Oxygen is not definitive evidence of life on habitable extrasolar planets

In summary, a recent study suggests that the presence of oxygen in the atmosphere of a habitable extrasolar planet may not necessarily be a definitive biomarker for life, as previously thought. The study proposes the possibility of abiotic sources of molecular oxygen, such as iron oxides in the mantle of the planet. This highlights the importance of considering interdisciplinary approaches in the search for life on other planets. While the presence of oxygen may still be a strong indicator of photosynthetic life, it is not a guarantee and should be further studied in conjunction with other factors.
  • #1
PF_SpaceNews
Oxygen is not definitive evidence of life on habitable extrasolar planets

The Earth's atmosphere contains oxygen because plants continuously produce it through photosynthesis. This abundant supply of oxygen allows life forms like animals to flourish. Therefore, oxygen had been thought to be an essential biomarker for life on extrasolar planets. But now, a research assistant professor Norio Narita of the Astrobiology Center of National Institutes of Natural Sciences (NINS), which was founded in April 2015, and an associate professor Shigeyuki Masaoka, of the Institute of Molecular Science of NINS, have presented a novel hypothesis that it could be possible for planets to have large quantities of abiotic (non-biologically produced) oxygen. This study is a good example of interdisciplinary studies that combine knowledge from different fields of science to promote astrobiology in the search for life on extrasolar planets. The study is published in Scientific Reports on Sep 10, 2015.

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  • #2
"Until now, it had been thought that if a planet has oxygen, that must mean that some form of plants are producing it through photosynthesis. Therefore, it had been assumed that when searching for signs of life on habitable extrasolar planets, the presence of oxygen in the atmosphere could be considered a definitive biomarker."

Read more at: http://phys.org/news/2015-09-oxygen-definitive-evidence-life-habitable.html#jCp

Bit of an overstatement to reach an obvious conclusion that "necessary" is not the same as "sufficient."
 
  • #3
Bystander said:
Bit of an overstatement to reach an obvious conclusion that "necessary" is not the same as "sufficient."
Where do you see that?

Before: "We don't know abiotic sources of molecular oxygen, if we find oxygen in an atmosphere it should come from life"
Now: "We know an abiotic source of molecular oxygen, if we find oxygen in an atmosphere we don't know where it comes from"
 
  • #4
mfb said:
Before: "We don't know abiotic sources of molecular oxygen
https://www.google.com/?gws_rd=ssl#q="iron+oxides"+"mantle+rocks"
See Lev Epplebaum (5th or 6th item in list) for clear statement of T, P stability of FeII over FeIII in mantle rock. Bottom line? Plenty of well-known sources of free oxygen in large quantities for atmospheres on rocky planets.
 
  • #5
OK so a planet with a substantial surface layer of Titanium Oxide orbiting a star with strong UV emission might have an atmosphere with a lot of free oxygen.
That doesn't make it less plausible that free oxygen is a strong marker of photosynthetic life.
In fact I think that Titanium Oxide coated planets would be considerably more rare than planets having surface water and an abundance of Carbon/Nitrogen/Oxygen compounds, the prerequisites for organic chemistry.
 

1. Why is oxygen not considered definitive evidence of life on habitable extrasolar planets?

There are several reasons why oxygen alone cannot be considered definitive evidence of life on habitable extrasolar planets. Firstly, oxygen can be produced through abiotic processes such as photochemistry and geological reactions. Secondly, it is possible for a planet to have a stable oxygen atmosphere without the presence of life, as seen on our own planet during the Archean era. Finally, there are other potential biomarkers that could indicate the presence of life, so oxygen alone cannot be considered conclusive evidence.

2. Is the presence of oxygen on a habitable extrasolar planet a strong indicator of life?

While the presence of oxygen may be a strong indicator of life, it is not definitive evidence. As mentioned earlier, there are other abiotic processes that can produce oxygen, and it is possible for a planet to have oxygen without the presence of life. Therefore, other factors and biomarkers need to be considered before concluding that a planet is habitable and has life.

3. What other biomarkers should be considered when searching for life on habitable extrasolar planets?

Apart from oxygen, other biomarkers that can indicate the presence of life on a habitable extrasolar planet include methane, water vapor, and certain ratios of gases such as carbon dioxide and nitrogen. Additionally, the presence of specific molecules such as amino acids and proteins can also be indicative of life.

4. Can the presence of oxygen on a habitable extrasolar planet be explained by non-biological processes?

Yes, the presence of oxygen on a habitable extrasolar planet can be explained by non-biological processes. For example, oxygen can be produced through photochemical reactions in the atmosphere or through geological processes like the breakdown of water molecules. Therefore, the presence of oxygen alone cannot be used to definitively conclude the presence of life on a planet.

5. How can scientists distinguish between biologically-produced oxygen and oxygen produced by other processes on a habitable extrasolar planet?

Scientists can use techniques such as spectroscopy to analyze the light that passes through a planet's atmosphere and identify the specific molecules present. This can help distinguish between biologically-produced oxygen and oxygen produced by other processes. Additionally, studying the ratios of different gases and molecules can also provide insight into the likelihood of life on a habitable extrasolar planet.

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