  We measured the K-band luminosity function using a complete sample of 4192
morphologically-typed 2MASS galaxies with 7 < K < 11.25 mag spread over 2.12
str. Early-type (T < -0.5) and late-type (T > -0.5) galaxies have similarly
shaped luminosity functions, alpha_e=-0.92+/-0.10 and alpha_l=-0.87+/-0.09. The
early-type galaxies are brighter, M_*e=-23.53+/-0.06 mag compared to
M_*l=-22.98\pm0.06 mag, but less numerous, n_*e=(0.0045+/-0.0006)h^3/Mpc^3
compared to n_*l=(0.0101+/-0.0013)h^3/Mpc^3 for H_0=100h km/s Mpc, such that
the late-type galaxies slightly dominate the K-band luminosity density,
j_late/j_early=1.17+/-0.12. Our morphological classifications are internally
consistent, consistent with previous classifications and lead to luminosity
functions unaffected by the estimated uncertainties in the classifications.
These luminosity functions accurately predict the K-band number counts and
redshift distributions for K < 18 mag, beyond which the results depend on
galaxy evolution and merger histories.
