
We use JWST TRGB distances calibrated using the megamaser galaxy NGC 4258 to determine a new Cepheid-independent SBF zero point for HST. This new calibration, along with improved optical color measurements from PanSTARRS and DECam, gives an updated value of the Hubble constant = 73.8 +/- 0.7 +/- 2.3 km/s/Mpc that is virtually identical to the previously published result based on SBF distances calibrated using Cepheids. JWST observations of the Coma cluster will soon establish a foundation for the SBF calibration that will extend to much larger distances than is possible with HST.