$A$ body $A$ of mass $m$ is moving in a circular orbit of radius $R$ about a planet. Another body $B$ of mass $\frac{m}{2}$ collides with $A$ with a velocity which is half $\left(\frac{\overrightarrow{v}}{2}\right)$ the instantaneous velocity $\overrightarrow{v}$ of $A$. The collision is completely inelastic. Then,the combined body

  • A
    starts moving in an elliptical orbit around the planet
  • B
    continues to move in a circular orbit
  • C
    falls vertically downwards towards the planet
  • D
    escapes from the planet's gravitational field

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