Other
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmgp41c..05g&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #GP41C-05
Other
0654 Plasmas, 0925 Magnetic And Electrical Methods (5109), 1517 Magnetic Anomalies: Modeling And Interpretation, 1540 Rock And Mineral Magnetism, 3929 Nmr, Mossbauer Spectroscopy, And Other Magnetic Techniques
Scientific paper
The thermal and tectonic history of planets can be gleaned from the ancient magnetic fields recorded in their rock records. Because meteorite impacts alter the magnetic signals of rocks, one can hope to work out an approximate magnetic stratigraphy of a planet based on the relative timing of core dynamo activity versus the age of meteorite impact. Such is the common perception for Mars, whose giant impact craters, Hellas and Argyre, possess significantly lower magnetizations than surrounding regions. The typical assumption is that rocks in the craters were shock demagnetized in the absence of a core dynamo. To test these assumptions and to better understand the effects of stress on the remanent magnetizations of rocks, we have been carrying out both laboratory and field experiments. Here we report stress demagnetization experiments on single and multi-domain magnetite, the magnetic mineral most likely to carry the magnetic remanence on Mars. We also report paleomagnetic and geomagnetic measurements in the Vredefort crater, whose basement rocks carry magnetite as the remanence-bearing magnetic mineral. We conclude that magnetic fields fossilized in the rock record of meteorite impacts cannot be used to ascertain the presence or absence of a planet`s dynamo as previously assumed.
Carporzen Laurent
Galdeano Armand
Gilder Stuart
Hart Rodger J.
Le Goff Maxime
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