SIMBAD references

2019A&A...624A...2D - Astronomy and Astrophysics, volume 624A, 2-2 (2019/4-1)

Tidal heating and the habitability of the TRAPPIST-1 exoplanets.

DOBOS V., BARR A.C. and KISS L.L.

Abstract (from CDS):


Context. New estimates of the masses and radii of the seven planets orbiting the ultracool M-dwarf TRAPPIST-1 star permit improved modelling of their compositions, heating by tidal dissipation, and removal of tidal heat by solid-state convection.
Aims. Here we compute the heat flux due to insolation and tidal heating for the inner four planets.
Methods. We apply a Maxwell viscoelastic rheology to compute the tidal response of the planets using the volume-weighted average of the viscosities and rigidities of the metal, rock, high-pressure ice, and liquid water/ice I layers.
Results. We show that TRAPPIST-1d and e can avoid entering a runaway greenhouse state. Planet e is the most likely to support a habitable environment, with Earth-like surface temperatures and possibly liquid water oceans. Planet d also avoids a runaway greenhouse, if its surface reflectance is at least as high as that of the Earth. Planets b and c, closer to the star, have heat fluxes high enough to trigger a runaway greenhouse and to support volcanism on the surfaces of their rock layers, rendering them too warm for life. Planets f, g, and h are too far from the star to experience significant tidal heating, and likely have solid ice surfaces with possible subsurface liquid water oceans.

Abstract Copyright: © ESO 2019

Journal keyword(s): planets and satellites: interiors - planets and satellites: terrestrial planets - methods: numerical - astrobiology

Simbad objects: 8

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2019A&A...624A...2D and select 'bookmark this link' or equivalent in the popup menu


2021.06.12-18:47:11

© Université de Strasbourg/CNRS

    • Contact