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Inner Solar System's elemental evolution

08.06.18 | Proceedings of the National Academy of Sciences

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Elemental analysis of dated meteorite chondrules, which record the early history of the Solar System, suggest that until around 4.567 billion years ago, oxygen and volatile element delivery from the outer Solar System to the inner Solar System increased; following this time point, oxygen from water began to decrease whereas volatiles continued to increase, lending support to a model of early formation of Mars under oxidizing conditions and accretion of Earth under relatively reducing conditions.

Article #18-07263: "Volatile element evolution of chondrules through time," by Brandon Mahan et al.

MEDIA CONTACT: Brandon Mahan, Institut de Physique du Globe de Paris, FRANCE; tel: +33 7 62 93 56 12; e-mail: < mahan@ipgp.fr >; Frédéric Moynier, Institut de Physique du Globe de Paris, FRANCE; tel: +33 1 83 95 77 88; e-mail: < moynier@ipgp.fr >

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Proceedings of the National Academy of Sciences

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Article Information

Contact Information

Brandon Mahan
mahan@ipgp.fr

How to Cite This Article

APA:
Proceedings of the National Academy of Sciences. (2018, August 6). Inner Solar System's elemental evolution. Brightsurf News. https://www.brightsurf.com/news/L7642Z41/inner-solar-systems-elemental-evolution.html
MLA:
"Inner Solar System's elemental evolution." Brightsurf News, Aug. 6 2018, https://www.brightsurf.com/news/L7642Z41/inner-solar-systems-elemental-evolution.html.