The Effect of Hydrostatic Pressure Up to 1.61 GPa on the Morin Transition of Hematite‐bearing Rocks: Implications for Planetary Crustal Magnetization

We present new experimental data on the dependence of the Morin transition temperature (T-M) on hydrostatic pressure up to 1.61 GPa, obtained on a well-characterized multidomain hematite-bearing sample from a banded iron formation. We used a nonmagnetic high-pressure cell for pressure application and a Superconducting Quantum Interference Device magnetometer to measure the isothermal remanent magnetization (IRM) under pressure on warming from 243 K to room temperature (T-0). IRM imparted at T-0 under pressure in 270 mT magnetic field (IRM270mT) is not recovered after a cooling-warming cycle. Memory effect under pressure was quantified as IRM recovery decrease of 10%/GPa. T-M, determined on warming, reaches T-0 under hydrostatic pressure 1.38-1.61 GPa. The pressure dependence of T-M up to 1.61 GPa is positive and essentially linear with a slope dT(M)/dP = (25 +/- 2) K/GPa. This estimate is more precise than previous ones and allows quantifying the effect of a pressure wave on the upper crust magnetization, with special emphasis on Mars.