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The direction of such a synthesis is a result of the absorption of the filtering gas by condensate and the formation of hydrocarbons and native sulfur in the condensate. The spatial position of the abiogenic synthesis zones is controlled by isosurfaces of critical temperatures and partial saturation pressures for CO\n                    <jats:sub>2<\/jats:sub>\n                    and H\n                    <jats:sub>2<\/jats:sub>\n                    S. Abiogenic synthesis of hydrocarbons ensures the occurrence of prebiological states. Since the condensation of CO\n                    <jats:sub>2<\/jats:sub>\n                    and H\n                    <jats:sub>2<\/jats:sub>\n                    S is controlled by the physical properties of these substances, it is possible to assess the conditions for the emergence of prebiological states on other planets. Venus demonstrates an example of an \u201coverheated\u201d planet on which the occurrence of prebiological states is unlikely in the past and impossible at the present time. Mars shows us a hypothetical example of a possible migration of prebiological states and protolife arising on their basis into the depths of a celestial body. Jupiter demonstrates an example of the localization of hydrocarbon synthesis zones and prebiological states in the gas envelope of the planet.\n                  <\/jats:p>","DOI":"10.1089\/ast.2024.0042","type":"journal-article","created":{"date-parts":[[2025,2,19]],"date-time":"2025-02-19T10:34:37Z","timestamp":1739961277000},"page":"133-149","update-policy":"https:\/\/doi.org\/10.1177\/sage-journals-update-policy","source":"Crossref","is-referenced-by-count":0,"title":["CO\n                    <sub>2<\/sub>\n                    and H\n                    <sub>2<\/sub>\n                    S in Abiogenic Hydrocarbon Synthesis and the Emergence of Prebiological States"],"prefix":"10.1177","volume":"25","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-4306-8000","authenticated-orcid":false,"given":"Aleksandr","family":"Malyshev","sequence":"first","affiliation":[{"name":"Institute of Geology and Geochemistry of the Ural Branch of the RAS, Ekaterinburg, Russia."}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Lidiia","family":"Malysheva","sequence":"additional","affiliation":[{"name":"Institute of Geology and Geochemistry of the Ural Branch of the RAS, Ekaterinburg, Russia."}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"179","published-online":{"date-parts":[[2025,2,18]]},"reference":[{"issue":"1","key":"e_1_3_5_2_1","first-page":"14","article-title":"Density and seismic profiles of the martian crust in the event of an extra-low temperature gradient","volume":"32","author":"Babeiko A","year":"1998","unstructured":"Babeiko A, , Zharkov VN. 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