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阿连德陨石中难熔包体与太阳星云气体之间的氧同位素交换。

Oxygen isotope exchange between refractory inclusion in Allende and solar nebula gas.

作者信息

Yurimoto H, Ito M, Nagasawa H

机构信息

Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Japan.

出版信息

Science. 1998 Dec 4;282(5395):1874-7.

PMID:9874638
Abstract

A calcium-aluminum-rich inclusion (CAI) from the Allende meteorite was analyzed and found to contain melilite crystals with extreme oxygen-isotope composition (approximately 5 percent oxygen-16 enrichment relative to terrestrial oxygen-16). Some of the melilite is also anomalously enriched in oxygen-16 compared with oxygen isotopes measured in other CAIs. The oxygen isotopic variation measured among the minerals (melilite, spinel, and fassaite) indicates that crystallization of the CAI started from oxygen-16-rich materials that were probably liquid droplets in the solar nebula, and oxygen isotope exchange with the surrounding oxygen-16-poor nebular gas progressed through the crystallization of the CAI. Additional oxygen isotope exchange also occurred during subsequent reheating events in the solar nebula.

摘要

对来自阿伦德陨石的一颗富钙铝包体(CAI)进行了分析,发现其中含有氧同位素组成极端的黄长石晶体(相对于地球的氧 - 16,氧 - 16富集约5%)。与在其他CAI中测得的氧同位素相比,一些黄长石中的氧 - 16也异常富集。在矿物(黄长石、尖晶石和斜硅钙钛矿)中测得的氧同位素变化表明,CAI的结晶始于可能是太阳星云液滴的富氧 - 16物质,并且随着CAI的结晶,与周围贫氧 - 16星云气体进行了氧同位素交换。在太阳星云随后的再加热事件中也发生了额外的氧同位素交换。

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