598 citations · 6.2k across the 94 of their papers we have counts for
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The young Sun's XUV-activity as a constraint for lower CO-limits in the Earth's Archean atmosphere
C. P. Johnstone, H. Lammer, K. G. Kislyakova +2
Despite their importance for determining the evolution of the Earth's atmosphere and surface conditions, the evolutionary histories of the Earth's atmospheric CO abundance duri…
Non-thermal escape of the Martian CO atmosphere over time: constrained by Ar isotopes
H. Lichtenegger, S. Dyadechkin, M. Scherf +5
The ion escape of Mars' CO atmosphere caused by its dissociation products C and O atoms is {simulated} from present time to billion years ago (Ga) by {numerical mode…
A critical assessment of the applicability of the energy-limited approximation for estimating exoplanetary mass-loss rates
Andreas F. Krenn, Luca Fossati, Daria Kubyshkina +1
Context: The energy-limited (EL) atmospheric escape approach is used to estimate mass-loss rates for a broad range of planets that host hydrogen-dominated atmospheres as well as fo…
Life as the Only Reason for the Existence of N2-O2-Dominated Atmospheres
Laurenz Sproß, Manuel Scherf, Valery I. Shematovich +2
The Earth's N2-dominated atmosphere is a very special feature. Firstly, N2 as main gas is unique on the terrestrial planets in the inner solar system and gives a hint for tectonic…
A pebble accretion model for the formation of the terrestrial planets in the Solar System
Anders Johansen, Thomas Ronnet, Martin Bizzarro +4
Pebbles of millimeter sizes are abundant in protoplanetary discs around young stars. Chondrules inside primitive meteorites - formed by melting of dust aggregate pebbles or in impa…
Formation of Venus, Earth and Mars: Constrained by isotopes
H. Lammer, R. Brasser, A. Johansen +2
We discuss the current state of knowledge of terrestrial planet formation from the aspects of different planet formation models and isotopic data from 182Hf-182W, U-Pb, lithophile-…