Trigonometric functions describe planetary motion in the context of physics using mathematical representations, aiding in predictions and celestial observations.
Trigonometric functions can be used to describe phenomena such as planetary motion. In this case, the movement of planets in their orbits around the Sun can be mathematically represented using trigonometric functions.
For example, the position of a planet at a given time can be expressed using sine and cosine functions, showcasing the cyclical nature of planetary motion as they revolve around a central point.
Understanding these functions helps astronomers predict the positions of planets in the sky at different times, aiding in celestial observations and calculations.
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