most citedMagma ocean evolution at arbitrary redox state

29 citations · 57 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.IM20255 cited

AGNI: A radiative-convective model for lava planet atmospheres

Harrison Nicholls, Raymond Pierrehumbert, Tim Lichtenberg

It is important that we are able to accurately model the atmospheres of (exo)planets. This is because atmospheres play a central role in setting a planet's thermochemical environme…

astro-ph.EP20255 cited

Absence of a Runaway Greenhouse Limit on Lava Planets

Iris D. Boer, Harrison Nicholls, Tim Lichtenberg

Climate transitions on exoplanets offer valuable insights into the atmospheric processes governing planetary habitability. Previous pure-steam atmospheric models show a thermal lim…

astro-ph.EP2025

Self-limited tidal heating and prolonged magma oceans in the L 98-59 system

Harrison Nicholls, Claire Marie Guimond, Hamish C. F. C. Hay +3

Rocky exoplanets accessible to characterisation often lie on close-in orbits where tidal heating within their interiors is significant, with the L 98-59 planetary system being a pr…

astro-ph.EP202418 cited

Convective shutdown in the atmospheres of lava worlds

Harrison Nicholls, Raymond T. Pierrehumbert, Tim Lichtenberg +2

Atmospheric energy transport is central to the cooling of primordial magma oceans. Theoretical studies of atmospheres on lava planets have assumed that convection is the only proce…

astro-ph.EP202429 cited

Magma ocean evolution at arbitrary redox state

Harrison Nicholls, Tim Lichtenberg, Dan J. Bower +1

Interactions between magma oceans and overlying atmospheres on young rocky planets leads to an evolving feedback of outgassing, greenhouse forcing, and mantle melt fraction. Previo…