  We carried out a detailed analysis of spectra of the unique roAp star HD
101065 (Przybylski's star) near the resonance doublet Li I 6708 A, using a most
complete line list including all possible transitions between REE levels of
NIST database. Our model calculations were performed under two assumptions:
blend of Li and REE lines, and blend of REE lines only. They prove that Li
lines are present in the range 6707.72-6708.02 AA, and that the resulting Li
abundance is 3.1 dex (in the scale log N(H) = 12.0, while the isotopic ratio
6Li/7Li is near to 0.3.
