How planets grow by pebble accretion - V. Silicate rainout delays the contraction of sub-Neptunes

Open Access

Fig. 9

Zoom-in on Fig. 8 in the first 1 Gyr in log timescale. Planets with significant radius inflation in the first 0.1 Gyr are vulnerable to mass loss by photoevaporation. As in Fig. 8, red signifies ΔR/R in the range of 0.25–1. The dashed curves show examples of estimated mass-loss tracks at 0.2 AU.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.