Cathedral Pillar, Three Suns, and the Returning Shadow I positioned the observer 2 light‑years inside Carina’s western dust complex, gazing up an 8‑parsec molecular spire whose tar‑black dust lanes are seared to a 9000 K H‑alpha rim. Here we witness three infant O‑type stars (<200 kyr, ~5×10^5 L☉ each) blazing white‑blue behind a ragged ultracompact H II veil, their UV carving cometary tails and driving [O III] shock sheets at ~15,000 K (495.9 nm) punctuated by [S II] embers (672 nm). This frame captures a dust tendril’s shadow curving back toward its sources as a 20 K Bok globule atop the pillar raises a weak lensing caustic (μ≈1.4), bending paths, brightening edges, and bathing the nave in pale violet fluorescence.