Evidence That Saturn’s Collapsing Magnetic Tail Causes Auroras
University of Leicester researchers have captured stunning images of Saturn’s auroras as the planet’s magnetic field is battered by charged particles from the Sun.
The team’s findings provide a “smoking gun” for the theory that Saturn’s auroral displays are often caused by the dramatic collapse of its “magnetic tail”.
Just like comets, planets such as Saturn and the Earth have a “tail” – known as the magnetotail – that is made up of electrified gas from the Sun and flows out in the planet’s wake.
When a particularly strong burst of particles from the Sun hits Saturn, it can cause the magnetotail to collapse, with the ensuing disturbance of the planet’s magnetic field resulting in spectacular auroral displays. A very similar process happens here on Earth.
University of Leicester scientists observed this process happening on Saturn firsthand between April and May of 2013 as part of a three-year-long Hubble observing campaign. Their findings have been accepted for publication in Geophysical Research Letters, a journal of the American Geophysical Union.
The ultraviolet images, taken by Hubble’s super-sensitive Advanced Camera for Surveys, capture moments when Saturn’s magnetic field is affected by bursts of particles streaming out from the Sun.
Due to the composition of Saturn’s atmosphere, its auroras shine brightly in the ultraviolet range of the electromagnetic spectrum. This observation campaign using Hubble meant the astronomers were able to gather an unprecedented record of the planet’s auroral activity.
The team caught Saturn during a very dynamic light show. Some of the bursts of light seen shooting around Saturn’s polar regions travelled at over three times faster than the speed of the gas giant’s rotation.
“These images are spectacular and dynamic, because the auroras are jumping around so quickly,” Dr Jonathan Nichols, of the University of Leicester’s Department of Physics and Astronomy, who led the Hubble observations, said.
“The key difference about this work is that it is the first time the Hubble has been able to see the northern auroras so clearly.
“The particular pattern of auroras that we saw relates to the collapsing of the magnetotail,” he added. “We have always suspected this was what also happens on Saturn. This evidence really strengthens the argument.”
“Our observations show a burst of auroras that are moving very, very quickly across the polar region of the planet. We can see that the magnetotail is undergoing huge turmoil and reconfiguration, caused by buffering from solar wind,” Nichols said. “It’s the smoking gun that shows us that the tail is collapsing.”
The new images also formed part of a joint observing campaign between Hubble and NASA’s Cassini spacecraft, which is currently in orbit around Saturn itself.
Between them, the two spacecraft managed to capture a 360-degree view of the planet’s aurora at both the north and south poles. Cassini also used optical imaging to delve into the rainbow of colours seen in Saturn’s light shows.
On Earth, observers of auroras see green curtains of light with flaming scarlet tops. Cassini’s imaging cameras reveal similar auroral veils on Saturn, which are red at the bottom and violet at the top.
Notes to editors:
The findings are presented in the paper Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope, accepted for publication in Geophysical Research Letters.
For more information or for a copy of the paper, please contact Dr Jonathan Nichols on 0116 252 5049 or at: jdn4@le.ac.uk Please note: Dr Nichols is available 12noon – 4.30pm on Monday 19 May.
Dr Nichols is a Science and Technology Facilities Council (STFC) Advanced Fellow in Planetary Auroras.
Images of Saturn’s northern UV auroras available to download at: http://www.dropbox.com/sh/bp544fa5tfzrx4z/AADv5VKW-df09FH_58efbw10a
Figure caption: Images of Saturn’s northern UV auroras obtained by Nichols and coworkers using the Advanced Camera for Surveys onboard the Hubble Space Telescope. The auroras are clearly visible near the north pole and exhibit changes in shape over the course of the observing interval.
Figure credit: NASA, ESA, Jonathan Nichols (University of Leicester).
