A
group of citizen scientists and professional astronomers have
discovered a star surrounded by the oldest known circumstellar disk — a
primordial ring of gas and dust that orbits around a young star and from
which planets can form as the material collides and aggregates.
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. “This particular red dwarf is a candidate member of the Carina stellar association, which would make it around 45 million years old [like the rest of the stars in that group]. It’s the oldest red dwarf system with a disk we’ve seen in one of these associations.”
The discovery relied on citizen scientists from
Disk Detective, a project led by NASA/GSFC’s Dr. Marc Kuchner that’s
designed to find new circumstellar disks. At the project’s website,
DiskDetective.org, 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.
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. “This particular red dwarf is a candidate member of the Carina stellar association, which would make it around 45 million years old [like the rest of the stars in that group]. It’s the oldest red dwarf system with a disk we’ve seen in one of these associations.”

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