  We present distributions of two molecular clouds having velocities of 2 km
s$^{-1}$ and 14 km s$^{-1}$ toward RCW 38, the youngest super star cluster in
the Milky Way, in the $^{12}$CO ($J=$1--0 and 3--2) and $^{13}$CO ($J=$1--0)
transitions. The two clouds are likely physically associated with the cluster
as verified by the high intensity ratio of the $J$=3--2 emission to the
$J$=1--0 emission, the bridging feature connecting the two clouds in velocity
and their morphological correspondence with the infrared dust emission. The
total mass of the clouds and the cluster is too small to gravitationally bind
the velocity difference. We frame a hypothesis that the two clouds are
colliding with each other by chance to trigger formation of the $\sim$20
candidate O stars which are localized within $\sim$0.3 pc of the cluster center
in the 2 km s$^{-1}$ cloud. We suggest that the collision is currently
continuing toward part of the 2 km s$^{-1}$ cloud where the bridging feature is
localized. This is the third super star cluster alongside of Westerlund2 and
NGC3603 where cloud-cloud collision triggered the cluster formation. RCW38 is
the most remarkable and youngest cluster, holding a possible sign of on-going O
star formation, and is the most promising site where we may be able to witness
the moment of O-star formation.
