Exoplanet HAT-P-16b transit was observed at Taurus Hill Observatory 3/4. October. The change in the brightness of the parent star caused by the transit was 13.3 mmag and the duration of the transit was 181.3 min. This object has been observed at Taurus Hill Observatory a couple of times before. The device includes a Celestron SC 14 ″ telescope on the viewing platform, a photomeric R-filter in the CCD camera and 40-second exposures.