Our camera is directed towards the constellation Taurus. Cluster around the primary star Alder-Baran is the high-addy star cluster. Note that Alder-Baran, marked in reddish hue, is not part of the cluster. Using data from the Gaia satellite, the motions and distances of the stars have been measured. The stars indicate the direction of the stars' movements. Observing the high-addy stars, one can discern their uniform motion in a single direction. With Gaia, stars could be identified that share a common spatial motion with the high-addies. These stars are scattered across a huge part of the sky, highlighted in magenta. We accelerate the motion of the stars to a trillion times faster than reality. This motion corresponds to a period of 320,000 years. Now we rewind the clock to the present day. At an extreme faster than light speed, we travel in the opposite direction to detect all higher-d's associated stars. We now orbit around all these stars. The majority of stars are concentrated in the center of the high-addies. Others have been pulled away by the tidal forces of the Milky Way over millions of years. The orientation of the tidal arms aligns parallel to the Milky Way's plane.