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Rapid Formation of Clathrate Hydrate From Liquid Ethane and Water Ice on Titan

Abstract 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...

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Bibliografische Detailangaben
Hauptverfasser: T. H. Vu, M. Choukroun, C. Sotin, V. Muñoz‐Iglesias, H. E. Maynard‐Casely
Format: Artigo
Sprache:Inglês
Veröffentlicht: Wiley 2020-02-01
Schriftenreihe:Geophysical Research Letters
Online-Zugang:https://doi.org/10.1029/2019GL086265
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