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Theoretical Insights into Gas Migration Within Ice on Earth and Icy Celestial Bodies

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dc.contributor.authorYi Yoo Soo-
dc.contributor.authorHan, Yeongcheol-
dc.date.accessioned2025-11-06T07:50:05Z-
dc.date.available2025-11-06T07:50:05Z-
dc.date.issued2024-
dc.identifier.urihttps://repository.kopri.re.kr/handle/201206/16357-
dc.description.abstractAtmospheric gases trapped in icy environments, such as Earth's polar regions and Jupiter's moon Europa, offer a unique opportunity to explore paleoclimate and astrogeological history. While previous studies have addressed the diffusive behaviors of these gases and their implications for paleoclimatological and geochronological reconstructions, the underlying mechanisms of gas migration in ice remain largely unexplored. Achieving an atomistic-level understanding of gas migration is therefore essential for improving our knowledge of the long-term behavior of gases in icy environments. In this study, we investigated the migration of noble gases encapsulated in isolated air bubbles within bulk ice using density functional theory calculations. We focused on both the dissolution at the gas-ice interface and the subsequent molecular diffusion through the ice lattice. Our results show that energy barriers for dissolution and molecular diffusion increase almost linearly with atomic size, leading to nonlinear, exponential-like decreases in solubility and diffusivity, due to their Arrhenius behavior in relation to the corresponding energy barriers. These energy barriers primarily arise from the structural distortions in the ice lattice, as it accommodates noble gas atoms. Additionally, our findings indicate that dissolution is energetically both more demanding and slower than molecular diffusion, making it the rate-limiting step in gas migration through ice. These findings provide valuable insights into gas migration and fractionation mechanisms in Earth's polar ice, highlighting the importance of incorporating atomic-level interactions into geochronological models. By deepening our fundamental understanding of gas mobility, this work not only advances methodologies for analyzing Earth's ice but also broadens our perspective on extraterrestrial icy environments, with potential implications for the search for life-supporting conditions beyond Earth.-
dc.languageEnglish-
dc.subject.classification해당사항없음-
dc.titleTheoretical Insights into Gas Migration Within Ice on Earth and Icy Celestial Bodies-
dc.title.alternative지구와 얼음이 있는 천체에서의 얼음 내 가스 이동에 관한 이론적 통찰-
dc.typeArticle-
dc.identifier.bibliographicCitationYi Yoo Soo, Han, Yeongcheol. 2024. "Theoretical Insights into Gas Migration Within Ice on Earth and Icy Celestial Bodies". <em>ACS EARTH AND SPACE CHEMISTRY</em>, 8(12): 2611-2620.-
dc.citation.titleACS EARTH AND SPACE CHEMISTRY-
dc.citation.volume8-
dc.citation.number12-
dc.identifier.doi10.1021/acsearthspacechem.4c00266-
dc.citation.startPage2611-
dc.citation.endPage2620-
dc.description.articleClassificationSCIE-
dc.description.jcrRateJCR 2022:33.333-
dc.subject.keywordAge dating-
dc.subject.keywordDensity functional theory-
dc.subject.keywordGas migration in ice-
dc.subject.keywordGeochronology-
dc.subject.keywordNoble gas-
dc.subject.keywordPaleoclimatology-
dc.identifier.localId2024-0228-
Appears in Collections  
2024-2024, 국제심부빙하시추 네트워크를 활용한 대기-빙상 상호작용의 자연적·인위적 특성 규명 (24-24) / 한영철 (PE24100)
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