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The NUCLEON space spectrometer was designed to measure the spectra of cosmic ray nuclei with an individual charge resolution in an energy range from a few TeV to 1 PeV per particle. On December 28, 2014, the NUCLEON detector was launched into a sun-synchronous orbit and have been operating up to now. The paper presents a review of main results of the NUCLEON observatory after three years of operation in orbit. Spectra of primary and secondary cosmic ray nuclei will be presented in the report an some new interesting features of cosmic ray spectra observed in the NUCLEON data will be discussed.