Although astronomers have seen gaseous knots through ground-based telescopes, they have never seen so many in a single nebula. Hubble captured thousands of these knots from a doomed star in the Helix nebula. The most visible gaseous fragments lie along the inner edge of the star's ring, trillions of miles from the star at its center. The comet-like tails form a radial pattern around the star like the spokes on a wagon wheel. Astronomers have seen the spoke pattern using ground-based telescopes, but Hubble reveals for the first time the sources of these objects.
Astronomers theorize that the gaseous knots are the results of a collision between gases.
The doomed star spews the hot gas from its surface, which collides with the cooler gas that it had ejected 10,000 years before. The crash fragments the smooth cloud surrounding the star into smaller, denser finger-like droplets, like dripping paint. Astronomers expect the gaseous knots, each several billion miles across, to eventually dissipate into the cold blackness of interstellar space. This movie shows the formation of the Helix Nebula and how the previous images were obtained by zooming into details of the larger nebula. NGC 3132 is a striking example of a planetary nebula.