|
|
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+ X; M: Z, G% b' k! f4 `
但在英文版中,这个“环”用了复数。
. s: V% \3 y- H/ S
7 G1 T# w1 o6 a5 ~) w"For a while, the two ripped-apart pieces were still connected ...
' R; i' N: e8 s/ T; a7 {& y; }) H. W" y! r) _* u
了解下“洛希极限”
1 i; D9 k6 u& ^/ Z, Z4 ^8 F# n- O+ v! r, h* @* t6 U: G
https://en.m.wikipedia.org/wiki/Roche_limit; S# [3 E/ a2 J
x! o. _1 P* t: B U/ LIn 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.
1 ]6 N9 |7 J' K
9 d0 a% Z+ O9 Y0 Y: ^6 mFar from the Roche limit (white line), the mass is practically spherical.
8 v# m# L+ `- E `3 h- S Y" h0 L/ Q6 E( z7 T. ?! U r
Closer to the Roche limit, the body is deformed by tidal forces.
]7 ?6 B h% \6 b+ O' v- F7 X' x) l$ | e3 I7 \; n
Within the Roche limit, the mass' own gravity can no longer withstand the tidal forces, and the body disintegrates.
. x3 r- T$ ^7 o% c, K& r' a k7 Q& Y# P
Particles closer to the primary move more quickly than particles farther away, as represented by the red arrows./ B4 j0 c K& G% I8 M7 k
' p9 G: f9 R: F
The varying orbital speed of the material eventually causes it to form a ring. |
|