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Fig. 14

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Comparison of the atmospheric radius for different core masses and headwind parameters. The Hill radius is by definition independent of the headwind parameter. We fit a power law to the data points Ratm/REarth = a · (Mc /MEarth)n using the relative least-squares method. When the headwind is included, we obtain a = 4.7 ± 0.6, n = 0.67 ± 0.08. Without the headwind, the result of the fit is a = 5.7 ± 0.3, n = 0.62 ± 0.04.

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