An asteroid of mass \(m\) is approaching earth, initially at a distance of \(10\ R_e\), with speed \(v_{i}\), it hits the earth with a speed \(v_{f}\)(\(R_{e}\) and \(M_{e}\) are radius and mass of earth), then ( )
A. \(v^{2}_{f}=v^{2}_{i}+\frac {2Gm}{M_{e}R}(1-\frac {1}{10})\)
B. \(v^{2}_{f}=v^{2}_{i}+\frac {2Gm_{e}}{R_{e}}(1+\frac {1}{10})\)
C. \(v^{2}_{f}=v^{2}_{i}+\frac {2Gm_{e}}{R_{e}}(1-\frac {1}{10})\)
D. \(v^{2}_{f}=v^{2}_{i}+\frac {2Gm}{R_{e}}(1-\frac {1}{10})\)