Kinetics of methane clathrate formation and dissociation under Mars relevant conditions

Icarus ◽  
2012 ◽  
Vol 218 (1) ◽  
pp. 513-524 ◽  
Author(s):  
S.R. Gainey ◽  
M.E. Elwood Madden
2014 ◽  
Vol 50 (10) ◽  
pp. 1244-1246 ◽  
Author(s):  
Weixing Wang ◽  
Peiyu Zeng ◽  
Xiyi Long ◽  
Jierong Huang ◽  
Yao Liu ◽  
...  

Kinetics of methane clathrate formation can be significantly accelerated by ingredients in tea infusions with a capacity of up to 172 v/v.


Author(s):  
Zhaoqian Su ◽  
Saman Alavi ◽  
John A. Ripmeester ◽  
Gedaliah Wolosh ◽  
Cristiano L. Dias

Fuel ◽  
2010 ◽  
Vol 89 (2) ◽  
pp. 294-301 ◽  
Author(s):  
Sebastien Bergeron ◽  
Juan G. Beltrán ◽  
Phillip Servio

2020 ◽  
Vol 117 (40) ◽  
pp. 24701-24708
Author(s):  
Liwen Li ◽  
Jie Zhong ◽  
Youguo Yan ◽  
Jun Zhang ◽  
Jiafang Xu ◽  
...  

Methane clathrates are widespread on the ocean floor of the Earth. A better understanding of methane clathrate formation has important implications for natural-gas exploitation, storage, and transportation. A key step toward understanding clathrate formation is hydrate nucleation, which has been suggested to involve multiple evolution pathways. Herein, a unique nucleation/growth pathway for methane clathrate formation has been identified by analyzing the trajectories of large-scale molecular dynamics (MD) simulations. In particular, ternary water-ring aggregations (TWRAs) have been identified as fundamental structures for characterizing the nucleation pathway. Based on this nucleation pathway, the critical nucleus size and nucleation timescale can be quantitatively determined. Specifically, a methane hydration layer compression/shedding process is observed to be the critical step in (and driving) the nucleation/growth pathway, which is manifested through overlapping/compression of the surrounding hydration layers of the methane molecules, followed by detachment (shedding) of the hydration layer. As such, an effective way to control methane hydrate nucleation is to alter the hydration layer compression/shedding process during the course of nucleation.


2013 ◽  
Vol 117 (14) ◽  
pp. 7081-7085 ◽  
Author(s):  
Satoshi Takeya ◽  
Hiroshi Fujihisa ◽  
Yoshito Gotoh ◽  
Vladimir Istomin ◽  
Evgeny Chuvilin ◽  
...  

2020 ◽  
Author(s):  
Mikkel T. Hornum ◽  
Andrew J. Hodson ◽  
Søren Jessen ◽  
Victor Bense ◽  
Kim Senger

Abstract. In the high Arctic valley of Adventdalen, Svalbard, sub-permafrost groundwater feeds several pingo springs distributed along the valley axis. The driving mechanism for groundwater discharge and associated pingo formation is enigmatic because wet-based glaciers in the adjacent highlands and the presence of continuous permafrost seem to preclude recharge of the sub-permafrost groundwater system by either a sub-glacial source or a precipitation surplus. Since the pingo springs enable methane that has accumulated underneath the permafrost to escape directly to the atmosphere, our limited understanding of the groundwater system brings significant uncertainty to the understanding of how methane emissions will respond to changing climate. We address this problem with a new conceptual model for open-system pingo formation wherein pingo growth is sustained by sub-permafrost pressure effects during millennial scale basal permafrost aggradation. We test the viability of this mechanism for generating groundwater flow with decoupled heat (1D-transient) and groundwater (2D-steady-state) transport modelling experiments. Our results show that the pingos in lower Adventdalen easily conform to this conceptual model. Simulations suggest that the generally low-permeability hydrogeological units cause groundwater residence times that exceed the duration of the Holocene. The likelihood of such pre-Holocene groundwater ages is also supported by the hydrogeochemistry of the pingo springs, which demonstrate a sea-wards freshening of groundwater, potentially supplied by paleo-subglacial melting during the Weichselian. Such waters form a sub-permafrost fresh water wedge that progressively thins inland, where the duration of permafrost aggradation is longest. The mixing ratio of the underlying marine waters therefore increases in this direction because less unfrozen freshwater is available for mixing. Although this unusual hydraulic system is most likely governed by permafrost aggradation, the potential for additional pressurization is also explored. We conclude that methane production and methane clathrate formation may also affect hydraulic the pressure in sub-permafrost aquifers, but additional research is needed to fully establish their influence.


2016 ◽  
Vol 94 (11) ◽  
pp. 2160-2167 ◽  
Author(s):  
Asheesh Kumar ◽  
Omkar Singh Kushwaha ◽  
Pramoch Rangsunvigit ◽  
Praveen Linga ◽  
Rajnish Kumar

2012 ◽  
Vol 116 (22) ◽  
pp. 12172-12180 ◽  
Author(s):  
Tricia D. Shepherd ◽  
Matthew A. Koc ◽  
Valeria Molinero

2003 ◽  
Vol 81 (1-2) ◽  
pp. 503-518 ◽  
Author(s):  
A Klapproth ◽  
E Goreshnik ◽  
D Staykova ◽  
H Klein ◽  
W F Kuhs

An overview of recent structural work focusing on the gas hydrates of methane and carbon dioxide is given. Both the crystal structure and the microstructure are considered. We report on the pressure-dependent molecular structure of methane clathrate hydrate using laboratory-made hydrogenous and deuterated samples investigated by neutron and hard-X-ray synchrotron diffraction experiments. The isothermal compressibilities are determined for hydrogenated and deuterated CH4 hydrate, and isotopic differences between both compounds are established for the first time. The cage filling of carbon dioxide and methane hydrate is determined and compared with predictions from statistical thermodynamic theory. In the case of small cages in methane hydrate, experimental results and predictions do not agree. Field-emission scanning electron microscopy reveals the meso- to macro-porous nature of gas hydrates formed with an excess of free gas. Furthermore, in situ measurements of the formation kinetics of porous hydrates are reported in which differences between methane and carbon dioxide are established quantitatively and the transient existence of a type II carbon dioxide structure is found. PACS Nos.: 82.75-z, 61.10Nz, 61.12Ld, 68.37Hk


2015 ◽  
Vol 29 (4) ◽  
pp. 2277-2288 ◽  
Author(s):  
Xingang Li ◽  
Chao Chen ◽  
Yingnan Chen ◽  
Yonghong Li ◽  
Hong Li

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