THE ROCHE LIMIT


DEFINITION

The Roche limit is the distance from a primary body (eg a planet) at which tidal forces will disrupt a small body (eg an asteroid) that is only held together by gravitation force (ie no other chemical forces holding it together). If the secondary body approaches the primary closer than the Roche limit it will pulled apart by tidal forces from the primary body. It is thought that this is how Saturn's rings were formed.

The Roche limit is found in many areas of astrophysics including the physics of black holes. Closer to home it may be used to decide whether loose surface material on an asteroid may be pulled off the surface of the asteroid during a close encounter with the Earth or other planetary body.


DERIVATION - 1

The simplest derivation may be done with reference to the diagram below:

Geometry for computing the Roche radius

The gravitational attraction between the two small bodies is:

The tidal force pulling the two bodies apart is: Equating the gravitational attraction to the tidal disruption force we have the Roche distance dR : where s = 2 r is the separation distance between the two small bodies (ie between their centres of mass).


DERIVATION - 2

A more useful formulation considers the problem of a boulder or a small grain of sand (mass μ) on the surface of a small asteroid (mass m) as per the diagram below:

Geometry for derivation 2

The gravitational force which holds the Boulder on the surface of the asteroid is:

The tidal disruptive force on the Boulder is: and eliminating numerator terms in r2 and denominator terms with r or r2 we have Equating Ft to Fa we have: It is generally not convenient to have r in this equation and we can eliminate it by using body densities: giving:

APPLICATION

The above formula might be used to determine if an asteroid in a close encounter with the Earth is likely to 'shed' loose material from its surface. The radius and density of the Earth is known, but you may have to estimate the asteroidal density.

If the asteroid is a "Rubble pile" it is likely to be totally disrupted if it comes closer than the Roche limit.

The Roche limit is important in many areas of astrophysics, including situations involving high energy processes.

Edouard Roche Edouard Roche who,
in the 1850's,
developed the concept
of the limit
named after him.



ASAAustralian Space Academy