Influence of fast rotator (purple line) or slow rotator (green line) stellar evolution in comparison to a simulation without considering induction heating (dotted black line) on the outgassing evolution for a planet mass of 1.8 M_⊕, a magnetic field inclination of 60°, 20 wt% iron content, and parameter case 4. Left: total outgassed pressure over time (limited between 1 and 3 Gyr for a better comparison). Right: difference in outgassing over time compared to a simulation where no induction heating was considered.