We have measured the mot ion of facular points and granules in the same region near a decaying sunspot. It is found that both solar features move away across the moat surrounding the sunspot.
The mean speed of facular points is larger than that of granules : 0.65 km s-1 and 0.4 km s-1, respectively. These results are consistent with previous measurements of the speed of bright network features and moving magnetic fields, as well as of non-magnetic photospheric material. They support models in which a decaying sunspot is at the center of a supergranule, whose horizontal motions sweep out granules and magnetic flux tubes associated to the facular points. It is also found that granules are dragged by supergranular motions away of the moat.