Given escape velocity, \(v = 7.15 \times 10^8\) m/s
Gravitational constant, \(G = 6.67 \times 10^{-11}\) N m²/kg²
Radius of the planet, \(R = 3.54 \times 10^6\) m
The escape velocity equation is given by:
\[ v = \sqrt{\frac{2GM}{R}} \]
Solving for the mass of
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