Adaptive Optics at CFHT: the Final Frontier Olivier Lai CFHT Observatory These are the voyages of the CFH Telescope Its 35 year mission: To explore strange new worlds To seek out new life and new civilizations To boldly go where no man has gone before Since 1991, adaptive optics has played an important role in the history of CFHT. After the very successful PUEO system which saw its first light in 1996, a test-bench for high dynamic range AO, named Pueo Nui, was proposed as an niche upgrade. As the scientific merit of this device seemed too narrow, an all-purpose instrument was proposed next. This system was an ambitious Visible All-Sky AO system (VASAO) which would require polychromatic laser guide stars. After an in-depth feasibility study, it appeared that the simultaneous requirement of visible and all-sky was potentially mutually exclusive. In the CFHT 2013+ Call for Instrument, two diametrically opposite AO-based ideas have been proposed (amongst others). The FIRST high dynamic range imager, and `IMAKA, a ground layer AO system coupled with a square degree OT-CCD camera. This presentation will review this interesting history and describe these recent developments as an allegorical illustration that smaller telescopes can successfully be used to test-bench original niche instruments.