Dia 2009

Trinidad mud volcanoes: where do the expelled fluids come from?

^†A. N. Dia^{, ,}¹, M. Castrec-Rouelle¹, J. Boulègue¹ and P. Comeau²

¹ Laboratoire de Géochimie et Métallogénie, Université Pierre et Marie Curie, Paris, France

² National Herbarium of Trinidad and Tobago, University of West Indies, St. Augustine, Trinidad and Tobago

Available online 9 July 1999.

Abstract

In order to establish the origin of fluids expelled from mud volcanoes in Trinidad, we analyzed their major-element, trace-element, and isotopic (H, O, Sr) compositions.

The mineralogical, chemical, and Sr isotope compositions of associated expelled muds were also determined.

On the basis of their chemical and Sr isotope compositions, the fluids were divided into two groups—those southwest and northeast of a major right lateral wrench fault (the Los Bajos fault) that both controls the chemical quality of the fluids and acts as a drain.

Strontium isotopes were derived via mixing between a radiogenic source (0.71135) and a nonradiogenic source (≤0.70671) for both southwest and northeast groups.

However, the nonradiogenic source possibly feeding the northeast group showed a lower Sr concentration than that of the southwest group.

H and O isotope data show that the fluids became enriched in δ¹⁸O through interaction with wall rocks.

The fluids were originally oceanic, but their properties were subsequently modified by diagenesis as evidenced by chemical data, and mixing between fluids issued from two deep-seated reservoirs and surface aquifer end-members.

The gas phase expelled with the mud and the fluid through the mud volcanoes is composed mainly of methane with minor carbon dioxide.

The amount of expelled gas seems the same in samples from both sides of the Los Bajos fault.

The almost unique methane content of the gas phase and the large positive δ18O shifts of the reservoir end-member, as well as B, Li, and Ba contents, reveal that the fluids from the deep-seated reservoirs inherited their chemical compositions at high-temperature fluid–rock interactions.

Estimates of equilibrium temperatures of the two deep-seated reservoirs suggest that, to acquire the estimated higher temperature (150°C), the mud volcanoes must have been fed partly by a reservoir located at a depth of more than 3 km.

This depth corresponds to previous geologic information, which located the deep-seated reservoir in Miocene sediments at such a comparable depth.

The mixing of the original fluids with a less deep-seated reservoir and meteoric waters on the ascending path suggests the presence of a recharge mechanism and contributes to the dynamics of the expulsion itself.

Article Outline

1. Introduction

2. Geologic setting and sample location

3. Sampling and analytical procedure

3.1. Sampling

3.2. Analytical procedure

4. Data

4.1. Fluid composition

4.1.1. Major- and trace-element contents

4.1.2. Origin of dissolved species—reactions with aluminosilicates

4.1.3. O and H isotopes

4.1.4. Sr isotopes