Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica

Intraplate volcanoes are associated with extensional tectonics, mantle upwelling and high heat flow. Erupted magmas have an alkaline nature and are rich in volatiles, especially CO2, that are inherited from fluid-rich magmatic sources in the mantle. Localized alkaline centers emit gas fluxes that ex...

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Main Authors: Oppenheimer C, P. Kyle, MORETTI, Roberto
Other Authors: Oppenheimer, C, Moretti, Roberto, P., Kyle
Format: Conference Object
Language:English
Published: European Geosciences Union 2009
Subjects:
Online Access:http://hdl.handle.net/11591/211807
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spelling ftuncampaniairis:oai:iris.unicampania.it:11591/211807 2024-01-14T10:00:32+01:00 Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica Oppenheimer C P. Kyle MORETTI, Roberto Oppenheimer, C Moretti, Roberto P., Kyle 2009 http://hdl.handle.net/11591/211807 eng eng European Geosciences Union place:Vienna ispartofbook:EGU General Assembly 2009 EGU General Assembly 2009 volume:11 firstpage:7456-1 lastpage:7456-1 journal:GEOPHYSICAL RESEARCH ABSTRACTS http://hdl.handle.net/11591/211807 info:eu-repo/semantics/conferenceObject 2009 ftuncampaniairis 2023-12-19T23:17:37Z Intraplate volcanoes are associated with extensional tectonics, mantle upwelling and high heat flow. Erupted magmas have an alkaline nature and are rich in volatiles, especially CO2, that are inherited from fluid-rich magmatic sources in the mantle. Localized alkaline centers emit gas fluxes that exceed what can be sustained by the rates of magma erupted. At Mount Erebus this dichotomy is evidenced by open-path Fourier transform infrared (FTIR) spectroscopy of gases released from the lava lake. Different gas signatures are associated with explosive and nonexplosive gas emissions, representative of volatile contents and redox conditions that identify the overlap between shallow and deep degassing sources. We show that this multiple signature of magma degassing provides a unique probe for magma differentiation and transfer of CO2-rich oxidized fluids from lithospheric roots up to the surface, and show how these processes operate in time and space. Magma deeper than 4 km equilibrates under vapour buffered conditions, whereas shallower magmas allow deep, CO2-rich fluids to accumulate and prior to release either via open-system degassing conditions and reduced oxidation states, or as volatile-enriched, phonolitic blobs that preserve the deep oxidized signature, and ascend as a closed-system to explode at the surface during Strombolian phases. Conference Object Antarc* Antarctica Università degli Studi della Campania "Luigi Vanvitelli": CINECA IRIS V: Lava Lake ENVELOPE(-128.996,-128.996,55.046,55.046) Mount Erebus ENVELOPE(167.167,167.167,-77.533,-77.533)
institution Open Polar
collection Università degli Studi della Campania "Luigi Vanvitelli": CINECA IRIS V:
op_collection_id ftuncampaniairis
language English
description Intraplate volcanoes are associated with extensional tectonics, mantle upwelling and high heat flow. Erupted magmas have an alkaline nature and are rich in volatiles, especially CO2, that are inherited from fluid-rich magmatic sources in the mantle. Localized alkaline centers emit gas fluxes that exceed what can be sustained by the rates of magma erupted. At Mount Erebus this dichotomy is evidenced by open-path Fourier transform infrared (FTIR) spectroscopy of gases released from the lava lake. Different gas signatures are associated with explosive and nonexplosive gas emissions, representative of volatile contents and redox conditions that identify the overlap between shallow and deep degassing sources. We show that this multiple signature of magma degassing provides a unique probe for magma differentiation and transfer of CO2-rich oxidized fluids from lithospheric roots up to the surface, and show how these processes operate in time and space. Magma deeper than 4 km equilibrates under vapour buffered conditions, whereas shallower magmas allow deep, CO2-rich fluids to accumulate and prior to release either via open-system degassing conditions and reduced oxidation states, or as volatile-enriched, phonolitic blobs that preserve the deep oxidized signature, and ascend as a closed-system to explode at the surface during Strombolian phases.
author2 Oppenheimer, C
Moretti, Roberto
P., Kyle
format Conference Object
author Oppenheimer C
P. Kyle
MORETTI, Roberto
spellingShingle Oppenheimer C
P. Kyle
MORETTI, Roberto
Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
author_facet Oppenheimer C
P. Kyle
MORETTI, Roberto
author_sort Oppenheimer C
title Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
title_short Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
title_full Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
title_fullStr Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
title_full_unstemmed Mantle to surface gas triggers of magmatic activity at Erebus volcano, Antarctica
title_sort mantle to surface gas triggers of magmatic activity at erebus volcano, antarctica
publisher European Geosciences Union
publishDate 2009
url http://hdl.handle.net/11591/211807
long_lat ENVELOPE(-128.996,-128.996,55.046,55.046)
ENVELOPE(167.167,167.167,-77.533,-77.533)
geographic Lava Lake
Mount Erebus
geographic_facet Lava Lake
Mount Erebus
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation ispartofbook:EGU General Assembly 2009
EGU General Assembly 2009
volume:11
firstpage:7456-1
lastpage:7456-1
journal:GEOPHYSICAL RESEARCH ABSTRACTS
http://hdl.handle.net/11591/211807
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