Atmospheric energy for subsurface life on Mars?
The location and density of biologically useful energy sources on Mars will limit the biomass, spatial distribution, and organism size of any biota. Subsurface Martian organisms could be supplied with a large energy flux from the oxidation of photochemically produced atmospheric H(2) and CO diffusin...
I tiakina i:
| I whakaputaina i: | Proc Natl Acad Sci U S A |
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| Ngā kaituhi matua: | , , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
National Academy of Sciences
2000
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| Ngā marau: | |
| Urunga tuihono: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC26444/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/10660689/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.030538097 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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