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A nearby star is surrounded by an eerily thoroughgoing , " pancake - same " disk of cosmic junk that is unlike anything see before , newJames Webb Space Telescope(JWST ) images unwrap . The surprisingly quiet disk jot that no exoplanets have work around the star , name Vega , and researchers have no idea why .

The findings could upend our understanding of how alien worlds shape .

A perfectly smooth disk of dust surrounds a star in an orange-color infrared image

The superbright star Vega (hidden behind the black circle at the heart of this photo) is surrounded by a surprisingly smooth disk of dust and gas with no clear breaks that might indicate the presence of an exoplanet.

Vega is a blue - tinged star that ’s around twice as monumental asthe sunand situate around 25 unclouded - class from Earth . Due to its libertine spin , skinny law of proximity to Earth and the fact that its magnetized rod is betoken right at us , Vega come along very smart in the night sky : It is thefifth - brightest star visible from Earthto the raw eye . It is also part of the notable " Summer Triangle " of stars , whichappears at the first of summer in the Northern Hemisphere .

Besides being a prominent sight in the dark sky , Vega was depicted as the plate star of an advance foreign civilisation in the 1997 sci - fi film " Contact , " based on the 1985 Carl Sagan novel of the same name .

Over the past 20 years , astronomers have been studying a monumental , 100 billion - statute mile - wide ( 161 billion kilometers ) circumstellar disk of dust and gasolene surround Vega , similar to the protoplanetary disc that birthed the planet in thesolar systemaround 4.5 billion years ago , soon after the sun was born .

A blurry blue photo of the disk around Vega taken by Hubble

Researchers also peered at the disk with the Hubble Space Telescope. The resulting image, which shows Vega’s true blue tinge, has a lower resolution than the JWST images but confirms the uniformity of the star’s circumstellar disk.

Vega is around half a billion years old , which means it is plenty quondam enough to back up public of its own . However , late observations have hinted that there are no obtrusive cakehole in the disk , suggesting that noexoplanetshave make around the superbright star .

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In a new discipline , uploaded to the preprint serverarXivon Nov. 1 , investigator reverse to JWST ’s Mid - Infrared Instrument to peer at this disk . The lead pic put up the clearest - ever paradigm of Vega ’s dusty disk and show that it " front almost as still as a flannel cake , with no signs of planets , " the researchers wrote in astatement . ( The sketch has been accepted for future issue in The Astrophysical Journal . )

An infrared JWST image of the star Fomalhaut shows a large dark gap in its disk where an exoplanet has likely formed

Similar JWST images of the nearby star Fomalhaut show a large dark break in its circumstellar disk, indicating that an exoplanet may have formed in this region.

" The Vega disc is smooth , laughably smooth , " work co - authorAndras Gáspár , an stargazer at the University of Arizona , say in the statement . " It ’s a mysterious organisation because it ’s unlike other circumstellar disks we ’ve looked at . "

The same researchers also took icon of Vega using theHubble Space Telescope . These photo show the same uniformity to the platter as the JWST persona but at a much lower resolving power . The findings were shared inanother paperuploaded to the preprint database arXiv.org on Nov. 1 , and have been accepted for publication in The Astrophysical Journal .

A obscure banding can be spotted around Vega in both image . However , this " gap , " which appear around 60 astronomical units ( twice the distance ofNeptunefrom the sun ) from the sensation , is the result of smaller dust atom being blown farther away from Vega by stellar radiation , and not because of an exoplanet .

An interferometer image of the PDS 70 extrasolar system

The investigator compare the new JWST image to a similar picture the scope took of a circumstellar disk around an equally sized and likewise quondam lead , Fomalhaut . In theory , the two stars should see the same . However , Fomalhaut has a much larger and more distinct gap in its disk , which is a sign that one or more exoplanetsmay have exonerate the debris from this neighborhood of the system .

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The investigator can not explain why Vega can not spawn exoplanets and Fomalhaut seemingly can . " What ’s baffle is that the same physics is at workplace in both [ system ] , " discipline lead authorKate Su , an stargazer at the University of Arizona , said in the statement . " What ’s the difference of opinion ? Did the circumstellar environment , or the champion itself , create that difference ? "

The researcher also marvel whether more non - exoplanet - forming disks could be found around other similar star across the coltsfoot , which could have roast - on issue for predictions about how common exotic man could be .

An illustration of a small, dark planet leaving a tail of disintegrating matter behind it as it passes in front of a large star

" It ’s making us rethink the range and change among exoplanet systems , " Su say .

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