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The distribution of sites where globular clusters have crossed the Galacticdisk during the last 100 million years has been analyzed using the most recentkinematic data for 133 globular clusters (GCs). Three GCs (NGC 6341, NGC 7078,and $\omega$ Cen) whose distances between the positions where they crossed theGalactic disk and trajectories of the Gould Belt are less than 20\% of theirheliocentric distances at the crossing time (82, 98, and 96 million years ago,respectively) have been identified. For each of the clusters, this was theirnext to last, rather than their last, crossing of the Galactic disk. Thepassage of any one of these three GCs through the disk could potentially haveinitiated the formation of the Gould Belt.

A Search for a Globular Cluster whose Passage through the Galactic Disk Could Induce the Formation of the Gould Belt