Saturn’s moon could have life, but only a little bit
- Titan, Saturn’s largest moon, may harbor life, but only in tiny amounts. A new study suggests that the moon’s subsurface ocean could support simple, microscopic life forms.
- The researchers used bioenergetic modeling to develop a realistic scenario of what life on Titan might look like, focusing on the moon’s plentiful organic content and its potential for supporting microbial life.
- The team found that only a small fraction of Titan’s organic material may be suitable for microbial consumption, suggesting that the moon’s biosphere would likely be very small, weighing only a few kilograms at most.
- Fermentation, a simple metabolic process that doesn’t require oxygen, is thought to have evolved early in Earth’s history and could potentially support life on Titan. The researchers focused on glycine, the simplest of all known amino acids, as a potential food source for microbes.
- The study suggests that finding life on Titan may be like looking for a needle in a haystack, unless future missions focus on exploring other areas of the moon beyond its surface organic content.
Saturn’s moon Titan could harbor life, but only a tiny amount, a new study finds.
Titan, Saturn’s largest moon, is a strange, alien world. Covered in rivers and lakes of liquid methane, icy boulders, and dunes of soot-like “sand,” its topography has long fascinated scientists and invited speculation on whether lifeforms might lurk beneath the moon’s thick, hazy atmosphere.
An international team of researchers co-led by Antonin Affholder at the University of Arizona ecology and evolutionary biology department of and Peter Higgins at Harvard University’s earth and planetary sciences department of set out to develop a realistic scenario of what life on Titan might look like if it does exist, where it is most likely to occur and how much of it might be present.
“In our study, we focus on what makes Titan unique when compared to other icy moons: its plentiful organic content,” says Affholder, who is a postdoctoral research associate.
Using bioenergetic modeling, the team found that Titan’s subsurface ocean, estimated to be as deep as about 300 miles, may support lifeforms that consume organic material. Published in The Planetary Science Journal, their study concludes that while Titan could possibly harbor simple, microscopic life, it likely could support only a few pounds of biomass overall.
Often described as “Earthlike on the surface, ocean world on the inside,” Titan is the target for future exploration via NASA’s Dragonfly mission. While much has been speculated about possible scenarios that could give rise to living organisms on Titan based on the moon’s abundant organic chemistry, previous estimates have suffered from what Affholder considers an overly simplistic approach.
“There has been this sense that because Titan has such abundant organics, there is no shortage of food sources that could sustain life,” Affholder says. “We point out that not all of these organic molecules may constitute food sources, the ocean is really big, and there’s limited exchange between the ocean and the surface, where all those organics are, so we argue for a more nuanced approach.”
At the core of the research lies a “back-to-basics” approach that attempted to come up with a plausible scenario for life on Titan that assumed one of the simplest and most remarkable of all biological metabolic processes: fermentation. Familiar to Earthlings for its use in sourdough breadmaking, beer brewing, and—less desirably—its role in spoiling forgotten leftovers, fermentation only requires organic molecules, but no “oxidant” such as oxygen, a crucial requirement for other metabolic processes, such as respiration.
“Fermentation probably evolved early in the history of Earth’s life, and does not require us to open any door into unknown or speculative mechanisms that may or may not have happened on Titan,” Affholder says, adding that life on Earth could have first emerged as feeding on organic molecules left over from Earth’s formation.
“We asked, could similar microbes exist on Titan?” Affholder says. “If so, what potential does Titan’s subsurface ocean have for a biosphere feeding off of the seemingly vast inventory of abiotic organic molecules synthesized in Titan’s atmosphere, accumulating at its surface and present in the core?”
The researchers specifically focused on one organic molecule, glycine, the simplest of all known amino acids.
“We know that glycine was relatively abundant in any sort of primordial matter in the solar system,” Affholder says. “When you look at asteroids, comets, the clouds of particles and gas from which stars and planets like our solar system form, we find glycine or its precursors in pretty much all those places.”
However, computer simulations revealed that only a small fraction of Titan’s organic material may be suitable for microbial consumption. Glycine-consuming microbes in Titan’s ocean would depend on a steady supply of the amino acid from the surface, through the thick icy shell. Previous work by the same team had shown that meteorites impacting the ice could leave behind “melt pools” of liquid water, which then sink through the ice and deliver surface materials to the ocean.
“Our new study shows that this supply may only be sufficient to sustain a very small population of microbes weighing a total of only a few kilograms at most—equivalent to the mass of a small dog,” Affholder says. “Such a tiny biosphere would average less than one cell per liter of water over Titan’s entire vast ocean.”
For a future mission to Titan, the odds of finding life—if it is indeed there—could be like looking for a needle in a haystack, unless Titan’s potential for life is to be found elsewhere than in its surface organic content, the team suggests.
“We conclude that Titan’s uniquely rich organic inventory may not in fact be available to play the role in the moon’s habitability to the extent one might intuitively think,” Affholder says.
The International Space Science Institute in Bern, Switzerland, funded the research.
Source: University of Arizona
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