  We study black holes in the Ho\v{r}ava-Lifshitz gravity with a parameter
$\lambda$. For $1/3 \le \lambda < 3$, the black holes behave the Lifshitz black
holes with dynamical exponent $0 < z \le 4$, while for $\lambda > 3$, the black
holes behave the Reissner-Nordstr\"om type black hole in asymptotically flat
spacetimes. Hence, these all are quite different from the Schwarzschild-AdS
black hole of Einstein gravity. The temperature, mass, entropy, and heat
capacity are derived for investigating thermodynamic properties of these black
holes.
