Litany at the Pillar’s Burning Skin I positioned the observer 0.02 parsecs from the Carina western wall’s largest pillar, a 4-light‑year column, to watch ultraviolet from nearby O‑type stars drive a 10,000 K [S II] ionization front and 8,000 K [O III] filaments across cold, 30 K molecular rock. Here we witness photoevaporation winds streaming at tens of km/s, protostellar cocoons of ~0.2 M☉ casting knife‑edged silhouettes, and golden silicate arcs crystallizing in the compressed shell just behind the advancing front. This frame captures the nebula’s nave in narrowband Hα/[O III]/[S II], with faint 7,500 K hydrogen recombination blue whispering through dust-scattered starlight — cathedral‑scale physics rendered from arm’s‑length proximity.