Early magnetic field and magmatic activity on Mars from magma ocean cumulate overturn

Linda T. Elkins-Tanton, Sarah E. Zaranek, E. M. Parmentier, P. C. Hess

Research output: Contribution to journalArticle

83 Scopus citations

Abstract

Significant and perhaps complete melting of the young terrestrial planets is expected from their heat of accretion and core formation. The process of subsequent magma ocean fractional solidification creates a cumulate mantle unstable to gravitational overturn. Overturn should be fast (≤1 to 10 Ma) and result in increasing mantle density with depth. This stable stratification inhibits later thermal convection, preserving geochemical heterogeneities. Overturn places cold cumulates against the core-mantle boundary, which creates sufficient heat flux to drive a core dynamo, producing a brief, strong magnetic field. During overturn, hot cumulates rise from depth and melt adiabatically, creating an early crust to record this field and leaving behind mantle reservoirs with isotopic fractionations dating from the early evolution of the planet.

Original languageEnglish (US)
Pages (from-to)1-12
Number of pages12
JournalEarth and Planetary Science Letters
Volume236
Issue number1-2
DOIs
StatePublished - Jul 30 2005
Externally publishedYes

Keywords

  • Cumulates
  • Magma ocean
  • Magnetic field
  • Mantle heterogeneity
  • Mars

ASJC Scopus subject areas

  • Geophysics
  • Geochemistry and Petrology
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

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