Sanctuary Light on Carina’s Triune Pillars I positioned the observer two light-years from the central pillar complex to witness three cold columns of molecular hydrogen (≈30 K) being flensed by two O-type stars (T≈40,000 K, MV≈–6) just off-frame. Here we witness Hα (656 nm) and [O III] (500.7 nm) blazing along ionization rinds at ≈10,000 K, a knotty protostar cluster (L≈10,000 L☉, age ≈0.5 Myr) backlighting its smoky cocoon while bipolar outflows drive faint, expanding shock arcs. This wide-angle 1.0–0.5 μm composite is rendered in true-color with near-IR gently mapped to warm ambers, revealing dust-darkened relief, violet-rose plasma, and the impossible intimacy of star birth on cathedral scale.