259 research outputs found
Implications of subduction rehydration for earth's deep water cycle
The âstandard modelâ for the genesis of the oceans is that they are exhalations from Earthâs deep interior continually rinsed through surface rocks by the global hydrologic cycle. No general consensus exists, however, on the water distribution within the deeper mantle of the Earth. Recently Dixon et al. [2002] estimated water concentrations for some of the major mantle components and concluded that the most primitive (FOZO) are significantly wetter than the recycling associated EM or HIMU mantle components and the even drier depleted mantle source that melts to form MORB. These findings are in striking agreement with the results of numerical modeling of the global water cycle that are presented here. We find that the Dixon et al. [2002] results are consistent with a global water cycle model in which the oceans have formed by efficient outgassing of the mantle. Present-day depleted mantle will contain a small volume fraction of more primitive wet mantle in addition to drier recycling related enriched components. This scenario is consis-tent with the observation that hotspots with a FOZO-component in their source will make wetter basalts than hotspots whose mantle sources contain a larger fraction of EM and HIMU components
On subducting slab entrainment of buoyant asthenosphere
Laboratory and numerical experiments and boundary layer analysis of the entrainment of buoyant asthenosphere by subducting oceanic lithosphere implies that slab entrainment is likely to be relatively inefficient at removing a buoyant and lower viscosity asthenosphere layer. Asthenosphere would instead be mostly removed by accretion into and eventual subduction of the overlying oceanic lithosphere. The lower (hot) side of a subducting slab entrains by the formation of a âŒ10â30 km-thick downdragged layer, whose thickness depends upon the subduction rate and the density contrast and viscosity of the asthenosphere, while the upper (cold) side of the slab may entrain as much by thermal 'freezing' onto the slab as by mechanical downdragging. This analysis also implies that proper treatment of slab entrainment in future numerical mantle flow experiments will require the resolution of âŒ10â30 km-thick entrainment boundary layers
Crustal structure of the propagating TAMMAR ridge segment on the Mid-Atlantic Ridge, 21.5°N
Active ridge propagation frequently occurs along spreading ridges and profoundly affects ridge crest segmentation over time. The mechanisms controlling ridge propagation, however, are poorly understood. At the slow spreading Mid-Atlantic Ridge at 21.5°N a seismic refraction and wide-angle reflection profile surveyed the crustal structure along a segment controlled by rapid ridge propagation. Tomographic traveltime inversion of seismic data suggests that the crustal structure along the ridge axis is controlled by melt supply; thus, crust is thickest, 8 km, at the domed segment center and decreases in thickness toward both segment ends. However, thicker crust is formed in the direction of ridge propagation, suggesting that melt is preferentially transferred toward the propagating ridge tip. Further, while seismic layer 2 remains constant along axis, seismic layer 3 shows profound changes in thickness, governing variations in total crustal thickness. This feature supports mantle upwelling at the segment center. Thus, fluid basaltic melt is redistributed easily laterally, while more viscose gabbroic melt tends to crystallize and accrete nearer to the locus of melt supply. The onset of propagation seems to have coincided with the formation of thicker crust, suggesting that propagation initiation might be due to changes in the melt supply. After a rapid initiation a continuous process of propagation was established. The propagation rate seems to be controlled by the amount of magma that reaches the segment ends. The strength of upwelling may govern the evolution of ridge segments and hence ultimately controls the propagation length
Morphology and tectonics of the Mid-Atlantic Ridge, 7°â12°S
