Evolution of the Solar System
by Hannes Alfven, Gustaf Arrhenius
Publisher: NASA 1976
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.
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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 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.
The Solar System comprises the Sun and its planetary system, 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.
by Elbert A. King - Lunar and Planetary Institute
The excitement of the Apollo program was that it accomplished a bold leap from the surface of the Earth to the Moon. The deed challenged our technology and engineering skill. Preparations are being made now for another and even more daring leap.