gravitational instability

gravitational instability

The tendency for fluctuations in an inhomogeneous medium to grow because of self-gravitation. It is opposed by pressure forces. The critical length-scale beyond which such condensations collapse is known as a Jeans length, and the Jeans mass it encloses eventually forms a stable gravitationally bound system. The Jeans length is thus often taken as a characteristic length-scale for gravitational collapse; an interstellar cloud larger than the Jeans length will fragment into clumps with this characteristic size. See also galaxies, formation and evolution.

gravitational instability

[‚grav·ə′tā·shən·əl ‚in·stə′bil·əd·ē] (mechanics) Instability of a dynamic system in which gravity is the restoring force.