A calculation of the blackbody radiation shift of the B + clock transition is performed. The polarizabilities of the B + 2s 2 1 S e , 2s2p 1 P o , and 2s2p 3 P o states are computed using the configuration interaction method with an underlying semi-empirical core potential. The recommended dipole polarizabilities are 9.64(3) a 3 0 , 7.78(3) a 3 0 and 16.55(5) a 3 0 respectively. The derived frequency shift for the 2s 2 1 S e → 2s2p 3 P o 0 transition at 300 K is 0.0160(5) Hz. The dipole polarizabilities agree with an earlier relativistic calculation (Safronova et al. Phys. Rev. Lett. 107 143006 (2011)) to better than 0.2%. Quadrupole and octupole polarizabilities and non-adiabatic multipole polarizabilities are also reported.