Growth of methanogens on a mars soil simulant

56Citations
Citations of this article
110Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Currently, the surface of Mars is probably too cold, too dry, and too oxidizing for life, as we know it, to exist. But the subsurface is another matter. Life forms that might exist below the surface could not obtain their energy from photosynthesis, but rather they would have to utilize chemical energy. Methanogens are one type of microorganism that might be able to survive below the surface of Mars. A potential habitat for existence of methanogens on Mars might be a geothermal source of hydrogen, possibly due to volcanic or hydrothermal activity, or the reaction of basalt and anaerobic water, carbon dioxide, which is abundant in the martian atmosphere, and of course, subsurface liquid water. We report here that certain methanogens can grow on a Mars soil simulant when supplied with carbon dioxide, molecular hydrogen, and varying amounts of water.

Cite

CITATION STYLE

APA

Kral, T. A., Bekkum, C. R., & McKay, C. P. (2004). Growth of methanogens on a mars soil simulant. Origins of Life and Evolution of the Biosphere, 34(6), 615–626. https://doi.org/10.1023/B:ORIG.0000043129.68196.5f

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free