{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,9,22]],"date-time":"2026-09-22T18:13:46Z","timestamp":1790100826422,"version":"4.0.1"},"reference-count":75,"publisher":"American Association for the Advancement of Science (AAAS)","issue":"32","content-domain":{"domain":["www.science.org"],"crossmark-restriction":true},"short-container-title":["Sci. Adv."],"published-print":{"date-parts":[[2025,8,8]]},"abstract":"<jats:p>\n                    Venus diverged from Earth\u2019s evolutionary path through the development of a carbon dioxide (CO\n                    <jats:sub>2<\/jats:sub>\n                    )\u2013dominated atmosphere, although studies dispute whether this atmosphere arose shortly after accretion or after a protracted period of surface habitability. Widespread volcanic features suggest that volcanic outgassing may have played a pivotal role in the transformation of Venus. However, the formation of volcanic units on Venus by basaltic lavas can only outgas a minor fraction of the CO\n                    <jats:sub>2<\/jats:sub>\n                    in the current atmosphere. Here, we model the erosion of long, meandering channels on Venus called canali and show that carbonatite lavas have the unique properties required to erode the canali. Our results suggest that eruption of these carbonatites may have delivered a total mass of CO\n                    <jats:sub>2<\/jats:sub>\n                    comparable to that of the modern atmosphere, resolving challenges to the formation of Venus\u2019 atmosphere within the recent past and suggesting that exoplanets in the \u201cVenus zone\u201d may exhibit the potential for prolonged habitability.\n                  <\/jats:p>","DOI":"10.1126\/sciadv.adw1621","type":"journal-article","created":{"date-parts":[[2025,8,6]],"date-time":"2025-08-06T17:58:27Z","timestamp":1754503107000},"update-policy":"https:\/\/doi.org\/10.34133\/aaas_crossmark","source":"Crossref","is-referenced-by-count":7,"title":["The importance of carbonatite lavas in outgassing Venus\u2019 modern-day atmosphere"],"prefix":"10.1126","volume":"11","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-7113-8782","authenticated-orcid":true,"given":"Allyson R.","family":"Trussell","sequence":"first","affiliation":[{"name":"School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1180-996X","authenticated-orcid":true,"given":"Joseph G.","family":"O\u2019Rourke","sequence":"additional","affiliation":[{"name":"School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-7930-9347","authenticated-orcid":true,"given":"David A.","family":"Williams","sequence":"additional","affiliation":[{"name":"School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-4410-3031","authenticated-orcid":true,"given":"Ian T. W.","family":"Flynn","sequence":"additional","affiliation":[{"name":"Department of Geology and Environmental Science, University of Pittsburgh, Pittsburgh, PA, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-4585-6438","authenticated-orcid":true,"given":"Benjamin A.","family":"Black","sequence":"additional","affiliation":[{"name":"Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1669-4989","authenticated-orcid":true,"given":"Madison E.","family":"Borrelli","sequence":"additional","affiliation":[{"name":"School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"221","reference":[{"key":"e_1_3_2_2_2","doi-asserted-by":"publisher","DOI":"10.1007\/s11214-023-00956-0"},{"key":"e_1_3_2_3_2","doi-asserted-by":"publisher","DOI":"10.1016\/S0012-821X(00)00195-3"},{"key":"e_1_3_2_4_2","doi-asserted-by":"publisher","DOI":"10.1029\/2019JE006276"},{"key":"e_1_3_2_5_2","doi-asserted-by":"publisher","DOI":"10.1007\/s11214-023-00966-y"},{"key":"e_1_3_2_6_2","doi-asserted-by":"publisher","DOI":"10.1029\/94JE00388"},{"key":"e_1_3_2_7_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.icarus.2011.03.010"},{"key":"e_1_3_2_8_2","doi-asserted-by":"publisher","DOI":"10.3847\/PSJ\/ac6033"},{"key":"e_1_3_2_9_2","unstructured":"J. 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