In order for a satellite such as the moon to travel in a circular orbit around a planet there needs to be a centripetal forceThe centripetal force keeping the moon in orbit is the Earth's gravitational force F = GMm/r2 where M is the mass of the Earth, m is the mass of the moon and r is the distance in metres between their centres of mass.
Satellites
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Specification: Edexcel Physics (9PH0), A-level, Topic 12: Gravitational Fields. Topic: Gravitational Fields.
More in Gravitational Fields
- Gravitational Potential.
- Equipotentials.
- The potential gradient.
- Newton's Law of Gravitation.
- Gravitational Field Strength - g.
- Gravitational Potential.
- Potential Gradients
- Area Under a Force vs Distance Graph
All 14 lessons in Gravitational Fields · All Edexcel A-level Physics topics