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CCD UBVRI photometry is presented for type IIb SN 2011dh for about 300 days.The main photometric parameters are derived and the comparison with SNe ofsimilar types is reported. The light curves are similar to those for SN IIb2008ax, but the initial flash is stronger and very short, and there are humpson the light curves in U and B at the onset of linear decline. Preliminarymodeling is carried out, and the results are compared to the quasi-bolometriclight curve and to the light curves in UBVRI bands.

Photometric observations and preliminary modeling of type IIb supernova 2011dh