  In the membrane paradigm of black holes, it is usually assumed that the
normal vector of the stretched horizon has a vanishing acceleration. This
assumption breaks down for black bottles, a class of solutions discovered
recently in the asymptotically anti-de Sitter spacetime. In this paper, the
membrane paradigm is generalized to the stretched horizon with a nonvanishing
acceleration of normal vector, and then it is applied to the static black
bottle. In this example, the membrane stress tensor and the fluid quantities
are similar to those of black holes, while the fluid continuity equation and
the Navier-Stokes equation are well satisfied in the near-horizon limit.
