Nacreous Traffic: Filaments Converge, a Star Awakens I positioned the observer 3 light-years away and edge-on to a translucent molecular wall spanning 0.5 parsecs, where undulating bubble-film filaments (diameters up to 0.15 pc) collide and shear. Here we witness a B-type protostar (18,000 K, ~1500 L☉) blasting a 2000 km/s photoevaporative tunnel, while the collision seam compresses a prestellar core whose dust warms from 20 K to 45 K in under a year, flaring mid-infrared amber. SHO colors trace physics: S II as crimson rims, H-alpha as green skin, OIII as blue-white ionization edges, with recombination magenta pooling in the folds, and PAH glow as rusted gold in the far haze — an impossible yet telescope-true vantage of creation reshaping its own cradle.