Type of Document Dissertation Author Esposito, Rosario Author's Email Address email@example.com URN etd-07132012-102229 Title Studies of volatile evolution in magmatic systems using melt inclusions Degree PhD Department Geosciences Advisory Committee
Advisor Name Title Bodnar, Robert J. Committee Chair De Vivo, Benedetto Committee Member Lima, Annamaria Committee Member Rimstidt, james Donald Committee Member Tracy, Robert J. Committee Member Keywords
- Melt Inclusion Assemblage
- Post Entrapment Crystallization
- Melt Inclusion
- Volatile Evolution
- Microscope Heating Stage
- Magma Degassing
Date of Defense 2012-07-02 Availability unrestricted AbstractUnderstanding volatile evolution associated with active volcanic magmatic systems is of paramount importance because volatiles control and determine the magnitude of an eruption owing to the large change in molar volume that volatile species show depending on their physical state (volatiles dissolved in silicate melts vs. volatiles exsolved as vapor). For active volcanic systems studying the volatile evolution can help to assess the potential hazard associated to a certain locality. Also, volatile evolution in magmatic system controls the formation of certain ore deposits.
Despite the importance of understanding volatile evolution of magmatic systems, concentrations of volatiles of evolving magmas are not easily available especially for magmas originated in the deep crust. Fortunately, sample of melts can be entrapped as melt inclusion (MI) into growing igneous minerals in crystalizing magma chamber. After the entrapment, the crystal works as an insulating capsule from the external magmatic environment.
Researchers have started to use MI because they provide some advantages in respect to the classical whole rock approach to petrological studies. One of the most important advantages is that MI often represent sample of a deep and non-degassed melt (glass) available at Earth’s surface. In fact, with the exception of deep ocean basalts, igneous whole rocks found at the Earth’s surface are degassed magmas.
This dissertation is a compilation of four publications produced during six years of research and is addressed to give a contribution in understanding the volatile evolution in magmatic systems and also to improve the present understanding of information that can be obtained using the melt inclusions technique.
In the first chapter, I present an alternative interpretation of H2O-CO2 trends obtained from MI. In this study, we demonstrate that these trends can be due to post entrapment crystallization on the wall of the MI and not to magma ascent. This alternative view is more realistic especially for cases where in the same phenocrysts MI show strongly different CO2 concentrations.
In the second chapter, I present a study to test for the MI reliability in recording volatile concentrations. We used the approach of the melt inclusion assemblage (MIA) that consists of analyzing groups of MI presumably entrapped at the same time and, thus, at same chemical and physical conditions. The results show that most of the MIA studied show consistent volatile concentrations corroborating the reliability of the MI technique. CO2 shows the highest degrees of variability and we have assessed this behavior mostly to C-contamination in the surface of the sample.
The third chapter is a study case (the Solchiaro eruption in Southern Italy) that shows the potential uses of MI to understanding the volatile evolution. I present a model showing the dynamic of the magma based on MI. This study also discusses the origin of anomalous MI and which MI provide the best information.
The final chapter is dedicated to test the applicability of the new Linkam TS1400XY heating stage. I was able to show how this new microthermometric tool is capable of homogenizing MI at high temperature and to quench MI to a homogeneous glass state.
Filename Size Approximate Download Time (Hours:Minutes:Seconds)
28.8 Modem 56K Modem ISDN (64 Kb) ISDN (128 Kb) Higher-speed Access Esposito_R_D_2012.pdf 13.53 Mb 01:02:38 00:32:12 00:28:11 00:14:05 00:01:12
If you have questions or technical problems, please Contact DLA.