The Scent of Cosmic Chemistry ✎ express

Original: "Infrared Spectroscopy and Photochemistry of Aromatic Nitriles in Para-Hydrogen Matrices"
arXiv:2608.09889v1 · 2026-08-10 · arXiv non-exclusive · independent analysis · 1 min
In cold clouds in space, aromatic molecules break down under ultraviolet light, leaving traces behind.

In the cold Taurus cloud, where stars are born, telescopes have detected molecules with the smell of bitter almonds — aromatic nitriles. On Earth, you can find them in peach pits, but in space they hang in icy dust. What happens to them under the harsh ultraviolet light of young stars? Chemists recreated this process in the lab.

In a special chamber at minus 268 degrees Celsius, benzonitrile and its cousins were irradiated with ultraviolet light at a wavelength of 193 nanometers. The molecules fell apart, and the main fragments turned out to be hydrogen cyanide (HCN) and its isomer HNC — the very ones already found in space. This means that light strips a group containing nitrogen and carbon from the ring, leaving a bare benzene core.

Ultraviolet light in the cloud acts like a knife, slicing side branches off the aromatic ring. Simple molecules remain, which then get incorporated into new, more complex ones.

Experiments with heavy hydrogen (deuterium) confirmed that the bond between the ring and the nitrile group breaks first, and only then do the fragments pick up hydrogen from the icy substrate. Such details help astronomers decipher the infrared spectra of distant clouds, where similar processes are happening right now.

Benzonitrile smells like bitter almonds, and in space it was found in a cloud where the temperature is only a few degrees above absolute zero.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterPaul Dirac
Concepts
silicon nitride benzene niobium nitride hydrogen cyanide nirspec lithium niobate