Following the recent laboratory detection of the ring-chain carbene C5
H2, we have now detected C5H2, the next longer member of the sequence
formed by substituting a carbon chain for one of the hydrogen atoms of
cyclic C3H2. The strongest lines, again obtained with a diacetylene-n
eon discharge, were roughly 15 times weaker than those of C5H2 Enough
rotational lines were detected in both the normal and doubly deuterate
d isotopic species to be certain of the identification and to obtain t
he rotational and leading centrifugal distortion constants accurately
enough for calculation of the entire rotational spectrum below 300 GHz
to a fraction of 1 km s(-1) in equivalent radial velocity. The ring c
hain here is calculated to be the most stable isomer of C7H2, and extr
emely polar, so it is of considerable astronomical interest. Several o
ther isomers of C7H2 may be detectable in the laboratory and in space
with present techniques.