Outgassing Composition of the Murchison Meteorite: Implications for Volatile Depletion of Planetesimals and Interior-atmosphere Connections for Terrestrial Exoplanets
Maggie A. Thompson, Myriam Telus, Graham Harper Edwards, Laura, Schaefer, Jasmeet Dhaliwal, Brian Dreyer, Jonathan J. Fortney, Kyle Kim

TL;DR
This study investigates the outgassing compositions of the Murchison meteorite through heating experiments, revealing insights into volatile depletion in planetesimals and implications for the early atmospheres of terrestrial exoplanets.
Contribution
It provides new experimental data on the outgassing of major and volatile elements from Murchison meteorite under different conditions, enhancing understanding of planetary formation processes.
Findings
Sulfur outgases significantly at high temperatures (800-1000°C).
Zinc outgasses under vacuum conditions.
Results inform models of volatile depletion in planetesimals.
Abstract
Outgassing is a central process during the formation and evolution of terrestrial planets and their atmospheres both within and beyond the solar system. Although terrestrial planets' early atmospheres likely form via outgassing during planetary accretion, the connection between a planet's bulk composition and its initial atmospheric properties is not well understood. One way to inform this connection is to analyze the outgassing compositions of meteorites, and in particular carbonaceous chondrites, because they are some of the most volatile-rich, primitive materials (in terms of their bulk compositions) that are available for direct study. In addition, they may serve as compositional analogs for the building block materials of terrestrial planets in our solar system and around other Sun-like stars. This study builds upon previous outgassing experiments that monitored the abundances of…
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