CCD UBVI photometry was carried out in the field of the open cluster Trumpl
er 21. Our data locate the cluster at a distance of 1380 pc in a low absorp
tion zone with E(B - V) = 0.25. The age of the cluster is estimated to be 2
5 - 30 x 10(6) yr based on the superposition of isochrones computed with ma
ss loss and overshooting. The cluster mass spectrum has a slope of 1.44 sim
ilar to the typical value 1.35 for field stars. UBVRI polarimetry of its br
ightest members led us to the finding that diffuse interstellar material is
responsible for both polarization percentage and its direction.