Chondrules


Book Description

An overview of state-of-the-art research into properties and possible formation mechanisms of chondrules, by leading cosmochemists and astrophysicists.




Chondrules and the Protoplanetary Disk


Book Description

This 1996 text reviews current ideas about the formation of chondrules in meteorites.







The Origin of Chondrules and Chondrites


Book Description

Chondrites are the largest group of meteorites. They can provide unique insights into the origins and early evolution of our Solar System, and even into the relationships between our Solar System and other stars in the vicinity of our Sun. The largest structural components of most chondrites are the glass-bearing chondrules, and there are numerous theories for their origin. This clear and systematic text summarizes the ideas surrounding the origin and history of chondrules and chondrites, drawing on research from the various scientific disciplines involved. With citations to a large number of published papers on the topic, it forms a comprehensive bibliography of the key research areas, and extensive illustrations provide a clear visual representation of the scientific theories. This text will be a valuable reference for graduate students and researchers in planetary science, geology, and astronomy.










Workshop on Chondrites and the Protoplanetary Disk, Kaua'i Hawai'i, 2004


Book Description

In November 2004, a diverse, multi-disciplinary group of scientists met to discuss the formation of the solar system. The main subject of their meeting was the formation of the foundation stones of the planets, samples of which fall upon the Earth in the form of meteorites.




Protoplanetary Dust


Book Description

The first comprehensive overview of planet formation for students and researchers in astronomy, cosmochemistry, laboratory astrophysics and planetary sciences.







Meteorites and the Early Solar System II


Book Description

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.