Escape velocity is the minimum speed that an object needs to achieve to break free from a celestial body's gravitational influence without further propulsion. This concept is crucial in space exploration and astrophysics, determining the requirements for launching spacecraft and understanding planetary formation.
Formula
The escape velocity is given by the following equation:
\[ v_e = \sqrt{\frac{2GM}{r}} \]
Where:
\( v_e \) is the escape velocity (m/s)
\( G \) is the gravitational constant (\( 6.67430 \times 10^{-11} \text{ N} \cdot \text{m}^2/\text{kg}^2 \))
\( M \) is the mass of the celestial body (kg)
\( r \) is the distance from the center of the celestial body (m)
Calculation Steps
Let's calculate the escape velocity from Earth's surface: