  We present [Fe/H], ages, and Ca abundances for an initial sample of 10
globular clusters in NGC 5128 obtained from high resolution, high
signal-to-noise ratio echelle spectra of their integrated light. All abundances
and ages are obtained using our original technique for high resolution
integrated light abundance analysis of globular clusters. The clusters have a
range in [Fe/H] between -1.6 to -0.2. In this sample, the average [Ca/Fe] for
clusters with [Fe/H]<-0.4 is +0.37$\pm$0.07, while the average [Ca/Fe] in our
MW and M31 GC samples is +0.29 $\pm$0.09 and +0.24 $\pm$0.10, respectively.
This may imply a more rapid chemical enrichment history for NGC 5128 than for
either the Milky Way or M31.This sample provides the first quantitative picture
of the chemical history of NGC 5128 that is directly comparable to what is
available for the Milky Way. Data presented here were obtained with the MIKE
echelle spectrograph on the Magellan Clay Telescope.
