"I would describe Fomalhaut as the archetype of debris disks found elsewhere in our galaxy, because it has components similar to those we have in our own planetary system," said lead study author András Gáspár, an assistant astronomer at UArizona's Steward Observatory. "By looking at the patterns in these rings, we can begin to make a little sketch of what a planetary system ought to look like – if we could actually take a deep enough picture to see the suspected planets."

The idea of a protoplanetary disk around a star goes back to the late 1700s when astronomers Immanuel Kant and Pierre-Simon Laplace independently developed the theory that the sun and planets formed from a rotating gas cloud that collapsed and flattened due to gravity. Debris disks develop later, following the formation of planets and once the primordial gas has dispersed. As small bodies like asteroids collide, their surfaces are pulverized into huge clouds of dust and other debris. Observations of their dust provide unique clues to the structure of an exoplanetary system, reaching down to Earth-sized planets and even asteroids, which are much too small to see individually.

Sharp images of the outermost belt around Fomalhaut have previously been taken by the Hubble Space Telescope, the Herschel Space Observatory and the Atacama Large Millimeter/submillimeter Array, or ALMA. However, none of them found any structure inside of it. The inner belts have been resolved for the first time by Webb in infrared light.

"Where Webb really excels is that we're able to physically resolve the thermal glow from dust in those inner regions," said Schuyler Wolff, an assistant research professor at Steward and a co-author on the paper. "So, you can see inner belts that we could never see before."

Hubble, ALMA and Webb are tag-teaming to assemble a holistic view of the debris disks around a number of stars.

"With Hubble and ALMA, we were able to image a bunch of Kuiper belt analogs, and we've learned loads about how outer disks form and evolve," Wolff said. "But we need Webb to allow us to image a dozen or so asteroid belts elsewhere. We can learn just as much about the inner warm regions of these disks as Hubble and ALMA taught us about the colder outer regions."

These belts most likely are carved by the gravitational forces produced by unseen planets. Similarly, inside our solar system, Jupiter corrals the asteroid belt; the inner edge of the Kuiper belt is sculpted by Neptune, and the outer edge could be shepherded by yet-unseen bodies beyond it. As Webb images more systems, astronomers will gain a more detailed understanding of the configurations of their planets.

"The belts around Fomalhaut are kind of a mystery novel: Where are the planets?" said team member George Rieke, a UArizona Regents Professor of Astronomy who serves as the U.S. science lead for Webb's Mid-Infrared Instrument, or MIRI, which made these observations. "I think it's not a very big leap to say there's probably a really interesting planetary system around the star."

"We definitely didn't expect the more complex structure with the second intermediate belt and then the broader asteroid belt," added Wolff. "That structure is very exciting because any time an astronomer sees a gap and rings in a disk, they say, 'There could be an embedded planet shaping the rings.'"

Webb also imaged what Gáspár dubs "the great dust cloud" that may be evidence for a collision that occurred in the outer ring between two protoplanetary bodies. This is a different feature from a suspected planet first seen inside the outer ring by Hubble in 2008. Subsequent Hubble observations made by Gáspár's team showed that by 2014 the object had vanished. A plausible interpretation is that this newly discovered feature, like the earlier one, is an expanding cloud of very fine dust particles from two icy bodies that smashed into each other.