97 citations · 744 across the 27 of their papers we have counts for
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Mercury, Moon, Mars: Surface expressions of mantle convection and interior evolution of stagnant-lid bodies
Nicola Tosi, Sebastiano Padovan
The evolution of the interior of stagnant-lid bodies is comparatively easier to model and predict with respect to the Earth's due to the absence of the large uncertainties associat…
Machine learning inference of the interior structure of low-mass exoplanets
Philipp Baumeister, Sebastiano Padovan, Nicola Tosi +4
We explore the application of machine learning based on mixture density neural networks (MDNs) to the interior characterization of low-mass exoplanets up to 25 Earth masses constra…
Carbon cycling and interior evolution of water-covered plate tectonics and stagnant lid planets
Dennis Höning, Nicola Tosi, Tilman Spohn
Aims: The long-term carbon cycle for planets with a surface entirely covered by oceans works differently from that of the present-day Earth because inefficient erosion leads to a s…
What factors affect the duration and outgassing of the terrestrial magma ocean?
Athanasia Nikolaou, Nisha Katyal, Nicola Tosi +3
The magma ocean (MO) is a crucial stage in the build-up of terrestrial planets. Its solidification and the accompanying outgassing of volatiles set the conditions for important pro…
The habitability of stagnant-lid Earths around dwarf stars
Mareike Godolt, Nicola Tosi, Barbara Stracke +4
The habitability of a planet depends on various factors, such as delivery of water during the formation, the co-evolution of the interior and the atmosphere, as well as the stellar…
Evolution and Spectral Response of a Steam Atmosphere for Early Earth with a coupled climate-interior model
Nisha Katyal, Athanasia Nikolaou, Mareike Godolt +4
The evolution of Earth's early atmosphere and the emergence of habitable conditions on our planet are intricately coupled with the development and duration of the magma ocean phase…
Bifurcation in the growth of continental crust
Dennis Höning, Nicola Tosi, Hendrik Hansen-Goos +1
Is the present-day water-land ratio a necessary outcome of the evolution of plate tectonic planets with a similar age, volume, mass, and total water inventory as the Earth? This wo…