Let $R_1, R_2$ and $R_3$ be the radii of three mercury drops. $A$ big mercury drop is formed from them under isothermal conditions. The radius of the resultant drop is

  • A
    $(R_1^3+R_2^3+R_3^3)^{\frac{1}{3}}$
  • B
    $(R_1^2+R_2^3-R_3^3)^{\frac{1}{3}}$
  • C
    $(R_1^3+R_2^3+R_3^3)$
  • D
    $(R_1+R_2+R_3)^3$

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$Reason :$ Excess pressure inside a drop is directly proportional to its surface area.

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