Climate Change Data Portal
DOI | 10.1073/pnas.2026129118 |
A 4,565-My-old andesite from an extinct chondritic protoplanet | |
Barrat J.-A.; Chaussidon M.; Yamaguchi A.; Beck P.; Villeneuve J.; Byrne D.J.; Broadley M.W.; Marty B. | |
发表日期 | 2021 |
ISSN | 00278424 |
卷号 | 118期号:11 |
英文摘要 | The age of iron meteorites implies that accretion of protoplanets began during the first millions of years of the solar system. Due to the heat generated by 26Al decay, many early protoplanets were fully differentiated with an igneous crust produced during the cooling of a magma ocean and the segregation at depth of a metallic core. The formation and nature of the primordial crust generated during the early stages of melting is poorly understood, due in part to the scarcity of available samples. The newly discovered meteorite Erg Chech 002 (EC 002) originates from one such primitive igneous crust and has an andesite bulk composition. It derives from the partial melting of a noncarbonaceous chondritic reservoir, with no depletion in alkalis relative to the Sun's photosphere and at a high degree of melting of around 25%. Moreover, EC 002 is, to date, the oldest known piece of an igneous crust with a 26Al-26Mg crystallization age of 4,565.0 million years (My). Partial melting took place at 1,220 °C up to several hundred kyr before, implying an accretion of the EC 002 parent body ca. 4,566 My ago. Protoplanets covered by andesitic crusts were probably frequent. However, no asteroid shares the spectral features of EC 002, indicating that almost all of these bodies have disappeared, either because they went on to form the building blocks of larger bodies or planets or were simply destroyed. © 2021 National Academy of Sciences. All rights reserved. |
英文关键词 | Andesitic magmatism; Differentiated meteorites; Early solar system; Planetary differentiation |
语种 | 英语 |
来源期刊 | Proceedings of the National Academy of Sciences of the United States of America
![]() |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/180283 |
作者单位 | Univ Brest, CNRS, IR4, Ifremer, LEMAR, Plouzané, F-29280, France; Institut de physique du globe de Paris, CNRS, Université de Paris, Paris, F-75005, France; National Institute of Polar Research, Tachikawa, Tokyo, 190-8518, Japan; CNRS, Institut de Planetologie et d'Astrophysique de Grenoble, Saint Martin d'Hères, F-38400, France; Université de Lorraine, CNRS, CRPG, Nancy, F-54000, France |
推荐引用方式 GB/T 7714 | Barrat J.-A.,Chaussidon M.,Yamaguchi A.,et al. A 4,565-My-old andesite from an extinct chondritic protoplanet[J],2021,118(11). |
APA | Barrat J.-A..,Chaussidon M..,Yamaguchi A..,Beck P..,Villeneuve J..,...&Marty B..(2021).A 4,565-My-old andesite from an extinct chondritic protoplanet.Proceedings of the National Academy of Sciences of the United States of America,118(11). |
MLA | Barrat J.-A.,et al."A 4,565-My-old andesite from an extinct chondritic protoplanet".Proceedings of the National Academy of Sciences of the United States of America 118.11(2021). |
条目包含的文件 | 条目无相关文件。 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。