Formation of extraterrestrial peptides and their derivatives
arXiv:2405.00744 · doi:10.1126/sciadv.adj7179
Abstract
The formation of protein precursors, due to the condensation of atomic carbon under the low-temperature conditions of the molecular phases of the interstellar medium, opens alternative pathways for the origin of life. We perform peptide synthesis under conditions prevailing in space and provide a comprehensive analytic characterization of its products. The application of 13C allowed us to confirm the suggested pathway of peptide formation that proceeds due to the polymerization of aminoketene molecules that are formed in the C + CO + NH3 reaction. Here, we address the question of how the efficiency of peptide production is modified by the presence of water molecules. We demonstrate that although water slightly reduces the efficiency of polymerization of aminoketene, it does not prevent the formation of peptides.
References in corpus (8)
- Photochemistry and astrochemistry: photochemical pathways to interstellar complex organic molecules
- Origin of the RNA World: The Fate of Nucleobases in Warm Little Ponds
- A pathway to peptides in space through the condensation of atomic carbon
- Carbon Atom Reactivity with Amorphous Solid Water: HO Catalyzed Formation of HCO
- Surface Diffusion of Carbon Atoms as a Driver of Interstellar Organic Chemistry
- Experimental Characterization of the Energetics of Low-temperature Surface Reactions
- A New "Non-energetic" Route to Complex Organic Molecules in Astrophysical Environments: The C + HO HCO Solid-state Reaction
- Did life originate from low-temperature areas of the Universe?