Extractos de residuos de la vitivinicultura : concentración de polifenoles

El objetivo del trabajo fue determinar la concentración de polifenoles en extractos de hojas de verano y otoño y de escobajo de variedades tintas de vitis vinifera, obtenidos por distintos métodos.Se trabajó con hojas de verano y de otoño de variedad Syrah y con hojas de otoño variedad Malbec, dividiéndolas por su color en rojas y amarillas, y con escobajo de variedad Malbec. Los extractos se obtuvieron por maceración en agua y baño María hirviente durante tres horas (BM), maceración en agua y agitación, a temperatura ambiente, durante 48 horas (AG). Se utilizó como referencia oleorresina de romero. El orden decreciente respecto de la cantidad de polifenoles expresados en g de quercitina / g de extracto seco fue el siguiente: oleorresina de romero: 56,3 ± 0,3 extracto de: hojas de otoño Syrah por maceración y agitación en agua a temperatura ambiente durante 48 horas: 7,5 ± 0,3; escobajo Malbec por maceración y agitación en agua a temperatura ambiente durante 48 horas: 24 ± 0,3; hojas de otoño rojas Malbec por maceración y agitación en agua a temperatura ambiente durante 48 horas: 22 ± 0,3; escobajo de Malbec: a baño María 21,4 ± 0,3; hojas de otoño Syrah 3 horas a baño María: 21,1 ±0,3; hojas de otoño amarillas Malbec por maceración y agitación en agua a temperatura ambiente durante 48 horas: 17 ± 0,3; hojas de verano Syrah 3 horas a baño María: 16,5 ± 0,3; hojas de otoño rojas Malbec 3 horas a baño María: 13,8 ± 0,3; hojas de otoño amarillas Malbec 3 horas a baño María: 12,4 ± 0,3; hojas de verano Syrah por maceración y agitación en agua a temperatura ambiente durante 48 horas: 12,2 ± 0,3. Se concluyó que las hojas de otoño contienen mayor cantidad de polifenoles que las de verano; la variedad Syrah posee más polifenoles en hojas que la variedad Malbec; el escobajo de Malbec contiene más olifenoles que las hojas de la misma variedad; y el mejor método de extracción para obtener estos compuestos activos fue por maceración en agua y agitación a temperatura ambiente durante 48 horas.

(Table 2) Major and trace element content of ODP Leg 130 basalts

Estimated relative errors on major and minor elements are 1%. For trace elements, errors (% standard deviation at levels measured) are estimated at 1 % for Cr, 3% for Ni, 3% for Rb at 30 ppm, and >20% at < 10 ppm; 2% for Sr and V, and 4% for Y and Zr.

Geochemistry of Ninetyeast Ridge basaltic glasses

The Ninetyeast Ridge (NER), a north-south striking, 5,000 km long, 77 to 43 Ma chain of basaltic submarine volcanoes in the eastern Indian Ocean formed as a hotspot track created by rapid northward migration of the Indian Plate over the Kerguelen hotspot. Based on the major and trace element contents of unaltered basaltic glasses from six locations along the NER, we show that the NER was constructed by basaltic magma derived from at least three geochemically distinct mantle sources: (1) a source enriched in highly incompatible elements relative to primitive mantle like the source of the 29-24 Ma flood basalts in the Kerguelen Archipelago; (2) an incompatible element-depleted source similar to the source of Mid-Ocean Ridge Basalt (MORB) erupted along the currently active Southeast Indian Ridge (SEIR); and (3) an incompatible element-depleted source that is compositionally and mineralogically distinct from the source of SEIR MORB. Specifically, this depleted mantle source was garnet-bearing and had higher Y/Dy and Nb/Zr, but lower Zr/Sm, than the SEIR MORB source. We infer that this third source formed as a garnet-bearing residue created during a previous melting event, perhaps an initial partial melting of the mantle hotspot. Subsequently, this residue partially melted over a large pressure range, from slightly over 3 GPa to less than 1 GPa, and to a high extent (~ 30%) thereby creating relatively high SiO2 and FeO contents in some NER basalts relative to SEIR MORB.

Rhenium and platinum-group element concentrations and Os isotope data for Philippine Sea Plate basalts from DSDP Legs 31, 58, and 59

Platinum-group elements (PGE), rhenium and osmium isotope data are reported for basalts from Deep Sea Drilling Project cores in the Philippine Sea Plate (PSP). Lithophile trace element and isotopic characteristics indicate a range of source components including DMM, EMII and subduction-enriched mantle. MORB-like basalts possess smooth, inclined chondrite-normalised PGE patterns with high palladium-PGE/iridium-PGE ratios, consistent with previously published data for MORB, and with the inferred compatibility of PGE. In contrast, while basalts with EMII-type lithophile element chemistry possess high Pt/Ir ratios, many have much lower Pd/Ir and unusually high Ru/Ir of >10. Similarly, back-arc samples from the Shikoku and Parece-Vela basins have very high Ru/Ir ratios (>30) and Pd/Ir as low as 1.1. Such extreme Pd/Ir and Ru/Ir ratios have not been previously reported in mafic volcanic suites and cannot be easily explained by variable degrees of melting, fractional crystallisation or by a shallow-level process such as alteration or degassing. The data appear most consistent with sampling of at least two mantle components with distinct PGE compositions. Peridotites with the required PGE characteristics (i.e. low Pd, but relatively high Ru and Re) have not been documented in oceanic mantle, but have been found in sub-continental mantle lithosphere and are the result of considerable melt depletion and selective metasomatic enrichment (mainly Re). The long-term presence of subduction zones surrounding the Philippine Sea Plate makes this a prime location for metasomatic enrichment of mantle, either through fluid enrichment or infiltration by small melt fractions. The Re-Os isotope data are difficult to interpret with confidence due to low Os concentrations in most samples and the uncertainty in sample age. Data for Site 444A (Shikoku Basin) give an age of 17.7+/-1.3 Ma (MSWD = 14), consistent with the proposed age of basement at the site and thus provides the first robust radiometric age for these samples. The initial 187Os/188Os of 0.1298+/-0.0069 is consistent with global MORB, and precludes significant metasomatic enrichment of Os by radiogenic slab fluids. Re-Os data for Sites 446A (two suites, Daito Basin) and 450 (Parece-Vela Basin) indicate ages of 73, 68 and 43 Ma, which are respectively, 30, 17 and >12 Ma older than previously proposed ages. The alkalic and tholeiitic suites from Site 446A define regression lines with different 187Os/188Osinitial (0.170+/-0.033 and 0.112+/-0.024, respectively) which could perhaps be explained by preferential sampling of interstitial, metasomatic sulphides (with higher time-integrated Re/Os ratios) by smaller percentage alkalic melts. One sample, with lithophile elements indistinguishable from MORB, is Os-rich (146 pg/g) and has an initial 187Os/188Os of 0.1594, which is at the upper limit of the accepted OIB range. Given the Os-rich nature of this sample and the lack of evidence for subduction or recycled crust inputs, this osmium isotope ratio likely reflects heterogeneity in the DMM. The dataset as a whole is a striking indication of the possible PGE and Os isotope variability within a region of mantle that has experienced a complex tectonic history.