The Evolution of Matter explains how all matter in the Universe
developed following the Big Bang and through subsequent stellar
processes. It describes the evolution of interstellar matter and
its differentiation during the accretion of the planets and the
history of the Earth. Unlike many books on geochemistry, this
volume follows the chemical history of matter from the very
beginning to the present, demonstrating connections in space and
time. It provides also solid links from cosmochemistry to the
geochemistry of Earth. The book presents comprehensive descriptions
of the various isotope systematics and fractionation processes
occurring naturally in the Universe, using simple equations and
helpful tables of data. With a glossary of terms and over 900
references, this volume is a valuable reference for researchers and
advanced students studying the chemical evolution of the Earth, the
Solar System and the wider Universe.
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