151. A thermally conductive Martian core and implications for its dynamo cessation.
- Author
-
Wen-Pin Hsieh, Deschamps, Frédéric, Yi-Chi Tsao, Takashi Yoshino, and Jung-Fu Lin
- Subjects
- *
ELECTRIC generators , *THERMAL conductivity , *CORE-mantle boundary , *ELECTRICAL resistivity , *IRON alloys , *MAGNETIC fields - Abstract
Mars experienced a dynamo process that generated a global magnetic field ~4.3 (or earlier) to 3.6 billion years ago (Ga). The cessation of this dynamo strongly affected Mars' history and is expected to be linked to thermochemical evolution of Mars' iron-rich liquid core, which is strongly influenced by its thermal conductivity. Here, we directly measured thermal conductivities of solid iron-sulfur alloys to pressures relevant to the Martian core and temperatures to 1023 Kelvin. Our results show that a Martian core with 16 weight % sulfur has a thermal conductivity of ~19 to 32 Watt meter-1 Kelvin-1 from its top to the center, much higher than previously inferred from electrical resistivity measurements. Our modeled thermal conductivity profile throughout the Martian deep-mantle and core indicates a ~4-to 6-fold discontinuity across the core-mantle boundary. The core's efficient cooling resulting from the depth-dependent, high conductivity diminishes thermal convection and forms thermal stratification, substantially contributing to cessation of Martian dynamo. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF