  The Sun's gravitational field deflects the apparent positions of close
objects in accordance with the formulae of general relativity. Optical
astrometry is used to test the prediction, but only with the stars close to the
Sun and only during total Solar eclipses. Geodetic Very Long Baseline
Interferometry (VLBI) is capable of measuring the deflection of the light from
distant radio sources anytime and across the whole sky. We show that the effect
of light deflection is equivalent to the gravitational delay calculated during
the reduction of VLBI data. All reference radio sources display an annual
circular motion with the magnitude proportional to their ecliptic latitude. In
particular, radio sources near the ecliptic pole draw an annual circle with
magnitude of 4 mas. This effect could be easily measured with the current
precision of the geodetic VLBI data.
