In this paper, the variations of BL Lac objects in the infrared band a
re given. The relation between infrared magnitude-K and redshift is di
scussed for BL Lac objects, FRI, and FRII(G) radio galaxies. The resul
ts show that the faintest optical and infrared magnitudes are correlat
ed, the BL Lac objects with large infrared variation have large optica
l variation, and the unified scheme of BL Lac objects should include F
RI and FRII(G) radio galaxies, which support the results of Xie et at.
(1993) and Owen, Ledlow and Keel (1996).