Japan Geoscience Union Meeting 2021

Presentation information

[J] Poster

M (Multidisciplinary and Interdisciplinary) » M-IS Intersection

[M-IS14] Aqua planetology

Sat. Jun 5, 2021 5:15 PM - 6:30 PM Ch.22

convener:Yasuhito Sekine(Earth-Life Science Insitute, Tokyo Institute of Technology), Takazo Shibuya(Japan Agency for Marine-Earth Science and Technology), Hidenori Genda(Earth-Life Science Institute, Tokyo Institute of Technology), Keisuke Fukushi(Institute of Nature & Environmental Technology, Kanazawa University)

5:15 PM - 6:30 PM

[MIS14-P09] Prediction of the composition of the primordial ocean just after its formation

*Hisahiro Ueda1, Takazo Shibuya1 (1.JAMSTEC)

Keywords:primordial ocean composition, ocean formation, water-rock reactions, Hadean, experiment

Hadean is an enigmatic period in the Earth’s history when ocean formation and the emergence of life occurred. However, minimal geological evidence is left from this period. Regarding the ocean in the early Earth, previous research indicates that seawater had weak acidity (pH 4–7) because the carbon dioxide concentration in the atmosphere was high compared to that today (e.g., Walker, 1985; Grotzinger and Kasting, 1993; Macleod et al., 1994), or it was strongly acidic (pH 1–2) because a large amount of halogen substance in the high-temperature vapor atmosphere eventually dissolved into seawater (Maruyama et al., 2013). Previously, pH, CO2 concentrations, and other elements were considered (Morse and Mackenzie, 1988) but these estimations did not provide information about the quantitative chemical compositions of seawater. To understand the primordial ocean’s composition, we focused on the ocean’s formation processes from CO2- and HCl-bearing water vapor in the high-temperature atmosphere. When the temperature of the lower atmosphere fell below the critical point, high-temperature rain reached the ground surface. Then, hydrothermal reactions between the subcritical fluid and primordial crust started. Eventually, a liquid ocean emerged on the completely altered crust as the temperature decreased to approximately 25 °C until the ocean’s temperature stabilized. Here, we conducted two experiments and modeling simulating the reactions between hypothetical primordial crustal rock (basalt or komatiite). The results indicate that the primordial ocean was mildly acidic and rich in CO2, Mg, and Ca relative to Na, irrespective of the rock type, which is different from the modern equivalents. Therefore, unlike the present seawater, the primordial seawater could have been carbonic, bitter, and harsh rather than salty. The ocean’s composition started to evolve once plate tectonics began on Earth.