Definition of The World’s Oldest Ophiolite
Ophiolites are a distinctive association of allochthonous rocks
interpreted to form at oceanic spreading centers in back arc
basins, forearcs, arcs, and in major oceans. A complete ophiolite
grades downward from pelagic sediments into a mafic volcanic
complex comprised mostly of pillow basalts, underlain by a sheeted
dike complex. These are underlain by gabbros exhibiting cumulus
textures, then tectonized peridotite, resting above a thrust fault that
marks the contact with underlying rock sequences. The term ophiolite
refers to this distinctive rock association, although many
workers interpret the term to mean allochthonous oceanic lithosphere
rocks formed exclusively at mid-ocean ridges.
Prior to 2001, no complete Phanerozoic-like ophiolite sequences
had been recognized in Archean greenstone belts, leading some
workers to the conclusion that no Archean ophiolites or oceanic
crustal fragments are preserved. These ideas were recently challenged
by the discovery of a complete 2.5 billion-year-old ophiolite
sequence in the North China craton. This remarkable rock sequence
includes chert and pillow lava, a sheeted dike complex, gabbro and
layered gabbro, cumulate ultramafic rocks, and a suite of strongly
deformed mantle harzburgite tectonites. The mantle rocks include a
distinctive type of intrusion with metallic chrome nodules called a
podiform chromite deposit, known to form only in oceanic crust.
Well-preserved black smoker chimney structures in metallic
sulfide deposits have also been discovered in some sections of the
Dongwanzi ophiolite belt, and these ancient seafloor hydrothermal
vents are among the oldest known. Deep-sea hydrothermal vents
host the most primitive thermophyllic, chemosynthetic, sulfatereducing
organisms known, believed to be the closest relatives of
the oldest life on Earth, with similar vents having possibly provided
nutrients and protected environments for the first organisms. These
vents are associated with some unusual microscale textures that
may be remnants of early life forms, most likely bacteria. These
ancient fossils provide tantalizing suggestions that early life may
have developed and remained sheltered in deep-sea hydrothermal
vents until surface conditions became favorable for organisms to
inhabit the land.
Archean oceanic crust was possibly thicker than Proterozoic
and Phanerozoic counterparts, resulting in accretion predominantly
of the upper basaltic section of oceanic crust. The crustal thickness
of Archean oceanic crust may in fact have resembled modern
oceanic plateaux. If this were the case, complete Phanerozoic-like
ophiolite sequences would have been very unlikely to be accreted
or obducted during Archean orogenies. In contrast, only the upper,
pillow-lava–dominated sections would likely be accreted. Remarkably,
Archean greenstone belts contain an abundance of tectonic
slivers of pillow lavas, gabbros, and associated deep-water sedimentary
rocks. The observation that Archean greenstone belts
have such an abundance of accreted ophiolitic fragments compared
with Phanerozoic orogens suggests that thick, relatively
buoyant, young Archean oceanic lithosphere may have had a rheological
structure favoring delamination of the uppermost parts during
subduction and collisional events.
sists of an ultramafic rock known as harzburgite, consisting
of olivine + orthopyroxene (± chromite), often forming
strongly deformed or transposed compositional layering,
forming a distinctive rock known as harzburgite tectonite. In
some ophiolites, harzburgite overlies lherzolite. The harzburgite
is generally interpreted to be the depleted mantle from
which overlying mafic rocks were derived, and the deformation
is related to the overlying lithospheric sequence flowing
away from the ridge along a shear zone within the harzburgite.
The harzburgite sequence may be six miles (10 km) or
more thick in some ophiolites, such as the Semail ophiolite in
Oman and the Bay of Island ophiolite in Newfoundland.
Resting above the harzburgite is a group of rocks that
were crystallized from a magma derived by partial melting of
the harzburgite. The lowest unit of these crustal rocks includes
crystal cumulates of pyroxene and olivine, forming distinctive
layers of pyroxenite, dunite, and other olivine + clinopyroxene
+ orthopyroxene peridotites including wehrlite, websterite, and
pods of chromite + olivine. The boundary between these rocks
(derived by partial melting and crystal fractionation) and those
below from which melts were extracted is one of the most fundamental
boundaries in the crust, known as the Moho, or base
of the crust. It is named after Andrija Mohorovicic, a Yugoslavian
geophysicist who noted a fundamental seismic boundary
beneath the continental crust. In this case, the Moho is a chemical
boundary, without a sharp seismic discontinuity. A seismic
discontinuity occurs about half a kilometer higher than the
chemical Moho in ophiolites.
The layered ultramafic cumulates grade upward into a
transition zone of interlayered pyroxenite and plagioclase-rich
cumulates, then into an approximately half-mile (1-km) thick
unit of strongly layered gabbro. Individual layers within this
thin unit may include gabbro, pyroxenite, and anorthosite.
The layered gabbro is succeeded upward by one to three miles
(2–5 km) of isotropic gabbro, which is generally structureless
but may have a faint layering. The layers within the isotropic
gabbro in some ophiolites define a curving trajectory, interpreted
to represent crystallization along the walls of a paleomagma
chamber. The upper part of the gabbro may contain
many xenoliths of diabase, pods of trondhjemite (plagioclase
plus quartz), and may be cut by diabase dikes.
The next highest unit in a complete, Penrose-style ophiolite
is typically a sheeted dike complex, consisting of a
0.3–1.25-mile (0.5–2-km) thick complex of diabasic, gabbroic,
to silicic dikes that show mutually intrusive relationships with
the underlying gabbro. In ideal cases, each diabase dike
intrudes into the center of the previously intruded dike, forming
a sequence of dikes that have chilled margins developed
only on one side. These dikes are said to exhibit one-way chilling.
In most real ophiolites, examples of one-way chilling may
be found, but statistically the one-way chilling may only show
directional preference in 50–60 percent of cases.
The sheeted dikes represent magma conduits that fed
basaltic flows at the surface. These flows are typically pillowed,
with lobes and tubes of basalt forming bulbous shapes
distinctive of underwater basaltic volcanism. The pillow
basalt section is typically 0.3–0.6-mile (0.5–1-km) thick.
Interstices between the pillows may be filled with chert, and
sulfide minerals are common.
Many ophiolites are overlain by deep-sea sediments,
including chert, red clay, in some cases carbonates, or sulfide
layers. Many variations are possible, depending on tectonic
setting (e.g., conglomerates may form in some settings) and
age (e.g., siliceous biogenic oozes and limestones would not
form in Archean ophiolites, before the life-forms that contribute
their bodies developed).
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