TY - JOUR
T1 - Sulfur Implantation into Water Ice with Propane
T2 - Implications for Organic Chemistry on the Surface of Europa
AU - Bouquet, Alexis
AU - da Costa, Cíntia Aparecida Pires
AU - Boduch, Philippe
AU - Rothard, Hermann
AU - Domaracka, Alicja
AU - Danger, Grégoire
AU - Schmitz, Isabelle
AU - Afonso, Carlos
AU - Schmitt-Kopplin, Philippe
AU - Hue, Vincent
AU - Nordheim, Tom A.
AU - Ruf, Alexander
AU - Duvernay, Fabrice
AU - Napoleoni, Maryse
AU - Khawaja, Nozair
AU - Postberg, Frank
AU - Javelle, Thomas
AU - Mousis, Olivier
AU - Tenelanda Osorio, Laura Isabel
N1 - Publisher Copyright:
© 2024. The Author(s). Published by the American Astronomical Society.
PY - 2024/4/1
Y1 - 2024/4/1
N2 - We performed experiments of implantation of energetic sulfur ions (105 keV) into 2:1 water:propane ices at 80 K and analyzed the resulting refractory organic matter with ultrahigh-resolution mass spectrometry. Our goal was to characterize the organic matter processed in the surface conditions of Europa, where it would receive a heavy flux of energetic particles, including sulfur ions, and determine whether organosulfurs could be formed in these conditions, using the simplest alkane that can exist in solid form on Europa’s surface. We find that the produced organic matter contains a large variety of both aliphatic and aromatic compounds (several thousand unique formulae), including polycyclic aromatic hydrocarbons (PAHs), with masses up to 900 amu. A large number of aromatic hydrocarbons is found along with oxygenated, mostly aliphatic, compounds. Organosulfurs are found in both CHS and CHOS form, demonstrating they can be formed from any organic compound through sulfur implantation. These organosulfurs’ properties (aromaticity, mass) appear similar to the rest of the organic matter, albeit their low quantity does not allow for a thorough comparison. Our results have implications for the type of refractory organic matter that could be observed by the JUICE and Europa Clipper space missions and how the surface of Europa could generate complex organics, including PAHs and organosulfurs, that could then enrich the subsurface ocean. In particular, they indicate that a large diversity of organic matter, including organosulfurs, can be formed from simple precursors in a geologically short time frame under the ion flux that reaches Europa.
AB - We performed experiments of implantation of energetic sulfur ions (105 keV) into 2:1 water:propane ices at 80 K and analyzed the resulting refractory organic matter with ultrahigh-resolution mass spectrometry. Our goal was to characterize the organic matter processed in the surface conditions of Europa, where it would receive a heavy flux of energetic particles, including sulfur ions, and determine whether organosulfurs could be formed in these conditions, using the simplest alkane that can exist in solid form on Europa’s surface. We find that the produced organic matter contains a large variety of both aliphatic and aromatic compounds (several thousand unique formulae), including polycyclic aromatic hydrocarbons (PAHs), with masses up to 900 amu. A large number of aromatic hydrocarbons is found along with oxygenated, mostly aliphatic, compounds. Organosulfurs are found in both CHS and CHOS form, demonstrating they can be formed from any organic compound through sulfur implantation. These organosulfurs’ properties (aromaticity, mass) appear similar to the rest of the organic matter, albeit their low quantity does not allow for a thorough comparison. Our results have implications for the type of refractory organic matter that could be observed by the JUICE and Europa Clipper space missions and how the surface of Europa could generate complex organics, including PAHs and organosulfurs, that could then enrich the subsurface ocean. In particular, they indicate that a large diversity of organic matter, including organosulfurs, can be formed from simple precursors in a geologically short time frame under the ion flux that reaches Europa.
UR - http://www.scopus.com/inward/record.url?scp=85191331945&partnerID=8YFLogxK
U2 - 10.3847/PSJ/ad3204
DO - 10.3847/PSJ/ad3204
M3 - Article
AN - SCOPUS:85191331945
SN - 2632-3338
VL - 5
JO - Planetary Science Journal
JF - Planetary Science Journal
IS - 4
M1 - 102
ER -