Magnetic properties of Antarctic shergottite meteorites EETA 79001 and ALHA 77005 - Possible relevance to a Martian magnetic field

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Achondrites, Magnetic Properties, Mars (Planet), Planetary Magnetic Fields, Antarctic Regions, Magnetization, Petrology, Remanence, Meteorites, Magnetic Properties, Antarctic Meteorites, Shergottites, Mars, Eeta79001, Elephant Moraine Meteorites, Alha77005, Allan Hills Meteorites, Magnetic Fields, Eucrites, Achondrites, Magnetization, Shock Effects, Formation, Samples, Meteorite, Magnetite, Strength

Scientific paper

The possibility that the parent body of the SNC meteorites is Mars implies that the magnetic properties of these meteorites may provide evidence concerning ancient Martian magnetic fields. EETA 79001 possesses a weak, very stable primary magnetization, the properties of which are consistent with its acquisition in an ambient magnetic field either during the meteorite's formation or during the severe shock event later in its history. The samples of ALHA 77005 studied possessed no measurable primary magnetization; the observed remanence appears to be a viscous magnetization acquired in local laboratory fields. The magnetic carriers in the meteorites are fine-grained magnetite and a lower Curie point mineral, probably titanomagnetite or pyrrhotite, present to the extent of less than 0.1 percent by weight. Estimates of the strength of the magnetizing field for EETA 79001 are in the range 1-10 microteslas.

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