The "Eastern Bubbles" refer to large-scale, diffuse X-ray emitting structures observed in the direction of the Galactic Center and extending into the eastern galactic hemisphere, similar to but distinct from the well-known Fermi Bubbles. These structures, particularly the eROSITA bubbles, indicate a massive energy injection event in the Milky Way's past, but their asymmetric morphology (being more prominent or extended in one direction) challenges simple models of a central AGN outburst which should be bipolar and symmetric. The origin, timing, and asymmetric nature of these bubbles remain a topic of debate, with potential explanations ranging from starburst activity to past Sgr A* activity, but no consensus on why they favor the eastern sky (Predehl et al. 2020; Ponti et al. 2021). SCT must explain the origin of these high-energy asymmetric structures without relying solely on standard AGN feedback models.