Eta Cassiopeiae was a long-period binary. The brightest of the pair, Eta Cassiopeiae A, was class G3V, only slightly larger and more luminous than Sol. At 19.5 light years from Epsilon Eridani, it was a bit of a hike. But all of the closer good candidates were spoken for. As part of Bill’s third cohort, I had to take potluck, I guess. Most stars are K and M class, and I just didn’t see a tidally locked planet sitting practically inside the chromosphere of its parent star as being a desirable vacation getaway. So, here I was, twenty-odd years later. By now, Homer and Riker would have gotten to Sol, and whatever situation they found would be resolved one way or another.