scholarly journals Mud volcano gas hydrates in the Caspian Sea

1994 ◽  
Vol 41 ◽  
pp. 95-100
Author(s):  
G. D. Ginsburg ◽  
V. A. x Soloviev

Two gas hydrate accumulations associated with mud volcano craters were investigated by means of sparker survey, bottom water and sediment sampling using gravity corer and subsequent chemical and isotopic studies of gas, bottom and porewater and carbonate inclusions. Hydrate contents in sediments were up to 35% per volume. Sometimes hydrates were encountered immediately on the seabed. Correlations have been established between hydrate contents, water contents (after dissociation of hydrates), chlorinity and the oxygen and hydrogen isotope composition of the pore water. The hydrate water is enriched with respect to deuterium. Liquid water in sediments contains higher 180 as result of isotopic exchange with carbonates. Hydrates are thought to have formed from the mud volcano brines (from their water and from dissolved light hydrocarbons which are thermogenic in origin). Each accumulation has its own deep source. The developed approach presents a thorough study of the hydrate and water contents in sediments along with the water composition.

2021 ◽  
Author(s):  
Sen Hu ◽  
Huicun He ◽  
Jianglong Ji ◽  
Yangting Lin ◽  
Hejiu Hui ◽  
...  

Abstract The distribution of water in the Moon’s interior carries key implications for the origin of the Moon1, the crystallisation of the lunar magma ocean2, and the duration of lunar volcanism2. The Chang’E-5 (CE5) mission returned the youngest mare basalt samples, dated at ca. 2.0 billion years ago3, from the northwestern Procellarum KREEP Terrane (PKT), providing a probe into the spatio-temporal evolution of lunar water. Here we report the water abundance and hydrogen isotope composition of apatite and ilmenite-hosted melt inclusions from CE5 basalts, from which we derived a maximum water abundance of 370 ± 30 μg.g-1 and a δD value (-330 ± 160‰) for their parent magma. During eruption, hydrogen degassing led to an increase in the D/H ratio of the residual melts up to δD values of 300-900‰. Accounting for low degrees of mantle partial melting followed by extensive magma fractional crystallisation4, we estimate a maximum mantle water abundance of 2-6 μg.g-1, which are too low for water contents alone to account for generating the Moon’s youngest basalts. Such modest water abundances for the lunar mantle are at the lower end of those estimated from mare basalts that erupted from ca. 4.0-2.8 Ga5, 6, suggesting the mantle source of CE5 basalts dried up by ca. 2.0 Ga through previous melt extraction from the PKT mantle during prolonged volcanic activity.


2021 ◽  
Vol 62 (4) ◽  
pp. 415-426
Author(s):  
E.I. Lastochkin ◽  
G.S. Ripp ◽  
D.S. Tsydenova ◽  
V.F. Posokhov ◽  
A.E. Murzintseva

Abstract —We consider the isotope-geochemical features of epithermal fluorite deposits in Transbaikalia, including the REE compositions, Sr isotope ratios, Sm–Nd systems, and isotope compositions of oxygen, carbon, hydrogen, and sulfur. The 87Sr/86Sr ratios in fluorites are within 0.706–0.708, and the εNd values are negative. Oxygen in quartz, the main mineral of the deposits, has a light isotope composition (δ18O = –3.4 to +2.6‰), and the calculated isotope composition of oxygen in the fluid in equilibrium with quartz (δ18O = –9 to –16‰) indicates the presence of meteoric water. The latter is confirmed by analysis of the isotope compositions of oxygen and hydrogen in gas–liquid inclusions in fluorites from three deposits. These isotope compositions are due to recycling caused by the impact of shallow basic plutons. The isotope composition of sulfur indicates its deep source. During ascent, sulfur became enriched in its light isotope (δ34S = –1.8 to –7.7‰). We assess the association of fluorite ores with basaltoids widespread in the study area. The isotope and geochemical parameters suggest their spatial proximity. Probably, the basaltoids were responsible for the recycling of meteoric water. It is shown that the epithermal fluorite deposits formed by the same mechanism as fissure–vein thermal waters in western Transbaikalia.


