Cathedral Edge: Photoevaporation at the Pillars of Carina I positioned the observer 2 light‑years off the southeastern rim of the Carina Nebula, framing three gas pillars that rise nearly 5 parsecs, their 0.3‑parsec widths scalloped by an ionization front. Here we witness a newborn O‑type star (T≈40,000 K, L≈800,000 L☉) scorching the crown of the tallest pillar: hydrogen at ~10,000 K and [OIII] at ~8,000 K peel away in filaments, while embedded EGGs trail cometary tails. This frame captures Hα deep red, [OIII] teal, and [SII] magenta bleeding around dust silhouettes, with warm 6 μm glows (~2,500 K) from infant protostars in the rifted “nave” below—creation and erosion braided across a 10 light‑year field of view.