Abstract:[1] We report new trace element concentrations and Sr, Nd, Hf, and Pb isotopic ratios for basalts from the three lava series of Mauritius. Older Series lavas, which represent the shield-building phase of Mauritius, are isotopically similar to other lavas produced by the Réunion mantle plume. The Intermediate and Younger Series lavas, erupted after a hiatus of millions of years, have more depleted isotopic signatures than the Older Series. Incompatible element abundances and major element compositions suggest t… Show more
“…Furthermore, Intermediate series and Younger Series lavas from Mauritius and Rodrigues show 3 He/ 4 He ratios of 6.5 to 8.4 R A [ Hanyu et al , 2001]. These helium isotope signatures suggest that the late‐stage lavas are derived from a mantle source that is dominated by a MORB‐like component, and they rule out melting of a heterogeneous “plum pudding” Réunion mantle component alone as the source of lavas in Mauritius [ Paul et al , 2005, 2007]. Consequently, we propose that the variations in 3 He/ 4 He ratios of glasses recovered along the off‐axis volcanic structures can only be explained by mixing of the (residual) hot spot component with partial melts derived from a MORB‐like mantle reservoir.…”
Section: Discussionmentioning
confidence: 99%
“…The island is composed of two volcanoes: Piton des Neiges, which was active between ∼2 Ma and 43 ka, and the still active Piton de la Fournaise, where volcanic activity began ∼530 ka ago [ Gillot and Nativel , 1989]. Mauritius is considered to be located on the former site of the Réunion hot spot [ Morgan , 1981; Paul et al , 2005]. Volcanic activity on Mauritius started with a shield‐building stage at 8 to 7 Ma (Older Series), with later stages at 3 to 2 Ma (Intermediate Series) and 0.7 to 0.2 Ma (Younger Series) [ McDougall and Chamalaun , 1969].…”
Section: Geologic Setting and Backgroundmentioning
[1] We report new helium abundance and isotope results for submarine basaltic glasses from the Central Indian Ridge (CIR) between the Marie Celeste (16.7°S) and Egeria fracture zones (FZ) (20.6°S); the adjacent Gasitao, Three Magi, and Rodrigues ridges; and for olivine separates from lavas and cumulate xenoliths from the Mascarene Islands (Réunion, Mauritius, and Rodrigues). Helium isotope ratios in basaltic glasses range from 7.1 to 12.2 R A (where R A = air 3 He/ 4 He) and lie between values of Mid-Ocean Ridge Basalt (MORB) (8 ± 1 R A ) and samples from Réunion Island (11.5 to 14.1 R A ). The highest 3 He/ 4 He values (up to 12.2 R A ) are found in glasses recovered off axis from the Three Magi and Gasitao ridges. Along the CIR axis, MORB-like 3 He/ 4 He ratios are found near the Egeria FZ, and there is a marked increase to values of ∼11 R A between ∼19°and 20°S. The lowest 3 He/ 4 He values (<8 R A ) are found immediately south of the Marie Celeste FZ, where incompatible trace element ratios (e.g., La/Sm) are highest. These low 3 He/ 4 He ratios can be explained by closed system radiogenic 4 He ingrowth in either (1) a "fossil" Réunion hot spot mantle component, embedded into the subridge mantle when the CIR migrated over the hot spot at ∼34 Ma or (2) trace element enriched MORB mantle. In contrast, the high 3 He/ 4 He ratios observed on the CIR axis adjacent to the Gasitao Ridge, and along the off-axis volcanic ridges, are consistent with flow of hot spot mantle material from Réunion (∼1100 km to the west) toward the CIR.