2021 ◽  
Author(s):  
Meisha Holloway-Philips ◽  
Jochem Baan ◽  
Daniel Nelson ◽  
Guillaume Tcherkez ◽  
Ansgar Kahmen

<p>The hydrogen isotope composition (δ<sup>2</sup>H) of cellulose has been used to assess ecohydrological processes and carries metabolic information, adding new understanding to how plants respond to environmental change. However, experimental approaches to isolate drivers of δ<sup>2</sup>H variation is limited to the Yakir & DeNiro model (1990), which is difficult to implement and largely unvalidated. Notably, the two biosynthetic fractionation factors in the model, associated with photosynthetic (ε<sub>A</sub>) and post-photosynthetic (ε<sub>H</sub>) processes are currently accepted as constants, and the third parameter – the extent to which organic molecules exchange hydrogen (f<sub>H</sub>) with local water – is usually tuned in order to resolve the difference between modelled and observed cellulose δ<sup>2</sup>H values. Thus, by virtue, the metabolically interpretable parameter is only f<sub>H</sub>, whilst from theory, metabolic flux rates will also impact on the apparent fractionations. To overcome part of this limitation, we measured the δ<sup>2</sup>H of extracted leaf sucrose from fully-expanded leaves of seven species and a phosphoglucomutase ‘starchless’ mutant of tobacco to estimate the isotopic offset between sucrose and leaf water (ε<sub>sucrose</sub>). Sucrose δ<sup>2</sup>H explained ~60% of the δ<sup>2</sup>H variation observed in cellulose. In general, ε<sub>sucrose</sub> was higher (range: -203‰ to -114‰; mean: -151 ± 21‰) than the currently accepted value of -171‰ (ε<sub>A</sub>) reflecting <sup>2</sup>H-enrichment downstream of triose-phosphate export from the chloroplast, with statistical differences in ε<sub>sucrose</sub> observed between species estimates. The remaining δ<sup>2</sup>H variation in cellulose was explained by species differences in f<sub>H </sub>(estimated by assuming ε<sub>H </sub>= +158‰). We also tested possible links between model parameters and plant metabolism. ε<sub>sucrose</sub> was positively related to dark respiration (R<sup>2</sup>=0.27) suggesting an important branch point influencing sugar δ<sup>2</sup>H. In addition, f<sub>H</sub> was positively related to the turnover time (τ) of water-soluble carbohydrates (R<sup>2</sup>=0.38), but only when estimated using fixed ε<sub>A </sub>= -171‰. To decipher and isolate the “metabolic” information contained within δ<sup>2</sup>H values of cellulose it will be important to assess δ<sup>2</sup>H values of non-structural carbohydrates so that hydrogen isotope fractionation during sugar metabolism can be better understood. This study provides the first attempt at such measurements showing species differences in both source and sink processes are important in understanding δ<sup>2</sup>H variation of cellulose.</p>


2014 ◽  
Vol 62 (20) ◽  
pp. 4493-4501 ◽  
Author(s):  
Luanzi Sun ◽  
Karl Auerswald ◽  
Rudi Schäufele ◽  
Hans Schnyder

1977 ◽  
Vol 60 (3) ◽  
pp. 311-315 ◽  
Author(s):  
Yoshimasu Kuroda ◽  
Tetsuro Suzuoki ◽  
Sadao Matsuo

1998 ◽  
Vol 145 (3-4) ◽  
pp. 249-261 ◽  
Author(s):  
Christophe Lécuyer ◽  
Philippe Gillet ◽  
François Robert

2008 ◽  
Vol 247 (1-2) ◽  
pp. 266-281 ◽  
Author(s):  
Sophie Verheyden ◽  
Dominique Genty ◽  
Olivier Cattani ◽  
Martin R. van Breukelen

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