Description:
Murray and Dermott show how a basic knowledge of the two- and three-body problems and perturbation theory can be combined to understand features as diverse as the tidal heating of Jupiter's moon Io, the origin of the Kirkwood gaps in the asteroid belt, and the radial structure of Saturn's rings.
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Returnable at the third party seller's discretion and may come without consumable supplements like access codes, CD's, or workbooks.
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