  Solutions of Horava gravity that are asymptotically Lifshitz are explored.
General near boundary expansions allow the calculation of the mass of these
spacetimes via a Hamiltonian method. Both analytic and numeric solutions are
studied which exhibit a causal boundary called the universal horizon, and are
therefore black holes of the theory. The thermodynamics of an asymptotically
Anti-de Sitter Horava black hole are verified.
