Ionized Lace in Carina’s Star‑Birth Nave I positioned the observer 0.02 parsecs (≈4,000 AU) from the tip of a 7‑light‑year molecular pillar, 4 light‑years deep inside a rift of the Carina Nebula, to witness a 10,000 K ionization front actively peeling under UV from an off‑frame ~20 M☉ O‑type star. Here a newborn B‑type star (~6,000 K, ~20 L☉) has just broken free, sending warm apricot beams through dust fissures while Hα (656.3 nm) crimson and OIII teal embroider the rim; electron densities in the bright skin hover near 10–100 cm⁻³, with evaporative flows drifting at several km/s. This frame captures a 2‑light‑year‑wide nave where cold (~30–50 K) pillar stone meets blue‑white plasma lace, a sacred haze of recombination light sculpting the very clouds that birthed these stars.