Image Details

Choose export citation format:

Mass–Radius Relationships for Irradiated Ocean Planets

  • Authors: Artyom Aguichine, Olivier Mousis, Magali Deleuil, and Emmanuel Marcq

2021 The Astrophysical Journal 914 84.

  • Provider: AAS Journals

Caption: Figure 8.

Comparison between mass–radius relationships computed with the Ma19+ model and those existing in literature. Our mass–radius relationships were computed for WMFs of 20%, 50%, and 100% with no metallic core, and temperatures of 400, 600, 800, and 1000 K. Thin solid lines and thin dashed lines are from Zeng et al. (2016) and Brugger et al. (2017), respectively. Empty triangles, solid circles, and stars correspond to planets subject to no atmospheric escape, to escape of H2 only, and to escape of both H2 and H2O (Jeans or blowoff), respectively. Planetary data are taken from the NASA Exoplanet Archive (https://exoplanetarchive.ipac.caltech.edu) and updated to 2020 July.

Other Images in This Article
Copyright and Terms & Conditions