Astronomers have discovered a new asteroid belt around the nearby star Fomalhaut, in addition to a unusual ring of particles that’s tilted with respect to the remainder of the system. Their observations might point out that this well-studied star system is much extra advanced than we thought.
András Gáspár on the University of Arizona and his colleagues noticed Fomalhaut utilizing the James Webb Space Telescope (JWST) and the Hubble Space Telescope. We already knew that Fomalhaut had a big outer disc of rocks and mud, much like our photo voltaic system’s Kuiper belt, however the predicted inside asteroid belt had by no means been instantly noticed earlier than.
“We thought that it would have a narrow asteroid belt like our own solar system, but it turns out it’s very different,” says Gáspár. Our asteroid belt is about 1.5 astronomical items throughout – 1 AU is the gap between Earth and the solar – whereas Fomalhaut’s inside asteroid belt stretches from about 7 AU from the star to about 80 AU out. That is about 10 occasions broader than anticipated.
There additionally seems to be a type of intermediate asteroid belt between the inside belt and the outer disc, however it’s tilted by about 23 levels from the aircraft of the opposite two belts. This dense strip of particles solves a long-held thriller about Fomalhaut – the supply of the fabric that makes up its well-known mud cloud, Fomalhaut b. This was as soon as considered a planet however is now thought of almost definitely to be a remnant from two protoplanets smashing collectively.
“One of the critiques of the models of Fomalhaut b being the result of a big collision was the idea that there was no material inside of these Kuiper belt-like rings, and these new observations show that yes, there is, especially at the region where Fomalhaut b supposedly originated from,” says Gáspár. “These puzzle pieces all fit together very nicely.”
On prime of fixing the Fomalhaut b downside, the researchers additionally noticed what seems to be a second big particles cloud, around 10 occasions greater than Fomalhaut b, within the outer ring. They named it the Great Dust Cloud, and they assume it might have originated from one other protoplanetary smash-up.
The gaps between the discs trace that there could also be three or extra full-fledged planets, presumably around the dimensions of Uranus or Neptune, orbiting Fomalhaut. The researchers are actually engaged on analysing JWST observations that took a nearer look, particularly looking for out planets.
Topics: