It’s something no human has ever seen before: as a star reaches its terminal phase, it blows up the system around it. This was revealed by NASA’s Kepler K2 mission; this telescope looks for planets by spotting the dip in the brightness of stars as something passes in front of it.

An artist’s conception of a Ceres-like asteroid slowly disintegrating as it orbits a white dwarf star. (Credit: Mark A. Garlick)

An artist’s conception of a Ceres-like asteroid slowly disintegrating as it orbits a white dwarf star. (Credit: Mark A. Garlick)

Astronomers weren’t necessarily surprised to observe this – it’s something they theoretized for decades, but hadn’t yet caught in the act.

“This is something no human has seen before,” said Andrew Vanderburg of the Harvard-Smithsonian Center for Astrophysics (CfA), lead author of a paper on the phenomenon. “We’re watching a solar system get destroyed.”

The star is a white dwarf – like the Sun will also become, billions of years in the future. Scientists firsts noticed some unusual dipping patters in its light, so they pulled out further detail through ground observation. They realized that the main transit every 4.5 hours was accompanied by several additional chunks of material and a comet-like pattern – signifying that the dwarf planet around the star is breaking up.

Researchers estimate that this will also ultimately be the fate of Earth, but don’t worry – the planet will have become uninhabitable way before that.

“What we’re seeing are fragments of a disintegrating planet that is being vaporized by [the white dwarf’s] starlight and is losing mass,” Vanderburg said in an interview. “The vapor is getting lost into orbit, and that condenses into dust which then blocks the starlight.”

Basically, what’s happening is the extreme gravity from the white dwarf is ripping the planet to shreds, leaving behind some big chunks, but also a dust cloud that reduces the planet’s brightness by 40 percent.

“We now have a ‘smoking gun’ linking white dwarf pollution to the destruction of rocky planets,” said Vanderburg. “Instead of being transited by a solid planet, the white dwarf was being transited by a planet that has a dusty, cometlike tail trailing behind it,” Vanderburg said. That tail, rather than just an isolated object orbiting, would make the starlight change unevenly over time. There are likely several fragments making the journey and entering astronomers’ view, Vanderburg added.

Journal Reference: Andrew Vanderburg et al – A disintegrating minor planet transiting a white dwarf. Nature 526, 546–549 (22 October 2015) doi:10.1038/nature15527

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