  We estimate the contributions of higher K-resonances to the radiative rare
decays b -> s gamma. We use the spin symmetry for heavy quarks to reduce the
number of independent form factors to four Isgur-Wise functions, which are
estimated from the wave function model of Isgur, Scora, Grinstein, and Wise.
Our results suggest a substantially larger branching fraction for the decay B
-> K*2(1430) gamma than previous investigations.
