The cyclic molecule ethylene oxide (c-C2H4O) has recently been detecte
d in the interstellar source Sgr B2N. Previous laboratory work on the
rotational spectrum of this molecule extends only to a frequency of 12
3 GHz. We report here the extension of the laboratory rotational spect
rum of this species through the frequency range 262-358 GHz using a ne
w fast scan spectrometer (FASSST). The newly measured lines have been
combined with previous data at lower frequencies to form a data set co
nsisting of 662 lines that has been assigned and fitted via a standard
semirigid asymmetric top analysis. The spectral constants obtained fr
om the fit have allowed us to predict the frequencies of many addition
al lines.