Formation of the Trappist-1 system in a dry protoplanetary disk

Open Access

Fig. 4.

Time evolution of the pebbles’ WMFs at the SL location. The phyllosilicate WMF is varied between 1 and 10%. The range of the WMF central values of the different Trappist-1 planets is bracketed by the dark orange box (Acuña et al. 2021), and the 1σ errors are shown in light orange.

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