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.
General
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