Concept: Escape velocity
Escape velocity is the minimum speed required for an object to escape a planet’s gravitational field without further propulsion:
\[
v = \sqrt{\frac{2GM}{R}}
\]
Step 1: Substitute known values
For Earth:
\[
G = 6.67 \times 10^{-11}, \quad M = 6 \times 10^{24} \text{ kg}, \quad R = 6.4 \times 10^6 \text{ m}
\]
Step 2: Calculate
\[
v = \sqrt{\frac{2 \times 6.67 \times 10^{-11} \times 6 \times 10^{24}}{6.4 \times 10^6}}
\]
\[
v \approx 1.26 \times 10^4 \text{ m/s}
\]
Step 3: Convert units
\[
v \approx 12.6 \text{ km/s}
\]
Final Answer:
\[
\boxed{12.6 \text{ km/s}}
\]
Note:
Escape velocity is independent of the mass of the object being projected.