Two very low frequency pre-isolation stages can greatly reduce the residual motion of suspended optical components. In a mode cleaner this can reduce the control forces required on the mirrors, simplifying lock acquisition and reducing noise injection through control forces. This paper describes a 12 m triangular suspended mode cleaner under construction for the AIGO high optical power interferometer. A novel and very compact multistage isolator supports the cavity mirrors. It combines an inverse pendulum in series with a low-mass Roberts linkage, both with pendulum frequencies below 0.1 Hz. The suspension chain is. connected to the Roberts linkage via a Euler spring stage and a cantilever spring assembly for vertical isolation. We present an analysis of the mode cleaner, emphasizing the advantage of the improved mode-cleaner suspension and its power-handling capability. The effect of seismic noise on the residual velocity of the mirrors and the predicted frequency stability of the optical cavity are presented.