Evolution of oceanic gabbros : in-situ and ancient examples
Evolution of oceanic gabbros : in-situ and ancient examples
Date
2004-06
Authors
Kvassnes, Astri Jæger Sweetman
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As Published
Date Created
Location
Atlantis Bank, Southwest Indian Ridge
DOI
10.1575/1912/1860
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Keywords
Mid-ocean ridges
Submarine geology
James Clark Ross (Ship) Cruise JR31
Kairei (Ship) Cruise MODE 98
Yokosuka (Ship) Cruise ABCDE
Submarine geology
James Clark Ross (Ship) Cruise JR31
Kairei (Ship) Cruise MODE 98
Yokosuka (Ship) Cruise ABCDE
Abstract
This study is a geochemical investigation into the accretion of lower oceanic crust
and processes of shallow melt-rock reaction at mid-ocean ridges. Major-, trace-elements,
and isotopes from whole-rocks and minerals from the Lyngen Gabbro, a 480-My old
dismembered ophiolite from the Scandinavian Caledonides, indicate that this igneous
complex was produced from hydrous supra-subduction zone magmas, a remnant of an
incipient ocean-arc. Such ophiolites are better models for the structural evolution than
the geochemical evolution of the lower oceanic crust at mid-ocean ridges.
Minerals in gabbros from Atlantis Bank, Southwest Indian Ridge, a modern, insitu
example of lower ocean-crust, were analyzed for major and trace-elements. The
MELTS algorithm indicates that these gabbros formed by near-fractional crystallzation
at mid-crustal pressures. The gabbroic crust is more evolved than the lavas and
represents melts fractionated 50-95% relative to a mantle-derived melt-composition,
supported by trace-element models. This argues against the often-cited gabbro-glacier
accretion model, where mantle-derived melts are transported to a shallow melt-lens and
fractionates there before eruption. There remain > 770-m of additional primitive
cumulates below 1500-m deep Hole 735B or within the underlying mantle. Thus, the
seismic Moho, beneath Hole 735B, could be the crust-mantle boundary, rather than an
alteration front as suggested elsewhere.
The Atlantis Bank gabbros have augites that are more primitive than plagioclases
and olivines with which they coexist. Melt-rock interaction, where ascending melts
dissolve the pre-existing gabbroic rocks and create hybrid magma may have caused this.
Dissolution-experiments for plagioclase-olivine and plagioclase-augite mineral pairs
were performed at 1180°-1330°C and 20-min - 24hrs. Dissolution occurs rapidly and out
of equilibrium, with the dissolution rates dependent on the ΔT above the solidus. Rocks
with small grain-boundary areas (coarse grained or nearly mono-mineralic) heat
internally when enclosed in hot magma, causing xenoliths or wall-rock to melt and
disaggregate. The dissolution-derived magma crystallizes minerals more refractory-looking
than the melts that precipitated the original gabbroic rocks. Assimilation of
gabbroic rocks increases the Na content and decreases the Fe content of the melt that
digests it, thus basaltic glasses formed after this hybridization will falsely reflect a lower
degree and pressure of mantle melting.
Description
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and Woods Hole Oceanographic Institution June 2004
Embargo Date
Citation
Kvassnes, A. J. S. (2004). Evolution of oceanic gabbros : in-situ and ancient examples [Doctoral thesis, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution]. Woods Hole Open Access Server. https://doi.org/10.1575/1912/1860