Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices

Oxygen-containing complex organic molecules are key precursors to biorelevant compounds fundamental for the origins of life. However, the untangling of their interstellar formation mechanisms has just scratched the surface, especially for oxygen-containing cyclic molecules. Here, we present the firs...

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Main Authors: Jia Wang, Chaojiang Zhang, Joshua H. Marks, Ralf I. Kaiser
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adc308
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author Jia Wang
Chaojiang Zhang
Joshua H. Marks
Ralf I. Kaiser
author_facet Jia Wang
Chaojiang Zhang
Joshua H. Marks
Ralf I. Kaiser
author_sort Jia Wang
collection DOAJ
description Oxygen-containing complex organic molecules are key precursors to biorelevant compounds fundamental for the origins of life. However, the untangling of their interstellar formation mechanisms has just scratched the surface, especially for oxygen-containing cyclic molecules. Here, we present the first laboratory simulation experiments featuring the formation of all three C _2 H _4 O isomers—ethylene oxide ( c –C _2 H _4 O), acetaldehyde (CH _3 CHO), and vinyl alcohol (CH _2 CHOH)—in low-temperature model interstellar ices composed of carbon monoxide (CO) and ethanol (C _2 H _5 OH). Ice mixtures were exposed to galactic cosmic-ray proxies with an irradiation dose equivalent to a cold molecular cloud aged (7 ± 2) × 10 ^5 yr. These biorelevant species were detected in the gas phase through isomer-selective photoionization reflectron time-of-flight mass spectrometry during temperature-programmed desorption. Isotopic labeling experiments reveal that ethylene oxide is produced from ethanol alone, providing the first experimental evidence to support the hypothesis that ethanol serves as a precursor to the prototype epoxide in interstellar ices. These findings reveal feasible pathways for the formation of all three C _2 H _4 O isomers in ethanol-rich interstellar ices, offering valuable constraints on astrochemical models for their formation. Our results suggest that ethanol is a critical precursor to C _2 H _4 O isomers in interstellar environments, representing a critical step toward unraveling the formation mechanisms of oxygen-containing cyclic molecules, aldehydes, and their enol tautomers from alcohols in interstellar ices.
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spelling doaj-art-fe7567480abb4dfa8b4cbe9c44f480c12025-08-20T03:11:32ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01984213810.3847/1538-4357/adc308Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog IcesJia Wang0https://orcid.org/0000-0002-3795-8699Chaojiang Zhang1https://orcid.org/0000-0003-3727-901XJoshua H. Marks2https://orcid.org/0000-0003-0492-2494Ralf I. Kaiser3https://orcid.org/0000-0002-7233-7206W. M. Keck Research Laboratory in Astrochemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USA ; ralfk@hawaii.edu; Department of Chemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USAW. M. Keck Research Laboratory in Astrochemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USA ; ralfk@hawaii.edu; Department of Chemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USAW. M. Keck Research Laboratory in Astrochemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USA ; ralfk@hawaii.edu; Department of Chemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USAW. M. Keck Research Laboratory in Astrochemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USA ; ralfk@hawaii.edu; Department of Chemistry, University of Hawaii at Manoa , Honolulu, HI 96822, USAOxygen-containing complex organic molecules are key precursors to biorelevant compounds fundamental for the origins of life. However, the untangling of their interstellar formation mechanisms has just scratched the surface, especially for oxygen-containing cyclic molecules. Here, we present the first laboratory simulation experiments featuring the formation of all three C _2 H _4 O isomers—ethylene oxide ( c –C _2 H _4 O), acetaldehyde (CH _3 CHO), and vinyl alcohol (CH _2 CHOH)—in low-temperature model interstellar ices composed of carbon monoxide (CO) and ethanol (C _2 H _5 OH). Ice mixtures were exposed to galactic cosmic-ray proxies with an irradiation dose equivalent to a cold molecular cloud aged (7 ± 2) × 10 ^5 yr. These biorelevant species were detected in the gas phase through isomer-selective photoionization reflectron time-of-flight mass spectrometry during temperature-programmed desorption. Isotopic labeling experiments reveal that ethylene oxide is produced from ethanol alone, providing the first experimental evidence to support the hypothesis that ethanol serves as a precursor to the prototype epoxide in interstellar ices. These findings reveal feasible pathways for the formation of all three C _2 H _4 O isomers in ethanol-rich interstellar ices, offering valuable constraints on astrochemical models for their formation. Our results suggest that ethanol is a critical precursor to C _2 H _4 O isomers in interstellar environments, representing a critical step toward unraveling the formation mechanisms of oxygen-containing cyclic molecules, aldehydes, and their enol tautomers from alcohols in interstellar ices.https://doi.org/10.3847/1538-4357/adc308Laboratory astrophysicsAstrochemistryMass spectrometryComplex organic moleculesInterstellar molecules
spellingShingle Jia Wang
Chaojiang Zhang
Joshua H. Marks
Ralf I. Kaiser
Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
The Astrophysical Journal
Laboratory astrophysics
Astrochemistry
Mass spectrometry
Complex organic molecules
Interstellar molecules
title Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
title_full Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
title_fullStr Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
title_full_unstemmed Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
title_short Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices
title_sort formation of all three c2h4o isomers ethylene oxide c c2h4o acetaldehyde ch3cho and vinyl alcohol ch2choh in ethanol containing interstellar analog ices
topic Laboratory astrophysics
Astrochemistry
Mass spectrometry
Complex organic molecules
Interstellar molecules
url https://doi.org/10.3847/1538-4357/adc308
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