Astrochemistry
Chemistry of the solar system
Katharina Lodders and Bruce Fegley, Jr
Cambridge, UK: Royal Society of Chemistry 2010 | 476pp | £29.95 (PB)
ISBN 9780854041282
Reviewed by Stephen Price

© Royal Society of Chemistry |
These themes are, in general, treated in significant depth, including many historical asides on the development of various key concepts. For example, the nine or so pages of discussion on the density and structure of the Earth present a chronological overview of the ideas developed in this field, beginning with William Gilbert in 1600.
I appreciated the abundant data, in tables and figures, to support the arguments presented. These data range from elemental abundance ratios in meteorites to the composition of the Earth's biosphere. The depth of treatment, the data presented and the associated detailed discussion perhaps make the book more a valuable resource for professional researchers rather than the general reader, although the latter is clearly identified as part of the target audience.
With a background in astrochemistry, most chapters of this book introduced me to a wealth of new information. However, the level of detail in the discussion does not make the book an easy read. The account also takes many pages to reach what a conventional chemist might recognise as 'real chemistry'. However, I felt the more overtly chemical topics that are discussed would be more familiar to the general chemist, but in a single chapter these large topics cannot be covered in sufficient detail for the specialist reader.
This book will be a tremendous resource for scientists wanting to familiarise themselves with the development of specific topics in planetary science. However, some of the topics are presented at a level of detail that might make the casual chemical reader a little wary.
RSC members can purchase this book direct from the RSC for a 35% discount.
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Chemistry of the Solar System
Copyright: 2010Katharina Lodders
Covers the chemical composition of bodies in the solar system, the major chemical processes that controlled the chemistry when they were formed and that operates on them today.
