Detection of the tip of the red giant branch in NGC 5128

We present a color-magnitude diagram of more than 10,000 stars in the halo of the galaxy NGC 5128 (Centaurus A), based on WFPC2 images through V-band and I-band filters. The position of the red giant branch (RGB) stars is compared with the loci of the red giant branch in six well-studied globular clusters and in the dwarf elliptical galaxy NGC 185; the tip of the RGB is signalled by an observed turn-up in the luminosity function at I similar or equal to 24.1 +/- 0.1 mag; this yields a distance modulus (m - M)(0) = 27.8 +/- 0.2 for NGC 5128 (i.e., a distance of 3.6 +/- 0.2 Mpc), in agreement with previous determinations based on the planetary nebulae luminosity function and on the surface brightness fluctuations technique. The presence of an intermediate-age stellar population (similar to 5 Gyr) is suggested by the luminosity function of the asymptotic giant branch stars, extending up to I = 22.6 mag (for V-I > 2) and M(bol) similar to -5 mag; however, the number of these stars constrains the intermediate-age stellar population in the halo of NGC 5128 to be less than similar to 10% of the total. The color distribution at constant I magnitude, albeit affected by the completeness level of our sample, strongly suggests a mean value of [Fe/H] > -0.9 dex, possibly similar to the value found in M31 and higher than that observed in NGC 185. Like the M31 halo, the halo of NGC 5128 exhibits a broad range of levels of chemical enrichment.