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Fig. 4

image

Impact of a change in the planetary mass on the orbital evolution for a planet located at the same distance as Kepler-444-d (initial value fixed to AU). The four red lines span a range of masses from 10 to 1000 M, with larger masses corresponding to more significant increases in the distances. The dashed lines, dotted lines, and shaded regions are the same as in Fig. 3 (top panel).

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