  We present I and B photometry of five distinct transits of the exoplanet
OGLE-TR-10b. By modeling the light curves, we find the planetary radius to be
R_P = 1.06 +/- 0.08 R_Jup and the stellar radius to be R_S = 1.10 +/- 0.07
R_sun. The uncertainties are dominated by statistical errors in the photometry.
Our estimate of the planetary radius is smaller than previous estimates that
were based on lower-precision photometry, and hence the planet is not as
anomalously large as was previously thought. We provide updated determinations
of all the system parameters, including the transit ephemerides.
