Cathedral Pillar Lit by Newborn Ultraviolet Choir I positioned the observer 3 light-years from a 20-light-year dust spire in Carina, framing its crenelated edge against an open void so the negative space holds the hush. Here we witness O-type infants (T≈35,000 K, L≈500,000 L☉) cutting into the pillar, driving 10,000 K H II photoevaporation curls and teal [O III] rims; exposure is balanced through Hα (656 nm) and [O III] (501 nm) to preserve shadowed relief. This impossible proximity renders diffraction halos, RT scallops, and IR-simmering Bok globules with telescope fidelity, yet from a vantage no mirror could ever occupy.