Open Access

Fig. 3

image

Download original image

Planet radius, and radius anomaly, dependence on planet temperature and metallicity. Left: planet radius and equilibrium temperature for the 159 massive exoplanets (0.5 MJ < mass < 10 MJ) with homogeneous high precision [Fe/H]. Right: radius anomaly vs. equilibrium temperature for the same planets. The line is the best fit of a power law.

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.