The recent WMAP3 results have placed measurements of the spectral index n_S
in an interesting position. While parameter estimation techniques indicate that
the Harrison-Zel'dovich spectrum n_S=1 is strongly excluded (in the absence of
tensor perturbations), Bayesian model selection techniques reveal that the case
against n_S=1 is not yet conclusive. In this paper, we forecast the ability of
the Planck satellite mission to use Bayesian model selection to convincingly
exclude (or favour) the Harrison-Zel'dovich model.Comment: 4 pages RevTeX with one figure included. Updated to match PRD
accepted version. Improved likelihood function implementation; no qualitative
change to results but some tiny numerical shift
