The November 2002 eruption of Piton de la Fournaise, Reunion: tracking the pre-eruptive thermal evolution of magma using melt inclusions | INSTITUT DE PHYSIQUE DU GLOBE DE PARIS

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  The November 2002 eruption of Piton de la Fournaise, Reunion: tracking the pre-eruptive thermal evolution of magma using melt inclusions

Type de publication:

Journal Article

Source:

Bulletin of Volcanology, Volume 71, Ticket 9, p.1077-1089 (2009)

ISBN:

0258-8900

Numéro d'accès:

ISI:000271025300007

URL:

http://www.springerlink.com/content/56222k15146r7222/?MUD=MP

Mots-clés:

UMR 7154 ; Volcanologie ; N° Contribution : 2463

Résumé:

The November 2002 eruption of Piton de la Fournaise in the Indian Ocean was typical of the activity of the volcano from 1999 to 2006 in terms of duration and volume of magma ejected. The first magma erupted was a basaltic liquid with a small proportion of olivine phenocrysts (Fo(81)) that contain small numbers of melt inclusions. In subsequent flows, olivine crystals were more abundant and richer in Mg (Fo(83-84)). These crystals contain numerous melt and fluid inclusions, healed fractures, and dislocation features such as kink bands. The major element composition of melt inclusions in this later olivine (Fo(83-84)) is out of equilibrium with that of its host as a result of extensive post-entrapment crystallization and Fe2+ loss by diffusion during cooling. Melt inclusions in Fo(81) olivine are also chemically out of equilibrium with their hosts but to a lesser degree. Using olivine-melt geothermometry, we determined that melt inclusions in Fo(81) olivine were trapped at lower temperature (1,182 +/- 1A degrees C) than inclusions in Fo(83-84) olivine (1,199-1,227A degrees C). This methodology was also used to estimate eruption temperatures. The November 2002 melt inclusion compositions suggest that they were at temperatures between 1,070A degrees C and 1,133A degrees C immediately before eruption and quenching. This relatively wide temperature range may reflect the fact that most of the melt inclusions were from olivine in lava samples and therefore likely underwent minor but variable amounts of post-eruptive crystallization and Fe2+ loss by diffusion due to their relatively slow cooling on the surface. In contrast, melt inclusions in tephra samples from past major eruptions yielded a narrower range of higher eruption temperatures (1,163-1,181A degrees C). The melt inclusion data presented here and in earlier publications are consistent with a model of magma recharge from depth during major eruptions, followed by storage, cooling, and crystallization at shallow levels prior to expulsion during events similar in magnitude to the relatively small November 2002 eruption.

Notes:

Vigouroux, Nathalie Williams-Jones, A. E. Wallace, Paul Staudacher, Thomas