GSTDTAP  > 气候变化
DOI10.1029/2019GL086265
Rapid Formation of Clathrate Hydrate From Liquid Ethane and Water Ice on Titan
Vu, T. H.1; Choukroun, M.1; Sotin, C.1; Munoz-Iglesias, V2; Maynard-Casely, H. E.3
2020-02-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2020
卷号47期号:4
文章类型Article
语种英语
国家USA; Spain; Australia
英文摘要

Liquid ethane is present in the lakes and seas observed on Titan's surface by the Cassini-Huygens mission. While interaction between liquid hydrocarbons and water ice is expected to result in the formation of clathrate hydrates, such reaction (and its kinetics) has not yet been demonstrated for cryogenic liquids under relevant planetary conditions. In this paper, we report the first experimental evidence for rapid formation of clathrates upon direct contact of liquid ethane with water ice at 1 bar using micro-Raman spectroscopy. Kinetics experiments conducted in the temperature range 150-173 K yield an activation energy of 14.8 +/- 2.2 kJ/mol, which is suggestive of a diffusion-controlled mechanism for clathrate formation. This implies that a clathrate reservoir can form within seasonal time scales on Titan if liquid ethane comes into contact with a pre-existing icy bedrock, which may hold important implications for the structure and dynamics of Titan's crust and its global evolution.


Plain Language Summary Saturn's moon Titan has a dense atmosphere and liquid lakes (of methane and ethane) on its surface. These organic compounds are the main constituents of natural gas on Earth. Water is completely frozen and comprises most of Titan's bedrock materials. Under the right conditions, it is common for water ice to form new solids that trap natural gas in their structures, called clathrate hydrates. On Earth, clathrate hydrates are often found in the permafrost and deep ocean. However, Titan is so much colder that these natural gases exist as liquids. We do not yet know if clathrates can form under such conditions, and if so, how quickly. In this study, we prepared small grains of water ice, bathed them in liquid ethane, and monitored the rate at which clathrate hydrates appear. Our data confirm that clathrates would indeed form on Titan from an ethane lake or rain event onto water ice, and they would do so very quickly (in just a few Earth years). This suggests that clathrate hydrates can be an important material on Titan that may be encountered by future missions there.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000529120100016
WOS关键词THERMAL-CONDUCTIVITY ; METHANE ; KINETICS ; EQUILIBRIUM ; SYSTEM ; HEAT
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/279647
专题气候变化
作者单位1.CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA;
2.Ctr Astrobiol CSIC INTA, Torrejon De Ardoz, Spain;
3.Australian Nucl Sci & Technol Org, Lucas Heights, NSW, Australia
推荐引用方式
GB/T 7714
Vu, T. H.,Choukroun, M.,Sotin, C.,et al. Rapid Formation of Clathrate Hydrate From Liquid Ethane and Water Ice on Titan[J]. GEOPHYSICAL RESEARCH LETTERS,2020,47(4).
APA Vu, T. H.,Choukroun, M.,Sotin, C.,Munoz-Iglesias, V,&Maynard-Casely, H. E..(2020).Rapid Formation of Clathrate Hydrate From Liquid Ethane and Water Ice on Titan.GEOPHYSICAL RESEARCH LETTERS,47(4).
MLA Vu, T. H.,et al."Rapid Formation of Clathrate Hydrate From Liquid Ethane and Water Ice on Titan".GEOPHYSICAL RESEARCH LETTERS 47.4(2020).
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