M408M Learning Module Pages
Main page Chapter 10: Parametric Equations and Polar CoordinatesChapter 12: Vectors and the Geometry of SpaceChapter 13: Vector FunctionsLearning module LM 13.1/2: Vector valued functionsLearning module LM 13.3: Velocity, speed and arc length:Position, velocity and accelerationSpeed and arc length Worked problems Learning module LM 13.4: Acceleration and curvature:Chapter 14: Partial DerivativesChapter 15: Multiple Integrals |
Position, velocity and accelerationRecall that when $${\bf r}(t) \ = \ x(t)\,{\bf i} + y(t)\,{\bf j} + z(t)\,{\bf k}$$ is a vector function whose values are vectors in ${\mathbb R}^3$, then a space curve is simply the path traced out by the tip of ${\bf r}(t)$ as $t$ varies. If this path is thought of as the trajectory of an object moving in space, the parameter $t$ is naturally time, so that the tip of ${\bf r}(t)$ gives the position of the object at time $t$. In terms of motion in space, the examples that we saw earlier,
might be motion on a spiral staircase or the path of an object caught up in a tornado so that it spirals around a cone. Again as we saw earlier, differentiation of a vector function is done one variable at a time: the first order and second order derivatives of ${\bf r}(t)$ are $${\bf r}' (t)\ = \ x'(t)\, {\bf i} + y'(t)\, {\bf j} + z'(t)\, {\bf k}\,, \qquad {\bf r}''(t)\ = \ x''(t)\, {\bf i} + y''(t)\, {\bf j} + z''(t)\, {\bf k}\,.$$ Both are vector functions; the first derivative ${\bf v}(t)={\bf r}'(t)$ is the velocity of the moving object, while the second derivative ${\bf a}(t)={\bf r}''(t)$ is its acceleration. Newton, of course, was really interested in starting with the acceleration!
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