Formation of Polyoxymethylenes in Extraterrestrial Ice Analogs of Formaldehyde Exposed to Ionizing Radiation

Abstract Polyoxymethylenes (POMs) have long been hypothesized as key organics in comets, as their decomposition products could account for the possible extended cometary formaldehyde (H 2 CO) source. However, POMs (X–(CH 2 O) n –Y; n > 2) are hitherto unobserved in deep space, and their possible formation mechanisms have still remained elusive. Here, we report on the laboratory formation of formaldehyde oligomers (H–(CH 2 O) n –H; n = 2−4) within extraterrestrial ice analogs of formaldehyde exposed to energetic electrons simulating secondary electrons generated by galactic cosmic rays passing through ices. The potential identification of these short-chain-length POMs, such as methoxymethanol (CH 3 OCH 2 OH), (methoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OH), and (methoxymethoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OCH 2 OH), is accomplished by utilizing the synchrotron vacuum ultraviolet photoionization reflectron time-of-flight mass spectrometry (SVUV-PI-ReTOF-MS) technique coupled with the temperature-programmed desorption method. A radical-induced formaldehyde polymerization mechanism is proposed to address the formation of POMs, with the competition between chain propagation and chain termination determining the chain length of the polymers and availability of reactive hydrogen atoms. The electron impact ionization of POMs as well as accompanied fragmentation of their cations are analyzed via a quadrupole mass spectrometer, with mass peaks compared with those collected by the Positive Ion Cluster Composition Analyzer instrument on board the Giotto spacecraft in the inner coma of comet 1P/Halley, and by the Ptolemy instrument on the comet 67P/Churyumov–Gerasimenko. Our findings might support the proposal that (small) POMs exist on comets and nominate hitherto unobserved POMs such as (methoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OH) and (methoxymethoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OCH 2 OH) for future astronomical searches.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-11-14
DOI
https://doi.org/10.3847/1538-4357/ae0cb7
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

Formation of Polyoxymethylenes in Extraterrestrial Ice Analogs of Formaldehyde Exposed to Ionizing Radiation

Tao Yang, Jiuzhong Yang, Jinghui Lu, Qiang Gong et al.
The Astrophysical Journal
Astrophysics and Star Formation Studies
article

Formation of Polyoxymethylenes in Extraterrestrial Ice Analogs of Formaldehyde Exposed to Ionizing Radiation

Tao Yang, Jiuzhong Yang, Jinghui Lu, Qiang Gong, Yang Pan, Ralf I. Kaiser, Zhenrong Sun, Xia Bai
article en

Abstract

Abstract Polyoxymethylenes (POMs) have long been hypothesized as key organics in comets, as their decomposition products could account for the possible extended cometary formaldehyde (H 2 CO) source. However, POMs (X–(CH 2 O) n –Y; n > 2) are hitherto unobserved in deep space, and their possible formation mechanisms have still remained elusive. Here, we report on the laboratory formation of formaldehyde oligomers (H–(CH 2 O) n –H; n = 2−4) within extraterrestrial ice analogs of formaldehyde exposed to energetic electrons simulating secondary electrons generated by galactic cosmic rays passing through ices. The potential identification of these short-chain-length POMs, such as methoxymethanol (CH 3 OCH 2 OH), (methoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OH), and (methoxymethoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OCH 2 OH), is accomplished by utilizing the synchrotron vacuum ultraviolet photoionization reflectron time-of-flight mass spectrometry (SVUV-PI-ReTOF-MS) technique coupled with the temperature-programmed desorption method. A radical-induced formaldehyde polymerization mechanism is proposed to address the formation of POMs, with the competition between chain propagation and chain termination determining the chain length of the polymers and availability of reactive hydrogen atoms. The electron impact ionization of POMs as well as accompanied fragmentation of their cations are analyzed via a quadrupole mass spectrometer, with mass peaks compared with those collected by the Positive Ion Cluster Composition Analyzer instrument on board the Giotto spacecraft in the inner coma of comet 1P/Halley, and by the Ptolemy instrument on the comet 67P/Churyumov–Gerasimenko. Our findings might support the proposal that (small) POMs exist on comets and nominate hitherto unobserved POMs such as (methoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OH) and (methoxymethoxymethoxy)methanol (CH 3 OCH 2 OCH 2 OCH 2 OH) for future astronomical searches.

The Astrophysical JournalVol. 994(1)
University of Hawaiʻi at Mānoa (US), University of Science and Technology of China (CN), Shanxi University (CN), Chinese Academy of Sciences (CN), Xinjiang Astronomical Observatory (CN), National Synchrotron Radiation Laboratory (CN), East China Normal University (CN)
Openalex Percentile: Top 76%
Astrophysics and Star Formation Studies
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