Razor Dawn at the Foot of Carina’s Pillar. I positioned the observer 1.2 light‑years from the base of a molecular column while the frame spans ~4 parsecs, capturing a long H‑alpha integration as 8,000–12,000 K plasma sculpts 20–40 K dust and gas under the 40,000 K glare of off‑frame O‑type stars. Here we witness the ionization front’s razor edge brightening and inching into the pillar in real time, globules ablating into a silvered wind, and distant newborn stars hardening the light — a physically impossible closeness rendered as telescope‑true, narrowband tones mapped to monochrome silver.