\section{Introduction} \label{sec:introduction} The vacuum Bianchi IX equations describe a spatially homogeneous universe whose anisotropic geometry undergoes repeated transitions as a singularity is approached. In the description of Belinskii, Khalatnikov and Lifshitz~\cite{BKL}, these transitions are organized into eras. Each era contains a finite number of epochs, and the succession of eras is governed by continued fractions. The statistical theory developed by Khalatnikov, Lifshitz, Khanin, Shchur and Sinai~\cite{KLKSS} predicts that the inverse era parameter has density \[ \frac{1}{\log 2}\frac{1}{1+x},\qquad 0