The rotational spectra of cis-and trans-HSSSH have been complemented u
p to 670 GHz ((r)Q(29) branch) and the spectra of several of its isoto
pomers have been recorded between 70 and 300 GHz. The derived rotation
al constants of HSSSH, (HSSSH)-S-34, (HSSSH)-S-34, HSSSD, and DSSSD pr
ovide the experimental basis for for deriving a substitution structure
(r(s)) for cis-HSSSH and and a r(epsilon I) structure for both specie
s, i.e. cis-and trans-HSSSH. The r(epsilon I) bond distances and angle
s are for the cis-conformer: R(SH)= 1.3435(14) Angstrom, R(SS) = 2.053
0(1) Angstrom, angle SSH = 97.37(15)degrees, angle SSS = 106.919(3)deg
rees, angle SSS-SSH = 90.82(16)degrees, and for the trans-conformer: R
(SH)= 1.3435(assumed) Angstrom, R(SS) = 2.0539(4) Angstrom, angle SSH
= 97.2(7)degrees, angle SSS = 107.02(2)degrees, angle SSS-SSH = 87.7(4
)degrees. These experimental structural results are in good agreement
with ab initio calculations. The spectra show no effect of internal ro
tation, in agreement with a theoretical barrier estimate of similar to
2900 cm(-1). (C) 1997 Elsevier Science B.V.