Petrological interpretation of deep crustal intrusive bodies beneath oceanic hotspot provinces
Author
dc.contributor.author
Richards, Mark
Author
dc.contributor.author
Contreras Reyes, Eduardo
es_CL
Author
dc.contributor.author
Lithgow Bertelloni, Carolina
es_CL
Author
dc.contributor.author
Ghiorso, Mark
es_CL
Author
dc.contributor.author
Stixrude, Lars
es_CL
Admission date
dc.date.accessioned
2014-03-06T20:15:08Z
Available date
dc.date.available
2014-03-06T20:15:08Z
Publication date
dc.date.issued
2013
Cita de ítem
dc.identifier.citation
Geochem. Geophys. Geosyst., 14, 604–619
en_US
Identifier
dc.identifier.issn
1525-2027
Identifier
dc.identifier.other
doi:10.1029/2012GC004448
Identifier
dc.identifier.uri
https://repositorio.uchile.cl/handle/2250/126428
General note
dc.description
Artículo de publicación ISI
en_US
Abstract
dc.description.abstract
Seismic refraction studies of deep-crustal and upper mantle structure beneath some oceanic hotspot
provinces reveal the presence of ultramafic bodies with P-wave velocities of Vp ~ 7.4–8.0 km/s lying at
or above the Moho, e.g., Hawaii, the Marquesas, and La Reunion. However, at other hotspot provinces such
as the Galapagos, Nazca Ridge, and Louisville the lower crust is intruded by large volumes of gabbroic
(mafic) rocks (Vp ~ 6.8–7.5 km/s). Ultramafic primary melts formed beneath mature oceanic lithosphere at
pressures of ~2–3 GPa (60–90 km depth), and ponded at the Moho due to their relatively high density,
can explain the observed ultramafic deep-crustal bodies. By contrast, plume melts formed at depths of
~15–30 km beneath thin lithosphere crystallize assemblages that are more gabbroic. The velocity and
density gradient is particularly strong in the pressure range 0.6–1.5 GPa due to the replacement of
plagioclase by olivine as melts become more MgO-rich with increasing pressure (and degree) of melting.
This anomalous density gradient suggests a possible filtering effect whereby plume melts equilibrated at
relatively shallow depths beneath very young and thin oceanic lithosphere may be expected to be of nearly
gabbroic (mafic) composition (~6–10% MgO), whereas ultramafic melts (MgO ~ 12–20%) formed beneath
older, thicker oceanic lithosphere must pond and undergo extensive olivine and clinopyroxene fractionation
before evolving residual magmas of basaltic composition sufficiently buoyant to be erupted at the surface. A
survey of well-studied hotspot provinces of highly-varying lithospheric age at the time of emplacement
shows that deep-crustal and upper mantle seismic refraction data are consistent with this hypothesis. These
results highlight the importance of large-volume intrusive processes in the evolution of hotspot magmas,
with intrusive volumes being significantly larger than those of the erupted lavas in most cases. Pyrolite
melting can account, to first order, for the total crustal column of magmatic products, whereas alternative
models such as selective melting of pyroxenite blobs probably cannot.