Electron-induced CO2 and hydrocarbon sputtering of functionalized hydrocarbons in icy planetary analogs
Sankhabrata Chandra, Bryana L. Henderson, Murthy S. Gudipati

TL;DR
This study investigates how electron-induced sputtering of organic molecules in icy planetary analogs produces CO2, revealing that acid-functionalized organics generate significantly more CO2, especially at higher temperatures, impacting our understanding of Europa's surface chemistry.
Contribution
It provides new insights into how functional groups in organic molecules influence CO2 production during sputtering, highlighting the role of acid groups in volatile release on icy planetary surfaces.
Findings
Acid-functionalized organics produce over 10x more CO2 than non-functionalized molecules.
CO2 production increases with temperature, being highest at 100-120 K.
Carboxylic acid groups significantly enhance volatile ejection in sputtering processes.
Abstract
CO2 has been detected in both the tenuous exosphere and surface chaos regions of Europa, but it is still unclear whether this CO2 is generated in situ by radiolysis or whether it is directly delivered by the ocean. In this work, we study the radiolysis pathway, and explore the possibility that organics upwelled from the subsurface oceans could be contributing to this signature on the surface and in the exosphere. Specifically, we report here on the evolution of carbon-containing byproducts generated by electron-induced sputtering of organics with different functional groups -- hexanoic acid, hexanol, and hexane -- in water ice. We found that, upon electron irradiation in vacuum, the acid-functionalized molecules generated a factor of over 10x more CO2 than either the non-functionalized or alcohol-functionalized molecules, but that all three species produced CO2 to some extent. The…
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Taxonomy
TopicsMass Spectrometry Techniques and Applications · Nuclear Physics and Applications · Advanced Chemical Physics Studies
