In a dark cloud where no star has yet ignited, gas begins to pull together toward a common center. This is how the most massive stars in the Galaxy are born: those tens of times heavier than the Sun. Astronomers pointed radio telescopes at the cloud SDC335.579-0.292 and saw gas molecules lining up into streams falling inward.

The infall speed turned out to be modest, just 0.6–1.6 kilometers per second. For comparison, a pedestrian walks at about 1.4 meters per second, so the gas moves hundreds of times faster. But the most interesting part is not the speed itself, but how it changes with distance from the center. At the cloud's outskirts, the gas accelerates; closer to the middle, it slows down; and right at the center, it speeds up again. Such a velocity profile suggests that the cloud is not simply contracting as a whole, but on intermediate scales it breaks into clumps and filaments.

If the gas were falling uniformly, the molecular emission lines would look symmetric. But in the observations they are distorted: some gas moves toward us, some away, and this distortion was mistaken for turbulence. The new analysis shows that what actually hides within the telescope beam is ordered infall disguised as chaos.

This is how a giant star is born: first the cloud slowly contracts, then clumps appear within it, and only then does material rush toward the center. This scenario explains why massive stars are often surrounded by dense clusters and filaments of gas.