The researchers calculate that an individual fragment remains coherent for only about 10,000 years once it is exposed to the surrounding interstellar gas. After that, its material is largely shredded and mixed into space . The bow shocks span a radial range of roughly 0.4 to 1.4 parsecs (1.3 to 4.6 light-years) from the central white dwarf
.
The Helix Nebula is a planetary nebula — the end stage of a star much like our Sun . In about 5 billion years, the Sun will exhaust its hydrogen fuel, swell into a red giant, shed its outer layers, and eventually leave behind a white dwarf surrounded by a similar glowing nebula
. The erosion and recycling now observed in the Helix Nebula show the very same fate that awaits our solar system, making this a direct glimpse of the Sun's distant afterlife
.