Noble gases in submarine pillow volcanic glasses

Fifteen submarine glasses from the East Pacific Rise (CYAMEX), the Kyushu-Palau Ridge (DSDP Leg 59) and the Nauru Basin (DSDP Leg 61) were analysed for noble gas contents and isotopic ratios. Both the East Pacific Rise and Kyushu-Palau Ridge samples showed Ne excess relative to Ar and a monotonic decrease from Xe to Ar when compared with air noble gas abundance. This characteristic noble gas abundance pattern (type 2, classified by Ozima and Alexander) is interpreted to be due to a two-stage degassing from a noble gas reservoir with originally atmospheric abundance. In the Kyushu-Palau Ridge sample, noble gases are nearly ten times more abundant than in the East Pacific Rise samples. This may be attributed to an oceanic crust contamination in the former mantle source. There is no correlation between the He content and that of the other noble gas in the CYAMEX samples. This suggests that He was derived from a larger region, independent from the other noble gases. Except where radiogenic isotopes are involved, all other noble gas isotopic ratios were indistinguishable from air noble gas isotopic ratios. The 3He/4He in the East Pacific Rise shows a remarkably uniform ratio of (1.21 +/- 0.07)10*-5, while the40Ar/36Ar ranges from 700 to 5600.

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Cite this as

Ozima, Minoru, Zashu, S (1983). Dataset: Noble gases in submarine pillow volcanic glasses. https://doi.org/10.1594/PANGAEA.723734

DOI retrieved: 1983

Additional Info

Field Value
Imported on November 29, 2024
Last update November 29, 2024
License CC-BY-3.0
Source https://doi.org/10.1594/PANGAEA.723734
Author Ozima, Minoru
Given Name Minoru
Family Name Ozima
More Authors
Zashu, S
Source Creation 1983
Publication Year 1983
Resource Type application/zip - filename: Ozima_Zashu_1983
Subject Areas
Name: Geophysics

Related Identifiers
Title: Noble gases in submarine pillow volcanic glasses
Identifier: https://doi.org/10.1016/0012-821X(83)90068-7
Type: DOI
Relation: IsSupplementTo
Year: 1983
Source: Earth and Planetary Science Letters
Authors: Ozima Minoru , Zashu S .