1 Two binary stars, masses 1020 kg and 2x1020 kg respectively, rotate about their common centre of mass with an angular velocity o. Assuming that the only force on a star is the mutual gravitational force between them, calculate @. Assuming the distance between the stars is 10° km and that G is 6.7 ×10-1" Nm²kg2. [4.5 x 10- rads1 -6-

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Chapter1: Units, Trigonometry. And Vectors
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1 Two binary stars, masses 1020 kg and
2 x1020 kg respectively, rotate about their
common centre of mass with an angular
velocity o. Assuming that the only force on a
star is the mutual gravitational force between
them, calculate @. Assuming the distance
between the stars is 10° km and that G is
6.7 ×10-1' Nm²kg2.
[4.5 x 10- rad s-
134
Transcribed Image Text:1 Two binary stars, masses 1020 kg and 2 x1020 kg respectively, rotate about their common centre of mass with an angular velocity o. Assuming that the only force on a star is the mutual gravitational force between them, calculate @. Assuming the distance between the stars is 10° km and that G is 6.7 ×10-1' Nm²kg2. [4.5 x 10- rad s- 134
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