Radiolytic Production, Trapping, and Desorption of H2 at Elevated Temperatures in Amorphous and Crystalline Astrophysical and Planetary H2O Ice Analogs
Rahul K. Kushwaha, Murthy S. Gudipati, Bryana L. Henderson
{"title":"Radiolytic Production, Trapping, and Desorption of H2 at Elevated Temperatures in Amorphous and Crystalline Astrophysical and Planetary H2O Ice Analogs","authors":"Rahul K. Kushwaha, Murthy S. Gudipati, Bryana L. Henderson","doi":"10.1021/acsearthspacechem.6c00205","DOIUrl":null,"url":null,"abstract":"<p>We have conducted a comprehensive study on trapping and\r\nsublimation\r\nof H<sub>2</sub> in H<sub>2</sub>O ice. The results demonstrate that\r\ncodeposited H<sub>2</sub>:H<sub>2</sub>O ices (1:5) at 7 K release\r\nH<sub>2</sub> in two temperature regions during temperature-programmed\r\ndesorption (TPD), at ∼25 K and ∼80 K, whereas H<sub>2</sub> produced in H<sub>2</sub>O ices via electron irradiation\r\nis released in three regions, at ∼25 K, ∼80 K, and ∼110\r\nK. The higher the electron energy, the greater the amount of H<sub>2</sub> trapped in and released from H<sub>2</sub>O ice at ∼110\r\nK. Following irradiation, the ∼80 K release of H<sub>2</sub> is observed in amorphous but not crystalline ice. To better understand\r\nthe trapping and release behavior of H<sub>2</sub> in H<sub>2</sub>O ice, we carried out systematic laboratory studies under different\r\nastrophysical and planetary conditions, as presented here, and compared\r\nthem with previous studies. The implications of our work will range\r\nfrom outgassing from cometary nuclei, protoplanetary disk ice chemistry,\r\nnongravitational acceleration of interstellar objects such as 1I/′Oumuamua,\r\nand outgassing of H<sub>2</sub> from irradiated icy bodies such as\r\nEuropa and Enceladus in the solar system. Our work also infers radiolytic\r\nproduction and storage of H<sub>2</sub> in the lunar permanently shadowed\r\nregions.</p>","PeriodicalId":15,"journal":{"name":"ACS Earth and Space Chemistry","volume":"10 9","pages":"2139–2150"},"PeriodicalIF":2.6000,"publicationDate":"2026-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"ACS Earth and Space Chemistry","FirstCategoryId":"92","ListUrlMain":"https://pubs.acs.org/doi/10.1021/acsearthspacechem.6c00205","RegionNum":3,"RegionCategory":"化学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/8/22 0:00:00","PubModel":"Epub","JCR":"Q2","JCRName":"CHEMISTRY, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
We have conducted a comprehensive study on trapping and
sublimation
of H2 in H2O ice. The results demonstrate that
codeposited H2:H2O ices (1:5) at 7 K release
H2 in two temperature regions during temperature-programmed
desorption (TPD), at ∼25 K and ∼80 K, whereas H2 produced in H2O ices via electron irradiation
is released in three regions, at ∼25 K, ∼80 K, and ∼110
K. The higher the electron energy, the greater the amount of H2 trapped in and released from H2O ice at ∼110
K. Following irradiation, the ∼80 K release of H2 is observed in amorphous but not crystalline ice. To better understand
the trapping and release behavior of H2 in H2O ice, we carried out systematic laboratory studies under different
astrophysical and planetary conditions, as presented here, and compared
them with previous studies. The implications of our work will range
from outgassing from cometary nuclei, protoplanetary disk ice chemistry,
nongravitational acceleration of interstellar objects such as 1I/′Oumuamua,
and outgassing of H2 from irradiated icy bodies such as
Europa and Enceladus in the solar system. Our work also infers radiolytic
production and storage of H2 in the lunar permanently shadowed
regions.
期刊介绍:
The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.