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...

Full description

Saved in:
Bibliographic Details
Published inScience (American Association for the Advancement of Science) Vol. 338; no. 6109; pp. 939 - 942
Main Authors Tarduno, John A., Cottrell, Rory D., Nimmo, Francis, Hopkins, Julianna, Voronov, Julia, Erickson, Austen, Blackman, Eric, Scott, Edward R.D., McKinley, Robert
Format Journal Article
LanguageEnglish
Published Washington, DC American Association for the Advancement of Science 16.11.2012
The American Association for the Advancement of Science
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary: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.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0036-8075
1095-9203
DOI:10.1126/science.1223932