Early Mars could have supported methane producing microbes much like Earth

Publicly released:
International
Image by Aynur Zakirov from Pixabay
Image by Aynur Zakirov from Pixabay

Early Mars could have been home to methane-producing microbes, much like early Earth was, according to computer simulations created by international researchers. The team analysed the interaction between the early environment on Mars and an ecosystem of microorganisms called methanogenic hydrogenotrophs, which gobble up hydrogen and produce methane. These microorganisms are considered to be some of the earliest forms of life on earth, and the author's simulations suggest the Martian crust was a viable place for this ecosystem, so long as it wasn't fully covered in ice. The team says the actions of these microbes would have triggered a feedback event with the climate on Mars, cooling it globally by up to more than 230°C and creating less habitable conditions closer to the surface. This would have forced the microbes to move progressively deeper within the planet’s crust, the scientists say.

Media release

From: Springer Nature

Early Mars was likely habitable for methane-producing microbes

The subsurface of early Mars was likely to have been habitable for microorganisms that feed on hydrogen and produce methane, according to a modelling study published in Nature Astronomy. The predicted biomass production may have been comparable to that of the early ocean of Earth and may have had a global cooling effect on Mars’s early climate.

The potential habitability of early Mars, more than 3.7 billion years ago, has been extensively debated. Evidence suggests that the red planet hosted — at least for part of its history — potentially favourable conditions for the development of life. The likelihood of such a scenario, however, has rarely been established quantitatively.

Boris Sauterey and colleagues model the interaction between the early environment on Mars and an ecosystem of methanogenic hydrogenotrophs — microorganisms that survive by consuming hydrogen and producing methane — which are considered to be among the earliest forms of life on Earth. The authors’ simulations predict that the Martian crust was a viable place for this ecosystem  — provided that the surface was not fully covered with ice  — and could have produced biomass similar to that of the early ocean of Earth. The team predicts that this ecosystem would have triggered a feedback event with the climate on Mars, cooling it globally by up to 40 degrees Kelvin and creating less habitable conditions closer to the surface. This would have forced the microbes to move progressively deeper within the planet’s crust.

Looking forward, the authors identify three sites; Hellas Planitia, Isidis Planitia and Jezero Crater, as the best places to look for signs of this early methanogenic life near the surface of Mars.

Journal/
conference:
Nature Astronomy
Research:Paper
Organisation/s: University of Arizona, USA
Funder: This work is supported by France Investissements d’Avenir programme (grant numbers ANR-10-LABX-54 MemoLife and ANR-10-IDEX-0001-02 PSL) through PSL IRIS OCAV and PSL–University of Arizona Mobility Program. R.F. acknowledges support from the US National Science Foundation, Dimensions of Biodiversity (DEB-1831493), Biology Integration Institute-Implementation (DBI-2022070), Growing Convergence in Research (OIA-2121155) and National Research Traineeship (DGE-2022055) programmes; and from the United States National Aeronautics and Space Administration, Interdisciplinary Consortium for Astrobiology Research program (award number 80NSSC21K059).
Media Contact/s
Contact details are only visible to registered journalists.