Giant impacts on early Mars and the cessation of the Martian dynamo

Details Giant impacts on early Mars and the cessation of the Martian dynamo Giant impacts on early Mars and the cessation of the Martian dynamo

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jgre..11404009r&link_type=abstract

Journal of Geophysical Research, Volume 114, Issue E4, CiteID E04009

Physics

21

Planetary Sciences: Solid Surface Planets: Interiors (8147), Planetary Sciences: Solar System Objects: Mars, Planetary Sciences: Solid Surface Planets: Impact Phenomena, Cratering (6022, 8136), Tectonophysics: Dynamics: Convection Currents, And Mantle Plumes, Planetary Sciences: Solid Surface Planets: Magnetic Fields And Magnetism

Scientific paper

Although Mars currently has no global dynamo-driven magnetic field, widespread crustal magnetization provides strong evidence that such a field existed in the past. The absence of magnetization in the younger large Noachian basins suggests that a dynamo operated early in Martian history but stopped in the mid-Noachian. Within a 100 Ma period, 15 giant impacts occurred coincident with the disappearance of the global magnetic field. Here we investigate a possible causal link between the giant impacts during the early and mid-Noachian and the cessation of the Martian dynamo at about the same time. Using three-dimensional spherical mantle convection models, we find that impact heating associated with the largest basins (diameters >2500 km) can cause the global heat flow at the core-mantle boundary to decrease significantly (10-40%). We suggest that such a reduction in core heat flow may have led to the cessation of the Martian dynamo.

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