Orbits of planets and satellites (AQA A-Level Physics): Flashcards

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Orbits of planets and satellites
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Kepler's 3rd law

T2∝r3T^2 \propto r^3

Lower orbit satellite: energy change

Loses GPE, gains KE

Escape velocity

Min speed to leave gravitational influence

Escape velocity formula

v=2GMrv = \sqrt{\frac{2GM}{r}}

Escape velocity & object mass

Independent of object's mass

Synchronous orbit

Period matches rotation period of orbited object

Geostationary orbit features

Above equator, 24h period, fixed position above Earth

Geostationary radius from Earth centre

42,000 km

Geostationary satellite uses

TV broadcasting & telecommunications

Low-orbit vs geostationary satellites

Faster; for weather monitoring, Earth observation, military

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