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| | Tectonics of the terrestrial planets |
 | | The major possibilities are nonuniform contraction, despinning, volcanism, isostatic adjustment, and several varieties of convection, including homogeneous, layered, plate-tectonic, delaminating, and plumose. |
 | | All of the five planets considered show volcanism and some isostatic adjustment in their early histories, supporting the concepts of hot accretion, early differentiation, and gradual cooling. |
 | | On the smaller planets (the Moon and Mercury), a global lithosphere formed early and remained unbroken, or was only slightly cracked, by the small strains of nonuniform contraction and perhaps despinning. |
| element.ess.ucla.edu /publications/1986_planetology/1986_planetology.htm (454 words) |
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