Revising the Giant Planet Mass–Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
Yayaati Chachan; Jonathan J. Fortney; Kazumasa Ohno; Daniel Thorngren; Ruth Murray‐Clay · 2025 · The Astrophysical Journal
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Abstract
Abstract The rate at which giant planets accumulate solids and gas is a critical component of planet formation models, yet it is extremely challenging to predict from first principles. Characterizing the heavy element (everything other than hydrogen and helium) content of giant planets provides important clues about their provenance. Using thermal evolution models with an updated H–He equation of state and atmospheric boundary conditions that vary with envelope metallicity, we quantify the bulk heavy element content of 147 warm (<1000 K) giant planets with well-measured masses and radii, mo
Abstract by Yayaati Chachan; Jonathan J. Fortney; Kazumasa Ohno; Daniel Thorngren; Ruth Murray‐Clay, The Astrophysical Journal (2025) — licensed CC BY 4.0.
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Metadata source: OpenAlex · DOI 10.3847/1538-4357/ae0cbf