A certain triple-star system consists of two stars, each of mass m = 1.9×1030 kg, revolving in the same circular orbit of radius r = 8.3x1011 m about a central star of mass M = 7.9×10³ kg (the figure). The two orbiting stars are always at opposite ends ofa diameter of the orbit. Calculate the period of revolution of the stars. M Number i 3.0e+11 Units

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Chapter3: Motion In Two Dimensions
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A certain triple-star system consists of two stars, each of mass m = 1.9×1030 kg, revolving in the same circular orbit of radius r=
8.3x1011 m about a central star of mass M = 7.9×103 kg (the figure). The two orbiting stars are always at opposite ends of a diameter
of the orbit. Calculate the period of revolution of the stars.
Number
i
3.0e+11
Units
Transcribed Image Text:A certain triple-star system consists of two stars, each of mass m = 1.9×1030 kg, revolving in the same circular orbit of radius r= 8.3x1011 m about a central star of mass M = 7.9×103 kg (the figure). The two orbiting stars are always at opposite ends of a diameter of the orbit. Calculate the period of revolution of the stars. Number i 3.0e+11 Units
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