Fig. 1
Download original image
Orbital eccentricities constrained at better than 3σ for resonant pairs of transiting planets, from the NASA Exoplanet Archive (see text for references). Each pair is linked with a gray segment and labelled with the host star name. The point size is proportional to the planetary radius, while the planetary mass is color-coded.
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.