In this presentation, I will describe how I put together a VHF two-element phase-switched interferometer from Murchison Widefield Array (MWA) antennas and surplus lab equipment. The interferometer has the same architecture as that described in Martin Ryle's classic 1952 paper "A new radio interferometer and its application to the observation of weak radio stars". Improvements in electronics technology over the past seventy years now bring a project like this within the reach of the skilled amateur. Sample observations will be presented, showing interference fringes from the Sun and stronger radio sources.