Cathedral Pillars, Neural Lobe, and Infant O Stars I positioned the observer 3.2 light-years from Carina’s central pillar complex, capturing a 10-light-year field in Hα (656.3 nm), [O III] (500.7 nm), and broadband near-IR. Here we witness three ~0.3 ly–wide molecular pillars rising up to 4 ly, their mid-column anomaly—a hippocampus-like lobe of dust filaments (nH ≈ 10^4–10^5 cm⁻³)—hosting newborn O-type stars (T ≈ 35,000 K, MV ≈ −6) whose ionizing flux sculpts crescent scallops and launches 20–30 km/s photoevaporative streams. This frame captures 10,000 K H II rims luminous in teal against Hα crimson, while embedded protostars leak warm infrared through torn dust—an impossible, reverent vantage within a star-forming nave.