Harry Y. McSween Jr – författare

Meteorites and Their Parent Planets provides an engrossing overview of a highly interdisciplinary field - the study of extraterrestrial materials. The second edition of this successful book has been thoroughly revised, and describes the nature of meteorites, where they come from, and how they get to Earth. Meteorites offer important insights into processes in stars and in interstellar regions, the birth of our solar system, the formation and evolution of planets and smaller bodies, and the origin of life. The first edition was immensely popular with meteorite collectors, scientists and science students in many fields, and amateur astronomers. In this second edition all of the illustrations have been updated and improved, many sections have been expanded and modified based on discoveries in the last decade, and a new final chapter on the importance of meteorites has been added. Everyone with an interest in meteorites will want a copy of this book.

Meteorites and Their Parent Planets provides an engrossing overview of a highly interdisciplinary field - the study of extraterrestrial materials. The second edition of this successful book has been thoroughly revised, and describes the nature of meteorites, where they come from, and how they get to Earth. Meteorites offer important insights into processes in stars and in interstellar regions, the birth of our solar system, the formation and evolution of planets and smaller bodies, and the origin of life. The first edition was immensely popular with meteorite collectors, scientists and science students in many fields, and amateur astronomers. In this second edition all of the illustrations have been updated and improved, many sections have been expanded and modified based on discoveries in the last decade, and a new final chapter on the importance of meteorites has been added. Everyone with an interest in meteorites will want a copy of this book.

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 synthesises our current understanding of the early solar system, summarising 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.