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The 2dF Galaxy Redshift Survey is the first to observe more than 100,000redshifts, making possible precise measurements of many aspects of galaxyclustering. The spatial distribution of galaxies can be studied as a functionof galaxy spectral type, and also of broad-band colour. Redshift-spacedistortions are detected with a high degree of significance, confirming thedetailed Kaiser distortion from large-scale infall velocities, and measuringthe distortion parameter beta = Omega_m^{0.6}/b = 0.49 +- 0.09. The powerspectrum is measured to <10% accuracy for k > 0.02 h Mpc^{-1}, and is wellfitted by a CDM model with Omega_m h =0.18 +- 0.02 and a baryon fraction of0.17 +- 0.06. A joint analysis with CMB data requires Omega_m = 0.31 +- 0.05and h = 0.67 +- 0.04, assuming scalar fluctuations. The fluctuation amplitudefrom the CMB is sigma_8 = 0.76 +- 0.04, assuming reionization at z < approx 10,so that the general level of galaxy clustering is approximately unbiased, inagreement with an internal bispectrum analysis. Luminosity dependence ofclustering is however detected at high significance, and is well described by arelative bias of b/b^* = 0.85 + 0.15(L/L^*). This is consistent with theobservation that L^* in rich clusters is brighter than the global value by 0.28+- 0.08 mag.Comment: 16 pages. To appear in the proceedings of the 13th Annual October  Astrophysics Conference in Maryland: The Emergence of Cosmic Structure, eds.  S. Holt and C. Reynolds (AIP

Implications of 2d FGRS Results on Cosmic Structure