Interior structure models of solid exoplanets using material laws in the infinite pressure limit

Details Interior structure models of solid exoplanets using material laws in the infinite pressure limit Interior structure models of solid exoplanets using material laws in the infinite pressure limit

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..214..366w&link_type=abstract

Icarus, Volume 214, Issue 2, p. 366-376.

Computer Science

3

Scientific paper

Structural models of solid exoplanet interiors are constructed using equations of state for the radial density distribution, which are compliant with the thermodynamics of the high-pressure limit. Trade-offs in predicted radii of terrestrial-type exoplanets of up to 10 Earth masses fall well within current observational limits. Deep exoplanet interiors are likely hotter than previously thought because of the pressure-induced, less vigorous convective heat transfer at depth.

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