Compound chondrule formation via collision of supercooled droplets
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- 作者：Sota Arakawa ; arakawa.s.ac@m.titech.ac.jp" class="auth_mail" title="E-mail the corresponding author ; Taishi Nakamoto
- 关键词：Collisional physics ; Meteorites ; Planetesimals ; Solar Nebula ; Thermal histories
- 刊名：Icarus
- 出版年：2016
- 出版时间：15 September 2016
- 年：2016
- 卷：276
- 期：Complete
- 页码：102-106
- 全文大小：486 K
文摘
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Most of the compound chondrules are nonporphyritic in ordinary chondrites.
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Primaries of compound chondrules are larger than secondaries.
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Most of the compound chondrules are formed from completely molten droplets.
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Completely molten levitated droplets invariably turn into supercooled droplets.
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The supercooled-collision model can reproduce the observed features.