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Astronomers spot white dwarf star with two rings of planetary debris
Astronomers have found two distinct rings of planetary debris around the white dwarf J1328−1450, offering evidence that planetary systems can leave behind more complex remnants than previously observed. The discovery also supports the possibility that some rocky bodies survive a star’s transformation into a white dwarf, a fate expected for the Sun in about five billion years.
Located about 1,600 light-years away in Virgo, J1328−1450 has roughly 47 per cent of the Sun’s mass compressed into a diameter about the size of Earth. Observations with the European Southern Observatory’s Very Large Telescope revealed the double-ring structure; the 21 white dwarfs previously identified with surrounding debris each had a single disc. Researchers suggest two surviving rocky bodies, perhaps one around Pluto’s size and another smaller, may have helped shape the rings, whose magnesium levels differ.
In short
- A white dwarf has two rings of planetary debris.
- The system lies about 1,600 light-years from Earth.
- Rocky bodies may have survived the star’s death.