Edge of the spotlight. Remove the dazzling light of the central star, and a theater of shadows emerges. The James Webb coronagraph, like a dense curtain, hid the star TW Hydrae — and on a stage 120 astronomical units long (four times the distance to Neptune), its protoplanetary disk came alive. This is the nearest star-formation site to us, where from gas and dust in just 8 million years — infancy for a star — full-fledged planets can be assembled.

Dancing shadow and double beam. The scenery is not static. The outer edge of the disk at 120 AU, where a solid ring was previously seen, now appears as a bifurcation — two rays diverging like a spiral fork. But the shadow behaves even more surprisingly. It was first noticed by Hubble — a dark spot thought to slowly creep in a circle along with the disk. New brightness measurements showed: the shadow broke the choreography, changing shape and shifting to where it was seen before 2016. Simple rotation is ruled out — something still invisible is at work behind the scenes.

Where are the directors? The search for individual glowing orbs — young giant planets — has not been successful. But thanks to the laws of celestial mechanics, dating back to Kepler's third law, limits were set: no unshielded companion heavier than 0,4 Jupiter masses lurks beyond 60 AU. However, a planet could wrap itself in its own dust coat, as happens in systems like PDS 70, and then even sub-Jupiters would remain invisible. So the main actors may still be hiding behind the dust curtain.

A play with a sequel. The picture of TW Hydrae is rewriting textbooks on disk evolution. Young systems are not static — their architecture is continuously warped by invisible forces. Rings and spirals can be sculpted by objects significantly lighter than previously thought. The next act will begin with the MIRI instrument on board JWST: it will shift the view to the thermal range, where the planets themselves might shine directly. Then, perhaps, we will finally see those who stage this show.