An Overview of the Solar System
Publisher: Wikipedia 2013
The Solar System comprises the Sun and its planetary system of eight planets, as well as a number of dwarf planets, satellites, and other objects that orbit the Sun. It formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud.
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by Hannes Alfven, Gustaf Arrhenius - NASA
A realistic attempt to reconstruct the early history of the solar system. The authors chose a procedure which reduces speculation as much as possible and connects the evolutionary models as closely as possible to experiment and observation.
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.
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 conventional divisions of this volume of space.
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.