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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- 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 ...
by Geoffrey A. Blake - California Institute of Technology
This course discusses the fundamental aspects of atomic and molecular spectra that enable one to infer physical conditions in astronomical, planetary and terrestrial environments from the analysis of their electromagnetic radiation.
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.
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.