A rock discovered by NASA's Curiosity Mars rover contains "the most diverse collection" of the building blocks of life ever seen on the Red Planet, including seven never found there before, new research confirms.

In 2020, Curiosity discovered and drilled into the rock, which has now been confirmed to contain organic molecules that bear the life-friendly element carbon. While scientists can't yet prove if the molecules formed due to biological or geologic processes, their findings add new evidence to the theory that ancient Mars was hospitable to life.

"Their discovery renewed confirmation that ancient Mars had the right chemistry to support life," officials at NASA's Jet Propulsion Laboratory (JPL), which manages the mission, wrote of the organics. "What's more, the molecules join a growing list of compounds known to be preserved in rocks even after billions of years of exposure on Mars to radiation, which can break down these molecules over time."

By the Martian seashore

The new analysis, published April 21 in the journal Nature Communications, shows that the rock sample included 21 carbon-containing molecules, including seven never seen before on the Red Planet. The newly found molecules included nitrogen heterocycle (a predecessor to RNA and DNA) as well as benzothiophene, which may have been key to bringing life-friendly chemistry to solar system planets aboard meteorites, the authors wrote.

The sample was nicknamed "Mary Anning 3," after the English paleontologist famous for discovering the first fossil ichthyosaur and plesiosaur. Much like the aquatic fossil environments Anning sought out, the Martian organics were found in an area of Mars that was teeming with lakes and streams before the planet dried out billions of years ago.

A region of Mars’ Mount Sharp where the ‘Mary Anning 3’ sample was discovered. (Image credit: NASA/JPL-Caltech/MSSS)

"This oasis surged and dried up multiple times in the planet's ancient past, eventually enriching the area with clay minerals, which are especially good at preserving organic compounds," JPL officials wrote.

Drilling for life

Last year, Curiosity also found the largest-ever organic molecules on Mars. These were "long-chain" hydrocarbons, including decane, undecane and dodecane.

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These organic finds in 2020 and 2025 used an instrument on Curiosity called Sample Analysis at Mars (SAM). Curiosity first drills rocks using its robotic arm. Then, it turns the rocks into powder samples and lets the powder fall into SAM. The instrument contains a high-temperature oven that heats up the powder, allowing the compositions of the gases inside the rover to be measured.

SAM also contains small cups of solvent that can perform "wet chemistry." The Mary Anning 3 sample was the first to use tetramethylammonium hydroxide (TMAH) — a substance that breaks apart organic molecules, of which Curiosity only carries two cups — because the sample was considered of the highest value.

Curiosity's findings were verified on Earth using a space rock that's well known to science, the Murchison meteorite, which is 4 billion years old and includes organic molecules.

"A Murchison sample exposed to TMAH was found to break much larger molecules into some of the ones seen in Mary Anning 3, including benzothiophene," JPL officials wrote. "That result verifies that the Martian molecules found in Mary Anning 3 could have been generated from the breakdown of even more complex compounds relevant to life."

Curiosity, which has been on Mars since 2012, recently used its last TMAH cup on "weblike boxwork ridges, which were formed by ancient groundwater," according to JPL. The results will be written up in a future study.

Williams, A. J., Eigenbrode, J. L., Millan, M., Williams, R. H., Mcintosh, O. M., Teinturier, S., Roach, J., Malespin, C., McAdam, A. C., Mahaffy, P., Bryk, A. B., Buch, A., Boulesteix, D., Chou, L., Dworkin, J. P., Fox, V., Franz, H. B., Freissinet, C., Glavin, D. P., . . . Vasavada, A. R. (2026). Diverse organic molecules on Mars revealed by the first SAM TMAH experiment. Nature Communications, 17(1). https://doi.org/10.1038/s41467-026-70656-0

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