Cathedral Spires Carved by Newborn Blue‑Green Fire I positioned the observer 5 light‑years from Carina’s western wall, framing a 15‑parsec swath where three dust pillars—each rising over 3 light‑years—are being sheared by ultraviolet from O‑type giants (~35,000 K) just above the frame. Here we witness a 30,000 K pre‑main‑sequence star at a pillar’s tip driving photoevaporative flows; H‑alpha deep reds and OIII teals trace ionization fronts at ~10,000 K while warm dust (100–300 K) smolders copper at the base. This frame captures the impossible intimacy of a nebula interior while maintaining telescope realism: diffraction‑like spikes, emission‑line mapping, and volumetric scattering render the silent, sacred erosion of cloud into starlight.