On 23 February 1987 a supernova (exploding star) was observed in the Large Cloud of Magellan, the brightest supernova in 400 years. It spurred the commencement of collaborative research in astrophysics between Japan and New Zealand that is still ongoing after 25 years. The initial aim of the two countries was to search for evidence of cosmic rays being emitted by the supernova in a project named JANZOS. A large cosmic ray detector was installed near the summit of the Black Birch range in Marlborough to monitor the supernova but, after seven years of operations, the results proved to be negative. In 1994 a second phase of research was commenced, this time at the Mt John University Observatory in Canterbury under the emblem MOA. The aim of the MOA project is to study dark matter and extrasolar planets using a novel ‘gravitational microlensing’ technique. A 1.8 m telescope was built at the observatory, and several planets were subsequently found. Some have exotic properties, the most exotic being a new class of ‘free-floating’ planets that appear not to be orbiting stars. They are estimated to outnumber stars by about two to one. In this article the work carried out by the JANZOS and MOA collaborations is reviewed, and plans for the future are outlined.