4.6 Review Book Chapter

The Stardust Mission: Analyzing Samples from the Edge of the Solar System

期刊

出版社

ANNUAL REVIEWS
DOI: 10.1146/annurev-earth-050212-124203

关键词

comet; Jupiter family comet; Solar System origin; Kuiper belt; meteorite; interplanetary dust; IDP; olivine; chondrule; calcium-aluminum inclusion; presolar grain; isotopic anomaly; solar nebula; accretion; Stardust; parent body; asteroid; KBO

向作者/读者索取更多资源

Comet samples returned to Earth by the NASA Stardust mission have provided a surprising glimpse into the nature of early Solar System materials and an epiphany on the origin of the initial rocky materials that once filled the cold regions of the solar nebula. The findings show that the cold regions of the early Solar System were not isolated and were not a refuge where interstellar materials could commonly survive. Wild 2, the sampled comet, appears to be a typical active Jupiter family comet, and yet most of its sampled micron and larger grains are familiar high-temperature meteoritic materials, such as chondrule fragments, that were transported to cold nebular regions. The rocky components in primitive asteroids and comets may differ because asteroid formation was dominated by local materials, whereas comets formed from mixed materials, many of which were transported from very distant locations.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.6
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据