A) \[{{m}^{0}}\]
B) \[{{m}^{1}}\]
C) \[{{m}^{2}}\]
D) \[{{m}^{3}}\]
Correct Answer: A
Solution :
\[{{v}_{esc}}=\sqrt{2gR}\], where R is radius of the planet. Hence escape velocity is independent of m.
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