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Fig. 1
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Post-formation outcome of the interior structure of planets assembled by pebble accretion (Ormel et al. 2021). We show the silicate mass fraction distribution (black) and the envelope temperature profile (red) in planets of 5 M⊕ (left), 10 M⊕ (middle), and 20 M⊕ (right), formed at 0.2 AU from a Sun-like star.
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