Press Release
Free Access

Fig. 6

image

Similar to Fig. 5, but now in units of fractional disk radius (see ordinate). a) Disk reflectivity (ks) is set to 0.2. b) Same model parameterization but now with disk reflectivity ks = 0.4. The negative slope in both panels indicates that the most massive giant planets have larger fractions of their disks fed with water ice and, consequently, relatively more space and material to form big moons.

This figure is made of several images, please see below:

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.