Abstract
The dicarbon molecule (C(2)) is found in flames, comets, stars, and the diffuse interstellar medium. In comets, it is responsible for the green color of the coma, but it is not found in the tail. It has long been held to photodissociate in sunlight with a lifetime precluding observation in the tail, but the mechanism was not known. Here we directly observe photodissociation of C(2) From the speed of the recoiling carbon atoms, a bond dissociation energy of 602.804(29) kJ·mol[Formula: see text] is determined, with an uncertainty comparable to its more experimentally accessible N(2) and O(2) counterparts. The value is within 0.03 kJ·mol(-1) of high-level quantum theory. This work shows that, to break the quadruple bond of C(2) using sunlight, the molecule must absorb two photons and undergo two "forbidden" transitions.