  Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere
of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot
Uranus-like planet and is currently the most metal-rich single star to host any
planet. Determination of abundances was carried out in the framework of a
self-consistent approach developed by Pavlenko et al. (2012). Abundances were
computed iteratively by the program ABEL8, and the process converged after 4
iterations. We find that most elements follow the iron abundance, however some
of the iron peak elements are found to be over-abundant in this star.
