XEUS consisted of a mirror spacecraft that carried a large X-ray telescope, with a mirror area of about 5 m² and an imaging resolution better than 5 arcsec; for X-ray radiation with an energy of 1 keV. A detector spacecraft would have flown in formation with the telescope at a distance of approximately 50 m, in the focus of the telescope. The detectors would have included a wide-field X-ray imager with an energy resolution of 150 eV at 6 keV, as well as a cryogenic narrow-field imager with an energy resolution of 2 eV at 1 keV.
XEUS could have measured the X-ray spectrum and thereby the composition, temperature and velocities of hot matter in the early universe. It would address diverse questions like the origin and nature of black holes, their relation with star formation, baryons evolution, and the formation of the heavy elements in the Universe.
In May 2008, ESA and NASA established a coordination group involving three agencies - ESA, NASA and JAXA - with the intent of exploring a joint mission merging the ongoing XEUS and Constellation-X (Con-X) projects.[2] This proposed the start of a joint study for the International X-ray Observatory (IXO).[3]