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-List Of Titles -A Complex network analysis of growth and mixing dynamics in natural metal-silicate systems

Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.14/170549

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Title
A Complex network analysis of growth and mixing dynamics in natural metal-silicate systems
Related
Goldschmidt Conference (21st : 2011) (14 - 19 August 2011 : Prague, Czech Republic)
Related
Mineralogical magazine, Vol. 75, No. 3, p.1768
Related
http://goldschmidt.info/2011/index.html
Publisher
London : Mineralogical Society
Date
2011
Author/Creator
Rushmer, Tracy
Author/Creator
Tordesillas, Antoinette
Author/Creator
Walker, David M
Description
The segregation of metallic cores from silicate mantles is one of the earliest, and most important, differentiation process involved in the evolution of terrestrial planetary bodies and reconciling our estimates of primary bulk silicate mantle with candidate planetary bulk compositions requires an understanding of the different regimes in which core forming material may have been mobile. This includes regimes that are dynamic and may result in transient states of high stress due to impact. Recent scenarios of core formation in planetesimals using calculations from extinct radionuclides (e.g. (super 26) Al, (super 60) Fe) call for segregation of a metal liquid (core) from partially molten silicate - a silicate mush matrix. This segregation scenario requires growth of molten core material into blebs large enough to overcome the strength of the mush matrix so that separation can occur. However, currently there is no satisfactory explanation as to how or why metallic liquid blebs in the presence of silicate melt actually grow. Experimental work has suggested deformation and shear can help coalesce metallic blebs. Here, we have developed an innovative approach that combines textures in experimental deformation experiments on a partially molten natural meteorite with complex network analyses. This approach can elucidate and quantify the growth of metallic blebs in regions where a silicate mush matrix is present and help predict separation.
Description
1 page(s)
Resource Type
conference paper abstract
Organisation
Macquarie University. Dept. of Earth and Planetary Sciences

Identifier
http://hdl.handle.net/1959.14/170549
Identifier
ISSN: 0026-461X
Identifier
mq_res-ext-pro885354550
Language
eng
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Citation Format
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Subject
"Mineralogical magazine"
 
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