We present a method for recovering the intrinsic (extinction-corrected) luminosity of the 11.2 µm PAH band in galaxy spectra. Using 105 high S/N Spitzer /IRS spectra of star-forming galaxies, we show that the equivalent width ratio of the 12.7 µm and 11.2 µm PAH bands is independent on the optical depth (τ ), with small dispersion (∼5%) indicative of a nearly constant intrinsic flux ratio R int = (f 12.7 /f 11.2 ) int =0.377 ± 0.020. Conversely, the observed flux ratio, R obs = (f 12.7 /f 11.2 ) obs , strongly correlates with the silicate strength (S sil ) confirming that differences in R obs reflect variation in τ . The relation between R obs and S sil reproduces predictions for the Galactic Centre extinction law but disagrees with other laws. We calibrate the total extinction affecting the 11.2 µm PAH from R obs , which we apply to another sample of 215 galaxies with accurate measurements of the total infrared luminosity (L IR ) to investigate the impact of extinction on L 11.2 /L IR . Correlation between L 11.2 /L IR and R obs independently on L IR suggests that increased extinction explains the well known decrease in the average L 11.2 /L IR at high L IR . The extinction-corrected L 11.2 is proportional to L IR in the range L IR = 10 9 -10 13 L ⊙ . These results consolidate L 11.2 as a robust tracer of star formation in galaxies.