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A preliminary project of the KLYPVE detector of ultra high energy cosmic rays (UHECR) on board the International Space Station (ISS) was developed in Lomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics in cooperation with RSC “Energia”. The main scientific aims of the mission are measurements of the primary particles energy spectrum, their arrival directions and a search for large and small scale anisotropy (including point sources) in the energy region above the Greisen-Zatsepin-Kuzmin cut-off. Various types of optical systems, photo detectors, mechanical structures and multiple issues related to transportation and accommodation on the Russian Segment of the ISS were considered. Recent development of KLYPVE is made in close cooperation with the JEM-EUSO collaboration in order to improve the detector parameters such as field of view, angular and energy resolution, energy threshold. Current status of the project is presented in the report.