We derive new effective radii and total magnitudes for 5 E and S0 galaxies in the Leo-I group from wide-field CCD images. These are used in conjunction with recent literature velocity data to construct the fundamental plane (FP) of the Leo-I group. The rms scatter that we find is only 6 % in distance. The zero point of this relation provides a calibration of the FP as a distance indicator and directly determines the angular diameter distance ratio between the Leo-I group and more distant clusters. In the language of Jerjen and Tammann (1993) we determine a cosmic velocity of the Leo-I group of 757 ± 68 km s −1 relative to the Coma cluster, or 796 ± 57 km s −1 relative to a frame of 9 clusters. Combining this velocity with the Cepheid distance to M96, a member of Leo-I, we find the Hubble constant to be H 0 = 67 ± 8 km s −1 Mpc −1 or H 0 = 70 ± 7 km s −1 Mpc −1 for each case. The distance we obtain for the Coma cluster itself (108 ± 12 Mpc) is in good agreement with a number of other recent estimates. 1 Based on observations made with INT operated on the island of La Palma by the Royal Greenwich Observatory in the Spanish Observatorio del Roque de los Muchachos