孟加拉湾克里希纳-戈达瓦里(K-G)盆地外甲烷渗漏点自生碳酸盐沉积的生物地球化学重建

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geochemistry Geophysics Geosystems Pub Date : 2024-10-27 DOI:10.1029/2024GC011801
S. P. K. Pillutla, A. Peketi, A. Mazumdar, Mohd. Sadique, K. Sivan, Anjali Zatale, S. Mishra, Swati Verma
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引用次数: 0

摘要

活跃的和遗存的海洋甲烷渗漏点广泛分布于全球各地,具有独特的地质、生物地球化学和生态系统。克里希纳-戈达瓦里(K-G)盆地甲烷渗漏点的发现为孟加拉湾的甲烷渗漏研究创造了令人兴奋的新机遇。在本研究中,我们记录了 K-G 盆地 SSD-045/4 甲烷渗漏点出现的自生碳酸盐,包括微晶文石壳(arg-crusts)与化合壳和高镁碳酸盐管状结构(HMC-tube)。HMC管(-54.5至-46.2‰)和氩壳(-57.6至-34.8‰)的δ13C值表明生物甲烷可能是碳源。促使碳酸盐沉淀的孔隙水碱度增强可能归因于微生物介导的 SO₄2--AOM 过程。此外,碳酸盐中残留有机物的δ13C值(-35.2 ± 8‰)表明,甲烷营养细菌的生物量也有贡献。HMC 和文石的 δ18Ocarb 值分别表明甲烷水合物的脱气和结晶途径。藻类填充的洞穴表明掘进生物对浅层 HMC 沉积物进行了再加工,而洞穴内的多相胶结物(文石和 HMC)则表明了早期和埋藏成岩途径。氩壳中ΣLREE/ΣHREE比值和Ceanom值范围较大,反映了氧化还原条件的微观空间变化,这可能是由于在开放和封闭成岩系统中都发生了胶结作用。相比之下,HMC管中的Ceanom值和ΣLREE/ΣHREE比值更为精确,表明硫酸条件持续存在。总之,这些发现提供了对 K-G 盆地甲烷渗漏点碳酸盐形成途径的见解,凸显了微生物过程、流体动力学和成岩改变之间复杂的相互作用。
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Biogeochemical Reconstruction of Authigenic Carbonate Deposits at Methane Seep Site off Krishna-Godavari (K-G) Basin, Bay of Bengal

Active and relic marine methane-seep sites are widely distributed globally and are distinguished by distinctive geology, biogeochemistry, and ecosystems. The discovery of methane-seep sites in the Krishna-Godavari (K-G) basin has created exciting new opportunities for methane-seep research in the Bay of Bengal. In this study, we document the occurrence of authigenic carbonates, including micro-crystalline aragonite crust (arg-crusts) admixed with chemosynthetic shells and high-magnesium carbonate tubular structures (HMC-tube), from the methane-seep site SSD-045/4 in the K-G basin. The δ13C values of HMC-tubes (−54.5 to −46.2‰) and arg-crusts (−57.6 to −34.8‰) indicate biogenic methane as the likely carbon source. Enhanced porewater alkalinity driving carbonate precipitation may be attributed to microbial-mediated SO₄2−-AOM processes. Additionally, δ13C values (−35.2 ± 8‰) of the residual organic matter within the carbonates suggest a contribution of methanotrophic bacterial biomass. The δ18Ocarb values of HMC and aragonite indicate methane hydrate degassing and crystallization pathways, respectively. Pelloid-filled burrows suggest the reworking of shallow HMC deposit by burrowing organisms, whereas the polyphase cementations (aragonite and HMC) within burrows indicate early and burial diagenetic pathways. The wide range in ΣLREE/ΣHREE ratios and Ceanom values in arg-crusts reflect micro-spatial variations in redox conditions, likely due to cementation occurring in both open and closed diagenetic systems. In contrast, more constrained Ceanom values and ΣLREE/ΣHREE ratios in HMC tubes suggest persistent sulfidic conditions. Overall, these findings provide insights into the pathways of carbonate formation at the K-G basin methane-seep site, highlighting the complex interplay of microbial processes, fluid dynamics, and diagenetic alterations.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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