Solar System Astrophysics: Background Science and the Inner Solar System

Solar System Astrophysics cover the field of solar system astrophysics beginning with basic tools of spherical astronomy, coordinate frames, and celestial mechanics. Historical introductions precede the development and discussion in most chapters. After a basic treatment of the two- and restricted three-body system motions, perturbations are discussed, followed by the Earth's gravitational potential field and its effect on satellite orbits. This is followed by a chapter on the observable properties of the Sun and then by analysis of the Earth-Moon system and the interior planets. The atmospheres chapters include detailed discussions of circulation, applicable also to the subsequent discussion of the gas giants. A comparative planetary approach is also given to discussions of the atmospheric and ionospheric chemistry, magnetospheres, and crustal properties.

The giant planets are discussed together, and the thermal excess of three of them highlighted. This is followed by chapters on moons and rings, mainly in the context of dynamical stability, comets and meteors, meteorites and asteroids, and concludes with an extensive discussion of extrasolar planets. The contents of Solar System Astrophysics have been field-tested by students for many years. Eugene F. Milone and William J.F. Wilson have written an entirely unique book that presents an up-to-date overview on all essential topics based on extensive experience in the classroom.