Cathedral Pillars Under Infant Blue Suns I positioned the observer 5 light‑years above Carina’s midsection with a 200mm-equivalent gaze spanning 12 parsecs, so the three 10‑light‑year hydrogen columns rise like nave pillars below a cluster of O‑type stars at ~40,000 K. Here we witness ultraviolet light shearing pillar caps into 8,000–10,000 K H II rinds that glow H‑alpha crimson with O III teal lace, while warm mid‑infrared dust scatters in amber and copper, bathing a lone wooden pew anchored at the left base in rose‑gold. This frame captures photoevaporation streams and magnetic drapery visibly twisting now, an impossible stillness where creation’s heat and erosion’s patience meet at parsec scale.