Suppose that a binary star system consists of two stars of equal mass. They are observed to be separated by 360 million kilometers and take 5.0 Earth years to orbit about a point midway between them. What is the mass of EACH?
Gravitational constant = G = 6.67 x 10-11 N.m2/kg2
Mass of each star = M
Distance between the two stars = D = 360 million km = 360 x 106 km = 360 x 109 m = 3.6 x 1011 m
Radius of orbit of the stars = R
R = 1.8 x 1011 m
Time period of orbit = T = 5 years = 5 x (365x24x60x60) sec = 1.5768 x 108 sec
Orbital speed of the stars = V
V = 7172.6 m/s
The gravitational force of the stars on each other provides the necessary centripetal force for their circular motion.
M = 5.55 x 1029 kg
Mass of each star = 5.55 x 1029 kg
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