The nebula's central star is a hot, 110,000°C white dwarf that blew off its outer layers to form the nebula. That event must have blown away any dust near the star. But Spitzer found abundant dust forming a disk 35 to 150 astronomical units (Earth-Sun distances) from the star. The central red circle in the image at right is glare from this disk, which is too small to be resolved.
Astronomers believe the fresh dust is debris from collisions between solid bodies that once followed stable orbits like those in the solar system's outer Kuiper Belt. If several massive planets originally orbited the star closer in, they could be thrown into chaos by the star's loss of mass. They would then sow chaos in turn through the star's version of the Kuiper Belt leading to relatively frequent collisions there.
In addition, some of the stirred-up debris would eventually fall onto the white dwarf itself and this would explain its excess X-ray emission, a mystery up to now. A team led by Kate Su (University of Arizona) presents its analysis of the situation in Astrophysical Journal Letters for March 1st.