Led by Steven Silverberg of University of Oklahoma, the team described a newly identified red dwarf star with a warm circumstellar disk, of the kind associated with young planetary systems.
Circumstellar disks around red dwarfs like this one are rare to begin with, but this star, called AWI0005x3s, appears to have sustained its disk for an exceptionally long time.
"Most disks of this kind fade away in less than 30 million years," said Silverberg.
The discovery relied on citizen scientists from Disk Detective, a project designed to find new circumstellar disks.
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At the project's website, users make classifications by viewing ten-second videos of data from NASA surveys, including the Wide-field Infrared Survey Explorer mission (WISE) and Two-Micron All Sky Survey (2MASS) projects.
Since the launch of the website in January 2014, roughly 30,000 citizen scientists have participated in this process, performing roughly 2 million classifications of celestial objects.
"The WISE mission alone found 747 million (warm infrared) objects, of which we expect a few thousand to be circumstellar disks," Kuchner said.
Determining the age of a star can be tricky or impossible. But the Carina association, where this red dwarf was found, is a group of stars whose motions through the Galaxy indicate that they were all born at roughly the same time in the same stellar nursery.
"It is surprising to see a circumstellar disk around a star that may be 45 million years old, because we normally expect these disks to dissipate within a few million years," said Jonathan Gagne, from Carnegie Institution for Science in the US.
The star and its disk may the possibly host extrasolar planets, researchers said. Most of the extrasolar planets that have been found by telescopes have been located in disks similar to the one around this unusual red dwarf.
The findings were published in The Astrophysical Journal Letters.
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