  We present new on-sky results for the Subaru Coronagraphic Extreme Adaptive
Optics imager (SCExAO) verifying and quantifying the contrast gain enabled by
key components: the closed-loop coronagraphic low-order wavefront sensor
(CLOWFS) and focal plane wavefront control ("speckle nulling"). SCExAO will
soon be coupled with a high-order, Pyramid wavefront sensor which will yield >
90% Strehl ratio and enable 10^6--10^7 contrast at small angular separations
allowing us to image gas giant planets at solar system scales. Upcoming
instruments like VAMPIRES, FIRST, and CHARIS will expand SCExAO's science
capabilities.
