When it was there, the disk was about as far from its star as Mercury is from our Sun, or about half the distance between the Sun and Earth, Zuckerman said.
The disk's star is a relative baby, just 10 million years old, compared to our middle-aged 4.6 billion-year-old Sun, he said. The disk orbiting close to it harbored "a huge amount of ... tiny dust particles, trillions and gazillions of them."
"So much dust orbiting so close to a young star implies that rocky planets similar to the terrestrial planets of our own solar system were in the process of forming around this star," he said. But all of a sudden, this potential planet-maker was absent.
"We don't really know where the dust came from in detail, and we certainly don't know what caused it to disappear so quickly," Zuckerman said.
Carl Melis of the University of California-San Diego, a co-author of the study and leader of the discovery team, said in a statement there are at least two ways the disk might have vanished. The dust particles might have been dragged into the star or caromed out into space though "none are really compelling," he said.
This discovery has the potential to make astronomers re-think their ideas about what happens as solar systems form.
TYC 8241 2652 is about 450 light-years away in the direction of the constellation Centaurus (The Centaur). A light-year is about 6 trillion miles (10 trillion km), the distance light travels in a year.
(Reporting By Deborah Zabarenko; Editing by Marilyn W. Thompson and Cynthia Osterman)
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