On the origin of the "kleine Kugelchen" called Chondrules

被引:44
作者
Connolly, HC
Desch, SJ
机构
[1] CUNY, Kingsborough Coll, Dept Phys Sci, Brooklyn, NY 11235 USA
[2] Amer Museum Nat Hist, Dept Earth & Planetary Sci, New York, NY 10024 USA
[3] Rutgers State Univ, Dept Geol Sci, Piscataway, NJ 08854 USA
[4] Arizona State Univ, Dept Phys & Astron, Tempe, AZ 85287 USA
关键词
chondrules; chondrule formation; chondrites; meteorites; protoplanetary disk; nebular processes;
D O I
10.1016/j.chemer.2003.12.001
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In this paper we investigate two major issues: (1) What are chondrules, and (2) why do they exist? We review the literature pertaining to each question and explore answers. We discuss the diversity of chondrules, especially with regard to their igneous textures and compositions. We review the constraints that have been placed experimentally on the thermal histories of chondrules and list those fundamental properties that all chondrule formation models must explain quantitatively in order to be considered predictive, quantitative models. We provide background on the three major classes of chondrule formation models currently being discussed, and scrutinize each with respect to how well they adhere to the experimental constraints placed on chondrule formation. Finally, we list several unresolved issues that are now or will soon be at the forefront of chondrule research. (C) 2004 Elsevier GmbH. All rights reserved.
引用
收藏
页码:95 / 125
页数:31
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