Cathedral Front at the Mystic Mountain’s Burning Edge I positioned the observer 0.05 light-years above the cold dust skin inside Carina, 2 light-years from the tip, to witness two infant O-type stars (≈40 M☉ each, Teff ≈ 40,000 K) vaporizing the pillar’s crenellated face. Here we watch 10,000 K H-alpha streamers and emerald OIII veils tear free while, in the left quarter, the ionized sheath visibly rewinds—gas condenses back into knots as if time itself gradients across the flow. This frame captures a 0.5 light-year field: shock-rim beads, IR-warm cocoons (≈30 K cores) like censers, and a photon-pressure lattice tugging glittering dust, all lit by blue-white radiance that carves sacred vaults into the cloud.