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Crustal Hydration Primed Early Mars with Warm and Habitable Conditions

Title: Crustal Hydration Primed Early Mars with Warm and Habitable Conditions
Authors: Adams, Danica; Scheucher, Markus; HU, RENYU; Thomas, Trent; Scheller, Eva; Lillis, Rob; Smith, Kayla; Wordsworth, Robin; Ehlmann, Bethany; Rauer, Heike; Yung, Yuk
Publisher Information: Springer Science and Business Media LLC
Publication Year: 2023
Description: Geological evidence suggests that ancient Mars held substantial volumes of surface liquid water [1–2] , lost over time due to crustal hydration [17] and atmospheric escape [7] . Resolving the Mars Faint Young Sun Paradox, or explaining how the atmosphere was kept warmer early on despite a less luminous sun, has remained a challenge. Reduced greenhouse gases like H 2 in a CO 2 atmosphere are known to induce warming through collision induced absorption [13–14] , but H 2 is short-lived and no long-lasting source at early Mars has been identified yet. Here we show that crustal hydration would have supplied significant H 2 fluxes, which, built up in the atmosphere over 10 5 -10 7 years, could have facilitated a warm, wet climate through collision-induced absorption with CO 2 and N 2 . This would only occur during a few major events lasting ~ million years, while shorter events could not have warmed the climate. Our results are the first to explain how long-lasting warm climates could have persisted at early Mars. As CO 2 was lost and the atmosphere cooled, it transitioned to a CO-dominated state in the Hesperian era, leading to a colder, drier climate. We anticipate that sharp climate and redox state changes may have been triggered by geological or obliquity changes.
Document Type: other/unknown material
Language: unknown
DOI: 10.21203/rs.3.rs-3497495/v1
Availability: https://doi.org/10.21203/rs.3.rs-3497495/v1; https://www.researchsquare.com/article/rs-3497495/v1; https://www.researchsquare.com/article/rs-3497495/v1.html
Rights: https://creativecommons.org/licenses/by/4.0/
Accession Number: edsbas.5044B4EB
Database: BASE