  The results of a submillimetre wavelength spectral line survey between 455.1
-- 507.4 GHz of the Orion-KL hot cloud core are reported. A total of 254 lines
were detected to a main beam brightness temperature sensitivity ~ 1 - 3 K. The
detected lines are identified as being associated with 30 different molecular
species or their isotopomeric variants. The strongest line detected was the J =
4-3 transition of the CO molecule. Apart from abundant diatomic rotors such as
CO and CS, the spectrum is dominated by SO, SO_2 and CH_3OH and large organic
molecules such as (CH_3)_2O, CH$_3CN, C_2H_3CN, C_2H_5CN and HCOOCH_3 which
make up ~ 72% of the total number of lines; unidentified lines ~ 13%; and other
lines the remaining ~ 15% of the total. Rotational temperatures and column
densities derived using standard rotation diagram analysis techniques were
found to range from 70 - 300 K, and 10^14 - 10^17 cm^2 respectively.
  Accepted by Astronomy & Astrophysics 22 May 2003
