Abstract
Fluids in rocks can be traced to great depths, and are found in crustal rocks
as well as in mantle rocks. Information about the deep fluid which is obtained
from fluid inclusions must be handled with care, for the way up after
entrapment in a crystal is long and full of interferences at
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different pressures
and temperatures. The fluid system may be a very complex mixture (H 20,
CO2 , CH4 , N2, CO, NH3, and H2 ) with distinct physical and chemical
proporties.
Chapter 1 indicates that many types of fluids have been recognized in
rocks, and that each type may be related to a distinct grade of
metamorphism (eg. Sorby 1858). For example, the type of fluid recognized in
inclusions from very deep rocks, like granulites and upper mantle rocks is
pure CO2 , Many interpretations of fluid inclusions are based on the
assumption that fluid inclusions do not change in density and composition
after entrapment. In recent years it was recognized that fluid densities may
change during the long way up, and some voices were heard argueing
compositional changes. In this study (Chapter 2 and Chapter 3) it is
experimentally proven that CO2-H2 0 fluid inclusions, which are synthesized in
Brazilian Quartz at 835 K and 200 MPa, leak preferentially H20 during reequilibration
at different conditions. The inclusions are submitted to an
internal overpressure and underpressure. The remaining inclusions become
relatively enriched in CO2, and the H20 must have diffused through the
crystal, for there are no traces of cracks. Several underpressurized inclusions
have "implosion halos" after re-eQuilibration, which consist of many small
secondary inclusions.
Transmission electron microscopy (TEM) observations of the reequilibrated
Brazilian Quartz and of Quartz lenses from Naxos, Greece,
(Chapter 4) indicate that dislocations adjacent to fluid inclusions account for
the non-decrepitative preferential H20 leakage. Ductile strain of the Quartz
neighbouring inclusions, which are overpressurized and underpressurized, is expressed in the localized occurrence of many dislocations. Selective
diffusion of H2 0 along dislocations, which are assumed to be inaccessible for
CO2 , results in the observed preferential H20 leakage. Additionally, a
solubility gradient of quartz in water between an underpressurized fluid
inclusion and a dislocation cause the growth of small secondary bubbles at
dislocations to optically visible ftimplosion halos" at the expense of the fluid
inclusion.
The fluid which should occur at great depths can be indirectly
obtained through thermodynamical calculations. The theoretical background
of these calculations is described in Chapter 5. The well documented
metamorphism from Rogaland (SW Norway) provides enough information to
proceed these fluid calculations (Chapter 6). The calculated gaseous fluid
inclusions are similar to the observed natural fluid inclusions. However, the
calculated aqeous fluids are not recognized or registered by natural fluid
inclusions. The absence of H2 0 in low density metastable CO2 -CH4 -rich
inclusions with graphite, and the occurrence of CH4-N2-rich inclusions are
both proposed to result from preferential H2 0 leakage.
The occurrence of CO2 rich inclusions in granulites and mantle rocks
may partly be caused by the fact that before exposure, these deep rocks
have usually suffered more intensive recrystallization during uplift than
shallow rocks. In future studies on fluid inclusions the effect of deformation
on aqueous inclusions can not be ignored
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