Certain neutron stars are believed to be rotating at about $1\,rev/\sec $. If such a star has a radius of $ 20\, km$, the acceleration of an object on the equator of the star will be

  • A

    $20 \times {10^8}m/{\sec ^2}$

  • B

    $8 \times {10^5}m/{\sec ^2}$

  • C

    $120 \times {10^5}m/{\sec ^2}$

  • D

    $4 \times {10^8}m/{\sec ^2}$

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