Amy Williams

Professor of geological sciences at the University of Florida and a member of both the curiosity-rover and perseverance-rover science teams.

Lead author of the April 2026 Nature Communications paper on the SAM/TMAH detection of more than 20 organic molecules in Gale Crater’s Glen Torridon clays — including a nitrogen-bearing DNA-precursor-like compound and benzothiophene (src-curiosity-mars-life-molecules-2026-04).

”In-situ + exogenous” framing (2026)

In src-mars-organics-fresh-clues-2026-04 (jeffrey-kluger, TIME), Williams articulates the modern origin-of-life consensus as the combination of geologically in-situ chemistry and meteorite-delivered prebiotic feedstocks (exogenous-organics) — citing Bennu’s 14 protein-forming amino acids and the Murchison meteorite’s hexamethylenetetramine as exogenous-delivery evidence — and applies the same combined frame to early Mars. She also confirms that SAM-class TMAH wet chemistry will fly on ESA’s rosalind-franklin-rover (2028) and NASA’s dragonfly-mission (2027), and that her team has run a second TMAH experiment at another Gale Crater site, results pending.