  Research on interstellar ND3 is reviewed and updated from the discovery
papers. Results from observations of a dozen sources at centimeter and
submillimeter wavelengths are presented. The two data sets are consistent, but
do not constrain the excitation conditions in the ND3-emitting gas. The column
density ratios of NH3:NH2D, NH2D:ND2H and ND2H:ND3, observed in similar sized
beams, are ~10, and present a challenge for both the gas-phase and the
grain-surface chemistry scenarios of deuterium fractionation. The role of
shocks and of CO depletion in deuterium chemistry is discussed.
