Skip Navigation


Journal of Petrology Advance Access originally published online on December 13, 2006
Journal of Petrology 2007 48(3):459-493; doi:10.1093/petrology/egl068
This Article
Right arrow Full Text Freely available
Right arrow FREE Full Text (PDF) Freely available
Right arrow Supplementary data
Right arrow All Versions of this Article:
48/3/459    most recent
egl068v2
egl068v1
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Add to My Personal Archive
Right arrow Download to citation manager
Right arrow Search for citing articles in:
ISI Web of Science (5)
Right arrowRequest Permissions
Google Scholar
Right arrow Articles by Fowler, S. J.
Right arrow Articles by De Vivo, B.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

© The Author 2006. Published by Oxford University Press. All rights reserved. For Permissions, please e-mail: journals.permissions@oxfordjournals.org

Phase Equilibria Constraints on the Chemical and Physical Evolution of the Campanian Ignimbrite

Sarah J. Fowler1,*, Frank J. Spera1, Wendy A. Bohrson2, Harvey E. Belkin3 and Benedetto De Vivo4

1Department of Earth Science and Institute for Crustal Studies, University of California, Santa Barbara, Santa Barbara, CA 93106, USA
2Department of Geological Sciences, Central Washington University, Ellensburg, WA 98926, USA
3956 National Center, US Geological Survey, Reston, VA 20192, USA
4Dipartimento di Scienze Della Terra, Università Di Napoli Federico II, 80134 Napoli, Italy

RECEIVED FEBRUARY 22, 2006; ACCEPTED OCTOBER 27, 2006


   Abstract

The Campanian Ignimbrite is a > 200 km3 trachyte–phonolite pyroclastic deposit that erupted at 39·3 ± 0·1 ka within the Campi Flegrei west of Naples, Italy. Here we test the hypothesis that Campanian Ignimbrite magma was derived by isobaric crystal fractionation of a parental basaltic trachyandesitic melt that reacted and came into local equilibrium with small amounts (5–10 wt%) of crustal rock (skarns and foid-syenites) during crystallization. Comparison of observed crystal and magma compositions with results of phase equilibria assimilation–fractionation simulations (MELTS) is generally very good. Oxygen fugacity was approximately buffered along QFM + 1 (where QFM is the quartz–fayalite–magnetite buffer) during isobaric fractionation at 0·15 GPa ({approx} 6 km depth). The parental melt, reconstructed from melt inclusion and host clinopyroxene compositions, is found to be basaltic trachyandesite liquid (51·1 wt% SiO2, 9·3 wt% MgO, 3 wt% H2O). A significant feature of phase equilibria simulations is the existence of a pseudo-invariant temperature, ~883 °C, at which the fraction of melt remaining in the system decreases abruptly from ~ 0·5 to < 0·1. Crystallization at the pseudo-invariant point leads to abrupt changes in the composition, properties (density, dissolved water content), and physical state (viscosity, volume fraction fluid) of melt and magma. A dramatic decrease in melt viscosity (from 1700 Pa s to ~ 200 Pa s), coupled with a change in the volume fraction of water in magma (from ~ 0·1 to 0·8) and a dramatic decrease in melt and magma density acted as a destabilizing eruption trigger. Thermal models suggest a timescale of ~ 200 kyr from the beginning of fractionation until eruption, leading to an apparent rate of evolved magma generation of about 10–3 km3/year. In situ crystallization and crystal settling in density-stratified regions, as well as in convectively mixed, less evolved subjacent magma, operate rapidly enough to match this apparent volumetric rate of evolved magma production.

KEY WORDS: assimilation; Campanian Ignimbrite; fractional crystallization; magma dynamics; phase equilibria


*Corresponding author.Telphone: (805) 893-4880. E-mail: fowler{at}umail.ucsb.edu


Add to CiteULike CiteULike   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us    What's this?


This article has been cited by other articles:


Home page
J PetrologyHome page
T. Kuritani, T. Yokoyama, and E. Nakamura
Rates of Thermal and Chemical Evolution of Magmas in a Cooling Magma Chamber: a Chronological and Theoretical Study on Basaltic and Andesitic Lavas from Rishiri Volcano, Japan
J. Petrology, July 1, 2007; 48(7): 1295 - 1319.
[Abstract] [Full Text] [PDF]



Disclaimer:
Please note that abstracts for content published before 1996 were created through digital scanning and may therefore not exactly replicate the text of the original print issues. All efforts have been made to ensure accuracy, but the Publisher will not be held responsible for any remaining inaccuracies. If you require any further clarification, please contact our Customer Services Department.