[ACS Central Science] Complex organic molecules in interstellar ices and carbonaceous asteroids record key steps in the chemical evolution toward life, yet the origin of branched carbonyl compounds a fundamental class of biorelevant molecules remains unresolved.

Here, we demonstrate the efficient formation of C4 carbonyls, isobutyraldehyde ((CH3)2CHCHO) and 2-butanone (CH3CH2COCH3) via barrierless radical-radical recombination in carbon monoxide-propane (CO-C3H8; 1:1.1 ± 0.2) and ethane-acetaldehyde (C2H6-CH3CHO; 1.5 ± 0.3:1) ice mixtures at 5 K irradiated with 5 keV electrons as proxies for secondary electrons generated by galactic cosmic rays.

Isobutyraldehyde arises from recombination of formyl (HĊO) and isopropyl (CH3ĊHCH3) radicals, whereas 2-butanone forms through acetyl (CH3ĊO) and ethyl (CH3ĊH2) radical coupling. Using isomer-selective photoionization mass spectrometry with isotopic labeling, we provided strong evidence for these products together with the enol 2-methylprop-1-en-1-ol ((CH3)2CCHOH) in the gas phase.

These results establish a plausible low-temperature mechanism for molecular mass growth that generates branched carbon skeletons without activation barriers, bridging a critical gap between simple interstellar species and structurally complex, biorelevant organics.

The demonstrated pathways operate under cosmic-ray-driven, nonequilibrium chemistry in icy grains, providing a plausible route to C4 backbone motifs found in prebiotic molecules, including amino acids and fatty acids.

Our findings show that chemical complexity – including carbon skeleton branching can emerge in deep space prior to planetary accretion, implying a plausible extraterrestrial origin for key molecular precursors delivered to early Earth and exo planetary systems.

Astrobiology,

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp...

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