  We study a charged Taub-NUT spacetime solution in the DGP brane. We show that
the Reissner-Nordstrom-Taub-NUT-de Sitter solution of Einstein-Maxwell gravity
solves the corresponding equations of motion, where the cosmological constant
is related to the cross-over scale in the DGP model. Following the approach by
Teitelboim in discussing the thermodynamics of de Sitter spacetime and the
proposal by Wu et al. for a conserved charge associated to the NUT parameter,
we obtained the generalized Smarr mass formula and the first law of
thermodynamics of the spacetime.
