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Identification of alteration mineral assemblages on Mars and potentially in ocean worlds such as Enceladus suggests the existence of extensive hydrothermal fluid\u2013igneous rock interactions of astrobiological interest in different planetary bodies. Here, we studied the terrestrial analog Cerro Caliente, a band of geothermal alterations located in the glaciovolcanic environment of Deception Island (Antarctica), with the aim of determining the mobility of major chemical elements (e.g., alkalis, phosphorus) and its implications in the habitability potential of such environments. We verified that the rock texture, particularly rich in volcanic glass, plays a major role in geochemical mobility, with permafrost delimiting the impact of hydrothermal activity by reducing the permeability of the lapilli tuff deposit. We studied the mineralogy and geochemistry of the alteration band by comparing borehole samples in different locations that represent different thermal regimes along the hydrothermal alteration band. The alteration products are characteristic of palagonitization processes, which favor the release of elements useful for life, such as phosphorus, although the basic alkalinity of the medium caused its precipitation in the form of tricalcium phosphate. In addition, lipid biomarker analyses were performed to assess the existence of possible potential ecological niches associated with these environments. On Mars, the circulation of low-temperature CO\n                    <jats:sub>2<\/jats:sub>\n                    -rich hydrothermal fluids through glass-bearing volcanic rocks results in a loss of silica content and a secondary mineral assemblage composed of palagonite, phyllosilicates, and zeolites, which establishes Cerro Caliente as a valid Mars analog for understanding such environments. In addition, our results support the hypothesis of a hydrothermal origin of phosphorous for the formation of Enceladus\u2019 phosphates recently detected in the plumes. We also determined that a fraction of the calcium in Cerro Caliente was sequestered as carbonates of biogenic origin, which produced a distinctive Raman signal that, together with the lipid content, would make it a relevant potential biosignature if similar findings were made in the search for life in such low-temperature hydrothermal environments. Key Words: Hydrothermal systems\u2014Palagonitization\u2014Phosphates\u2014Lipid biomarkers\u2014Mars\u2014Ocean worlds. Astrobiology 25, 777\u2013792.\n                  <\/jats:p>","DOI":"10.1177\/15311074251392901","type":"journal-article","created":{"date-parts":[[2025,11,6]],"date-time":"2025-11-06T16:50:53Z","timestamp":1762447853000},"page":"777-792","update-policy":"https:\/\/doi.org\/10.1177\/sage-journals-update-policy","source":"Crossref","is-referenced-by-count":1,"title":["Geochemical Mobility of Elements in Antarctic Environments Affected by CO\n                    <sub>2<\/sub>\n                    -Rich Hydrothermal Fluids: Astrobiological Implications"],"prefix":"10.1177","volume":"25","author":[{"given":"Ana","family":"de Dios-Cubillas","sequence":"first","affiliation":[{"name":"Centro de Astrobiolog\u00eda (CAB), CSIC-INTA, Madrid, Spain."},{"name":"Departamento de Biolog\u00eda, Geolog\u00eda, F\u00edsica y Qu\u00edmica Inorg\u00e1nica, Tecvolrisk Research Group. ESCET, Universidad Rey Juan Carlos, M\u00f3stoles, Madrid, Spain."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Olga","family":"Prieto-Ballesteros","sequence":"additional","affiliation":[{"name":"Centro de Astrobiolog\u00eda (CAB), CSIC-INTA, Madrid, Spain."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Daniel","family":"Carrizo","sequence":"additional","affiliation":[{"name":"Centro de Astrobiolog\u00eda (CAB), CSIC-INTA, Madrid, Spain."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Iv\u00e1n","family":"L\u00f3pez","sequence":"additional","affiliation":[{"name":"Departamento de Biolog\u00eda, Geolog\u00eda, F\u00edsica y Qu\u00edmica Inorg\u00e1nica, Tecvolrisk Research Group. 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