Grain size measurements of natural gas hydrates

被引:25
|
作者
Klapp, Stephan A. [1 ]
Hemes, Susanne [2 ]
Klein, Helmut [2 ]
Bohrmann, Gerhard [1 ]
MacDonald, Ian [3 ]
Kuhs, Werner F. [2 ]
机构
[1] Univ Bremen, Ctr Marine Environm Sci, MARUM, D-28334 Bremen, Germany
[2] Univ Gottingen, Geowissensch Zentrum, Abt Kristallog, D-37077 Gottingen, Germany
[3] Texas A&M Univ, Corpus Christi, TX 78412 USA
关键词
gas hydrates; grain sizes; crystallite size distribution; synchrotron radiation; Black Sea; Gulf of Mexico; Indian Ocean; METHANE CLATHRATE HYDRATE; NEUTRON-DIFFRACTION; CASCADIA MARGIN; CARBON-DIOXIDE; KINETICS; ICE; TEXTURE; GROWTH; MICROSTRUCTURE; PRECIPITATION;
D O I
10.1016/j.margeo.2010.03.007
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Methane hydrates are present in marine seep systems and occur within the gas hydrate stability zone. Very little is known about their crystallite sizes and size distributions because they are notoriously difficult to measure. Crystal size distributions are usually considered as one of the key petrophysical parameters because they influence mechanical properties and possible compositional changes, which may occur with changing environmental conditions. Variations in grain size are relevant for gas substitution in natural hydrates by replacing CH4 with CO2 for the purpose of carbon dioxide sequestration. Here we show that crystallite sizes of gas hydrates from some locations in the Indian Ocean, Gulf of Mexico and Black Sea are in the range of 200-400 mu m; larger values were obtained for deeper-buried samples from ODP Leg 204. The crystallite sizes show generally a log-normal distribution and appear to vary sometimes rapidly with location. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码:85 / 94
页数:10
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