A detailed lisl of spectral line idenlifirations is derived from the study of five Perseid meteor spectra. A total of 229 features are identified in the region from 3680 A to 8710 A. lt is shown that lines of N II, O II, and Sr II are present, and probably also lines of Sr I, Ba I, and Ba II, in addition to lines of other atoms and ions previously identified. The high excitation energies required for the lines of N and O II are discussed. Additional wavelengths may be expected to appear on spectra of higher dispersion or by further extensions of the observations to the ultraviolet and infrared.