Ammonia cluster cations are a chemical species that has recently attracted considerable research attention as an ion−molecule reaction species in the planetary atmosphere, surface reaction species in materials chemistry, and super-alkali species. Reactions of the radical cation of an ammonia cluster, [(NH 3 ) n ] + (n = 2−6), following the ionization of the parent neutral cluster, were investigated using direct ab initio molecular dynamics to elucidate the reactions of the ammonia cluster cation under astrochemical conditions. The calculations showed that two competing reaction channelsproton transfer (PT) channel and complex formation channeloperate after the ionization of neutral clusters. In the PT channel, a proton of NH 3 + was transferred to a neighboring ammonia molecule. The PT channel was found in all clusters (n = 2−6). Reaction via the PT channel became faster with increasing cluster size and saturated around n = 5− 6. In the complex formation channel, a face-to-face complex having a H 3 N−NH 3 + structure (with a N−N bond) was formed. This channel was found only in larger clusters (n = 5−6). Time scales of PT and complex formation channels were calculated to be 20− 30 and 40−50 fs, respectively. The reaction mechanism was discussed based on the results of theoretical calculations.