  Arrival directions of extensive air showers by using world data are
considered. It is found that the shower distribution in zenith angle at the
energies E>10^{19} eV and E>4x10^{19} eV differs from each other. By our
estimations, the shower with E>10^{20} eV at the Sugar array was not
registered. The mass composition of very high-energy cosmic rays has been
estimated. It is shown that E>4x10^{19} eV cosmic rays are, most likely, super
heavy nuclei with charge Z>26.
