Astronomers discover four moons orbiting the exoplanet Zeus

PHYSICS · Multi-part · A Level · Physics · Fields and their consequences · Fields and their consequences

Problem

Astronomers discover four moons orbiting the exoplanet Zeus. Their measured orbital data are listed below.
MoonOrbital radius RR (×106 m\times10^{6}\,\text{m})Orbital period TT (days)
A1.500.80
B2.301.46
C3.603.10
D5.105.75
Assume the moons travel in nearly circular orbits and that the mass of each moon is negligible compared with the mass MZM_Z of Zeus. (a) Transform the data so that a single straight-line graph can be produced that tests the relationship between TT and RR for circular orbital motion. State clearly what quantities you would plot on each axis and explain why this transformation yields a linear graph. (b) Using the transformed data, calculate the numerical value of the slope of the best-fit line. Show all working, including any unit conversions required. (c) Derive an expression that relates the slope obtained in part (b) to the mass MZM_Z of Zeus, and then compute MZM_Z. Express your answer in kilograms. (d) Identify two possible systematic errors in the astronomical measurements that could cause the computed mass to differ from the true mass. For each error, indicate whether it would tend to make the calculated mass too large or too small, and justify your reasoning.

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