(astronomy) The formation of a dynamic equilibrium in a system of collisionless particles modelled as being subject only to Newtonian gravity (galaxy, other stellar system, or galaxy cluster)..
현재 검증된 한국어 뜻은 준비 중이며 영어 정의는 “(astronomy) The formation of a dynamic equilibrium in a system of collisionless particles modelled as being subject only to Newtonian gravity (galaxy, other stellar system, or galaxy cluster).”입니다.