Compositional layering in io driven by magmatic segregation and volcanism

The compositional evolution of volcanic bodies like Io is not well understood. Magmatic segregation and volcanic eruptions transport tidal heat from Io's interior to its surface. Several observed eruptions appear to be extremely high temperature (≥1600 K), suggesting either very high degrees of...

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Main Authors: Spencer, DC, Katz, RF, Hewitt, IJ, May, DA, Keszthelyi, LP
Format: Journal article
Language:English
Published: Wiley 2020
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author Spencer, DC
Katz, RF
Hewitt, IJ
May, DA
Keszthelyi, LP
author_facet Spencer, DC
Katz, RF
Hewitt, IJ
May, DA
Keszthelyi, LP
author_sort Spencer, DC
collection OXFORD
description The compositional evolution of volcanic bodies like Io is not well understood. Magmatic segregation and volcanic eruptions transport tidal heat from Io's interior to its surface. Several observed eruptions appear to be extremely high temperature (≥1600 K), suggesting either very high degrees of melting, refractory source regions, or intensive viscous heating on ascent. To address this ambiguity, we develop a model that couples crust and mantle dynamics to a simple compositional system. We analyze the model to investigate chemical structure and evolution. We demonstrate that magmatic segregation and volcanic eruptions lead to stratification of the mantle, the extent of which depends on how easily high temperature melts from the more refractory lower mantle can migrate upwards. We propose that Io's highest temperature eruptions originate from this lower mantle region and that such eruptions act to limit the degree of compositional stratification.
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spelling oxford-uuid:41288f16-b486-4efd-84c8-83c770d760ad2022-03-26T14:41:55ZCompositional layering in io driven by magmatic segregation and volcanismJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:41288f16-b486-4efd-84c8-83c770d760adEnglishSymplectic ElementsWiley2020Spencer, DCKatz, RFHewitt, IJMay, DAKeszthelyi, LPThe compositional evolution of volcanic bodies like Io is not well understood. Magmatic segregation and volcanic eruptions transport tidal heat from Io's interior to its surface. Several observed eruptions appear to be extremely high temperature (≥1600 K), suggesting either very high degrees of melting, refractory source regions, or intensive viscous heating on ascent. To address this ambiguity, we develop a model that couples crust and mantle dynamics to a simple compositional system. We analyze the model to investigate chemical structure and evolution. We demonstrate that magmatic segregation and volcanic eruptions lead to stratification of the mantle, the extent of which depends on how easily high temperature melts from the more refractory lower mantle can migrate upwards. We propose that Io's highest temperature eruptions originate from this lower mantle region and that such eruptions act to limit the degree of compositional stratification.
spellingShingle Spencer, DC
Katz, RF
Hewitt, IJ
May, DA
Keszthelyi, LP
Compositional layering in io driven by magmatic segregation and volcanism
title Compositional layering in io driven by magmatic segregation and volcanism
title_full Compositional layering in io driven by magmatic segregation and volcanism
title_fullStr Compositional layering in io driven by magmatic segregation and volcanism
title_full_unstemmed Compositional layering in io driven by magmatic segregation and volcanism
title_short Compositional layering in io driven by magmatic segregation and volcanism
title_sort compositional layering in io driven by magmatic segregation and volcanism
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AT katzrf compositionallayeringiniodrivenbymagmaticsegregationandvolcanism
AT hewittij compositionallayeringiniodrivenbymagmaticsegregationandvolcanism
AT mayda compositionallayeringiniodrivenbymagmaticsegregationandvolcanism
AT keszthelyilp compositionallayeringiniodrivenbymagmaticsegregationandvolcanism