Position and velocity vectors are fundamental concepts in physics and vector calculus. A position vector \( \vec{r} \) describes the position of an object in space as a function of time. For example, the vector \( \vec{r} = bt^2\hat{\imath} + ct^3\hat{\jmath} \) gives the object's position along the \( x \)- and \( y \)-axes as time evolves. Velocity vectors, on the other hand, express how fast the object is moving and its direction. It is derived by differentiating the position vector with respect to time. This yields the velocity vector \( \vec{v} = 2bt\hat{\imath} + 3ct^2\hat{\jmath} \). The components of velocity tell us the rate of change along each axis:
- \( 2bt \hat{\imath} \) indicates the velocity in the \( x \)-direction.
- \( 3ct^2 \hat{\jmath} \) describes the velocity in the \( y \)-direction.
By analyzing these vectors, we can determine how objects change position over time and their respective motion paths. Understanding this relationship is essential for predicting future positions and velocities from a set of initial conditions.