75. Two equal-mass stars maintain a constant distance apart of 8.0 x 10" m and revolve about a point midway between them at a rate of one revolution every 12.6 yr. (a) Why don't the two stars crash into one another due to the gravitational force between them? (b) What must be the mass of each star?

Glencoe Physics: Principles and Problems, Student Edition
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Author:Paul W. Zitzewitz
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Chapter7: Gravitation
Section: Chapter Questions
Problem 68A
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75. Two equal-mass stars maintain a constant distance apart
of 8.0 x 101" m and revolve about a point midway between
them at a rate of one revolution every 12.6 yr. (a) Why
don't the two stars crash into one another due to the
gravitational force between them? (b) What must be the
mass of each star?
Transcribed Image Text:75. Two equal-mass stars maintain a constant distance apart of 8.0 x 101" m and revolve about a point midway between them at a rate of one revolution every 12.6 yr. (a) Why don't the two stars crash into one another due to the gravitational force between them? (b) What must be the mass of each star?
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