A&A 605, A71 (2017) Astronomy DOI: 10.1051/0004-6361/201730728 & c ESO 2017 Astrophysics The habitability of a stagnant-lid Earth N. Tosi1; 2, M. Godolt1; 2, B. Stracke2, T. Ruedas3; 2, J. L. Grenfell2, D. Höning2, A. Nikolaou1; 2, A.-C. Plesa2, D. Breuer2, and T. Spohn2 1 Technische Universität Berlin, Department of Astronomy and Astrophysics, Hardenbergstr. 36, 10623 Berlin, Germany e-mail:
[email protected] 2 Institute for Planetary Research, German Aerospace Center (DLR), Rutherfordstr. 2, 12489 Berlin, Germany 3 Westfälische Wilhelms-Universität Münster, Institute of Planetology, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany Received 3 March 2017 / Accepted 24 June 2017 ABSTRACT Context. Plate tectonics is considered a fundamental component for the habitability of the Earth. Yet whether it is a recurrent feature of terrestrial bodies orbiting other stars or unique to the Earth is unknown. The stagnant lid may rather be the most common tectonic expression on such bodies. Aims. To understand whether a stagnant-lid planet can be habitable, i.e. host liquid water at its surface, we model the thermal evolution of the mantle, volcanic outgassing of H2O and CO2, and resulting climate of an Earth-like planet lacking plate tectonics. Methods. We used a 1D model of parameterized convection to simulate the evolution of melt generation and the build-up of an atmosphere of H2O and CO2 over 4.5 Gyr. We then employed a 1D radiative-convective atmosphere model to calculate the global mean atmospheric temperature and the boundaries of the habitable zone (HZ). Results. The evolution of the interior is characterized by the initial production of a large amount of partial melt accompanied by a rapid outgassing of H2O and CO2.