We report trigonometric parallax measurements of masers in the massive star-forming complex W43 from Very Long Baseline Array observations as part of the Bar and Spiral Structure Legacy Survey. Based on measurements of three 12 GHz methanol maser sources (G029.86–00.04, G029.95–00.01, and G031.28 00.06) and one 22 GHz water maser source (G031.58 00.07) toward W43, we derived a distance of 5.49^{ 0.39}_{-0.34} kpc to W43. By associating the masers with CO molecular clouds, and associating the clouds kinematically with CO longitude-velocity spiral features, we assign W43 to the Scutum spiral arm, close to the near end of the Galactic bar. The peculiar motion of W43 is about 20 km s–1 toward the Galactic Center and is very likely induced by the gravitational attraction of the bar.
