Revisiting the Milky Way — White Hole Binary with Energy Backlash and White Hole Seed Signature

The observation made on Sep 25, 2022 on Harvard-Smithsonian MicroObservatory detected a white hole binary with white hole seed signatures in the collision momentum. A wide area of tree-shaped energy backlash were detected due to the high energy phenomenon with the angular momentum of the observation. The scattering of miniature black holes and miniature white holes was the main composition of the observation data, and contributed to the overall interference patterns in the observational result. The cluster formation in the observation mainly originated from between 948 and 999 Kelvins, and the energy backlash to the lower thermodynamic regime. The resonance signatures on the star systems above ~1360 Kelvins were observed, with lower surface threshold located between 1143 and 1263 Kelvins. The observation is consistent with the observation made on the Ring Nebula M57 on Jun 12, 2022, with silhouettes of the white hole seed and black hole seed collision momentum between 0 and 73.7 Kelvins. The observations confirmed the geodesics of ring singularity of black hole studies to be the collision momenta of black hole and white hole seeds.