Chemical and isotopic composition of interstitial waters and hydrocarbon composition at ODP Site 184-1146

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Main Authors: Zhu, Youhai, Huang, Yongyang, Matsumoto, Ryo, Wu, Bihao
Format: Dataset Open Access
Language:en
Published: PANGAEA 2003
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author Zhu, Youhai
Huang, Yongyang
Matsumoto, Ryo
Wu, Bihao
author_facet Zhu, Youhai
Huang, Yongyang
Matsumoto, Ryo
Wu, Bihao
collection Datos científicos de ciencias marinas y ambientales
contents Bottom-simulating reflectors were observed beneath the southeastern slope of the Dongsha Islands in the South China Sea, raising the potential for the presence of gas hydrate in the area. We have analyzed the chemical and isotopic compositions of interstitial water, headspace gas, and authigenic siderite concretions from Site 1146. Geochemical anomalies, including a slight decrease of chlorine concentration in interstitial water, substantial increase of methane concentration in headspace gas, and 18O enrichment in the authigenic siderite concretion below 400 meters below seafloor are probably caused by the decomposition of gas hydrate. The low-chlorine pore fluids contain higher molecular-weight hydrocarbons and probably migrate to Site 1146 along faults or bedded planes.
format Dataset Open Access
id pangaea_https___doi_org_10_1594_PANGAEA_784852
institution PANGAEA
language en
publishDate 2003
publisher PANGAEA
record_format pangaea
spellingShingle Chemical and isotopic composition of interstitial waters and hydrocarbon composition at ODP Site 184-1146
Zhu, Youhai
Huang, Yongyang
Matsumoto, Ryo
Wu, Bihao
184-1146A; 184-1146C; DRILL; Drilling/drill rig; Joides Resolution; Leg184; Ocean Drilling Program; ODP; South China Sea
Bottom-simulating reflectors were observed beneath the southeastern slope of the Dongsha Islands in the South China Sea, raising the potential for the presence of gas hydrate in the area. We have analyzed the chemical and isotopic compositions of interstitial water, headspace gas, and authigenic siderite concretions from Site 1146. Geochemical anomalies, including a slight decrease of chlorine concentration in interstitial water, substantial increase of methane concentration in headspace gas, and 18O enrichment in the authigenic siderite concretion below 400 meters below seafloor are probably caused by the decomposition of gas hydrate. The low-chlorine pore fluids contain higher molecular-weight hydrocarbons and probably migrate to Site 1146 along faults or bedded planes.
title Chemical and isotopic composition of interstitial waters and hydrocarbon composition at ODP Site 184-1146
topic 184-1146A; 184-1146C; DRILL; Drilling/drill rig; Joides Resolution; Leg184; Ocean Drilling Program; ODP; South China Sea
url https://doi.org/10.1594/PANGAEA.784852