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
Voyager Encounters Jupiter- National Aeronautics and Space Administration
Passing by Jupiter in 1979, the Voyager spacecraft have collected an enormous amount of data that may prove to be a keystone in understanding our solar system. This publication provides an early look at the Jovian planetary system ...
(3253 views)
Solar System- Wikipedia
The Solar System consists of the Sun and its planetary system of eight planets, their moons, and other non-stellar objects. It formed 4.6 billion years ago from the collapse of a molecular cloud. The majority of the system's mass is in the Sun...
(7771 views)
Planetary Ringsby Matthew S. Tiscareno - arXiv
Understanding of disks in general can be enhanced by understanding the dynamical processes observed at close-range planetary rings. We review the known ring systems of the four giant planets, and the prospects for ring systems yet to be discovered.
(7268 views)
A Photographic Atlas of Rock Breakdown Features in Geomorphic Environmentsby Mary Bourke, Heather Viles - Planetary Science Institute
A comprehensive image collection of rock breakdown features observed on boulders. This atlas is intended as a tool for planetary geoscientists and their students to assist in identifying surface features found on rocks on planetary surfaces.
(21476 views)