The Roche limit is proportional to the cube root of the ratio of the black hole's mass and the orbiting body's density.
42.
The equations for the Roche limits relate the minimum sustainable orbital radius to the ratio of the two objects'densities and the Radius of the primary body.
43.
For this reason, it is also known as the "'Roche sphere "'( not to be confused with the Roche limit ).
44.
(Note that the Roche limit should not be confused with the concept of the Roche lobe or Roche sphere, which are also named after �douard Roche.
45.
Typically, the Roche limit applies to a satellite disintegrating due to tidal forces induced by its " primary ", the body about which it orbits.
46.
At that time, the orbit of Shoemaker Levy 9 passed within Jupiter's Roche limit, and Jupiter's tidal forces had acted to pull apart the comet.
47.
However, once the Moon comes within the Roche limit, wouldn't it break into pieces anyway ? talk ) 20 : 10, 27 March 2008 ( UTC)
48.
Is there an article concerning the subject of orbital tidal radii ( and I'm not referring to the Roche limit, which " orbital radius " redirects to )?
49.
For instance, comet Shoemaker Levy 9's decaying orbit around Jupiter passed within its Roche limit in July 1992, causing it to fragment into a number of smaller pieces.
50.
He described a method of calculating the distance at which an object held together only by gravity would break up due to tidal forces; this distance became known as the Roche limit.
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