activity
20122020
most citedGlobal modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution

351 citations · 405 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2020

Lunar Near-Surface Volatile Sample Return

Igor Aleinov, Michael J. Way, Christopher W. Hamilton +1

The origin, distribution, depth and volume of lunar volatiles remain open questions. One of the possible sources of Moon's volatiles is their volcanic outgassing during the peak of…

astro-ph.IM2020

Venus as a Nearby Exoplanetary Laboratory

Stephen R. Kane, Giada Arney, Paul Byrne +9

The key goals of the astrobiology community are to identify environments beyond Earth that may be habitable, and to search for signs of life in those environments. A fundamental as…

astro-ph.EP2019

Venus as a Laboratory for Exoplanetary Science

Stephen R. Kane, Giada Arney, David Crisp +9

The current goals of the astrobiology community are focused on developing a framework for the detection of biosignatures, or evidence thereof, on objects inside and outside of our…

astro-ph.EP2019

The environmental effects of very large bolide impacts on early Mars explored with a hierarchy of numerical models

Martin Turbet, Cédric Gillmann, François Forget +4

We use a hierarchy of numerical models (a 3-D Global Climate Model, a 1-D radiative-convective model and a 2-D Mantle Dynamics model) to explore the environmental effects of very l…

astro-ph.EP201754 cited

3D Modelling of the climatic impact of outflow channel formation events on Early Mars

M. Turbet, F. Forget, J. W. Head +1

Mars was characterized by cataclysmic groundwater-sourced surface flooding that formed large outflow channels and that may have altered the climate for extensive periods during the…

astro-ph.EP2012351 cited

Global modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution

R. Wordsworth, F. Forget, E. Millour +3

We discuss 3D global simulations of the early Martian climate that we have performed assuming a faint young Sun and denser CO2 atmosphere. We include a self-consistent representati…