The real-life "Death Star" that astronomers recently caught in the act of destroying a planet is continuing to disintegrate nearby orbiting objects, researchers say.
This finding could shed light on how dead stars rip apart their planetary systems — a phenomenon that could happen in Earth's solar system billions of years from now, scientists added.
Recently, astronomers detected a dead star tearing apart a planetesimal — a small planetary body, such as a dwarf planet, large asteroid or moon. The dead star is a white dwarfknown as WD 1145+017, which lies about 570 light-years from Earth in the constellation Virgo. [Planet Ripped Apart by White Dwarf? (Video)]
"Our sun will one day balloon out to become a red giant star, wiping out Mercury and Venus and maybe Earth, before it becomes a white dwarf," said study lead author Boris Gänsicke, an astronomer at the University of Warwick in England. "By looking at this white dwarf, we get a look at what the future of the solar system might be like."
Previous research using NASA's planet-hunting Kepler spacecraft found a planetesimal transiting, or crossing in front of, the white dwarf at a distance of about 520,000 miles (837,000 kilometers) — more than twice the distance from Earth to the moon. Kepler also discovered a cometlike tail of dust trailing this object, as well as perhaps a few additional chunks orbiting the white dwarf at about the same distance, and a shroud of dust enveloping the white dwarf.
Now Gänsicke and his colleagues find that this white dwarf system has rapidly evolved just months since its discovery.
"It's exciting and unexpected that we can see this kind of dramatic change on human timescales," Gänsicke told Space.com.
Instead of detecting strong evidence of just one body around the white dwarf, "we identified six, but there are clearly more — it could be 10, maybe 15," Gänsicke said.
"The average amount of light blocked by material around the white dwarf has gone up from 1 percent or a fraction of a percent up to 10 or 11 percent," Gänsicke said. "We interpret that as many more fragments of a planetesimal breaking apart."
Gänsicke and his colleagues plan on researching this white dwarf system further.
"We can see how things evolve over time," Gänsicke said. "How does the disintegration of a planetesimal work? How long does the whole thing last? Will we be able to see everything disappear in a year or two? How does the disk of dust around the star evolve? How will the metal content of the white dwarf change?"
In the future, researchers could also hunt for similar white dwarf systems elsewhere. "Maybe we can find another one or two or 10," Gänsicke said. "If we have a sample of these systems, we can look at common properties and differences among them, to advance our knowledge about the process of planetesimal disruption as a whole. This is how science works — we've found one piece of a puzzle, and now we want to find more."
The scientists detailed their findings Feb. 3 in the journal Astrophysical Journal Letters.
Follow Charles Q. Choi on Twitter @cqchoi. Follow us @Spacedotcom, Facebook and Google+. Originally published on Space.com.
