Trans-Neptunian Objects: An Overview
Publisher: Wikipedia 2014
A trans-Neptunian object is any minor planet in the Solar System that orbits the Sun at a greater average distance (semi-major axis) than Neptune. The Kuiper belt, scattered disk, and Oort cloud are three conventional divisions of this volume of space.
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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.
by William Sheehan - University of Arizona Press
Sheehan offers an accessible history of the men who collected data about Mars and interpreted it. The central story is the coherent and compelling narrative of Giovanni Schiaparelli, Percival Lowell and the description of the 'canals' of Mars.
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 Jonathan P. Williams, Lucas A. Cieza - arXiv
Flattened disks of cool dust and gas are found around almost all low mass stars shortly after their birth. This review addresses observations of the outer parts of protoplanetary disks with a focus on recent infrared and (sub-)millimeter results.