We report on molecular abundances and distributions in a starless dense core L492. We have found that the abundances of carbon-chain molecules such as CCS, C3S, HC3N, HC5N, and HC7N are comparable to those in chemically young dark cloud cores called ”carbon-chain–producing regions”, such as L1495B, L1521B, L1521E, and TMC-1. This is the first dark cloud core with extremely rich in carbon-chain-...