Coupled atmospHere Interior modeL Intercomparison (CHILI). I. Evolutionary Modelling -- Primordial Magma Oceans of Earth and Venus
Abstract
Earth and Venus represent two evolutionary outcomes arising from initially molten 'magma ocean' periods, followed by lifetimes of chemical and geophysical divergence. Their physics is common to all rocky planets and is accessible to simulations that adopt coupled interior-atmosphere modelling approaches. Our understanding of planet histories and interpretation of current states is dependent on this modelling, yet existing codes vary in their approximations. Here, we present the first results from the Coupled atmospHere Interior modeL Intercomparison (CHILI) project; benchmarking planetary evolution codes in the context of Earth and Venus to identify key model sensitivities. Our 'nominal' Earth models predict magma ocean solidification timescales within 4 Myr of thermal evolution, and are consistent with empirical constraints on Earth's early history. Venus scenarios exhibit more diverse behaviours where prolonged magma ocean stages can be conditionally sustained for 50 Myr. Cooling timescales correlate with initial hydrogen and carbon budgets, but model-specific treatments of volatile partitioning and vertical energy transport introduce substantial inter-model variance. Different parametrisations of mantle geodynamics, convection, melting curves, rheological properties, and radiative transfer give rise to divergent evolutionary behaviours. Discrepancies in atmospheres generated by magma ocean outgassing underscore these differences, although C-H-O compositions with surface pressures exceeding 100 bar are favoured. This intercomparison identifies critical sensitivities in volatile partitioning, escape processes, mantle viscosity, and melting. Validating these treatments is essential for enabling deep insight into the early histories of the Solar System's terrestrial planets, and for drawing meaningful interpretations from ongoing observational exoplanet campaigns.
Authors 25
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Affiliation as printed
Kapteyn Astronomical Institute , University of Groningen , The Netherlands
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Affiliation as printed
Stanford University , USA
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National Astronomical Observatory of Japan
Affiliation as printed
National Astronomical Observatory of Japan , Japan
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Laboratoire de Mathématiques Blaise Pascal
Affiliation as printed
Laboratoire de Mathématiques de Versailles , France
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Centre National de la Recherche Scientifique · Institut de physique du globe de Paris · Université Paris Cité
Affiliation as printed
Université Paris Cité , Institut de physique du globe de Paris , CNRS , Paris , France
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Affiliation as printed
University of Washington , USA
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Affiliation as printed
Johns Hopkins University , USA
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Leiden University · Leiden Observatory · Space Research Organisation Netherlands
Affiliation as printed
Leiden Observatory , University of Leiden , Einsteinweg 55 , 2333CA Leiden , The Netherlands
SRON Netherlands Research Organisation Netherlands , Niels Bohrweg 4 , 2333CA Leiden , The Netherlands
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Affiliation as printed
School of Physics , University of Bristol , UK
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Leiden University · Leiden Observatory · Space Research Organisation Netherlands
Affiliation as printed
Leiden Observatory , University of Leiden , Einsteinweg 55 , 2333CA Leiden , The Netherlands
SRON Netherlands Research Organisation Netherlands , Niels Bohrweg 4 , 2333CA Leiden , The Netherlands
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Centre National de la Recherche Scientifique · Institut de physique du globe de Paris · Université Paris Cité
Affiliation as printed
Université Paris Cité , Institut de physique du globe de Paris , CNRS , Paris , France
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Laboratoire atmosphères, milieux, observations spatiales
Affiliation as printed
Laboratoire Atmospheres Milieux Observations Spatiales , France
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Affiliation as printed
Institut für Geologische Wissenschaften , Freie Universität Berlin , Germany
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Affiliation as printed
University of Central Florida , USA
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Affiliation as printed
Kapteyn Astronomical Institute , University of Groningen , The Netherlands
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Affiliation as printed
Stanford University , USA
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