From Disks to Planets
by Andrew N. Youdin, Scott J. Kenyon
Publisher: arXiv 2012
Number of pages: 70
This pedagogical chapter covers the theory of planet formation, with an emphasis on the physical processes relevant to current research. After summarizing empirical constraints from astronomical and geophysical data, we describe the structure and evolution of protoplanetary disks. We consider the growth of planetesimals and of larger solid protoplanets, followed by the accretion of planetary atmospheres, including the core accretion instability.
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by Andrew J. Butrica - NASA History Division
A comprehensive history of this surprisingly significant scientific discipline. Quite rigorous and systematic in its methodology, To See the Unseen explores the development of the radar astronomy specialty in the larger community of scientists.
- Pergamon Press
The theme of this book is the study of basaltic volcanism on the terrestrial planets as a stage in planetary evolution: to use the eruption of lava from the interior of a planet as evidence of the thermal and chemical processes of the planet.
by Stuart Ross Taylor - Lunar and Planetary Institute
The technical triumph of manned landings on the Moon and the return of samples from the lunar surface has provided scientists with a unique opportunity to advance our understanding of the nature, evolution and origin of the solar system.
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A detailed introduction to impact processes, crater formation, and shock metamorphism. The book is intended for geoscientists of all kinds: students, professors and professional geologists who may encounter an impact structure in the field area.