Binary stars rotate under mutual gravitational force at separation `2(G/(omega^(2)))^(1/3)`
Channel: Doubtnut
Date: 26/01/2020

Binary stars rotate under mutual gravitational force at separation `2(G/(omega^(2)))^(1/3)`, where `omega` is the angular velocity of each of the star about centre of mass of the system. If difference between the mass of stars is `6` units. Find the ratio of mass of bigger star to smaller star.