Limestone assimilation and skarn formation are important processes in magmatic systems emplaced within carbonate-rich crust and can affect the composition of the magma and that of associated volcanic gas. In this studywe focus on marble and calc-silicate (skarn) xenoliths fromcontact reactions between magma and carbonate wall-rock of the Vesuvius volcanic system. We present new elemental and C-O isotope data for marble and skarn xenoliths as well as for igneous rocks collected from the AD 79 (Pompeii) and AD 472 (Pollena) eruptions. The igneous samples have consistently high δ18Ovalues (9.3to10.8‰), but lowH2O contents (≤1.5%), indicating that magma–crust interaction prior to eruption took place. The marble xenoliths, in turn, record initial decarbonation reactions and fluid-mass exchange in their textures and δ13C and δ18O ranges, while the skarn xenoliths reflect prolonged magma–carbonate interaction and intense contact metamorphism. Skarn-xenoliths record Ca and Mg release from the original carbonate and uptake of Al and Si and span the full δ18O data range from unmetamorphosed carbonate (N18‰) to values typical for Vesuvius magmatic rocks (~7.5‰), which implies that skarn xenoliths comprise carbonate and magmatic components. Textural and chemical evidence suggest that direct carbonate dissolution into the host magmas occurred aswell as post-metamorphic skarn recycling, resulting in progressive Ca andMgliberation fromthe skarn xenoliths into themagma.Magma–carbonate interaction is an additional source of CO2 during carbonate break-down and assimilation and we calculate the amount of extra volatile components likely liberated by contact metamorphic reactions before and during the investigated eruptions. We find that the extra CO2 added into the volcanic systemcould have outweighed the magmatic CO2 component by ≥ factor seven and thus likely increased the intensity of both the Pompeii and the Pollena eruptive events.
Skarn xenolith record crustal CO2 liberation during Pompeii and Pollena eruptions, Vesuvius volcanic system, central Italy / Jolis, E. M; Troll, V. R.; Harris, C.; Freda, C.; Gaeta, Mario; Orsi, G.; Siebe, C.. - In: CHEMICAL GEOLOGY. - ISSN 0009-2541. - 415:(2015), pp. 17-36. [10.1016/j.chemgeo.2015.09.003]
Skarn xenolith record crustal CO2 liberation during Pompeii and Pollena eruptions, Vesuvius volcanic system, central Italy
GAETA, Mario;
2015
Abstract
Limestone assimilation and skarn formation are important processes in magmatic systems emplaced within carbonate-rich crust and can affect the composition of the magma and that of associated volcanic gas. In this studywe focus on marble and calc-silicate (skarn) xenoliths fromcontact reactions between magma and carbonate wall-rock of the Vesuvius volcanic system. We present new elemental and C-O isotope data for marble and skarn xenoliths as well as for igneous rocks collected from the AD 79 (Pompeii) and AD 472 (Pollena) eruptions. The igneous samples have consistently high δ18Ovalues (9.3to10.8‰), but lowH2O contents (≤1.5%), indicating that magma–crust interaction prior to eruption took place. The marble xenoliths, in turn, record initial decarbonation reactions and fluid-mass exchange in their textures and δ13C and δ18O ranges, while the skarn xenoliths reflect prolonged magma–carbonate interaction and intense contact metamorphism. Skarn-xenoliths record Ca and Mg release from the original carbonate and uptake of Al and Si and span the full δ18O data range from unmetamorphosed carbonate (N18‰) to values typical for Vesuvius magmatic rocks (~7.5‰), which implies that skarn xenoliths comprise carbonate and magmatic components. Textural and chemical evidence suggest that direct carbonate dissolution into the host magmas occurred aswell as post-metamorphic skarn recycling, resulting in progressive Ca andMgliberation fromthe skarn xenoliths into themagma.Magma–carbonate interaction is an additional source of CO2 during carbonate break-down and assimilation and we calculate the amount of extra volatile components likely liberated by contact metamorphic reactions before and during the investigated eruptions. We find that the extra CO2 added into the volcanic systemcould have outweighed the magmatic CO2 component by ≥ factor seven and thus likely increased the intensity of both the Pompeii and the Pollena eruptive events.File | Dimensione | Formato | |
---|---|---|---|
Jolis_Skarn_2015.pdf
solo gestori archivio
Tipologia:
Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza:
Tutti i diritti riservati (All rights reserved)
Dimensione
5.3 MB
Formato
Adobe PDF
|
5.3 MB | Adobe PDF | Contatta l'autore |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.