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 Max Fairbairn
The text covers principles of planetary photometry: radiance and the equation of transfer, diffuse reflection and transmission, albedo, scattering and absorption, net flux and exitance, and a brief history of the Lommel-Seeliger law.
by Elbert A. King - The Lunar and Planetary Institute
The origins of chondrules are fundamental problems of most stony meteorites and some planetary surface samples. The contents of this volume are designed to provide the reader with a broad overview of current ideas in this area of research.
by John Lindsay - Elsevier
Lunar Stratigraphy and Sedimentology is an attempt to organize some of the information now available about the sedimentary rocks forming the lunar crust in a way that allows some comparison with the terrestrial sedimentary environment.
by W. K. Hartmann, R. J. Phillips, G. J. Taylor - Lunar and Planetary Institute
Contents: History; Dynamical Constraints; Geochemical Constraints; Geophysical Constraints; Theories and Processes of Origin: Lunar Formation Involving Capture or Fission; Lunar Formation Triggered by Large Impact; and more.