作者: Robert J. Malcuit
DOI: 10.1007/978-3-319-11388-3_2
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摘要: The origin of the Solar System has intrigued scientists for centuries. As recently as five decades ago models were still very general and concerned mainly with collapse a cloud stellar dust gas roughly solar composition transformation that into rapidly rotating disk-shaped mass around proto-sun. next few dominated by calculations equilibrium chemical condensation from cooling nebula based on temperature pressure conditions Cameron Pine. Identification high-temperature condensates [calcium-aluminum inclusions (CAIs)] in Allende meteorite was critical event development more sophisticated evolution System. After discovery CAIs it important to develop explain (a) chondrules (the main constituent chondritic meteorites), (b) CAIs, well (c) fine-grained matrix meteorites.