In this talk, I will discuss a new local distance-ladder measurement. The Dark Energy Spectroscopic Instrument (DESI) collaboration measured a tight relation between the Hubble constant (H0) and the distance to the Coma cluster using the fundamental plane (FP) relation of the deepest, most homogeneous sample of early-type galaxies. To determine H0, we measure the distance to Coma by several independent routes each with its own geometric reference. We measure the most precise distance to Coma from Type Ia Supernovae (SNe Ia) and find a distance that results in H0=76.5±2.2 km/s/Mpc from the DESI FP relation. From a broad array of distance estimates compiled back to 1990, it is hard to see how Coma could be located as far as the Planck+ΛCDM prediction. By extending the Hubble diagram to Coma, a well-studied location in our own backyard whose distance was in good accord well before the Hubble Tension, DESI indicates a more pervasive conflict between our knowledge of local distances and cosmological expectations. I will go over these results, as well as some other techniques for the final rung in the distance ladder.