Invisible Molecule Teaches Chemistry of Space express

Original: "Collisional energy transfer in ethanimine + He system"
arXiv:2606.08846 · 2026-06-07 · CC BY 4.0 · 2 min
Astronomers spotted a prebiotic molecule at the center of the Galaxy that behaves unlike the textbooks — and built a collision map for it.

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Two guitar strings are stretched on the same neck. They are almost identical, but one is slightly shorter — and they sound different. That's roughly how the two isomers of ethanimine work: molecules with the same set of atoms but rotated differently in space. Astronomers spotted this molecule in the dense clouds near the center of our Galaxy. Ethanimine is interesting because it belongs to the "prebiotic" class — from such building blocks, the first steps toward life might have assembled.

In cold gas, molecules constantly collide with neighbors — mostly helium atoms and hydrogen molecules. Each jolt makes the molecule spin faster or slower. Usually, frequent collisions bring rotation to equilibrium: fast and slow "spinning tops" settle into a strict distribution, like sand that has settled after a shake. But observations showed that ethanimine behaves differently: its rotational states are frozen in a non-equilibrium pattern. This means that collisions and the emission of energy into space pull the blanket in different directions, and neither wins.

Ethanimine is one of the few prebiotic compounds found directly in space, not "reconstructed" from indirect evidence.

To sort this out, the authors built a detailed map of how a helium atom interacts with each of the two isomers. They obtained "potential energy surfaces" — essentially, the landscape of forces acting between particles as they approach. Then they played out three collision scenarios on this map: fully quantum (most accurate but heavy), simplified quantum, and mixed quantum-classical. It turned out that upon impact, the molecule prefers to change its rotation in a strictly defined way: either "roll" around one axis without changing speed around the other, or vice versa. This is like a spinning top that changes its tilt when flicked but keeps its spin speed.

The difference in energy transfer between the two isomers is about 10%. Seems like a small thing, but in astronomical observations such a subtlety can decide whether we correctly identified the molecule.

The most practical of the findings is that the mixed quantum-classical method works well at high collision energies. It's like switching from hand engraving to lithography: faster, cheaper, and you hardly lose any detail. Now, plugging the computed transition probabilities into radiation transfer models, astronomers can more accurately read the chemical composition of distant clouds — the very ones where, from ethanimine and its neighbors, the first organic chains might have been born.

Ethanimine consists of just 8 atoms (two carbons, five hydrogens, and one nitrogen), but its two isomers differ like left and right gloves — and space "sees" that difference.

In Carl Sagan's novel "Contact," the alien signal contained blueprints for a machine, but building it required understanding the chemistry of the interstellar medium — exactly what collision calculations refine.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterJames Clerk Maxwell
Concepts
energy transfer helium burning charge transfer states energy exchange elastic scattering hydrogen cyanide titanium electron transition nuclear collision methanol tritium triple-alpha process (Hoyle process) inverse compton scattering transition collision fuel cell helium flash chemical enrichment heat transport mass–energy equivalence