Kepler's second law (law of areas) of planetary motion leads to law of conservation of
In the travelling plane wave equation given by \( y = A \sin \omega \left( \frac{x}{v} - t \right) \), where \( \omega \) is the angular velocity and \( v \) is the linear velocity.
The dimension of \( \omega t \) is:
Kepler's second law (law of areas) of planetary motion leads to law of conservation of