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Evidence for a Dynamo in the Main Group Pallasite Parent Body
Understanding the origin of pallasites, stony-iron meteorites made mainly of olivine crystals and FeNi metal, has been a vexing problem since their discovery. Here, we show that pallasite olivines host minute magnetic inclusions that have favorable magnetic recording properties. Our paleointensity m...
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Published in: | Science (American Association for the Advancement of Science) 2012-11, Vol.338 (6109), p.939-942 |
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container_issue | 6109 |
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container_title | Science (American Association for the Advancement of Science) |
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creator | Tarduno, John A. Cottrell, Rory D. Nimmo, Francis Hopkins, Julianna Voronov, Julia Erickson, Austen Blackman, Eric Scott, Edward R.D. McKinley, Robert |
description | Understanding the origin of pallasites, stony-iron meteorites made mainly of olivine crystals and FeNi metal, has been a vexing problem since their discovery. Here, we show that pallasite olivines host minute magnetic inclusions that have favorable magnetic recording properties. Our paleointensity measurements indicate strong paleomagnetic fields, suggesting dynamo action in the pallasite parent body. We use these data and thermal modeling to suggest that some pallasites formed when liquid FeNi from the core of an impactor was injected as dikes into the shallow mantle of a ~200-kilometer-radius protoplanet. The protoplanet remained intact for at least several tens of millions of years after the olivine-metal mixing event. |
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Here, we show that pallasite olivines host minute magnetic inclusions that have favorable magnetic recording properties. Our paleointensity measurements indicate strong paleomagnetic fields, suggesting dynamo action in the pallasite parent body. We use these data and thermal modeling to suggest that some pallasites formed when liquid FeNi from the core of an impactor was injected as dikes into the shallow mantle of a ~200-kilometer-radius protoplanet. The protoplanet remained intact for at least several tens of millions of years after the olivine-metal mixing event.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1223932</identifier><identifier>PMID: 23161997</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Asteroids ; Boundaries ; Cooling ; Core mantle boundary ; Cosmochemistry. 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subjects | Asteroids Boundaries Cooling Core mantle boundary Cosmochemistry. Extraterrestrial geology Crystals Demagnetization Earth sciences Earth, ocean, space Exact sciences and technology Liquids Magnetic fields Magnetization Meteorites Meteorites. Tectites. Impactites Meteors & meteorites Olivine Parents Planets Protoplanets Rotating generators |
title | Evidence for a Dynamo in the Main Group Pallasite Parent Body |
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