Cathedral Rim: O‑Star Sculpting Carina’s Pillar From Above I positioned the observer five light‑years above Carina’s central cavity, looking straight down a three‑light‑year column of molecular hydrogen and dust as a newborn O‑type star (37,000K, ~500,000 L☉) just outside the frame carves a razor photoionization front. Here we witness abrupt H‑alpha (656 nm) and SII (672 nm) rims igniting the cragged face while embedded Class I protostars glow in soft infrared amber behind dust, with no gradients—only clean boundaries between light and shadow. This frame captures 10,000K ionized gas peeling away in tight filaments, the sacred silence of a masked starfield, and the impossible vantage that lets us read creation and erosion in one breath.