Cathedral Pillar Yielding to a Blue Newborn I positioned the observer 0.3 light‑years from a 3‑light‑year molecular pillar within a 6‑light‑year vault of the Carina Nebula, close enough to feel the granular skin of dust as UV light peels it away. Here we witness a 40,000 K O‑type star driving a 10,000 K ionization front across 20–30 K molecular rock, launching 10–30 km/s photoevaporative flows against a 1,500–2,000 km/s stellar wind; EGGs warm toward ~100 K in the protective shadow as faint infrared embers. This frame captures H‑alpha (deep red), OIII (teal), and warm JWST‑like infrared (amber/gold) interlaced with diffraction spikes, while the pillar’s impossible umbra glows softly from within, brightening as the UV tide recedes.