Step 1: Calculating the velocity.
When a body falls from infinity, its velocity on reaching the surface of the Earth can be calculated using the formula for gravitational potential energy:
\[
\frac{GMm}{R} = \frac{1}{2} mv^2
\]
where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, \( R \) is the radius of the Earth, \( m \) is the mass of the body, and \( v \) is the velocity.
Substituting the known values:
\[
G = 6.67 \times 10^{-11} \, \text{Nm}^2/\text{kg}^2, \, M = 5.97 \times 10^{24} \, \text{kg}, \, R = 6400 \times 10^3 \, \text{m}
\]
We find that the velocity \( v \) is approximately 11.2 km/s.
Step 2: Calculating the kinetic energy.
The kinetic energy of the body can be calculated using the formula:
\[
K = \frac{1}{2} mv^2
\]
Substituting the value of \( v \) and the mass of the body:
\[
K = \frac{1}{2} (1)(11.2 \times 10^3)^2 = 12.54 \times 10^7 \, \text{J}
\]
Step 3: Conclusion.
Thus, the velocity \( v = 11.2 \, \text{km/s} \) and the kinetic energy \( k = 12.54 \times 10^7 \, \text{J} \).
Final Answer: (B) 11.2 km/s; \( 12.54 \times 10^7 \) J