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Fig. 3

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Iron-mass fractions, Feplanet%, of the 57 rocky exoplanets as a function of their equilibrium temperature, Teq. The data points are divided by the spectral type of their host stars into two groups: planets around M stars (red squares) and around FGK stars (blue triangles). The Feplanet% of the two groups show different correlations with equilibrium temperature. Green stars denote the results for the four terrestrial planets in our Solar System.

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