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 r(t) = x(t)i+y(t)j+z(t)k is a vector function whose values are vectors in R3, then a space curve is simply the path traced out by the tip of 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 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 r(t) are r′(t) = x′(t)i+y′(t)j+z′(t)k,r″(t) = x″(t)i+y″(t)j+z″(t)k. Both are vector functions; the first derivative v(t)=r′(t) is the velocity of the moving object, while the second derivative a(t)=r″(t) is its acceleration. Newton, of course, was really interested in starting with the acceleration!
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