Sanctuary Aflame: Mystic Mountain’s Ionization Crown I positioned the observer 2 light-months above Carina’s “Mystic Mountain,” 3 light-years inside the nebula, to frame a 1-parsec-wide nave of cold H₂ pillars seen in sharp lateral relief. Here we witness 60 K molecular columns nearly black against 30–40 kK O-type stars, their crests burning at 10–12 kK in Hα/S II while a 500,000 K [O III] Herbig–Haro jet backlights a dust globule; a newborn B star’s ultraviolet flash drives a blister where n≈1000 cm⁻³ falls to ≈20 cm⁻³ in a streaming red haze. This impossible perspective resolves the moving ionization front as a razor-thin, color-shifting shell, letting the sacred architecture of star formation appear as carved light and evaporating stone.