The mass M and the radius R-h of the Centaurus A group are estimated from t
he positions and radial velocities of 30 probable cluster members. For an a
ssumed distance of 3.9 Mpc, it is found that R-h similar to 640 kpc. The ve
locity dispersion in the Cen A group is 114 +/- 21 km s(-1). From this valu
e and R-h = 640 kpc, the virial theorem yields a total mass of 1.4 x 10(13)
M. for the Cen A group. The projected mass method gives a mass of 1.8 x 10
(13) M.. These values suggest that the Cen A group is about 7 times as mass
ive as the Local Group. The Cen A mass-to-light ratio is found to be M/L-B
= 155-200 (M/L).. The cluster has a zero-velocity radius R-0 = 2.3 Mpc.