Two bodies of equal masses revolve in circular orbits of radii ${R_1}$ and ${R_2}$ with the same period. Their centripetal forces are in the ratio
Two bodies of equal masses revolve in circular orbits of radii ${R_1}$ and ${R_2}$ with the same period. Their centripetal forces are in the ratio
- A
${\left( {\frac{{{R_2}}}{{{R_1}}}} \right)^2}$
- B
$\frac{{{R_1}}}{{{R_2}}}$
- C
${\left( {\frac{{{R_1}}}{{{R_2}}}} \right)^2}$
- D
$\sqrt {{R_1}{R_2}} $
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