 w
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"For a while, the two ripped-apart pieces were still connected ... 2 L+ O. j* l* b6 E
; t- `( }5 x% h6 Z了解下“洛希极限”
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) N4 L) {3 _5 G& p3 e. Mhttps://en.m.wikipedia.org/wiki/Roche_limit# e1 a# v; W0 y; s
% A2 x7 @) o- k( @, DIn 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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+ |. \" g/ ^4 x' u0 `. M9 mFar from the Roche limit (white line), the mass is practically spherical./ Y1 ] e8 @5 ~, h* \1 Z R
2 |& ~+ @# f& G, X" ?Closer to the Roche limit, the body is deformed by tidal forces., G- ]# T" B$ E" b- P" X9 b
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Within the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.( B. {3 T% e4 k
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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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0 l+ l' Y* U3 o: | ]; i3 EThe varying orbital speed of the material eventually causes it to form a ring. |
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