Aerobic Microbes: Imre Friedmann Research on Mars

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In summary: The researchers suggest that the ice caps could be melted and raised as a shield over large parts of the planet, including the equator."I think that this idea is a good one, however I don't think that it would be easy to do. There are a lot of challenges that would need to be overcome.
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Hello all skilled biologists reading this post.

Researcher Imre Friedmann et al. have selected a couple of critters suited for Mars if man were to warm it up. Two of these are aerobic; Matteia and Deinococcus radiodurans. I was wondering if the oxygen pressure on Mars is high enough for aerobic bacteria to breath there. If not, is the problem easily engineered?

http://www.users.globalnet.co.uk/~mfogg/pioneer.htm

I appreciate all answers..
 
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If the bacteria strict aerobes, the amosphere pressure will probably not be sufficient for the bacteria to grow. However, if the bacteria can grow in the absent of oxygen or at low oxygen level, then there is a chance of survival.
I did not find any information regarding there specifics of the respiratory chain.

The bacteria could be engineered to use another electron acceptor. However several changes would have to be made.
 
  • #3
D. radiodurans is a very hardy bacteria, I would doubt it would be highly adaptable. Like extreme barophiles I think it is too specialized to adapt. Why not e.coli which is both fermentative (therefore anaerobic) and aerobic. Facultative anaerobes are really good, cyanobacteria would be a good choice as well.
 
  • #4
The problem with E. coli and cyanobacteria is that these bacteria may not survive the stresses encounter on mars. However, use some of the D. radiodurans resistance gene and inserted inside a falcutative anaerobe.

As you mention, D. radiodurans can surive extreme stress. the idea would be the insert new genetic information insinde D. radiodurans and Matteia. As far as i know,D. radiodurans can be transformed by some establised protocol.
 
  • #5
With reference to e.coli AND cyanobacteria is to basically propose a autotrophic bacteria that demonstrats high levels of adaptability. Lol e.coli (enterobacter strains) can't survive in our terrestrial environment for long forget mars. But they were the only examples I could come up with at the top of my head.

Radiodurans is infact a very cool microorganism because it has chaperones for its proteins and really good "fixing" mechanisms for DNA. But this is just repsonse generated due to massive amounts ionizing radiation in its environement, which it has adapted to via these processes. Other microorganisms use ca2+ based organic acids and mn2+ for their preservation of genetic material (with respect to free radicals and temperature). This is also why I mentioned barophiles as some barophiles (who also happen to be thermophillic) like pyrolobus fumari also have these chapperon proteins.

Radiodiurans has most of these adaptive features neatly packed in it, however because I am not a cosmologist or astronomer I have not clue how radiation or temperature is of consequence to mars. Yet I would have thought microorganisms that can function and adapt very well to the depletion of essential nutrients would be ideal for this. I understand the cloning bit with Radiodurans genes but, how will that help us? I mean there are just so many (eu)bacteria and archea which have specialization for extreme environments so what makes Radiodurans so special particularly for mars.

I think I might do some reading on the atomsphere (if there is one) of mars; but after exams. Ciao!
 
  • #6
google said:
have not clue how radiation or temperature is of consequence to mars.
Well, Mars is much colder than Earth, but there's probably sufficient warmth to support a hearty microbe...
from http://www.seds.org/billa/tnp/mars.html
While the average temperature on Mars is about 218 K (-55 C, -67 F), Martian surface temperatures range widely from as little as 140 K (-133 C, -207 F) at the winter pole to almost 300 K (27 C, 80 F) on the day side during summer.

Solar radiation is a big problem for life on Mars. With no ozone layer on Mars, lots more sterilizing UV light hits the surface. This also seems to have converted Martian soil into something highly oxidative (destroys organic matter).

Microbes would likely do better in the subsurface under current conditions.

I think I might do some reading on the atomsphere (if there is one)
yep, there's an atmosphere...
from http://www.seds.org/billa/tnp/mars.html
Mars has a very thin atmosphere composed mostly of the tiny amount of remaining carbon dioxide (95.3%) plus nitrogen (2.7%), argon (1.6%) and traces of oxygen (0.15%) and water (0.03%). The average pressure on the surface of Mars is only about 7 millibars (less than 1% of Earth's), but it varies greatly with altitude from almost 9 millibars in the deepest basins to about 1 millibar at the top of Olympus Mons.
 
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  • #7
Phobos said:
Solar radiation is a big problem for life on Mars. With no ozone layer on Mars, lots more sterilizing UV light hits the surface. This also seems to have converted Martian soil into something highly oxidative (destroys organic matter).

Microbes would likely do better in the subsurface under current conditions.

For protection from the UV rays of the sun, how about going beneath the Martian ice caps?

NASA is has also been thinking about this. (reference)
"Data from a Nasa probe has revealed that enough heat from inside the Red Planet might be trapped at the poles to melt underground water ice. This could create lakes below the ice caps - and where there is water, there could be life."

They go on to say there is carbon dioxide trapped under the caps as well which could help retain the heat. If CO2 is trapped below the ice, it would be reasonable guess there is some oxygen which had been dissolved in the ice that is trapped down there as well. Perhaps a probe like the Global Surveyor, has already verified this.
 

1. What are aerobic microbes?

Aerobic microbes are organisms that require oxygen to survive and carry out their metabolic processes. These microbes can be found in various environments on Earth, such as soil, water, and even our own bodies.

2. Who is Imre Friedmann and what is his research on Mars?

Imre Friedmann was a prominent microbiologist who studied the microbial life in extreme environments. He was also one of the pioneers in the field of astrobiology, which focuses on the study of life on other planets. Friedmann's research on Mars involved studying the possibility of microbial life on the red planet, specifically focusing on the discovery of aerobic microbes in the harsh conditions of the Martian environment.

3. How did Imre Friedmann's research on Mars impact our understanding of microbial life?

Friedmann's research on Mars was groundbreaking as it challenged the traditional belief that life could only exist in habitable conditions similar to Earth. His discovery of aerobic microbes in extreme environments on Earth and the possibility of their existence on Mars expanded our understanding of the potential for life to exist in a wide range of environments.

4. What does Friedmann's research on Mars suggest about the potential for life on other planets?

Friedmann's research on Mars suggests that life could potentially exist in even the harshest of environments, as long as there is a source of energy and basic nutrients. This has opened up the possibility for the existence of microbial life on other planets, such as Mars, Europa, and Enceladus, which were previously thought to be uninhabitable.

5. What is the significance of studying aerobic microbes on Mars?

Studying aerobic microbes on Mars is significant because it provides insights into the potential for life on other planets and the conditions that could support it. This research also helps us understand the origins and evolution of life on Earth and the possibility of finding similar life forms on other planets in our solar system or beyond.

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