Free Access
Fig. 4
Sketch of the inner envelope’s saturation level (Z) in the envelope’s deep interior during the four evolutionary stages. The planet is initially saturated (phase I), but dilutes as nebular gas flows in (phases II and III). The envelope can eventually become saturated again if it cools down sufficiently (phase IV).
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.