When discussing motion along a circular path, such as the movements of objects A and B, understanding the velocity function is crucial. The velocity function represents the rate of change of position over time. For a circular motion, velocity is not only about speed but also direction.
For object A, given by the position function \[ \mathbf{r}(t) = \langle \cos t, \sin t \rangle, \]the velocity function is derived by differentiating the position with respect to time. It yields \[ \mathbf{v}(t) = \langle -\sin t, \cos t \rangle. \]
Notice that the velocity vector rotates with the same angle as displacement but is perpendicular to the radius. It remains tangent to the circular path.
- This results in a constant speed on the circle's edge.
- The direction changes as the object maintains circular motion.
For object B, with position \[ \mathbf{r}(t) = \langle \cos 3t, \sin 3t \rangle, \]the velocity function becomes:\[ \mathbf{v}(t) = \langle -3\sin 3t, 3\cos 3t \rangle. \]
This velocity is three times the magnitude of object A's velocity. The higher coefficients reflect that object B moves faster around the circle, completing the path three times more quickly.
- Object B's motion is faster, evident from its velocity's factor of 3.
- Both velocity vectors are perpendicular to their respective radius vectors, ensuring tangential motion.
Understanding these velocity functions help explain how objects move swiftly and consistently along a circular orbit.