EPSC Abstracts Vol. 8, EPSC2013-986-1, 2013 European Planetary Science Congress 2013 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2013 Super-dense remnants of gas giant exoplanets A. Mocquet (1), O. Grasset (1) and C. Sotin (2) (1) Laboratoire de Planétologie et Géodynamique UMR 6112, Nantes University, France (
[email protected] / Fax:+33-2-51125268, (2) Jet Propulsion Laboratory, Caltech, Pasadena, California, USA Abstract of metallic materials is performed through the Mie- Grüneisen-Debye theory, which provides comparable The masses that have been observed for three large results to both ANEOS and Thomas-Fermi-Dirac exoplanets, Kepler-52b, Kepler-52c, and Kepler-57b, formulations up to a few tens of TPa [2]. The are between 30 and 100 times the Earth mass, which mechanical effects induced by the loss of the massive implies densities higher than iron planets of the same atmosphere are described by a pressure unloading of sizes. We propose that these planets could represent the solid core surface, and by a consequent increase the naked solid cores of gas giants that would have of volume and decrease of the density. Following the lost their atmospheres, for instance during their methods employed to investigate the deformation of migration towards their star, and investigate the the Earth’s mantle by surface loads [4], the evolution conditions under which the density of these cores of the unloading and associated decompression could remain close to their initial highly pressurized processes, is assessed by the convolution of a time- state. dependent source, the extensive surface stress, with the time varying viscoelastic response of the 1.