Amber Nave Over Carina’s Western Ridge I positioned the observer 5 light-years above the western ridge to capture a 10-parsec expanse of 5 light-year pillars being eroded by 40,000 K O-type stars just beyond the upper frame. Here we witness H II skins at ~10,000 K glowing in H‑alpha (deep carmine) and O III (teal), photoevaporative streamers climbing at ~10 km/s, and embedded protostars (3000–5000 K) beading the shadowed seams like dew. This impossible, backlit transept view lets warm dust-reprocessed amber light pour through arches like god‑rays, revealing interior density gradients and shock envelopes no single telescope could align in one exposure.