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define-escape-speed

๐Ÿš€ Gravitation is a fundamental force that attracts two bodies towards each other. The force of gravitation is responsible for the motion of planets, moons, and artificial satellites. Escape velocity is the minimum speed needed for an object to break free from the gravitational attraction of a celestial body without any further propulsion. For Earth, this speed is approximately 11.2 km/s. Understanding escape velocity is crucial for launching satellites and spacecraft into orbit or beyond.

Theory Explanation

Understanding Gravitational Force

The gravitational force between two masses is given by Newton's law of universal gravitation, which states that every point mass attracts every other point mass with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

\[ F = G \frac{m_1 m_2}{r^2} \]
Deriving Escape Velocity

To derive the escape velocity, we equate the kinetic energy of the object to the gravitational potential energy at the surface of the celestial body. The kinetic energy (KE) is given by \( KE = \frac{1}{2} mv^2 \) and the gravitational potential energy (PE) is given by \( PE = -G \frac{Mm}{r} \). Setting these equal allows us to solve for the escape velocity (v).

\[ \frac{1}{2} mv^2 = G \frac{Mm}{r} \Rightarrow v = \sqrt{\frac{2GM}{r}} \]

Key Points

  • ๐ŸŽฏ Escape velocity is the speed needed to break free from a gravitational field.
  • ๐ŸŽฏ It depends on the mass of the celestial body and the distance from its center.
  • ๐ŸŽฏ For Earth, the escape velocity is approximately 11.2 km/s.

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Examples:💡

Calculate the escape velocity from the surface of the Earth.

Solution:

Step 1: Taking the square root gives v โ‰ˆ 10,583 m/s or approximately 10.6 km/s.

Common Mistakes

  • Mistake: Confusing escape velocity with the speed of a satellite in orbit.

    Correction: Escape velocity is the speed needed to leave a gravitational field, while orbital speed is the speed needed to maintain a stable orbit.

  • Mistake: Not considering the mass of the celestial body when calculating escape velocity.

    Correction: Always use the mass of the celestial body in the escape velocity formula.