Séminaires LLR

Une histoire précoce de la Terre à la lumière du paradoxe du xénon manquant

par Mme Chrystèle Sanloup (Institut de Minéralogie, de Physique des matériaux et de Cosmochimie)

Europe/Paris
salle de conférence (LLR)

salle de conférence

LLR

Description

Xenon (Xe), due to its radiogenic isotopes, is a key tracer of atmosphere formation. Indeed, as for other noble gases, Xe is considered inert, volatile, and thus expected to degas upon rock melting and accumulate in the atmosphere. But Xe is atypical. Compared to lighter noble gases, Xe is extremely fractionated both isotopically and elementally. These observations led us to test Xe chemical reactivity at the extreme pressures and temperatures of planetary interiors, and to evidence the retention of its heaviest isotopes in minerals. Unexpectedly, these results have cast light on the very early stages of terrestrial planets, revealing that upon each planetary embryos impacts, magma oceans are formed while atmosphere is massively lost, a scenario repeated about ten times.

Beyond Earth sciences, the understanding of Xe chemistry in planetary interiors has revealed a new synthesis pathway for high energy Xe compounds, and opens applied research perspectives for nuclear reactors or spatial propulsion where similar conditions are found.