activity
20172022
most citedSolubility of water in peridotite liquids and the prevalence of steam atmospheres on rocky planets

54 citations · 117 across the 3 of their papers we have counts for

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Showing astro-ph.EPShow all

8 papers · 1 filter

astro-ph.EP202254 cited

Solubility of water in peridotite liquids and the prevalence of steam atmospheres on rocky planets

Paolo A. Sossi, Peter M. E. Tollan, James Badro +1

Atmospheres are products of time-integrated mass exchange between the surface of a planet and its interior. On Earth and other planetary bodies, magma oceans likely marked signific…

astro-ph.EP202126 cited

Hemispheric Tectonics on super-Earth LHS 3844b

Tobias G. Meier, Dan J. Bower, Tim Lichtenberg +2

The tectonic regime of rocky planets fundamentally influences their long-term evolution and cycling of volatiles between interior and atmosphere. Earth is the only known planet wit…

astro-ph.EP2021

Vertically resolved magma ocean-protoatmosphere evolution: H, HO, CO, CH, CO, O, and N as primary absorbers

Tim Lichtenberg, Dan J. Bower, Mark Hammond +4

The earliest atmospheres of rocky planets originate from extensive volatile release during magma ocean epochs that occur during assembly of the planet. These establish the initial…

astro-ph.EP2020

Lithologic Controls on Silicate Weathering Regimes of Temperate Planets

Kaustubh Hakim, Dan J. Bower, Meng Tian +6

Weathering of silicate rocks at a planetary surface can draw down CO from the atmosphere for eventual burial and long-term storage in the planetary interior. This process is th…

astro-ph.EP2020

The influence of bulk composition on long-term interior-atmosphere evolution of terrestrial exoplanets

Rob J. Spaargaren, Maxim D. Ballmer, Dan J. Bower +2

Aims: The secondary atmospheres of terrestrial planets form and evolve as a consequence of interaction with the interior over geological time. We aim to quantify the influence of p…

astro-ph.EP2019

Linking the evolution of terrestrial interiors and an early outgassed atmosphere to astrophysical observations

Dan J. Bower, Daniel Kitzmann, Aaron S. Wolf +3

A terrestrial planet is molten during formation and may remain so if subject to intense insolation or tidal forces. Observations continue to favour the detection and characterisati…