Published November 20, 2020 | Version v1
Journal article Open

Oceanic and atmospheric methane cycling in the cGENIE Earth system model – release v0.9.14

  • 1. Georgia Institute of Technology
  • 2. University of Chicago
  • 3. University of California, Riverside
  • 4. University of Bremen

Description

The methane (CH4) cycle is a key component of the Earth system that links planetary climate, biological metabolism, and the global biogeochemical cycles of carbon, oxygen, sulfur, and hydrogen. However, currently lacking is a numerical model capable of simulating a diversity of environments in the ocean, where CH4 can be produced and destroyed, and with the flexibility to be able to explore not only relatively recent perturbations to Earth's CH4 cycle but also to probe CH4 cycling and associated climate impacts under the very low-O2 conditions characteristic of most of Earth's history and likely widespread on other Earth-like planets. Here, we present a refinement and expansion of the ocean–atmosphere CH4 cycle in the intermediate-complexity Earth system model cGENIE, including parameterized atmospheric O2–O3–CH4 photochemistry and schemes for microbial methanogenesis, aerobic methanotrophy, and anaerobic oxidation of methane (AOM). We describe the model framework, compare model parameterizations against modern observations, and illustrate the flexibility of the model through a series of example simulations. Though we make no attempt to rigorously tune default model parameters, we find that simulated atmospheric CH4 levels and marine dissolved CH4 distributions are generally in good agreement with empirical constraints for the modern and recent Earth. Finally, we illustrate the model's utility in understanding the time-dependent behavior of the CH4 cycle resulting from transient carbon injection into the atmosphere, and we present model ensembles that examine the effects of atmospheric pO2, oceanic dissolved $SO_4^{2-}$ and the thermodynamics of microbial metabolism on steady-state atmospheric CH4 abundance. Future model developments will address the sources and sinks of CH4 associated with the terrestrial biosphere and marine CH4 gas hydrates, both of which will be essential for comprehensive treatment of Earth's CH4 cycle during geologically recent time periods.

Data availability

The rate data used to construct Fig. 2 are also included in the Supplement and as an accessory dataset with the DOI https://doi.org/10.5281/zenodo.4081700 (Reinhard, 2020).

Files

gmd-13-5687-2020.pdf

Files (4.0 MB)

Name Size Download all
Supplement
md5:1a72bace9c3974bcd2eba206a260d37c
94.8 kB Preview Download
Article
md5:5bb85b271981debde35645ff816a132e
3.9 MB Preview Download

Additional details

Identifiers

DOI
10.5194/gmd-13-5687-2020
Other
oai:uchicago.tind.io:13991

Funding

NASA Astrobiology Institute
CAN7
NASA Exobiology Program
18-EXO18-0005

UChicago Information

Division(s)
Physical Sciences Division
Department(s)
Geophysical Sciences