by Staff Writers
Boston MA (SPX) Nov 07, 2017
Jupiter's intense northern and southern lights, or auroras, behave independently of each other according to a new study using NASA's Chandra X-ray and ESA's XMM-Newton observatories. Using XMM-Newton and Chandra X-ray observations from March 2007 and May and June 2016, a team of researchers produced maps of Jupiter's X-ray emissions (shown in inset) and identified an X-ray hot spot at each pole. Each hot spot can cover an area equal to about half the surface of the Earth.
The team found that the hot spots had very different characteristics. The X-ray emission at Jupiter's south pole consistently pulsed every 11 minutes, but the X-rays seen from the north pole were erratic, increasing and decreasing in brightness - seemingly independent of the emission from the south pole.
This makes Jupiter particularly puzzling. X-ray auroras have never been detected from our solar system's other gas giants, including Saturn. Jupiter is also unlike Earth, where the auroras on our planet's north and south poles generally mirror each other because the magnetic fields are similar.
To understand how Jupiter produces its X-ray auroras, the team of researchers plans to combine new and upcoming X-ray data from Chandra and XMM-Newton with information from NASA's Juno mission, which is currently in orbit around the planet. If scientists can connect the X-ray activity with physical changes observed simultaneously with Juno, they may be able to determine the process that generates the Jovian auroras and by association X-ray auroras at other planets.
One theory that the X-ray and Juno observations may help to prove or disprove is that Jupiter's X-ray auroras are caused by interactions at the boundary between Jupiter's magnetic field, which is generated by electrical currents in the planet's interior, and the solar wind, a high-speed flow of particles streaming from the Sun.
The interactions between the solar wind and Jupiter's magnetic field can cause the latter to vibrate and produce magnetic waves. Charged particles can surf these waves and gain energy. Collisions of these particles with Jupiter's atmosphere produce the bright flashes of X-rays observed by Chandra and XMM-Newton. Within this theory the 11-minute interval would represent the time for a wave to travel along one of Jupiter's magnetic field lines.
The difference in behavior between the Jovian north and south poles may be caused by the difference in visibility of the two poles. Because the magnetic field of Jupiter is tilted, we are able to see much more of the northern aurora than the southern aurora.
Therefore for the north pole we may be able to observe regions where the magnetic field connects to more than one location, with several different travel times, while for the south pole we can only observe regions where the magnetic field connects to one location. This would cause the behavior of the north pole to appear erratic compared to the south pole.
A larger question is how does Jupiter give the particles in its magnetosphere (the realm controlled by Jupiter's magnetic field) the huge energies needed to make X-rays? Some of the X-ray emission observed with Chandra can only be produced if Jupiter accelerates oxygen ions to such high energies that when they violently collide with the atmosphere all eight of their electrons are torn off.
Scientists hope to determine what impact these particles, which crash into the planet's poles at thousands of kilometers per second, have on the planet itself. Do these high-energy particles affect the Jovian weather and the chemical composition of its atmosphere?
Can they explain the anomalously high temperatures found in certain places in Jupiter's atmosphere? These are the questions that Chandra, XMM-Newton, and Juno may be able to help answer in the future.
"The Independent Pulsations of Jupiter's Northern and Southern X-ray Auroras," William R. Dunn (University College London) et al., 2017 Oct. 30, Nature Astronomy
Pasadena CA (JPL) Nov 03, 2017
Data returned Tuesday, Oct. 31, indicate that NASA's Juno spacecraft successfully completed its eighth science flyby over Jupiter's mysterious cloud tops on Tuesday, Oct. 24. The confirmation was delayed by several days due to solar conjunction at Jupiter, which affected communications during the days prior to and after the flyby. Solar conjunction is the period when the path of communicat ... read more
Chandra X-Ray Center
The million outer planets of a star called Sol
|The content herein, unless otherwise known to be public domain, are Copyright 1995-2017 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement|