Illustration of NASA’s Cassini spacecraft diving through the plume of Saturn’s moon Enceladus.
NASA/JPL-California Institute of Technology
The plumes of water vapor spewing from Enceladus’ surface appear to contain hydrogen cyanide, which, perhaps counterintuitively, suggests that there may be life in the oceans beneath the surface of this icy moon of Saturn. It shows that it is possible.
The Cassini spacecraft flew through Enceladus’ plume several times in the early 2000s, capturing samples as it hurtled past. Preliminary analyzes of these samples have revealed several elements and compounds that may be important for life, but many are not, as the molecules tend to fracture after impacting Cassini’s sampling chamber at high speeds. It has been difficult to identify specific compounds.
Jonah Peter Researchers at Harvard University performed a reanalysis of the Cassini data using new statistical methods and were able to extract more compounds present in the plume. They found evidence of several previously undetected compounds, including hydrogen cyanide, acetylene, ethane, and even trace amounts of the alcohol methanol.
All of these compounds could be part of chemical reactions important to life, but hydrogen cyanide is particularly promising.
“We still don’t have a complete picture of the molecules that are there and are necessary for the origin of life. We don’t even know how the origin of life occurred on Earth,” Peter said. say. “But we know a lot about some of the building blocks that are necessary for the beginning of life, and hydrogen cyanide is one of those very versatile building blocks.”
We know that it can be a building block for amino acids, RNA, and other large biomolecules, so its presence in the plume points to the possibility of life in Enceladus’ subsurface ocean. That’s a good sign.
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Source: www.newscientist.com
