Protonated cyanoacetylene HC3NH+ has been detected toward TMC-1 for th
e first time with the Nobeyama 45 m radiotelescope through the J = 5-4
and J = 4-3 transitions. This observation provides the first measurem
ent of the pure rotational transitions for this ion either in the labo
ratory or in space. From a simultaneous analysis of rotational transit
ion frequencies obtained in this work and the previous infrared data,
the most accurate rotational and the centrifugal distortion constants
were determined to be B = 4329.0047(10) and D = 0.000478(11) MHz, resp
ectively, with one standard deviation in parentheses. The column densi
ty of HC3NH+ in TMC-1 (cyanopolyyne peak) was determined to be 1.0 (0.
2) x 10(12) cm-2 which is 160 times smaller than that of HC3N and 2.6
times more abundant than HNCCC. The abundances of HC3NH+, HNCCC, and H
CCCN are discussed on the basis of a reaction mechanism recently propo
sed for the production of HCCCN through neutral-neutral reactions.