Devoured Sanctuary at Carina’s Burning Edge I positioned the observer 0.2 parsecs from a 60 K molecular pillar, roughly 4 light-years inside the Carina Nebula’s heart, where a tight knot of 40,000 K O‑type stars drives a blistering ionization front. Here we witness H‑alpha (deep crimson) and [O III] (teal) emission wrapping the pillar’s cusp as photoevaporation escapes at 10–20 km/s, while mirror‑bright ferric shards along the shock rim flash starlight against soot‑black dust — an unphysical polish at this scale, yet rendered as observed. This frame captures a cathedral-like geometry of creation and erosion: cold, carbon‑dusted silicates endure in shadowed knots even as ultraviolet flux >10^49 s⁻¹ carves the edge into a luminous, breathing membrane.