Definition
Mars is the fourth Planet from the Sun and one of the terrestrial planets. It is named after the Roman god of war.
Overview
Mars accreted rapidly in a couple of million years (Brasser 2013) and differentiated within a few tens of millions years after the formation of the Solar System into a core, mantle, and crust, as indicated by isotope geochemistry (Lee and Halliday 1997; Mezger et al. 2013). It is commonly thought that the bulk composition of Mars is “chondritic” (Dreibus and Wänke 1985), i.e., similar to the composition of Carbonaceous Chondrites, the most primitive materials in the Solar System. The Fe-Ni-FeS core is dense and metal rich (Fig. 1) and its radius is about 50 % of the surface radius, the exact value depending on its content of lighter elements like sulfur. The remnant magnetization of parts of the Martian crust indicates that core convection induced by energy from core cooling and/or inner core growth might have produced a core magnetic dynamo and a...
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Forget, F., Hauber, E. (2015). Mars. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-44185-5_938
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