4.4.3

Escape Velocity & Synchronous Orbits

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Escape Velocity

Escape velocity is the velocity needed for an object to escape a planet's gravitational pull.

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Equations for escape velocity

  • The escape velocity, ve, needed for an object to leave the gravitational influence of a planet can be estimated by equating the expressions:
    • KE=12mv2KE = \frac12 mv^2
    • GPE=mΔV=0(GMmRP)=GMmRPGPE = m\Delta V = 0 - (-\frac{GMm}{R_P}) = \frac{GMm}{R_P}
  • Where M is the mass of the planet, RP is the radius of the planet and m is the mass of the satellite.
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Calculation for escape velocity

  • When an object is removed from a planet’s gravitational pull, it loses kinetic energy equal to the gravitational potential energy it gains.
  • The kinetic energy lost is equal to the potential energy gained when the object is moved an infinite distance from the planet and has zero velocity.
    • 12mve2=GMmRP\frac12 m v_e^2=\frac{GMm}{R_P}
    • ve2=2GMRPv_e^2 = \frac{2GM}{R_P}
    • ve=2GMRPv_e = \sqrt{\frac{2GM}{R_P}}
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Earth's escape velocity

  • For the Earth, RP = 6.4 × 106 m and M = 6.0 × 1024 kg.
  • This gives ve of approximately 11 km/s.

Synchronous Orbits

A geosynchronous orbit has a period of exactly one day.

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Satellites

  • A satellite in a geosynchronous orbit remains at the same point above the Earth at all times.
  • These satellites can be used for weather mapping and observation as they can watch the same place for long periods of time.
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Calculation

  • By definition, a geosynchronous orbit has a period of one day, this can be used to calculate the radius of the orbit.
    • r3=GmT2/4π2r^3=GmT^2/4{\pi}^2
  • Remember to convert the period into seconds and the take the cubed root to find r.

Jump to other topics

1Space, Time & Motion

2The Particulate Nature of Matter

3Wave Behaviour

4Fields

4.1Circular Motion

4.2Newton's Law of Gravitation

4.3Fields

4.4Fields at Work

4.5Electric Fields

4.6Magnetic Effect of Electric Currents

4.7Heating Effect of Currents

4.8Electromagnetic Induction

4.9Power Generation & Transmission

4.10Capacitance

5Nuclear & Quantum Physics

6Measurements

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