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NASA NTRS · 19740057511

Temperatures inside Mars - Is the core liquid or solid

Abstract

If internal heating in the mantle of Mars is similar to that in the earth, solid-state convection is the mechanism preventing large scale melting of the Martian mantle. Convection is efficient enough in transporting heat to preclude the existence of a liquid core and hence a dynamo-driven intrinsic magnetic field, if the viscosity of mantle material is lower than 10 to the 22nd to 10 to the 23rd sq cm/sec at temperatures in excess of about 1500 C. The Martian lithosphere is probably several hundred kilometers thick, intermediate in size between that of the earth and Moon.

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BibTeXRIS

Young, R. E., Schubert, G.. 1974-08-01. Temperatures inside Mars - Is the core liquid or solid. https://ntrs.nasa.gov/citations/19740057511

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