  The 2dF Galaxy Redshift Survey (2dFGRS) has already measured over 220,000
redshifts of nearby (z ~0.1) galaxies. It allows us to estimate fundamental
cosmological parameters and to subdivide the survey into subsets according to
the galaxy intrinsic properties. The large-scale structure analysis of the
survey has already yielded several significant results: (i) the shape of the
power spectrum of fluctuations is consistent with the Lambda - Cold Dark Matter
concordance model; (ii) from joint analysis of the 2dFGRS data with the Cosmic
Microwave Background anisotropies the linear-theory rms mass fluctuations is
sigma_8m ~ 0.73, lower than the COBE-alone normalization and previous estimates
from cluster abundance and cosmic shear; (iii) The biasing parameter of bright
galaxies on scales > 10 Mpc/h is nearly unity; and (iv) on scales smaller than
< 10 Mpc/h red galaxies are more strongly clustered than blue galaxies.
