scholarly journals A Low-Pressure, N2/CO2 Atmosphere Is Suitable for Cyanobacterium-Based Life-Support Systems on Mars

2021 ◽  
Vol 12 ◽  
Author(s):  
Cyprien Verseux ◽  
Christiane Heinicke ◽  
Tiago P. Ramalho ◽  
Jonathan Determann ◽  
Malte Duckhorn ◽  
...  

The leading space agencies aim for crewed missions to Mars in the coming decades. Among the associated challenges is the need to provide astronauts with life-support consumables and, for a Mars exploration program to be sustainable, most of those consumables should be generated on site. Research is being done to achieve this using cyanobacteria: fed from Mars's regolith and atmosphere, they would serve as a basis for biological life-support systems that rely on local materials. Efficiency will largely depend on cyanobacteria's behavior under artificial atmospheres: a compromise is needed between conditions that would be desirable from a purely engineering and logistical standpoint (by being close to conditions found on the Martian surface) and conditions that optimize cyanobacterial productivity. To help identify this compromise, we developed a low-pressure photobioreactor, dubbed Atmos, that can provide tightly regulated atmospheric conditions to nine cultivation chambers. We used it to study the effects of a 96% N2, 4% CO2 gas mixture at a total pressure of 100 hPa on Anabaena sp. PCC 7938. We showed that those atmospheric conditions (referred to as MDA-1) can support the vigorous autotrophic, diazotrophic growth of cyanobacteria. We found that MDA-1 did not prevent Anabaena sp. from using an analog of Martian regolith (MGS-1) as a nutrient source. Finally, we demonstrated that cyanobacterial biomass grown under MDA-1 could be used for feeding secondary consumers (here, the heterotrophic bacterium E. coli W). Taken as a whole, our results suggest that a mixture of gases extracted from the Martian atmosphere, brought to approximately one tenth of Earth's pressure at sea level, would be suitable for photobioreactor modules of cyanobacterium-based life-support systems. This finding could greatly enhance the viability of such systems on Mars.

2011 ◽  
Vol 37 (7) ◽  
pp. 784-789 ◽  
Author(s):  
V. N. Sychev ◽  
M. A. Levinskikh ◽  
T. S. Gurieva ◽  
I. G. Podolsky

1996 ◽  
Vol 18 (12) ◽  
pp. 265-268 ◽  
Author(s):  
N.S Pechurkin ◽  
L.A Somova ◽  
J.I Gitelson ◽  
R.C Huttenbach

1996 ◽  
Vol 39 (8) ◽  
pp. 617-622 ◽  
Author(s):  
S.I. Bartsev ◽  
J.I. Gitelson ◽  
G.M. Lisovsky ◽  
V.V. Mezhevikin ◽  
V.A. Okhonin

1993 ◽  
Vol 62 (6) ◽  
pp. S9-S15 ◽  
Author(s):  
G. I. Meleshko ◽  
T. S. Guryeva ◽  
Ye. Ya. Shepelev ◽  
I. A. Abakumova

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