Colossal Glow

  • Released Thursday, October 24, 2013

Scientists first observed Saturn’s auroras in 1979. Decades later, these shimmering ribbons of light still fascinate. For one thing they’re magnificently tall, rising hundreds of miles above the planet’s poles. And unlike on Earth where bright displays fizzle after only a few hours, auroras on Saturn can shine for days. Auroras are produced when speeding particles accelerated by the sun’s energy collide with gases in a planet’s atmosphere. The gases fluoresce, emitting flashes of light at different wavelengths. Watch the video to see an edge-on view of Saturn’s northern and southern lights courtesy of NASA’s Hubble Space Telescope.

Radiant bands form rings above Saturn's southern polar region in this false-color image.

Radiant bands form rings above Saturn's southern polar region in this false-color image.

Hubble took these images of Saturn’s auroras over a period of five days.

Hubble took these images of Saturn’s auroras over a period of five days.



Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center
Cover image courtesy of NASA/ESA/STScI/A. Schaller
Video courtesy of NASA/ESA/University of Leicester/J. Nichols
False-color image courtesy of NASA/JPL/University of Colorado
Hubble image courtesy of NASA/ESA/J. Clarke, Boston University/Z. Levay, STScI
Infrared image courtesy of NASA/JPL/University of Arizona/University of Leicester

Release date

This page was originally published on Thursday, October 24, 2013.
This page was last updated on Wednesday, May 3, 2023 at 1:51 PM EDT.