Petrogenesis of Erg Chech 002 Achondrite and Implications for an Altered Magma Ocean

• Published in: The Astrophysical journal Vol. 965; no. 1; pp. 24 - 31
• Main Authors: Jin, Ziliang, Zhang, Yishen, Bose, Maitrayee, Glynn, Sarah, Couffignal, Frédéric
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.04.2024; IOP Publishing
• Subjects: Achondrites; Atomic properties; Crystals; Evaporation; Lava; Magma; Meteorites; Meteors & meteorites; Oceans; Petrogenesis; Planetary system evolution; Planetesimals; Solar system
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ad2ea7

Abstract This study conducts mineralogical and chemical investigations on the oldest achondrite, Erg Chech 002 (∼4565 million yr old). This meteorite exhibits a disequilibrium igneous texture characterized by high-Mg-number (atomic Mg/(Mg + Fe 2+ )) orthopyroxene xenocrysts (Mg number = 60–80) embedded in an andesitic groundmass. Our research reveals that these xenocrysts were early formed crystals, loosely accumulated or scattered in the short-period magma ocean on the parent body. Subsequently, these crystals underwent agitation due to the influx of external materials. The assimilation of these materials enriched the 16 O component of the magma ocean and induced a relatively reduced state. Furthermore, this process significantly cooled the magma ocean and inhibited the evaporation of alkali elements, leading to elevated concentrations of Na and K within the meteorite. Our findings suggest that the introduced materials are probably sourced from the reservoirs of CR clan meteorites, indicating extensive transport and mixing of materials within the early solar system.