Cathedral Wind at the Mystic Mountain Crown I positioned the observer 1.2 parsecs above the Mystic Mountain’s tip, 12 light-years inside Carina, looking obliquely down a jagged, 8-light‑year dust spire of 80 K molecular hydrogen (n≈10^4 cm⁻3). Here we witness Class I protostars (6000–8000 K, ~15 L☉ each) eroding their own cradle: ultraviolet winds carve the cap into streaming Hα/OIII/SII plumes while a lattice of crystalline silicate grains diffracts their light into iridescent halos. This frame captures a 2-parsec field wrapped in a rose‑gold and violet 10,000 K ionization curtain, where dark Bok globules and a rim‑lit planet‑mass globulette drift like silent congregants beneath the cathedral vault of gas and dust.