4.4.3
Escape Velocity & Synchronous Orbits
Escape Velocity
Escape Velocity
Escape velocity is the velocity needed for an object to escape a planet's gravitational pull.


Equations for escape velocity
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:
- Where M is the mass of the planet, RP is the radius of the planet and m is the mass of the satellite.


Calculation for escape velocity
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.


Earth's escape velocity
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
Synchronous Orbits
A geosynchronous orbit has a period of exactly one day.


Satellites
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.


Calculation
Calculation
- By definition, a geosynchronous orbit has a period of one day, this can be used to calculate the radius of the orbit.
- Remember to convert the period into seconds and the take the cubed root to find r.
1Space, Time & Motion
1.1Motion
1.2Forces
1.3Momentum & Impulse
2The Particulate Nature of Matter
2.1Thermal Concepts
3Wave Behaviour
3.1Oscillations
3.2Travelling Waves
3.3Wave Characteristics
3.4Wave Behaviour
3.5Standing Waves
3.6Simple Harmonic Motion
3.7Single Slit Diffraction
3.8Interference
3.9Doppler Effect
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
5Nuclear & Quantum Physics
5.1Discrete Energy & Radioactivity
5.2Nuclear Reactions
5.3The Interaction of Matter with Radiation
6Measurements
6.1Measurements & Errors
6.2Uncertainties & Errors
6.3Vectors & Scalars
Jump to other topics
1Space, Time & Motion
1.1Motion
1.2Forces
1.3Momentum & Impulse
2The Particulate Nature of Matter
2.1Thermal Concepts
3Wave Behaviour
3.1Oscillations
3.2Travelling Waves
3.3Wave Characteristics
3.4Wave Behaviour
3.5Standing Waves
3.6Simple Harmonic Motion
3.7Single Slit Diffraction
3.8Interference
3.9Doppler Effect
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
5Nuclear & Quantum Physics
5.1Discrete Energy & Radioactivity
5.2Nuclear Reactions
5.3The Interaction of Matter with Radiation
6Measurements
6.1Measurements & Errors
6.2Uncertainties & Errors
6.3Vectors & Scalars
Unlock your full potential with Seneca Premium
Unlimited access to 10,000+ open-ended exam questions
Mini-mock exams based on your study history
Unlock 800+ premium courses & e-books