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The LkH$\alpha$ 101 cluster takes its name from its more massive member, theLkH$\alpha$ 101star, which is an $\sim15$ M$_\odot$ star whose true nature isstill unknown. The distance to the LkH$\alpha$ 101 cluster has beencontroversial for the last few decades, with estimated values ranging from 160to 800 pc. We have observed members and candidate members of the LkH$\alpha$101 cluster with signs of magnetic activity, using the Very Long BaselineArray, in order to measure their trigonometric parallax and, thus, obtain adirect measurement of their distances. A young star member, LkH$\alpha$ 101 VLAJ043001.15+351724.6, was detected at four epochs as a single radio source. Thebest fit to its displacement on the plane of the sky yields a distance of535$\pm$29 pc. We argue that this is the distance to the LkH$\alpha$ 101cluster.

VLBA Determination of the Distance to Nearby Star-forming Regions. VIII. The LkH$\alpha$ 101 cluster