activity
20172026
most citedVolatile loss following cooling and accretion of the Moon revealed by chromium isotopes

88 citations · 323 across the 18 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

22 papers · 1 filter

astro-ph.EP2026

Super-Earth Interiors Shrink by About 10% as They Crystallise

Tim Lichtenberg, Mara Attia, Harrison Nicholls +26

Super-Earth exoplanets are among the most abundant planets known, yet their bulk densities leave the interior state degenerate. The static structure models used to interpret them,…

astro-ph.EP2026

Low-spin ferrous iron suppresses mantle oxidation beyond Earth-like pressures

Alice Girani, Sylvain Petitgirard, Sergey Yaroslavstsev +5

The Earth's mantle has elevated Fe relative to those of other rocky bodies, yet the oxidation- and electronic state of iron at extreme pressures is poorly known. We present…

astro-ph.EP2025★ 5 cited

Physicochemical Controls on the Compositions of the Earth and Planets

Paolo A. Sossi, Remco C. Hin, Thorsten Kleine +2

Despite the fact that the terrestrial planets formed from the protoplanetary disk, their compositions show marked departures from that of solar nebula condensates. Metallic cores f…

astro-ph.EP2025★ 7 cited

Water solubility in silicate melts: The effects of melt composition under reducing conditions and implications for nebular ingassing on rocky planets

Maggie A. Thompson, Paolo A. Sossi, Dan J. Bower +3

Rocky planet atmospheres form and evolve through interactions between the planet's surface and interior. If a growing rocky planet acquires enough mass prior to the dissipation of…

astro-ph.EP2025

A massive primordial atmosphere on early Mars

Sarah Joiret, Alessandro Morbidelli, Rafael de Sousa Ribeiro +2

Mars finished forming while the solar nebula was still present, and acquired its primordial atmosphere from this reservoir. The absence of a detectable cometary xenon signature in…

astro-ph.EP2025★ 2 cited

Volatile-bearing mineral atmospheres of hot rocky exoplanets as probes of interior state and composition

Fabian L. Seidler, Paolo A. Sossi, Dan J. Bower +1

The atmospheres of hot rocky exoplanets (HREs), should they persist, are products of interactions with underlying magma oceans. Spectra collected by the James Webb Space Telescope…