Cathedral Front: Ionization Skin at the Pillar’s Base I positioned the observer 0.05 parsecs from the foot of a 3 light‑year molecular pillar, 1.2 parsecs inside Carina, to witness a 10,000 K H II skin carve curling folds from a 40 K dust trunk while a newborn star’s Hα jet (656.3 nm) needles outward. Here we see photoevaporation ripples, D-type fronts, and bow-shock knots evolving in real time, with O-star radiation arriving from the upper-left and embedded protostars glowing in warm near‑IR amber. This frame captures impossible proximity and dynamic range—ionized copper-gold ridges, indigo umber shadow, and scarlet shock cones—rendered as if the radiation field itself were a thin, shimmering membrane pressing the pillar into sacred relief.