A satellite orbits a planet at radius

PHYSICS · Multi-part · Fermi University Physics · Scientific Practice & Experimental Methods · Mathematical Methods for Physics · Uncertainty in measurement

Mathematical Methods for Physics, Ch The derivative as a physical instrument

Problem

A satellite orbits a planet at radius r=4.216×107 mr = 4.216\times10^{7}\,\mathrm{m}, measured with an uncertainty δr=1.0×105 m\delta r = 1.0\times10^{5}\,\mathrm{m}. For a given planet, Kepler's third law gives T2∝r3T^2 \propto r^3, so T∝r3/2T \propto r^{3/2}. At this radius the period is T=8.640×104 sT = 8.640\times10^{4}\,\mathrm{s}. ((a)) Find the fractional error δr/r\delta r/r. ((b)) Use the differential of T∝r3/2T \propto r^{3/2} to estimate the fractional error δT/T\delta T/T, and hence the absolute uncertainty δT\delta T in the period, in seconds.

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