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Journal article

Magnetic Properties Experiments on the Mars exploration Rover Spirit at Gusev crater

By Bertelsen, Pernille1; Goetz, W.; Madsen, M.B.; Kinch, K.M.; Hviid, S.F.; Knudsen, J.M.; Gunnlaugsson, H.P.; Merrison, J.; Nornberg, P.; Squyres, S.W.; Bell, J.F.; Herkenhoff, K.E.; Gorevan, S.; Yen, A.S.; Myrick, T.; Klingelhofer, G.; Rieder, R.; Gellert, R. ...and 8 more

From

Department of Management Engineering, Technical University of Denmark1

The magnetic properties experiments are designed to help identify the magnetic minerals in the dust and rocks on Mars-and to determine whether liquid water was involved in the formation and alteration of these magnetic minerals. Almost all of the dust particles suspended in the martian atmosphere must contain ferrimagnetic minerals (such as maghemite or magnetite) in an amount of similar to2% by weight.

The most magnetic fraction of the dust appears darker than the average dust. Magnetite was detected in the first two rocks ground by Spirit.

Language: English
Publisher: American Association for the Advancement of Science
Year: 2004
Pages: 827-829
ISSN: 10959203 , 00368075 and 03686396
Types: Journal article
DOI: 10.1126/science.1100112
ORCIDs: 0000-0001-8909-5111
Keywords

Atmosphere Extraterrestrial Environment Ferrosoferric Oxide Geologic Sediments Iron Magnetics Mars Minerals Oxides Water

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