Orbits refer to the path followed by planets and satellites as they revolve around another celestial body under gravitational influence.
Centripetal Force: Centripetal force is a force directed toward a fixed center that keeps an object moving along a circular path. In orbits, it is provided by gravitational forces.
Kepler's Laws of Planetary Motion: These laws describe how planets move in elliptical orbits around stars. They provide insights into various aspects such as orbital shape, speed, and time taken for one complete orbit.
Geostationary Orbit: A geostationary orbit is when a satellite orbits Earth at an altitude where its orbital period matches Earth's rotation period. This allows the satellite to appear stationary relative to an observer on Earth.
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