The abiotic synthesis of histidine under experimental prebiotic conditions has proven to be chemically promising and plausible. Within this context, the present results suggest that histidine amino acid may function as a simple prebiotic catalyst able to enhance amino acid polymerization. This work describes an experimental and computational approach to the self-assembly and stabilization of DL-histidine on mineral surfaces using antigorite ((Mg, Fe)SiO(OH)), pyrite (FeS), and aragonite (CaCO) as representative minerals of prebiotic scenarios, such as meteorites, and subaerial and submarine hydrothermal systems.
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