Gravitational Deformation in Shaping Ast
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Evgeniy N. Slyuta; Sergey A. Voropaev
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Article
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1997
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Elsevier Science
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English
β 339 KB
percent of their mean radii (R m ), but the roughness of the latter as a class (''planetary bodies'') is below 0.01R m . A variety of techniques have demonstrated that some of the solid bodies of the Solar System have distinct irregular shapes, Furthermore, the maximum topographic relief of small w