We present swath bathymetric, gravity, and magnetic data from the Mid-Atlantic Ridge between the Ascension and the Bode Verde fracture zones, where significant ridgeâhot spot interaction has been inferred. The ridge axis in this region may be divided into four segments. The central two segments exhibit rifted axial highs, while the northernmost and southernmost segments have deep rift valleys typical of slow-spreading mid-ocean ridges. Bathymetric and magnetic data indicate that both central segments have experienced ridge jumps since ~1 Ma. Mantle Bouguer anomalies (MBAs) derived from shipboard free air gravity and swath bathymetric data show deep subcircular lows centered on the new ridge axes, suggesting that mantle flow has been established beneath the new spreading centers for at least ~1 Myr. Inversion of gravity data indicates that crustal thicknesses vary by ~4 km along axis, with the thickest crust occurring beneath a large axial volcanic edifice. Once the effects of lithospheric aging have been removed, a model in which gravity variations are attributed entirely to crustal thickness variations is more consistent with data from an axis-parallel seismic line than a model that includes additional along-axis variations in mantle temperature. Both geophysical and geochemical data from the region may be explained by the melting of small (<200 km) mantle chemical heterogeneities rather than elevated temperatures. Therefore, there may be no Ascension/Circe plume
Melt generation, crystallization, and extraction beneath segmented oceanic transform faults
Author Posting. © American Geophysical Union, 2009. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 114 (2009): B11102, doi:10.1029/2008JB006100.We examine mantle melting, fractional crystallization, and melt extraction beneath fast slipping, segmented oceanic transform fault systems. Three-dimensional mantle flow and thermal structures are calculated using a temperature-dependent rheology that incorporates a viscoplastic approximation for brittle deformation in the lithosphere. Thermal solutions are combined with the near-fractional, polybaric melting model of Kinzler and Grove (1992a, 1992b, 1993) to determine extents of melting, the shape of the melting regime, and major element melt composition. We investigate the mantle source region of intratransform spreading centers (ITSCs) using the melt migration approach of Sparks and Parmentier (1991) for two end-member pooling models: (1) a wide pooling region that incorporates all of the melt focused to the ITSC and (2) a narrow pooling region that assumes melt will not migrate across a transform fault or fracture zone. Assuming wide melt pooling, our model predictions can explain both the systematic crustal thickness excesses observed at intermediate and fast slipping transform faults as well as the deeper and lower extents of melting observed in the vicinity of several transform systems. Applying these techniques to the Siqueiros transform on the East Pacific Rise we find that both the viscoplastic rheology and wide melt pooling are required to explain the observed variations in gravity inferred crustal thickness. Finally, we show that mantle potential temperature Tp = 1350°C and fractional crystallization at depths of 9â15.5 km fit the majority of the major element geochemical data from the Siqueiros transform fault system.This research was supported by WHOI Academic Programs
Office (PMG), NSF grants OCE-0649103 and OCE-0623188 (MDB),
and the Charles D. Hollister Endowed Fund for Support of Innovative
Research at WHOI (J.L.)
Upper crustal structure and axial topography at intermediate spreading ridges : seismic constraints from the southern Juan de Fuca Ridge
Author Posting. © American Geophysical Union, 2005. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 110 (2005): B12104, doi:10.1029/2005JB003630.We use multichannel seismic reflection data to image the upper crustal structure of 0-620
ka crust along the southern Juan de Fuca Ridge (JdFR). The study area comprises two
segments spreading at intermediate rate with an axial high morphology with narrow
(Cleft) and wide (Vance) axial summit grabens (ASG). Along most of the axis of both
segments we image the top of an axial magma chamber (AMC). The AMC along Cleft
deepens from south to north, from 2.0 km beneath the RIDGE Cleft Observatory and
hydrothermal vents near the southern end of the segment, to 2.3 km at the northern end
near the site of the 1980âs eruptive event. Along the Vance segment, the AMC also
deepens from south to north, from 2.4 km to 2.7 km. Seismic layer 2A, interpreted as the
basaltic extrusive layer, is 250-300 m thick at the ridge axis along the Cleft segment, and
300-350 m thick along the axis of the Vance segment. However off-axis layer 2A is
similar in both segments (500-600 m), indicating ~90% and ~60% off-axis thickening at
the Cleft and Vance segments, respectively. Half of the thickening occurs sharply at the
walls of the ASG, with the remaining thickening occurring within 3-4 km of the ASG.
