The work was led by Amy Williams of the University of Florida, together with Jennifer Eigenbrode of NASA’s Goddard Space Flight Center and an international collaboration, using Curiosity’s Sample Analysis at Mars (SAM) instrument suite. Where previous SAM runs had relied on thermal decomposition — heating rock until molecules fragmented — this campaign used a reagent called TMAH (tetramethylammonium hydroxide) to gently cleave larger, complex organics into pieces small enough to reach SAM’s mass spectrometer with their structural information intact.
The technique matters because Mars has a habit of destroying its own evidence. Billions of years of ultraviolet radiation and oxidizing soils tend to shred anything chemically delicate at the surface. TMAH circumvents that problem by derivatizing the sample in a way that preserves molecular architecture rather than smashing it. Only two TMAH doses were ever loaded onto Curiosity, and one of them was spent on this experiment.

Glen Torridon: the right rock, the right moment
The run was performed in 2020 on three drilled samples inside Glen Torridon, a region of Gale crater where clay minerals mark what was once a long-lived lake bed. Clay matters in astrobiology because it clings to organic molecules and shelters them from the harshest surface chemistry. If anywhere on Mars was likely to have held onto a chemical autobiography for 3.5 billion years, this was a prime candidate.
And the chemistry delivered. Beyond the more than twenty organic species identified, two finds stand out. The first is a nitrogen-bearing molecule whose architecture echoes the compounds that build nucleic acids on Earth — the first time anything of that family has been flagged on Mars. The second is benzothiophene, a double-ringed, sulfur-containing hydrocarbon frequently found in meteorites, a clue that at least part of the Martian organic inventory may be of extraterrestrial infall origin rather than in-situ geochemistry.
Chemistry is not biology — yet
Williams and her coauthors are careful on the critical point, and so should the rest of us be: these molecules do not prove that Mars once hosted life. The SAM experiment cannot cleanly separate organics produced by biology from those forged by abiotic geochemistry or delivered by meteorites. A definitive answer will almost certainly require bringing pieces of Mars back to Earth, where laboratory instruments can chase the isotopic fingerprints that telegraph a biological origin.

What the result does establish is that Mars is a chemically informative archive. Complex organics can survive for roughly 3.5 billion years in the shallow subsurface, which means any ancient biosignatures that may have existed had a reasonable shot at being preserved. That is not a discovery of life. It is something nearly as important: a demonstration that the search is not hopeless.
A test case for the next decade of planetary exploration
The technique validated by Curiosity in 2020 is already booked for future flights. Europe’s Rosalind Franklin rover, designed to drill nearly two meters beneath the Martian surface and well below the UV-damaged zone, will carry a TMAH-based experiment. So will NASA’s Dragonfly rotorcraft, bound for Saturn’s moon Titan and its stupendously rich hydrocarbon chemistry.
Curiosity, meanwhile, continues to climb Mount Sharp more than a decade past its nominal mission. A rover that landed in 2012 has now extended its scientific reach into experiments that were not part of its original playbook when it launched — and in doing so has handed astrobiology one of the most detailed organic inventories ever produced off-world.
The study, Diverse organic molecules on Mars revealed by the first SAM TMAH experiment, is published in Nature Communications (DOI: 10.1038/s41467-026-70656-0).
© 2026 SKYCR.ORG | Homer Dávila Gutiérrez, FRAS. All rights reserved. Total or partial reproduction without express authorization is prohibited. Original source: phys.org / University of Florida.
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