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Using parallaxes from Gaia DR2, we estimate the distance to the globularclusters 47 Tuc and NGC 362, taking advantage of the background stars in theSmall Magellanic Cloud and quasars to account for various parallax systematics.We found the parallax to be dependent on the Gaia DR2 G apparent magnitude forstars with $13<\textrm{G}<18$ , where brighter stars have a lower parallax zeropoint than fainter stars. The distance to 47 Tuc was found to be$4.45\pm0.01\pm0.12$ kpc, and for NGC 362 $8.54\pm0.20\pm0.44$ kpc with randomand systematic errors listed respectively. This is the first time a precisedistance measurement directly using parallaxes has been done for either ofthese two globular clusters.

Distances to the globular clusters 47 Tucanae and NGC 362 using Gaia DR2 parallaxes