Magnetic classification of stony meteorites: 3. Achondrites
A database of magnetic susceptibility measurements of stony achondrites (acapulcoitelodranite clan, winonaites, ureilites, angrites, aubrites, brachinites, howardite-eucrite-diogenite (HED) clan, and Martian meteorites, except lunar meteorites) is presented and compared to our previous work on chond...
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The Meteoritical Society
2009
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ftingv:oai:www.earth-prints.org:2122/5061 |
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Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
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English |
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meteorites magnetic susceptibility rock magnetism 04. Solid Earth::04.05. Geomagnetism::04.05.07. Rock magnetism |
| spellingShingle |
meteorites magnetic susceptibility rock magnetism 04. Solid Earth::04.05. Geomagnetism::04.05.07. Rock magnetism Rochette, P. Gattacceca, J. Bourot-Denise, M. Consolmagno, G. Folco, L. Kohout, T. Pesones, L. Sagnotti, L. Magnetic classification of stony meteorites: 3. Achondrites |
| topic_facet |
meteorites magnetic susceptibility rock magnetism 04. Solid Earth::04.05. Geomagnetism::04.05.07. Rock magnetism |
| description |
A database of magnetic susceptibility measurements of stony achondrites (acapulcoitelodranite clan, winonaites, ureilites, angrites, aubrites, brachinites, howardite-eucrite-diogenite (HED) clan, and Martian meteorites, except lunar meteorites) is presented and compared to our previous work on chondrites. This database provides an exhaustive study of the amount of iron-nickel magnetic phases (essentially metal and more rarely pyrrhotite and titanomagnetite) in these meteorites. Except for ureilites, achondrites appear much more heterogeneous than chondrites in metal content, both at the meteorite scale and at the parent body scale. We propose a model to explain the lack of or inefficient metal segregation in a low gravity context. The relationship between grain density and magnetic susceptibility is discussed. Saturation remanence appears quite weak in most metal-bearing achondrites(HED and aubrites)compared to Martian meteorites. Ureilites are a notable exception and can carry a strong remanence, similar to most chondrites. Published 405 - 427 2.2. Laboratorio di paleomagnetismo JCR Journal reserved |
| author2 |
Rochette, P.; CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Gattacceca, J.; CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Bourot-Denise, M.; Museum National d’Histoire Naturelle, Paris, France Consolmagno, G.; Specola Vaticana, Vatican City State Folco, L.; Museo Nazionale dell'Antartide, Università di Siena, Italy Kohout, T.; 5University of Helsinki, Finland Pesones, L.; 5University of Helsinki, Finland Sagnotti, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Museum National d’Histoire Naturelle, Paris, France Specola Vaticana, Vatican City State Museo Nazionale dell'Antartide, Università di Siena, Italy 5University of Helsinki, Finland Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia |
| format |
Article in Journal/Newspaper |
| author |
Rochette, P. Gattacceca, J. Bourot-Denise, M. Consolmagno, G. Folco, L. Kohout, T. Pesones, L. Sagnotti, L. |
| author_facet |
Rochette, P. Gattacceca, J. Bourot-Denise, M. Consolmagno, G. Folco, L. Kohout, T. Pesones, L. Sagnotti, L. |
| author_sort |
Rochette, P. |
| title |
Magnetic classification of stony meteorites: 3. Achondrites |
| title_short |
Magnetic classification of stony meteorites: 3. Achondrites |
| title_full |
Magnetic classification of stony meteorites: 3. Achondrites |
| title_fullStr |
Magnetic classification of stony meteorites: 3. Achondrites |
| title_full_unstemmed |
Magnetic classification of stony meteorites: 3. Achondrites |
| title_sort |
magnetic classification of stony meteorites: 3. achondrites |
| publisher |
The Meteoritical Society |
| publishDate |
2009 |
| url |
http://hdl.handle.net/2122/5061 |
| genre |
Polar Research |
| genre_facet |
Polar Research |
| op_relation |
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ftingv:oai:www.earth-prints.org:2122/5061 2023-05-15T18:02:44+02:00 Magnetic classification of stony meteorites: 3. Achondrites Rochette, P. Gattacceca, J. Bourot-Denise, M. Consolmagno, G. Folco, L. Kohout, T. Pesones, L. Sagnotti, L. Rochette, P.; CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Gattacceca, J.; CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Bourot-Denise, M.; Museum National d’Histoire Naturelle, Paris, France Consolmagno, G.; Specola Vaticana, Vatican City State Folco, L.; Museo Nazionale dell'Antartide, Università di Siena, Italy Kohout, T.; 5University of Helsinki, Finland Pesones, L.; 5University of Helsinki, Finland Sagnotti, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia CEREGE, CNRS Aix-Marseille University, BP80 13545 Aix en Provence, Cedex 4, France Museum National d’Histoire Naturelle, Paris, France Specola Vaticana, Vatican City State Museo Nazionale dell'Antartide, Università di Siena, Italy 5University of Helsinki, Finland Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia 2009 http://hdl.handle.net/2122/5061 en eng The Meteoritical Society Meteoritics & Planetary Science 3 / 44 (2009) Bouhifd M. A., Richet P., Besson P., Roskosz M., and Ingrin J. 2004. Redox state, microstructure and viscosity of a partially crystallized basalt melt. Earth and Planetary Science Letters 218:31–44. Brecher A. and Furhman M. 1979. The magnetic effects of brecciation and shock in meteorites: II. The ureilites and evidence for strong nebula magnetic fields. The Moon and the Planets 20:251–263. Brecher A., Furhman M., and Stein J. 1979. The magnetic effects of brecciation and shock in meteorites: III. The achondrites. The Moon and the Planets 20:265–279. Britt D. T. and Consolmagno G. J. 2003. Stony meteorite porosities and densities: A review of the data through 2001. Meteoritics & Planetary Science 38:1161–1180. Burroni and Folco L. 2008. Frontier Mountain meteorite specimens of the acapulcoite-lodranite clan: Petrography, pairing and parent-rock lithology of an unusual intrusive rock. Meteoritics & Planetary Science 43:1–14. Carmichael R. S. 1989. 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Rock magnetism article 2009 ftingv 2022-07-29T06:05:19Z A database of magnetic susceptibility measurements of stony achondrites (acapulcoitelodranite clan, winonaites, ureilites, angrites, aubrites, brachinites, howardite-eucrite-diogenite (HED) clan, and Martian meteorites, except lunar meteorites) is presented and compared to our previous work on chondrites. This database provides an exhaustive study of the amount of iron-nickel magnetic phases (essentially metal and more rarely pyrrhotite and titanomagnetite) in these meteorites. Except for ureilites, achondrites appear much more heterogeneous than chondrites in metal content, both at the meteorite scale and at the parent body scale. We propose a model to explain the lack of or inefficient metal segregation in a low gravity context. The relationship between grain density and magnetic susceptibility is discussed. Saturation remanence appears quite weak in most metal-bearing achondrites(HED and aubrites)compared to Martian meteorites. Ureilites are a notable exception and can carry a strong remanence, similar to most chondrites. Published 405 - 427 2.2. Laboratorio di paleomagnetismo JCR Journal reserved Article in Journal/Newspaper Polar Research Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Geophysical Research Letters 34 14 |