Source: wikibot/gravitational-instability
= Gravitational instability
{wiki=Gravitational_instability}
Gravitational instability refers to a situation in which a cloud of gas, dust, or other matter becomes susceptible to gravitational collapse due to its own weight, leading to the formation of denser regions. This concept is crucial in astrophysics and cosmology, particularly in the context of star formation and the large-scale structure of the universe.