Mars
Microbiology
In the process known as respiration, microorganisms break
down organic compounds, such as sugars, as food to produce energy. Another way of saying this is that the
organic compounds are oxidized. The organisms use the energy to power cell functions and make
cell material. Anaerobic respiration
occurs in the absence of oxygen (nevertheless we still say that the the organic
compounds used as fuel are oxidized in the process) but produces
much less energy per sugar molecule than aerobic respiration, although the
latter requires molecular oxygen (O2) as a substrate.
Because the Martian atmosphere does not contain significant
amounts of O2 astrobiologists do not believe that aerobic respiration
occurs on Mars. However, if Martian
life forms exist, then some form of anaerobic respiration may be part of their
metabolism and if so they would be capable of metabolizing small organic
compounds. Therefore, one of the
experiments sent to Mars during the 1970s as part of Project Viking was
designed to look for evidence of anaerobic respiration in the Martian
soil. The experiment, designed by
Gilbert Levin was known as the Labeled Release (LR) Experiment, because it
employed a solution of test nutrients, labeled with carbon-14 (14C). In other words each carbon atom of each
molecule of nutrient in the LR test solution was of the isotope 14C,
instead of the more common 12C and 13C. However, unlike the other two carbon
isotopes, 14C is radioactive, so its presence can be detected with a
radiation sensor.
At both Viking landing sites when Martian soil was placed
within a special container and treated with the LR test solution, radioactivity
was detected in the air space above the soil.
This means that the some or all of the 14C-containing liquid
nutrients were converted chemically into 14C-containing gases,
because only a gas would rise above the soil sample to produce a radioactive
signal in the overhead space. For
example, one of the the 14C-containing nutrients in the LR test
solution was formic acid which in many terrestrial microorganisms is oxidized
to carbon dioxide (CO2) during the process of respiration, whether
aerobic or anaerobic. Here is the
reaction, which in many species requires two enzymes as well as co-factor
called NAD+.

The radioactivity was detected following treatment with
nutrient solution only in those samples that were not heated prior to
testing. In samples that were heated to
160 degrees C for three hours before testing, the results were negative,
suggesting that microorganisms had been the resson for the positive response in
unheated samples but had been killed in the heated samples. To appreciated the value of using heat sterilization
as a control for a life detection expetiment, try Classroom Experiment # 1 (see section II).
Initially the Viking scientists were very excited about
these results. However, because another
instrument designed to look for carbon-containing (organic) compounds produced
negative results, most of the scientists began to think that a non-biological
oxidizing agent, such as hydrogen peroxide (H2O2) had
mimicked the effects of life on the LR test solution –like this:
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Photosynthetic
microorganisms: Microcystis aeruginosa strain PCC
7806. Autofluorescence image. From Cyanobacterial Image Gallery
http://www-cyanosite.bio.purdue.edu/images/images.html
In a way, photosynthesis is the opposite of
respiration. In photosynthesis, the carbon
contained within CO2 is used to make organic nutrient compounds
through a process called reduction, the opposite of
oxidation. Photosynthetic organisms can
then oxidize the compounds through respiration or they can be saved and/or used
by other organisms. Thus,
photosynthetic organisms use to CO2 make their own food! In order to do this, they need sunlight and
water and as a by product they produce O2, which they can use during
respiration in the dark or which can be used by non-photosynthetic organisms
–humans for example.
Plants are famous for being
photosynthetic but did you know that many microorganisms are also
photosynthetic? During Project Viking, scientists tested for the
possibility that photosynthetic microorganisms might inhabit Mars. They employed the Pyrolytic Release
Experiment (PR) developed by Norman Horiwitz.
In a way, the PR was the opposite of the LR. While the LR treated Martian soil samples with 14C-containing
liquid nutrients, the PR exposed soil samples to 14C-containing gases,
CO2 and carbon monoxide (CO), because both of these gases are
present in the Martian atmosphere.
After exposure to the gases, the soil was studied to see whether it can
taken in any radioactivity, which would indicate that the 14C-containing
CO2 and/or CO had been reduced to organic compounds within the soil.
When the PR experiment was
performed, very small amounts of carbon from the gases were found to have
become part of the soil, indicating reduction.
However this occurred in both unheated samples and those heated prior to
testing, suggesting that the effect had been the result of some non-living
agent/s process in the soil. Also, the
small amount of reduction occurred both in the light and the dark and thus the
experiment did not detect photosynthesis.
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Methanogenic microorganisms produce the gas CH4
(methane). On Earth, the substrates
usually are H2 and CO2 both of which are gases at
standard temperature and pressure. In
the process of synthesizing methane, the carbon atom is changed from its most
oxidized state (in CO2) to its most reduced state (in CH4)
and energy is produced, energy which the organisms use to make food and cell
material. Here is the overall reaction:
4H2 +
CO2 CH4
+ 2H2O
For methanogenic organisms, the methane is a waste product,
released into the atmosphere, just as CO2 is released as waste by
humans. Earth’s atmosphere thus
contains some methane, although compared the concentration of nitrogen and
oxygen, the levels of methane in our atmosphere is very very tiny. Even so, Earth’s atmospheric methane can be
detected from space, using special instruments.
If life forms exists on Mars, it is plausible that some of
them might use methanogenesis for energy.
It is possible that the gas released during the Viking Labeled Release
Experiment (LR) was CH4 rather than CO2, but this is not
the only reason why a Martian version of methanogen may inhabit the Red
Planet. In 2004 a European Space Agency
(ESA) probe, Mars Express, detected
methane in the Martian atmosphere.
Although volcanic activity is a possible non-biological source of
methane, there is no evidence for contemporary volcanic activity on Mars. On the other hand, Mars Express also detected trace amounts of HCHO
(formaldehyde). Formaldehyde is an
intermediate of methanogenesis, a compound produced along the way during the
biosynthesis of methane from H2 and CO2. It cannot be made through volcanic
activity. ESA plans to continue to
study the Martian atmosphere and scientists in both ESA and NASA plan
additional probes in the near future to confirm the Mars Express findings. But
if it turns out that the Martian atmosphere contains methane with a sprinkling
of formadehyde, it would mean that methanogenic microorganisms are native to
Mars. Stay tuned.
1. Take some baker’s yeast and divide it into two portions. Heat one sample for 3 hours at 160 degrees
C. For each sample (heated and unheated)
place in nutrient solution (which teacher will prepare). The solution will be made from PBS to which
sugar or vinegar will be added as food for the yeast. Let the yeast incubate in the nutrient solution, then after 2
hours look for bubbles. Compare the
result for the heated and unheated yeast.