Fig. 2.
Energy release inside the planet HD 3167b assuming a conductivity profile with an iron mass fraction of 40% and various strengths of the stellar magnetic field. The orbital inclination is 85°. The energy is released in the upper 10% of the planet’s mantle. The shaded region shows the radiogenic heat sources at the formation time of the system (upper limit) and at the age of 6 Gyr (lower limit).
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