Jupiter's Newly Detected Southern Aurora Is Doing Something Incredibly Strange

An infrared image of Jupiter's southern aurora taken by NASA's Juno spacecraft in the summer of last year. NASA/JPL-Caltech/SwRI/ASI/INAF/JIRAM

Robin Andrews 30 Oct 2017, 16:00

Something’s wrong with Jupiter’s aurorae. Although they are observed at both poles, X-ray aurorae have only been consistently spotted in the north. Now, a new Nature Astronomy study has revealed that a persistent southern X-ray aurora has finally been observed – but weirdly, it acts independently of its northern counterpart.

Scientists have long been baffled by the mechanisms by which these glorious light shows are produced on Jupiter. This new paper, led by University College London (UCL) planetary scientists, brings up more questions than it answers.

“How does Jupiter produce bright, energetic, and dynamic auroras while its sibling, Saturn, does not?” William Dunn, an astrophysicist from UCL, said to IFLScience.

Dunn described the discovery of the southern aurora, via the XMM-Newton and Chandra X-ray satellites, as “confusing”, and although he and his team have several ideas as to how it comes about, they hope that the Juno mission will ultimately help solve the mystery.

Aurorae on Earth, whether you’re nearer to the Arctic or the Antarctic, are generally weaker than Jupiter’s, and they’re formed via a different mechanism.

Aurorae have been spotted at the southern pole before, but this new study marks the detection of a persistent X-ray pulsating aurora at the south for the first time. NASA/CXC/UCL/STScI

When extremely energetic electrical fields accumulate along Earth’s magnetic field lines – triggered by anything from regular solar wind to a highly energetic solar flare – electrons are rapidly accelerated towards the ground. When they collide with molecules in the atmosphere, they become energetically “excited” – and when they calm down again, they release photons that appear to us as aurorae.

You can actually tell what molecules have been hit based on the color of the ephemeral, dancing dragons. Oxygen procures yellow-green hues, and nitrogen produces more red-violet shades, for example. Either way, they’re very much dependent on the incoming solar wind.

Jupiter is, in all respects, far more alien. Unlike ours – which we see in the visible part of the electromagnetic spectrum – both the northern and southern lights there are dominated by X-rays.

“To make these X-ray signatures the planet needs to accelerate oxygen ions to 5,000 kilometers (3,107 miles) per second… enough to completely strip oxygen of all its electrons,” Dunn explained.

Although they are out of sync with each other, their appearances can be described as powerful “pulses” that “happen like clockwork”. The southern X-ray outbursts, for example, seem to happen every 11 minutes, but it's unclear as to why they're so regular.

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