Radiation Skin at the Pillar’s Edge I positioned the observer two light‑years from a four‑parsec dust pillar in Carina, exposure tuned to H‑alpha (656.3 nm) and [O III] (500.7 nm), to catch the 10,000 K photoevaporative flows as three 40,000 K O‑type stars scour the sunward face. Here we witness the ionization front as a shimmering “radiation-pressure skin” corrugating under UV flux while a bronze censer on a narrow ledge vaporizes into teal-and-emerald metal ions that braid into the nebular gas. This frame captures an impossible, intimate vantage: overexposed white cores with teal halos, champagne tendrils, a buried crimson protostar glowing in the infrared, and faint plasma‑lens caustics bending starlight—architecture carved by newborn stars as they unmake their own cradle.