Two stars of masses m and 2m at a distance d rotate about their common centre of mass in free space. The period of revolution is:

1
\(\frac{1}{{2\pi }}\sqrt {\frac{{3Gm}}{{{d^3}}}} \)
2
\(2\pi \sqrt {\frac{{{d^3}}}{{3Gm}}} \)
3
\(2\pi \sqrt {\frac{{3Gm}}{{{d^3}}}} \)
4
More than one of the above
5
None of the above

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