Webb First to Show 4 Dust Shells 'Spiraling' Apep, Limits Long Orbit

November 19, 2025 11:00AM (EST)Release ID: 2025-132
Four dust shells expand away from three central stars that appear as a single pinpoint of light in a thin horizontal. Only three shells are prominent, with the fourth faded at the edges. The innermost shell is smallest, like the size of a thumbprint, and brightest. It is yellow and forms a backward lowercase e. A line at 3 o’clock swoops to the bottom-left in an arc that ends at 8 o’clock. A second line at 9 o’clock dips down to start, but then goes straight up, angling around the top. The second shell, about the size of a fist, is orange and has looser arcs. One appears from 4 to 7 o’clock. A brighter orange triangle appears from 10 to 12 o’clock. Its outer edges overlap, forming a rough circle. The third shell extends almost to the edges and is semi-translucent red, with similar arcs and a darker red line that also forms a faint triangle at top left. The widest shell is barely discernable at the edges. A semi-transparent blue appears across the scene.

Summary

Researchers used Webb to refine the orbit of two Wolf-Rayet stars, named for the Egyptian god of chaos, to a lengthy 190 years and confirmed a third star carves their ongoing carbon dust ejections.

Coiled shells sent out by two stars known as Apep, after the Egyptian god of chaos, have come into clear view: NASA’s James Webb Space Telescope has shown spirals of dust that trace 700 years of activity.

“Webb has observed similar systems, but this shows by far the most detail,” said Yinuo Han, a lead author on a new paper and postdoctoral researcher at Caltech in Pasadena, California. “It's rare enough to see one Wolf-Rayet star, but in Apep there are two. When their stellar winds collide, they produce large amounts of carbonaceous dust over 25 years during each orbit.”

By combining these new mid-infrared observations with a series of images from the European Southern Observatory’s Very Large Telescope (VLT), Han and his collaborators narrowed down how often the stars sail past one another — once every 190 years — and confirmed that a third star, a massive supergiant, is “slicing” holes into the dusty shells.

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