ERC Starting Grant · 2024
Volatile evolution on terrestrial planets
Volatile elements, such as water, carbon and nitrogen, with low condensation temperatures, are needed to achieve and sustain habitable conditions. They also regulate planets geodynamics and climate evolution. However, how these volatiles were delivered to terrestrial planets and how they subsequently evolved is actively debated. Due to their inertness and high volatility, the noble gases krypton and xenon are unique geochemical tracers of volatiles. Their non-radiogenic isotopes have kept the signatures of the sources that delivered volatiles to planets and of the evolutionary processes subsequent to accretion, like recycling via subduction. Yet the non-radiogenic krypton and xenon isotopes…
From the public funding record at EU CORDIS. Describes the funded project, not the reviews below.
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