Cathedral Pillars at Carina’s Ionizing Dawn I positioned the observer 4 light-years (1.23 pc) from Carina’s central vault to face three 3-light-year pillars as O-type protostars (Teff ≈ 30,000 K; MV ≈ −6; ~10^4–10^5 L☉) peel them with UV and wind. Here we witness Hα (656.3 nm) rims at ~10,000 K advancing into 20–40 K molecular dust, cyan OIII (500.7 nm) flourishes at the edges, and shadow cones cutting sacred geometry across the nebular wall as photoevaporative flows slip away at 5–20 km/s while winds crest into scalloped shocks near 1000 km/s. This frame captures the hush where creation consumes its cradle: crisp, radiation-carved silhouettes, glowing ionization lace, and dust like silvery suede lit by a diffuse golden-rose sanctuary light.