most citedThe habitability of a stagnant-lid Earth

97 citations · 177 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201740 cited

Radioactive heat production of six geologically important nuclides

Thomas Ruedas

Heat production rates for the geologically important nuclides Al, K, Fe, Th, U, and U are calculated on the basis of recent…

astro-ph.EP201726 cited

On the relative importance of thermal and chemical buoyancy in regular and impact-induced melting in a Mars-like planet

Thomas Ruedas, Doris Breuer

We ran several series of two-dimensional numerical mantle convection simulations representing in idealized form the thermochemical evolution of a Mars-like planet. In order to stud…

astro-ph.EP201797 cited

The habitability of a stagnant-lid Earth

N. Tosi, M. Godolt, B. Stracke +7

Plate tectonics is 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 Eart…

astro-ph.EP201711 cited

Globally smooth approximations for shock pressure decay in impacts

Thomas Ruedas

New forms of empirical formulae that provide an approximate description of the decay of shock pressure with distance in hypervelocity impacts are proposed. These forms, which are i…

astro-ph.EP20103 cited

Habitability of Planets Orbiting Cool Stars

Rory Barnes, Victoria S. Meadows, Shawn D. Domagal-Goldman +6

Terrestrial planets are more likely to be detected if they orbit M dwarfs due to the favorable planet/star size and mass ratios. However, M dwarf habitable zones are significantly…

astro-ph.EP2010

Predicted dynamos for terrestrial extra-solar planets and their influence in habitability

Natalia Gomez-Perez, Mercedes Lopez-Morales, Thomas Ruedas

In this paper, we find the internal stratification for terrestrial planets with given mass-radius pairs, and use the core size and density to estimate their maximum dipolar magneti…