Consider a binary star system of star A and star B with masses mA and mB revolving in a circular orbit of radii rA and rB, respectively. If TA and TB are the time period of star A and star B, respectively, then:
Held on 20 Jul 2021 · Verified 6 Jul 2026.
TBTA=(rBrA)23
TA=TB
TA>TB (if mA>mB)
TA>TB (if rA>rB)
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