Along the full length of both segments, layer 2A is thinner within the ASG, compared to
the ridge flanks. Previous studies argued that the ASG is a cyclic feature formed by
alternating periods of magmatism and tectonic extension. Our observations agree with
the evolving nature of the ASG. However, we suggest that its evolution is related to large
changes in axial morphology produced by small fluctuations in magma supply. Thus the
ASG, rather than being formed by excess volcanism, is a rifted flexural axial high. The
changes in axial morphology affect the distribution of lava flows along the ridge flanks,
as indicated by the pattern of layer 2A thickness. The fluctuations in magma supply may
occur at all spreading rates, but its effects on crustal structure and axial morphology are
most pronounced along intermediate spreading rate ridges.This study was supported by the National Science Foundation grants OCE-0002551 to
Woods Hole Oceanographic Institution, OCE-0002488 to Lamont-Doherty Earth
Observatory, and OCE-0002600 to Scripps Institution of Oceanography
Morphology and segmentation of the western GalĂĄpagos Spreading Center, 90.5°â98°W : plume-ridge interaction at an intermediate spreading ridge
Author Posting. © American Geophysical Union 2003. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geochemistry Geophysics Geosystems 4 (2003): 8515, doi:10.1029/2003GC000609.Complete multibeam bathymetric coverage of the western GalĂĄpagos Spreading Center (GSC) between 90.5°W and 98°W reveals the fine-scale morphology, segmentation and influence of the GalĂĄpagos hot spot on this intermediate spreading ridge. The western GSC comprises three morphologically defined provinces: A Western Province, located farthest from the GalĂĄpagos hot spot west of 95°30âČW, is characterized by an axial deep, rift valley morphology with individual, overlapping, E-W striking segments separated by non-transform offsets; A Middle Province, between the propagating rift tips at 93°15âČW and 95°30âČW, with transitional axial morphology strikes âŒ276°; An Eastern Province, closest to the GalĂĄpagos hot spot between the âŒ90°50âČW GalĂĄpagos Transform and 93°15âČW, with an axial high morphology generally less than 1800 m deep, strikes âŒ280°. At a finer scale, the axial region consists of 32 individual segments defined on the basis of smaller, mainly <2 km, offsets. These offsets mainly step left in the Western and Middle Provinces, and right in the Eastern Province. Glass compositions indicate that the GSC is segmented magmatically into 8 broad regions, with Mg # generally decreasing to the west within each region. Striking differences in bathymetric and lava fractionation patterns between the propagating rifts with tips at 93°15âČW and 95°30âČW reflect lower overall magma supply and larger offset distance at the latter. The structure of the Eastern Province is complicated by the intersection of a series of volcanic lineaments that appear to radiate away from a point located on the northern edge of the GalĂĄpagos platform, close to the southern limit of the GalĂĄpagos Fracture Zone. Where these lineaments intersect the GSC, the ridge axis is displaced to the south through a series of overlapping spreading centers (OSCs); abandoned OSC limbs lie even farther south. We propose that southward displacement of the axis is promoted during intermittent times of increased plume activity, when lithospheric zones of weakness become volcanically active. Following cessation of the increased plume activity, the axis straightens by decapitating southernmost OSC limbs during short-lived propagation events. This process contributes to the number of right stepping offsets in the Eastern Province.This work was supported by NSF grants OCE98-
18632 to the University of Hawaiâi and OCE98-19117 to the
Woods Hole Oceanographic Institution; support was provided to M. B. by a CIW/DTM Postdoctoral Fellowshi
How and when plume zonation appeared during the 132 Myr evolution of the Tristan Hotspot
Increasingly, spatial geochemical zonation, present as geographically distinct, subparallel
trends, is observed along hotspot tracks, such as Hawaii and the Galapagos. The origin of this
zonation is currently unclear. Recently zonation was found along the last B70 Myr of the
Tristan-Gough hotspot track. Here we present new SrâNdâPbâHf isotope data from the older
parts of this hotspot track (Walvis Ridge and Rio Grande Rise) and re-evaluate published data
from the Etendeka and Parana flood basalts erupted at the initiation of the hotspot track. We
show that only the enriched Gough, but not the less-enriched Tristan, component is present in
the earlier (70â132 Ma) history of the hotspot. Here we present a model that can explain the
temporal evolution and origin of plume zonation for both the Tristan-Gough and Hawaiian
hotspots, two end member types of zoned plumes, through processes taking place in the
plume sources at the base of the lower mantle
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