In detecting alien life on a faraway planet, methane may be the key
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[March 29, 2022]
By Will Dunham
WASHINGTON (Reuters) - For humankind,
evidence for life beyond Earth is unlikely to be as dramatic as an alien
spaceship landing, say, next to the Eiffel Tower in Paris. It is more
likely to come from telescope observations of a faraway planet bearing
atmospheric chemicals suggestive of biological activity.
Researchers on Monday said methane may be the first detectable sign of
extraterrestrial life if discovered in the atmosphere of a rocky planet
orbiting in the "habitable zone" - the area not too hot and not too cold
for liquid water to exist on the planetary surface - around a sun-like
star.
Scientists are working to understand the indicators of life -
biosignatures - that might be present in observations of planets in
other solar systems, called exoplanets, knowing that increasingly
capable telescopes soon will be available.
The researchers, in a study published in the journal Proceedings of the
National Academy of Sciences, showed that abundant atmospheric methane
could be a persuasive sign of life in the right planetary context.
Methane is an important trace gas in Earth's atmosphere, at less than 2
parts per million by volume.
Unlike other potential biosignatures such as atmospheric oxygen, methane
is one of the few gases that should be readily detectable using the
James Webb Space Telescope, launched by NASA in December and due to
become operational within months.
"On Earth, the vast majority of methane is produced by life," said study
lead author Maggie Thompson, a University of California, Santa Cruz
graduate student in astronomy and astrophysics.
Most of it is generated directly by life: methane-producing microbes in
wetlands, rice fields or in the guts of large animals. Methane is also
generated through human activities such as burning fossil fuels
including coal and oil, which are remnants of dead organisms. The
proportion of Earth's nonbiologically generated methane is miniscule.
The researchers made a three-part case for methane as a promising
biosignature.
"First, it would be unsurprising for life elsewhere to produce methane.
Even if the biochemistry of alien life was radically different to that
of Earth's biosphere, methanogenesis is an obvious and easy metabolic
strategy for any carbon-based life given the energy sources likely to be
present on rocky exoplanets," said co-author Joshua Krissansen-Totton, a
NASA Sagan Fellow in UCSC's Department of Astronomy and Astrophysics.
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An artist's depiction of the exoplanet Kepler-62e is shown in this
NASA handout provided November 4, 2013. Kepler-62e is a super
Earth-size planet in the habitable zone of a star smaller and cooler
than the sun, located about 1,200 light-years from Earth in the
constellation Lyra. REUTERS/NASA Ames/JPL-Caltech/Handout via
Reuters
Secondly, they said, methane would
not persist for long in atmospheres of habitable rocky planets
without constant replenishment, possibly by living organisms. On
Earth, atmospheric methane is unstable - destroyed by the chemical
effects of light - but has constant biologically-generated
replenishment.
Thirdly, they said, it would be difficult for
nonbiological processes such as volcanism or chemical reactions in
mid-ocean ridges and hydrothermal vents to maintain replenishment
without leaving a "fingerprint" indicating the methane was not
biologically generated.
Gas-spewing volcanoes, for instance, would release carbon monoxide
alongside methane, but biological activity tends to devour carbon
monoxide and reduce its atmospheric concentrations. Thus, they said,
nonbiological processes cannot easily produce rocky planet
atmospheres rich in both methane and carbon dioxide, as on Earth,
but with little or no carbon monoxide.
Scientists are expecting greater insight into exoplanet atmospheres
using Webb and other new telescopes, examining their chemistry as
these distant worlds pass in front of their host stars from the
perspective of Earth.
Oxygen, more plentiful in Earth's atmosphere than methane, is
another potential biosignature. It too is fed into Earth's
atmosphere via biological processes - in this case photosynthesis by
plants and microbes. But oxygen could elude Webb's detection.
"Methane is not a hypothetical biosignature. We know life on Earth
has been producing methane for essentially its entire history, and
atmospheric methane concentrations may have been high on the early
Earth, before there was oxygen in the atmosphere," Krissansen-Totton
said. "But it's important to note that the diversity of planetary
environments elsewhere is probably vast, and there could be other
non-biological methane-making producing processes that no one has
yet considered."
(Reporting by Will Dunham, Editing by Rosalba O'Brien)
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