Mantle plume-midocean ridge interaction : geophysical observations and mantle dynamics
Mantle plume-midocean ridge interaction : geophysical observations and mantle dynamics
Date
1996-09
Authors
Ito, Garrett T.
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Location
Galapagos Spreading Center
DOI
10.1575/1912/5708
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Keywords
Mid-ocean ridges
Plumes
Structural geology
Plate tectonics
Submarine geology
Mantle
Plumes
Structural geology
Plate tectonics
Submarine geology
Mantle
Abstract
We analyze bathymetric and gravity anomalies at five plume-ridge systems to constrain
crustal and mantle density structure at these prominent oceanic features. Numerical models
are then used to explore the physical mechanisms controlling plume-ridge interaction and to
place theoretical constraints on the temperature anomalies, dimensions, and fluxes of the
Icelandic and Galapagos plumes.
In Chapter 1 we analyze bathymetric and gravity anomalies along the hotspot-influenced
Galapagos Spreading Center. We find that the Galapagos plume generates
along-axis bathymetric and mantle-Bouguer gravity anomalies (MBA) that extend >500 km
east and west of the Galapagos Islands. The along-axis MBA becomes increasingly
negative towards the plume center, reaching a minimum of ~-90 mGal near 91°W, and axial
topography shallows by ~1.1 km toward the plume. These variations in MBA and
bathymetry are attributed to the combined effects of crustal thickening and anomalously low
mantle densities, both of which are due to a mantle temperature anomaly imposed beneath
the ridge by the Galapagos plume. Passive mantle flow models predict a temperature
anomaly of 50±25°C is sufficient to produce the 2-4 km excess crust required to explain the
along-axis anomalies. 70-75% of the along-axis bathymetric and MBA variations are
estimated to arise from the crust with the remaining 25-30% generated by the anomalously
hot, thus low-density mantle. Along Cocos-plate isochrons, bathymetric and MBA
variations increase with increasing isochron age, suggesting the subaxial mantle
temperature anomaly was greater in the past when the plume was closer, to the ridge axis.
In addition to the Galapagos plume-ridge system, in Chapter 2 we examine alongisochron
bathymetric and MBA variations at four other plume-ridge systems associated
with the Iceland, Azores, Easter and Tristan hotspots. We show that residual bathymetry
(up to 4.7 km) and mantle-Bouguer gravity anomalies (up to -340 mGal) are greatest at on-axis
plumes and decreases with increasing ridge-hotspot separation distance, until
becoming insignificant at a plume-ridge separation of ~500 km. Along-isochron widths of
bathymetric anomalies (up to 2700 km) decrease with increasing paleo-spreading rate,
reflecting the extent to which plume material flows along-axis before being swept away by
the spreading lithosphere. Scaling arguments suggest an average ridgeward plume flux of
-2.2x106 km/my. Assuming that the amplitudes of the MBA and bathymetric anomalies
reflect crustal thickness and mantle density variations, passive mantle flow models predict maximum subaxial mantle temperature anomalies to be 150-225°C for ridge-center plumes,
which decrease as the ridges migrate away from the plumes.
The dynamics of mantle flow and melting at ridge-centered plumes are investigated in
Chapters 3 using three-dimensional, variable-viscosity, numerical models. Three
buoyancy sources are examined: temperature, melt depletion, and melt retention. The
width W to which a plume spreads along a ridge axis depends on plume volume flux Q,
full spreading rate U, buoyancy number B = (QΔρg)/(48η0U2), and ambient/plume
viscosity contrast ϒ according to W=2.37(Q/U)l/2(Bϒ)0.04. Thermal buoyancy is first
order in controlling along-axis plume spreading while latent heat loss due to melting, and
depletion and retention buoyancy forces contribute second order effects. Two end-member
models of the Iceland-Mid-Atlantic Ridge (MAR) system are examined. The first endmember
model has a broad plume source of radius 300 km, temperature anomaly of 75°C,
and volume flux of 1.2xl07 km3/my. The second model has a narrower plume source of
radius 60 km, temperature anomaly of l70°C, and flux of 2.1 x106 km3/my. The first
model predicts successfully the observed crustal thickness, topographic, and MBA
variations along the MAR, but the second model requires substantial along-axis melt
transport in order to explain the observed along-axis variations in crustal thickness,
bathymetry, and gravity. We favor this second model because it predicts a mantle P-wave
velocity reduction in the plume of ~2% as consistent with recent seismic observations
beneath Iceland.
Finally in Chapter 4 we use three-dimensional numerical models to investigate the
interaction of plumes and migrating midocean ridges. Scaling laws of axial plume
spreading width Ware derived first for stationary ridges and off-axis plumes, which yield
results consistent with those obtained from independent studies of Ribe [1996]. Wand the
maximum plume-ridge interaction distance Xmax again scale with (Q/U)l/2 as in the case of
ridge-centered plumes and increase with ϒ and buoyancy number. In the case of a
migrating ridge, Xmax is reduced when a ridge migrates toward the plume due to excess
drag of the faster-moving leading plate, and enhanced when a ridge migrates away from the
plume due to reduced drag of the slower-moving trailing plate. Thermal erosion of the
lithospheric boundary layer by the previously ridge-centered plume further enhances Wand
Xmax but to a degree that is secondary to the differential migration rates of the two plates.
Model predictions are compared with observed along-isochron bathymetric and MBA
variations at the Galapagos plume-ridge system. The anomaly amplitudes and widths, as
well as the increase in anomaly amplitude with age are predicted with a plume source
temperature anomaly of 80-120°C, radius of 80-100 km, and volume flux of 4.5x106
km3/m.y. Our numerical models also predict crustal production rates of the Galapagos
Islands consistent with those estimated independently using the observed island
topography. Predictions of the geochemical signature of the plume along the present-day
ridge suggest that mixing between the plume and ambient mantle sources is unlikely to
occur in the asthenosphere or shallow crust, but most likely deeper in the mantle possibly
by entrainment of ambient mantle as the plume ascends through the depleted portion of the
mantle from its deep source reservoir.
Description
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1996
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Citation
Ito, G. T. (1996). Mantle plume-midocean ridge interaction : geophysical observations and mantle dynamics [Doctoral thesis, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution]. Woods Hole Open Access Server. https://doi.org/10.1575/1912/5708