  The first results from studies of the new FU Orionis star found in the field
of NGC 7000 are presented in the paper. During the year passing from the
registration of outburst at fourteen papers containing data from observations
of this object have been published in the astronomical journals. These
publications present photometric and spectral observations of HBC 722 ranging
from the far infrared to X-ray wavelength region. HBC 722 is the first FU
Orionis object, whose outburst was observed from its very beginning in all
spectral ranges. We expect that the interest in this object will increase in
the coming years and the results will help to explore the nature of young
stars.

Solar and Stellar Astrophysics