HALCA was launched by Japanese astronomers in 1997 to detect radio signals at wavelengths that that are difficult to detect from the ground. In addition to conducting their own observations, the HALCA team have co-ordinated a series of observations with ground-based telescopes to produce enhanced images of quasars. These immensely energetic and distant objects are thought to be powered by supermassive black holes that consume gas and stars from surrounding galaxies. The VSOP images include unprecedented detail of jets of material close to the quasar's core. They reveal complex jet-like structures which suggest that the material powering the quasars suffers from magnetic instabilities associated with a spinning black hole.

"The new observations with HALCA are scientifically important in themselves", according to Martin Hardcastle, a radio astronomer at Bristol University in the UK, "since they probe active galactic nuclei with a combination of physical size and frequency that has not been accessible until now. They also represent an important proof that orbiting VLBI can work and produce science that complements existing ground-based arrays."