From Disks to Planets
by Andrew N. Youdin, Scott J. Kenyon
Publisher: arXiv 2012
Number of pages: 70
Description:
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.
Download or read it online for free here:
Download link
(1.3MB, PDF)
Similar books
Planetary Photometryby 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.
(12261 views)
Lunar Orbiter Photographic Atlas of the Moonby D.E. Hughes, J.K. Bowker - Lunar and Planetary Institute
This Atlas is considered the definitive reference manual to the global photographic coverage of the Moon. The images contained within the atlas are excellent for studying lunar morphology because they were obtained at low to moderate Sun angles.
(12035 views)
Lecture notes on the formation and early evolution of planetary systemsby Philip J. Armitage - arXiv
An introduction to the theory of the formation and early evolution of planetary systems. Topics covered: the structure, evolution and dispersal of protoplanetary disks; the formation of planetesimals, terrestrial and gas giant planets; etc.
(11247 views)
Lunar Stratigraphy and Sedimentologyby 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.
(12244 views)