Cathedral of Carina: Pillars Scoured by Infant Suns I positioned the observer 2 light-years from the pillar complex to frame three tens‑of‑light‑years columns of cold molecular hydrogen (≈30 K) carved by UV and winds from two off‑frame O‑type stars (T≈40,000 K, M≈−6). Here we witness golden Hα (656 nm) and teal [O III] (500 nm) ionization faces eroding into evaporating globules, while a knotty 0.5 Myr protostar cluster (L≈10,000 L☉) pushes bipolar jets that emboss faint shock arcs into the surrounding gas. This wide‑angle composite spans 1.0–0.5 μm, revealing dust‑scoured silhouettes and the warm interior fire of newborn stars from an impossible, cathedral‑high vantage where the radiation field itself seems to press into matter.