TY - JOUR
T1 - Subduction zone thermal structure and mineralogy and their relationship to seismic wave reflections and conversions at the slab/mantle interface
AU - Helffrich, George R.
AU - Stein, Seth
AU - Wood, Bernard J.
PY - 1989
Y1 - 1989
N2 - Seismological studies of the interface between downgoing
slabs of subducted lithosphere and the overriding mantle provide constraints
against which models of mantle and slab temperature and bulk composition can be
tested. These studies, employing waves reflected and converted at the
slab/mantle interface, suggest that a velocity contrast of 5–10% occurs over a
distance of 10–20 km to depths of at least 350 km. We have investigated whether
such sharp contrasts can result from thermal structure, compositional
differences, phase changes, or other effects such as preferred mineral
orientation. Using a mantle and slab temperature model, a petrologic model of
mantle and slab mineralogy, and a data base of elastic properties of mantle and
slab phases, theoretical seismic velocities were calculated and compared with
the observed velocity contrast and boundary thickness constraints. At 9.6 GPa
and 1000°C (conditions modeled at the slab/mantle interface at ∼280-km
depth), cooler temperatures in the slab interior produce, at constant
composition, only approximately a 1.75% Vp increase
into the slab in any of the peridotitic and eclogitic mineralogies
investigated. Variation in Vp among the different bulk
compositions is only approximately 0.5%. These contrasts are substantially
lower than those obtained from the seismological studies and indicate that
temperature and bulk compositional differences between mantle and slab are
inadequate to cause the observed velocity contrasts. We propose that phase
transformations in mantle and slab mineralogies, notably elevation of the
olivine-spinel phase change normally occurring at 400-km depth, are important
factors in these sharp contrasts. Other contributing effects may include
preferential mineral orientation near the slab surface and, at shallower
depths, the presence of partial melt or hydrous fluid evolved from dehydration
reactions along the interface.
AB - Seismological studies of the interface between downgoing
slabs of subducted lithosphere and the overriding mantle provide constraints
against which models of mantle and slab temperature and bulk composition can be
tested. These studies, employing waves reflected and converted at the
slab/mantle interface, suggest that a velocity contrast of 5–10% occurs over a
distance of 10–20 km to depths of at least 350 km. We have investigated whether
such sharp contrasts can result from thermal structure, compositional
differences, phase changes, or other effects such as preferred mineral
orientation. Using a mantle and slab temperature model, a petrologic model of
mantle and slab mineralogy, and a data base of elastic properties of mantle and
slab phases, theoretical seismic velocities were calculated and compared with
the observed velocity contrast and boundary thickness constraints. At 9.6 GPa
and 1000°C (conditions modeled at the slab/mantle interface at ∼280-km
depth), cooler temperatures in the slab interior produce, at constant
composition, only approximately a 1.75% Vp increase
into the slab in any of the peridotitic and eclogitic mineralogies
investigated. Variation in Vp among the different bulk
compositions is only approximately 0.5%. These contrasts are substantially
lower than those obtained from the seismological studies and indicate that
temperature and bulk compositional differences between mantle and slab are
inadequate to cause the observed velocity contrasts. We propose that phase
transformations in mantle and slab mineralogies, notably elevation of the
olivine-spinel phase change normally occurring at 400-km depth, are important
factors in these sharp contrasts. Other contributing effects may include
preferential mineral orientation near the slab surface and, at shallower
depths, the presence of partial melt or hydrous fluid evolved from dehydration
reactions along the interface.
UR - http://www.scopus.com/inward/record.url?scp=0024569235&partnerID=8YFLogxK
U2 - 10.1029/JB094iB01p00753
DO - 10.1029/JB094iB01p00753
M3 - Article
AN - SCOPUS:0024569235
SN - 0148-0227
VL - 94
SP - 753
EP - 763
JO - Journal of Geophysical Research
JF - Journal of Geophysical Research
IS - B1
ER -