“…Furthermore, Intermediate series and Younger Series lavas from Mauritius and Rodrigues show 3 He/ 4 He ratios of 6.5 to 8.4 R A [ Hanyu et al , 2001]. These helium isotope signatures suggest that the late‐stage lavas are derived from a mantle source that is dominated by a MORB‐like component, and they rule out melting of a heterogeneous “plum pudding” Réunion mantle component alone as the source of lavas in Mauritius [ Paul et al , 2005, 2007]. Consequently, we propose that the variations in 3 He/ 4 He ratios of glasses recovered along the off‐axis volcanic structures can only be explained by mixing of the (residual) hot spot component with partial melts derived from a MORB‐like mantle reservoir.…”
Section: Discussionmentioning
confidence: 99%
“…The island is composed of two volcanoes: Piton des Neiges, which was active between ∼2 Ma and 43 ka, and the still active Piton de la Fournaise, where volcanic activity began ∼530 ka ago [ Gillot and Nativel , 1989]. Mauritius is considered to be located on the former site of the Réunion hot spot [ Morgan , 1981; Paul et al , 2005]. Volcanic activity on Mauritius started with a shield‐building stage at 8 to 7 Ma (Older Series), with later stages at 3 to 2 Ma (Intermediate Series) and 0.7 to 0.2 Ma (Younger Series) [ McDougall and Chamalaun , 1969].…”
Section: Geologic Setting and Backgroundmentioning
[1] We report new helium abundance and isotope results for submarine basaltic glasses from the Central Indian Ridge (CIR) between the Marie Celeste (16.7°S) and Egeria fracture zones (FZ) (20.6°S); the adjacent Gasitao, Three Magi, and Rodrigues ridges; and for olivine separates from lavas and cumulate xenoliths from the Mascarene Islands (Réunion, Mauritius, and Rodrigues). Helium isotope ratios in basaltic glasses range from 7.1 to 12.2 R A (where R A = air 3 He/ 4 He) and lie between values of Mid-Ocean Ridge Basalt (MORB) (8 ± 1 R A ) and samples from Réunion Island (11.5 to 14.1 R A ). The highest 3 He/ 4 He values (up to 12.2 R A ) are found in glasses recovered off axis from the Three Magi and Gasitao ridges. Along the CIR axis, MORB-like 3 He/ 4 He ratios are found near the Egeria FZ, and there is a marked increase to values of ∼11 R A between ∼19°and 20°S. The lowest 3 He/ 4 He values (<8 R A ) are found immediately south of the Marie Celeste FZ, where incompatible trace element ratios (e.g., La/Sm) are highest. These low 3 He/ 4 He ratios can be explained by closed system radiogenic 4 He ingrowth in either (1) a "fossil" Réunion hot spot mantle component, embedded into the subridge mantle when the CIR migrated over the hot spot at ∼34 Ma or (2) trace element enriched MORB mantle. In contrast, the high 3 He/ 4 He ratios observed on the CIR axis adjacent to the Gasitao Ridge, and along the off-axis volcanic ridges, are consistent with flow of hot spot mantle material from Réunion (∼1100 km to the west) toward the CIR.
“…) after analysing 50 mg. Paul et al . () obtained the highest Mo mass fraction (0.42 μg g −1 ) from a 25‐mg test portion. This phenomenon is perhaps due to a specific chemical/mineral form of Mo in the basalt BIR‐1 and could also occur in other rock samples.…”
The influence of the mixtures HF‐HNO3 and HF‐NH4F‐HNO3 in bomb digestion for trace element determination from different rock types was studied using ICP‐MS. It is shown that the HF concentration, not the ratio of reagents in the decomposing mixture, controls the digestion process of a rock. Data for Zr in the granite G‐2 as a function of HF concentration gave the same results as reaction mixtures of various compositions. A complete digestion in 50‐mg sample bombs was achieved by 1.0 ml of HF alone, or with a mixture of other acids at a HF concentration of at least 35% m/m at 196 °C over 18 h. The results of the analysis of basalts BCR‐1, BIR‐1, mica schist SDC‐1, shale SBC‐1, granites G‐2, SG‐1A, garnet‐biotite plagiogneiss GBPg‐1, rhyolite RGM‐1, granodiorite GSP‐1, trachyandesite MTA‐1 and rhyolite MRh‐1 are given and compared against available data. The reproducibility of the element determinations by ICP‐MS and XRF as an independent non‐destructive analysis for a quality check in the range of concentrations typical for routine rock samples is given.
“…There are important differences, however. Rejuvenescent lavas are only slightly less silica saturated and, in contrast to Hawaii, are slightly less incompatible element-enriched than shield stage lavas (e.g., Paul et al, 2005;Moore et al, 2011). Furthermore, the rejuvenescent phase has been extraordinarily long (~3.5 million years) and is interrupted by a hiatus of ~600,000 years separating the so-called Intermediate and Younger Series.…”
Section: The Mystery Of Rejuvenescent Volcanismmentioning
confidence: 99%
“…Further downstream, a bulge or arch develops in response to this loading, relieve horizontal compressive stresses and allowing magma to reach the surface. In combination, a long melting tail and lithospheric flexure could explain both the volcanism and the hiatus (e.g., Paul et al, 2005;Garcia et al, 2010). Bianco et al (2005) extended the flexure model, arguing that sufficient upwelling occurs in the asthenosphere as the lithosphere arches upward to generate the small melt fractions that characterise the rejuvenescent magmas.…”
Section: The Mystery Of Rejuvenescent Volcanismmentioning
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