Japan Geoscience Union Meeting 2021

Presentation information

[E] Oral

M (Multidisciplinary and Interdisciplinary) » M-IS Intersection

[M-IS02] Astrobiology

Thu. Jun 3, 2021 3:30 PM - 5:00 PM Ch.26 (Zoom Room 26)

convener:Hikaru Yabuta(Hiroshima University, Department of Earth and Planetary Systems Science), Seiji Sugita(Department of Earth and Planetary Science, Graduate School of Science Sciece, The University of Tokyo), Misato Fukagawa(National Astronomical Observatory of Japan), Fujishima Kosuke(Tokyo Institute of Technology, Earth-Life Science Institute), Chairperson:Fujishima Kosuke(Tokyo Institute of Technology, Earth-Life Science Institute), Misato Fukagawa(National Astronomical Observatory of Japan), Seiji Sugita(Department of Earth and Planetary Science, Graduate School of Science Sciece, The University of Tokyo), Hikaru Yabuta(Hiroshima University, Department of Earth and Planetary Systems Science)

4:30 PM - 4:45 PM

[MIS02-09] A mechanism for non-linear amplification of methane flux in the early Earth system with primitive biosphere

*Aika Akahori1, Yasuto Watanabe1, Eiichi Tajika1 (1.Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo)


Keywords:Archean, Atmospheric photochemical model, Marine microbial ecosystem, Faint young Sun paradox, Earth-like exoplanet

Geological records indicate that the climate of the Archean Earth was warm or even warmer than the modern Earth. On the other hand, the standard evolution model of the Sun suggests that early solar luminosity was 30~20% dimmer than the present value. The atmosphere containing high levels of greenhouse gases would be a key to explain the paradox. Methane (CH4) produced by methanogens had probably played an important role in the Archean Earth, in addition to carbon dioxide (CO2). Ozaki et al. (2018) developed a coupled atmosphere-ocean ecosystem model, and evaluated CH4 concentrations in the Archean atmosphere for two cases; one assumed ecosystem based on hydrogen (H2)-using anoxygenic photoautotrophs, and the other assumed ecosystem based on H2-using and iron (Fe)-using anoxygenic photoautotrophs, with carbon monoxide (CO)-consuming acetogens and methanogens. They found that the CH4 flux increases non-linearly in the latter case against volcanic H2 outgassing flux, which can explain the high CH4 levels in the atmosphere of the Archean Earth. The mechanism of non-linear amplification of CH4 flux, however, remains unclear.
Here, we investigate the mechanism for non-linear amplification of CH4 flux by detailed analysis with a coupled model of atmospheric photochemistry and marine ecosystem. We found that the difference between the two cases is derived from difference in redox balance at the same outgassing flux of H2. A net flux of reducing power increases with activity of Fe-using anoxygenic photoautotrophs. Two positive feedbacks for the production of H2 and CO, strongly impact on the CH4 flux and concentrations. Biogenic CH4 is converted back to H2 and CO by photolysis in the atmosphere, which are recycled by marine microbial ecosystem, forming organic matters followed by decomposition to produce CH4 again. That is, increase of H2 and CO concentrations owing to photolysis of CH4 in the atmosphere triggers positive feedback of CH4 flux. Increase of H2 concentration increases linearly, while CO concentration increases non-linearly with an increase in the CH4 flux. This result indicates that positive feedback with CO should contribute to amplification for CH4 flux more stronger than the positive feedback with H2.
We will also discuss on application of this model to Earth-like exoplanets orbiting around stars with different masses and spectral types.