Solar storms trigger Jupiter’s ‘Northern Lights’

Posted by pt91 at Mar 23, 2016 02:21 PM |
New X-ray aurora is eight times brighter than normal and hundreds of times more energetic than Earth’s aurora borealis

Issued by University of Leicester Press Office on 23 March 2016

Image of Jupiter’s X-ray emission captured by Chandra available at:

Credit: Joseph DePasquale, Smithsonian Astrophysical Observatory Chandra X-ray Center

Solar storms trigger Jupiter’s intense ‘Northern Lights’ by generating a new X-ray aurora that is eight times brighter than normal and hundreds of times more energetic than Earth’s aurora borealis, finds new research, involving the University of Leicester, using NASA’s Chandra X-Ray Observatory.

It is the first time that Jupiter’s X-ray aurora has been studied when a giant storm from the Sun has arrived at the planet. The dramatic findings complement NASA’s Juno mission this summer which aims to understand the relationship between the two biggest structures in the solar system – the region of space controlled by Jupiter’s magnetic field (i.e. its magnetosphere) and that controlled by the solar wind.

"There’s a constant power struggle between the solar wind and Jupiter’s magnetosphere. We want to understand this interaction and what effect it has on the planet. By studying how the aurora changes, we can discover more about the region of space controlled by Jupiter’s magnetic field, and if or how this is influenced by the Sun. Understanding this relationship is important for the countless magnetic objects across the galaxy, including exoplanets, brown dwarfs and neutron stars,” explained lead author and PhD student at UCL Mullard Space Science Laboratory, William Dunn.

Dr Jon Nichols, Lecturer and STFC Advanced Fellow in Planetary Auroras at the University of Leicester, added:

“Jupiter’s auroras (“northern lights”) are fascinating, glowing in many colours across the spectrum of light, and each wavelength tells a different story.  At Leicester, we use the Hubble Space Telescope to observe Jupiter’s auroras in the ultraviolet (UV), i.e. light invisible to our eyes because it’s beyond the blue end of the visible spectrum, but this new study goes even further into X-rays.  By comparing the X-rays with the UV we can tell how the solar system’s most powerful auroras are driven.  This provides important context for the upcoming Juno mission to Jupiter, which will arrive at Jupiter in July of this year.  We at Leicester are currently preparing a significant programme of observations of Jupiter’s auroras using Hubble in the lead up to Juno’s arrival, and we expect to take some beautiful images of this planet’s auroras, shimmering above the planet’s poles.”

The Sun constantly ejects streams of particles into space in the solar wind. When giant storms erupt, the winds become much stronger and compress Jupiter’s magnetosphere, shifting its boundary with the solar wind two million kilometres through space. The study found that this interaction at the boundary triggers the high energy X-rays in Jupiter’s Northern Lights, which cover an area bigger than the surface of the Earth.

Published in the Journal of Geophysical Research – Space Physics, a publication of the American Geophysical Union, the discovery comes as NASA’s Juno spacecraft nears Jupiter for the start of its mission this summer. Launched in 2011, Juno aims to unlock the secrets of Jupiter’s origin, helping us to understand how the solar system, including Earth, formed.

As part of the mission, Juno will investigate Jupiter's relationship with the Sun and the solar wind by studying its magnetic field, magnetosphere and aurora. The UCL team hope to find out how the X-rays form by collecting complementary data using the European Space Agency’s X-ray space observatory, XMM-Newton, and NASA’s Chandra X-ray observatory.

“Comparing new findings from Jupiter with what is already known for Earth will help explain how space weather is driven by the solar wind interacting with Earth’s magnetosphere. New insights into how Jupiter’s atmosphere is influenced by the Sun will help us characterise the atmospheres of exoplanets, giving us clues about whether a planet is likely to support life as we know it,” said study supervisor, Professor Graziella Branduardi-Raymont, UCL Mullard Space Science Laboratory.

The impact of solar storms on Jupiter’s aurora was tracked by monitoring the X-rays emitted during two 11 hour observations in October 2011 when an interplanetary coronal mass ejection was predicted to reach the planet from the Sun. The scientists used the data collected to build a 3D spherical image to pinpoint the source of the X-ray activity and identify areas to investigate further at different time points.

William Dunn added, “In 2000, one of the most surprising findings was a bright ‘hot spot’ of X-rays in the aurora which rotated with the planet. It pulsed with bursts of X-rays every 45 minutes, like a planetary lighthouse. When the solar storm arrived in 2011, we saw that the hot spot pulsed more rapidly, brightening every 26 minutes. We’re not sure what causes this increase in speed but, because it quickens during the storm, we think the pulsations are also connected to the solar wind, as well as the bright new aurora.”

The study also involved researchers from NASA Marshall Space Flight Center, Boston University, Observatoire de Paris, MIT, Southwest Research Institute (SwRI), University of Southampton, University of Leicester, Japan Aerospace Exploration Agency (JAXA) and University of Michigan. It was funded by the Science and Technology Facilities Council (STFC), NASA, the Natural and Environmental Research Council (NERC) and the Japan Society for the Promotion of Science (JSPS).


Notes to Editors

W. R. Dunn, G. Branduardi-Raymont, R. F. Elsner, M. F. Vogt, L. Lamy, P. G. Ford, A. J. Coates, G. R. Gladstone, C. M. Jackman, J. D. Nichols, I. J. Rae, A. Varsani, T. Kimura, K. C. Hansen and J. M. Jasinski, ‘The impact of an ICME on the Jovian X-ray aurora’ will be published by the Journal of Geophysical Research on 22nd March 2016, 4pm US Eastern time DOI: 10.1002/2015JA021888.

About NASA’s Chandra X-ray Observatory

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations. |

Share this page:

Older press releases

For press releases issued before 4 October 2010, please visit the old eBulletin site.

Get in touch

T: +44 (0)116 252 2160


The Press Office is open 9.00am-5.00pm, Monday to Friday.

For general enquiries about the University, contact the main switchboard on +44 (0)116 252 2522.