Terrestrial planet evolution in the stagnant-lid regime: Size effects and the formation of self-destabilizing crust

Physics & Astronomy

• planetary mass 100%
• terrestrial planets 94%
• crusts 88%
• eclogite 88%
• Earth mantle 83%
• planetary crusts 54%
• viscosity 50%
• rheology 49%
• planetary evolution 41%
• plates (tectonics) 40%
• lithosphere 36%
• basalt 33%
• scaling 32%
• principal components analysis 29%
• mars 27%
• extrasolar planets 25%
• hydration 24%
• regression analysis 23%
• escape 22%
• temperature gradients 20%
• convection 20%
• simulation 17%
• temperature 6%

Earth & Environmental Sciences

• size effect 81%
• planet 62%
• crust 53%
• viscosity 40%
• mantle 38%
• eclogite 38%
• rheology 35%
• planetary evolution 28%
• brittle deformation 22%
• ductile deformation 21%
• thermal evolution 21%
• crustal thickness 20%
• deformation mechanism 20%
• plate tectonics 19%
• phase transition 18%
• temperature gradient 17%
• hydration 16%
• Mars 16%
• lithosphere 15%
• simulation 15%
• principal component analysis 14%
• basalt 14%
• convection 13%
• effect 8%
• temperature 6%