A binary star consists of two stars A (mass 2.2M_(s)), and B of mass (11M_(s)) where M_(s) is the mass of the sun. They are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary start to the angular momentum of star B about the centre of mass is

A binary star consists of two stars A (mass 2.2M_(s)), and B of mass (

1.	A binary star consists of two stars A (mass 2.2M_(s)), and B of mass (11M_(s)) where M_(s) is the mass of the sun. They are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary start to the angular momentum of star B about the centre of mass is
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