Meteorites and the early solar system II
Meteorites and the early solar system II
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发表时间：
2006
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通讯作者：
D. Lauretta;H. McSween
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作者：
D. Lauretta;H. McSween
它们的大小从微小的颗粒到数吨的质量不等。小行星和太阳系其他岩石天体的地质多样性表现在陨石中观察到的各种各样的纹理和矿物。原始陨石的成分、化学和矿物学共同为各种各样的化学和物理过程提供了证据。这本书综合了我们目前对早期太阳系的理解，总结了有关其形成之前发生的过程的信息。它将是行星科学研究生教育的宝贵教科书，也是全世界有关领域的陨石学家和研究人员的参考资料。
They range in size from microscopic particles to masses of many tons. The geologic diversity of asteroids and other rocky bodies of the solar system are displayed in the enormous variety of textures and mineralogies observed in meteorites. The composition, chemistry, and mineralogy of primitive meteorites collectively provide evidence for a wide variety of chemical and physical processes. This book synthesizes our current understanding of the early solar system, summarizing information about processes that occurred before its formation. It will be valuable as a textbook for graduate education in planetary science and as a reference for meteoriticists and researchers in allied fields worldwide.