|
发表于 2022-12-8 11:07:53
|
显示全部楼层
弹钢琴 发表于 2022-12-8 10:22
' r- P( O/ x7 r! W% r但在英文版中,这个“环”用了复数。. _% d+ m5 F* R* {* }, F
& E# d0 r% X) P7 p. A
"For a while, the two ripped-apart pieces were still connected ...
/ W X0 o6 O' Q9 i0 `+ u" n+ ?& {- z2 k* t+ M0 M( h6 Z7 g
了解下“洛希极限”
/ y/ {3 k* e6 T' ^
; E. ^ E: F0 ~- k7 `& G6 T! |0 c: x, dhttps://en.m.wikipedia.org/wiki/Roche_limit
7 c4 f( s, l# z$ {# {. e
4 I; g- w, Z# `# w3 ~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.
@9 j% v0 T3 e$ g/ F. n( ?+ ~6 W3 q) v2 w
Far from the Roche limit (white line), the mass is practically spherical.2 Y. _1 ^4 ~, T1 r3 r0 c" Z
5 F |. P/ z- c9 X' K. A8 f! qCloser to the Roche limit, the body is deformed by tidal forces.: |! o0 k/ n9 @$ t1 t
/ [5 c5 a+ S! {1 l) y2 sWithin the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.
4 y3 ~( A6 D, u0 K% T$ r3 K: S* v6 g! V
Particles closer to the primary move more quickly than particles farther away, as represented by the red arrows.$ S9 @" |0 S& W. L
! R* u* H; K1 u4 k
The varying orbital speed of the material eventually causes it to form a ring. |
|