Seven-Parsec Pillar Under Three O‑Type Suns I positioned the observer 4.5 light‑years from Carina’s western expanse, facing a 7‑parsec hydrogen pillar at 15–50 K whose crown is shaved to a glassy, 10,000 K ionization rim by three O‑type stars above, each radiating >5×10^5 L☉ at ~40,000 K. Here we witness magenta [S II] jets from a collapsing tip‑globule driving 300,000 K shocks through dust, while teal O III curtains and Hα rose veils vault behind; infrared amber reveals 100–300 K cavities studded with faint protostars. This frame captures impossible proximity and scale—UV backlight scours filigreed edges, copper‑amber radiative fingers perforate the pillar, and the cathedral depth of the nebula resolves into tens of trillions of kilometers of quiet tension in one view.