An Archean atmosphere rich in sulfur biomolecules. Journal Article uri icon

Overview

abstract

  • The abiotic production of sulfur-containing biomolecules under mild and globally relevant conditions has been an elusive endeavor in prebiotic chemistry experiments. As a result, a disconnect has emerged between understanding the origins of life and the later stages of biological evolution; the former potentially occurred independent of sulfur while the latter is universally dependent on it. Here, we demonstrate that planetary organic haze chemistry produces a suite of sulfur biomolecules including cysteine, coenzyme M, taurine, and potentially methionine and homocysteine. These compounds may form high in the atmosphere and subsequently deposit to early surface environments in sufficient amounts to support a budding global biosphere. Our findings thus challenge long-standing assumptions that sulfur biomolecules such as cysteine must have been biological "inventions."

publication date

  • December 9, 2025

Date in CU Experts

  • December 10, 2025 11:33 AM

Full Author List

  • Reed NW; Christensen CM; Surratt JD; McGlynn SE; Wing BA; Neubauer C; Tolbert MA; Browne EC

author count

  • 8

Other Profiles

Electronic International Standard Serial Number (EISSN)

  • 1091-6490

Additional Document Info

start page

  • e2516779122

volume

  • 122

issue

  • 49