“…Previous high-temperature circumstellar reaction networks borrowed from sooty hydrocarbon flames have revealed limited efficiencies under conditions prevailing in circumstellar envelopes to synthesize fullerenes predominantly due to the lack of constrained and validated mechanisms leading to PAHs and fullerenes. 58,62 These high temperature reaction mechanisms in carbon rich circumstellar envelopes are similaralbeit under the exclusion of oxygento the bottom-up formation of PAHs probed in sooting combustion flames of, e.g., methane, 63 acetylene, 64 and benzene 65 revealing the ubiquitous presence of aromatics like fluoranthene, benzo[ghi]fluoranthene, and corannulene along with fullerenes (C60,C70). The reaction pathways to corannulene revealed in the present study and the potential role of corannulene in the formation of fullerenes gain strong support from sophisticated examinations of carbonaceous chondrites.…”