In a dense molecular cloud, at the edge of glowing gas, an invisible assembly line is at work. It takes simple scraps — single atoms and light pairs — and glues them together step by step into long carbon chains and rings. The first piece of this assembly line has long eluded our eyes. Now it has been found.

The ion in question is C2H+ (ethynyl cation): a tiny charged particle where two carbon atoms hold one hydrogen atom. It's like the zipper on a jacket: small on its own, but without it you can't close the whole thing. Astronomers caught its signal in a region called the Orion Bar, where radiation from young stars strips the neighboring cloud. The APEX telescope, with its 12-meter dish operating in the submillimeter range, picked up radio waves at a frequency of about 211 GHz — roughly one and a half times higher than that of a microwave oven. The signal was neatly split into several spikes, like a comb with sparse teeth — exactly as recent laboratory measurements had predicted.

The discovery matters not on its own but as a missing link. Models calculated at the Meudon Observatory showed that it is precisely here, on the illuminated edge of the cloud, that the C2H+ ion passes the baton onward, turning into C2H2+ and C2H3+. This kicks off growth from simple to complex — bottom-up. Previously, astronomers debated whether such a pathway could exist in real space, or whether large molecules assemble differently. Now the 'small bricks' scenario has a solid observational foundation. The next step is to look for C2H+ in other nebulae. Each new find will be like a signature on a blueprint: yes, this is how nature builds carbon structures, from which, perhaps, the building blocks of life will later emerge.