H, O, Sr, and Nd isotope ratios and water, Rb, Sr, Sm, and Nd content of ODP Hole 116-717C and 116-718C samples (Table 2)


Autoria(s): Bouquillon, Anne; France-Lanord, Christian; Michard, Annie; Tiercelin, Jean-Jacques
Cobertura

MEDIAN LATITUDE: -0.975350 * MEDIAN LONGITUDE: 81.395600 * SOUTH-BOUND LATITUDE: -1.020900 * WEST-BOUND LONGITUDE: 81.390100 * NORTH-BOUND LATITUDE: -0.929800 * EAST-BOUND LONGITUDE: 81.401100 * DATE/TIME START: 1987-07-10T00:00:00 * DATE/TIME END: 1987-07-20T00:00:00 * MINIMUM ELEVATION: -4746.0 m * MAXIMUM ELEVATION: -4741.0 m

Data(s)

24/01/1990

Resumo

Mineralogical and H, O, Sr, and Nd isotope compositions have been analyzed on a set of representative samples from the 17-m.y. section in ODP Leg 116 Holes 717C and 718C. Based on the mineralogical composition of the fraction <2 µm together with the lithogenic-biogenic composition of the fraction >63 µm, the whole section can be subdivided into three major periods of sedimentation. Between 17.1 and 6 m.y., and between 0.8 m.y. to present, the sediments are characterized by sandy and silty turbiditic inputs with a high proportion of minerals derived from a gneissic source without alteration. In the fraction <2 µm, illite and chlorite are dominant over smectite and kaolinite. The granulometric fraction >63 µm contains quartz, muscovite, biotite, chlorite, and feldspars. The 6-to 0.8-m.y. period is represented by an alternation of sandy/silty horizons, muds, and calcareous muds rich in smectite, and kaolinite (50% to 85% of the fraction <2 µm) and bioclastic material. The presence of smectite and kaolinite, as well as the 18O/16O and the 87Sr/86Sr ratios of the fraction <2 µm, imply an evolution in a soil environment and exchanges with meteoric ground water. The ranges of isotopic compositions are limited throughout the section: d18O quartz = 11.7 to 13.3 per mil, 87Sr/86Sr = 0.733 to 0.760 and epsilon-Nd (0) = -17.4 to -13.8. These values are within those of the High Himalaya Crystalline series, and they are considered to reflect this source region. The data imply that, since 17 Ma, this formation has supplied the major part of the eroded material.

Formato

text/tab-separated-values, 304 data points

Identificador

https://doi.pangaea.de/10.1594/PANGAEA.756369

doi:10.1594/PANGAEA.756369

Idioma(s)

en

Publicador

PANGAEA

Direitos

CC-BY: Creative Commons Attribution 3.0 Unported

Access constraints: unrestricted

Fonte

Supplement to: Bouquillon, Anne; France-Lanord, Christian; Michard, Annie; Tiercelin, Jean-Jacques (1990): Sedimentology and isotopic chemistry of the Bengal Fan sediments: the denudation of the Himalaya. In: Cochran, JR; Stow, DAV; et al. (eds.), Proceedings of the Ocean Drilling Program, Scientific Results, College Station, TX (Ocean Drilling Program), 116, 43-58, doi:10.2973/odp.proc.sr.116.117.1990

Palavras-Chave #116-717C; 116-718C; delta 18O; delta Deuterium; DRILL; Drilling/drill rig; epsilon-Neodymium (0); Event label; Joides Resolution; Leg116; Neodymium; Neodymium 143/Neodymium 144; Neodymium 143/Neodymium 144, error; Ocean Drilling Program; ODP; ODP sample designation; Rubidium; Samarium; Sample code/label; Sample comment; South Indian Ridge, South Indian Ocean; Strontium; Strontium 87/Strontium 86 ratio; Water in rock
Tipo

Dataset