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, researchers Norio Narita and Shigeyuki Masaoka from Japan's National Institutes of Natural Sciences (NINS), have presented a novel hypothesis that it could be possible for planets to have large quantities of abiotic (non-biologically produced) oxygen.
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.
However, non-biological chemical reactions can also affect atmospheric compositions of extrasolar planets.
A research team led by Narita has shown that, abiotic oxygen produced by the photocatalytic reaction of titanium oxide, which is known to be abundant on the surfaces of terrestrial planets, meteorolites, and the Moon in the Solar System, cannot be discounted.
In addition, the team estimated the amount of possible oxygen production for habitable planets around other types of host stars with various masses and temperatures.
They found that even in the least efficient production case of a low-temperature star, the photocatalytic reaction of the titanium oxide on about 3 per cent of the planetary surface could maintain this level of atmospheric oxygen through abiotic processes.
"To search for life on extrasolar planets through astronomical observation, we need to combine the knowledge from various scientific fields and to promote astrobiology researches to establish the decisive signs of life," Narita said.
"Although oxygen is still one of possible biomarkers, it becomes necessary to look for new biomarkers besides oxygen from the present result," Narita added.
The study was published in the journal Scientific Reports.
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