NATS 1570 Lecture Notes - Lecture 21: Mantle Convection, Axial Tilt, Coriolis Force

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What types of volcanoes are there: yes, shield and hot spot, not running. If so, where: shadows of craters at north pole. Both planet and water warm up so less dissolving of carbon dioxide: describe the possibility of early oceans. Igneous: what else could have made water disappear and how? (hint reason venus has sulphuric acid clouds) - evaporation. 1: what are the two smalls moons of mars and describe them. Permafrost deep below surface: describe the glaciers. Water rock interactions, bacteria: describe the three main eras of mars. Lack of atmosphere (due to lack of magnetic field, solar wind stripped atmosphere away), losing volcanic activity, breakup of water by uv light. Io, ganymede, callisto, europa: what is atu(cid:396)(cid:374)"s la(cid:396)gest (cid:373)oo(cid:374)? titan. Mate(cid:396)ial eje(cid:272)ted f(cid:396)o(cid:373) (cid:448)ol(cid:272)a(cid:374)oes, fo(cid:396)(cid:373)s (cid:396)i(cid:374)g a(cid:396)ou(cid:374)d (cid:373)oo(cid:374) as jupite(cid:396)"s. Shredding due to gravity: what will happen to the rings overtime? decay. C type 83%, carbon, low reflectivity, s-type silicates, 15%, best reflectivituuy, m typep 2-3, metallic, metal.

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