Publication | Closed Access
Isotopic and geochemical provinces of the western Indian Ocean Spreading Centers
317
Citations
71
References
1989
Year
India-asia Collision ZoneVolcanologyEngineeringMarine ChemistryIndia-asia CollisionOceanographyEarth ScienceBasalt GlassesCentral Indian RidgeCrustal MeltingGeochemical ProvincesMarine GeologyMagmatismIgneous PetrogenesisGeographyGeologyTriple JunctionMantle GeochemistryTectonicsStructural GeologyEconomic GeologyEarth SciencesGeochemistryCrust-mantle InteractionPetrology
Basalt glasses from the Central Indian Ridge are distinct isotopically from mid‐ocean ridge basalts (MORB) of the Indian Ocean triple junction and western few hundred kilometers of the Southeast Indian Ridge. In particular, very low 206 Pb/ 204 Pb and high 87 Sr/ 86 Sr signatures, which characterize the latter region, are absent over most of the Central Indian Ridge. In turn, lavas from the unusually deep eastern 1100–1500 km of the Southwest Indian Ridge are different chemically and isotopically from those of the above areas. A rather abrupt eastern boundary to Southwest Indian Ridge‐type compositions occurs at or very near the geographic triple junction. This provinciality in western Indian Ocean ridge basalts partly mirrors fundamental regional differences in the underlying mantle but, at least between the eastern Southwest Indian Ridge and the western Southeast Indian Ridge and triple junction, also may reflect variations in extent and depth of melting in a vertically zoned upper mantle. A pronounced low ε Nd , high 206 Pb/ 204 Pb, high 87 Sr/ 86 Sr anomaly exists on the Central Indian Ridge at the Marie Celeste Fracture Zone and on the adjacent ridge segment to the south. Despite the great distance (>1100 km) of Réunion Island from the ridge, this zone appears to demark a region of mantle containing substantial Réunion hotspotlike material. Several old (35–60 m.y.) Deep Sea Drilling Project basalts which erupted on the ancestral Central Indian Ridge also record a significant Réunion hotspotlike influence, whereas a 46‐m.y.‐old sample that formed farther from the presumed locus of the hotspot possesses isotopic values identical to many present (non‐Marie Celeste area) Central Indian Ridge MORB. The variably expressed and/or heterogeneous low 206 Pb/ 204 Pb material partly responsible for the isotopic distinctiveness of Indian Ocean ridge basalts may have entered into the Indian MORB mantle as a result of continental lithospheric remobilization preceding the breakup of Gondwana, particularly from the portion that would eventually become Greater India.
| Year | Citations | |
|---|---|---|
Page 1
Page 1