Your browser doesn't support javascript.
loading
Microbial growth in actual martian regolith in the form of Mars meteorite EETA79001.
Naz, Neveda; Harandi, Bijan F; Newmark, Jacob; Kounaves, Samuel P.
Afiliação
  • Naz N; Department of Chemistry, Tufts University, Medford, MA 02155 USA.
  • Harandi BF; Department of Chemistry, Tufts University, Medford, MA 02155 USA.
  • Newmark J; Department of Chemistry, Tufts University, Medford, MA 02155 USA.
  • Kounaves SP; Department of Chemistry, Tufts University, Medford, MA 02155 USA.
Commun Earth Environ ; 4(1): 381, 2023.
Article em En | MEDLINE | ID: mdl-38665180
ABSTRACT
Studies to understand the growth of organisms on Mars are hampered by the use of simulants to duplicate martian mineralogy and chemistry. Even though such materials are improving, no terrestrial simulant can replace a real martian sample. Here we report the use of actual martian regolith, in the form of Mars meteorite EETA79001 sawdust, to demonstrate its ability to support the growth of four microorganisms, E. coli. Eucapsis sp., Chr20-20201027-1, and P. halocryophilus, for up to 23 days under terrestrial conditions using regolithwater ratios from 41 to 110. If the EETA79001 sawdust is widely representative of regolith on the martian surface, our results imply that microbial life under appropriate conditions could have been present on Mars in the past and/or today in the subsurface, and that the regolith does not contain any bactericidal agents. The results of our study have implications not only for putative martian microbial life but also for building bio-sustainable human habitats on Mars.
Palavras-chave

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article