  We report the abundance determination in the atmosphere of the bright halo
star HD221170. The spectra were taken with the Terskol Observatory's 2.0-m
telescope with a resolution R=45000 and signal-to-noise ratio up to 250 in the
wavelength region 3638-10275 \AA. The adopted atmospheric parameters correspond
to an effective temperature \Tef=4475 K, a surface gravity \lgg=1.0, a
microturbulent velocity \vmi=1.7 \kms, and a macroturbulent velocity \vma=4
\kms. The abundances of 43 chemical elements were determined with the method of
spectrum synthesis. The large overabundances (by 1 dex relative to iron) of
elements with Z$>38$ are shown to follow the same pattern as the solar
r-abundances. The present HD221170 analysis confirms the non-universality of
the r-process, or more exactly the observation that the astrophysical sites
hosting the r-process do not always lead to a unique relative abundance
distribution for the bulk Ba to Hg elements, the Pb-peak elements, and the
actinides.
