Three point masses,each of mass $m$,are kept at the corners of an equilateral triangle of side $L$. The system rotates about the center of the triangle without any change in the separation of masses during rotation. The period of rotation is directly proportional to

  • A
    $L$
  • B
    $L^{1/2}$
  • C
    $L^{3/2}$
  • D
    $L^{-2}$

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