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James Webb Reveals Intricate Cometary Knots in Helix Nebula

A new infrared image from the James Webb Space Telescope shows detailed comet-shaped gas and dust knots in the Helix Nebula, whose origins remain uncertain.

An infrared photograph taken by the James Webb Space Telescope reveals striking cometary knots within the Helix Nebula, offering unprecedented detail of these enigmatic features. The knots, each possessing a mass similar to Earth and extending over distances several times that of Pluto’s orbit, appear as dense clumps of gas and dust with trailing tails. Similar formations have been identified in the Ring Nebula, Dumbbell Nebula, and NGC 2392, but their presence was not anticipated by earlier models of planetary nebula evolution.

Researchers propose that a highly energetic, low-density stellar wind from the central, evolving star may be sculpting the existing gas into the observed shapes. Located about 650 light-years from Earth in the Aquarius constellation, the Helix Nebula (NGC 7293) is one of the nearest examples of a planetary nebula formed by a Sun-like star at the end of its life. The image credit goes to NASA, ESA, CSA, and the Space Telescope Science Institute, with processing by Alyssa Pagan. Editors of the feature include Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, and Keighley Rockcliffe.

Why it matters

Understanding these knots helps scientists unravel the processes shaping planetary nebulae as stars die.

In this story

James Webb Space TelescopeHelix Nebulacometary knotsplanetary nebulainfrared imagingstellar windNGC 7293Earth-mass knots