{"id":1103,"date":"2021-08-04T08:15:00","date_gmt":"2021-08-04T08:15:00","guid":{"rendered":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/?p=1103"},"modified":"2025-02-26T13:37:28","modified_gmt":"2025-02-26T13:37:28","slug":"leicester-planetary-scientists-reveal-secret-behind-jupiters-energy-crisis","status":"publish","type":"post","link":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/2021\/08\/04\/leicester-planetary-scientists-reveal-secret-behind-jupiters-energy-crisis\/","title":{"rendered":"Leicester planetary scientists reveal secret behind Jupiter\u2019s \u2018energy crisis\u2019"},"content":{"rendered":"\n<p><strong><em>New research published in\u00a0Nature\u00a0has revealed the solution to Jupiter\u2019s \u2018energy crisis\u2019, which has puzzled astronomers for decades.<\/em><\/strong><br><br><\/p>\n\n\n\n<p>Space scientists at the University of Leicester worked with colleagues from the Japanese Space Agency (JAXA), Boston University, NASA\u2019s Goddard Space Flight Center and the National Institute of Information and Communications Technology (NICT) to reveal the mechanism behind Jupiter\u2019s atmospheric heating.<br><br><\/p>\n\n\n\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\"><div class=\"wp-block-embed__wrapper\">\n<iframe loading=\"lazy\" title=\"The secret behind Jupiter\u2019s \u2018energy crisis\u2019\" width=\"620\" height=\"349\" src=\"https:\/\/www.youtube.com\/embed\/JE3bv9gCSPY?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/div><\/figure>\n\n\n\n<p><br>Now, using data from the Keck Observatory in Hawai\u2019i, astronomers have created the most-detailed yet global map of the gas giant\u2019s upper atmosphere, confirming for the first time that Jupiter\u2019s powerful aurorae are responsible for delivering planet-wide heating.<br><br><\/p>\n\n\n\n<p>Dr James O\u2019Donoghue is a researcher at JAXA and completed his PhD at Leicester, and is lead author for the research paper.<br><br><\/p>\n\n\n\n<p>He said: \u201cWe first began trying to create a global heat map of Jupiter\u2019s uppermost atmosphere at the University of Leicester. The signal was not bright enough to reveal anything outside of Jupiter\u2019s polar regions at the time, but with the lessons learned from that work we managed to secure time on one of the largest, most competitive telescopes on Earth some years later.<br><br><\/p>\n\n\n\n<p>\u201cUsing the Keck telescope we produced temperature maps of extraordinary detail. We found that temperatures start very high within the aurora, as expected from previous work, but now we could observe that Jupiter\u2019s aurora, despite taking up less than 10% of the area of the planet, appear to be heating the whole thing.<br><br><\/p>\n\n\n\n<p>\u201cThis research started in Leicester and carried on at Boston University and NASA before ending at JAXA in Japan. Collaborators from each continent working together made this study successful, combined with data from NASA\u2019s Juno spacecraft in orbit around Jupiter and JAXA\u2019s Hisaki spacecraft, an observatory in space.\u201d<br><br><\/p>\n\n\n\n<p>Dr Tom Stallard and Dr Henrik Melin are both part of the School of Physics and Astronomy at the University of Leicester. Dr Stallard added: \u201cThere has been a very long-standing puzzle in the thin atmosphere at the top of every Giant Planet within our solar system.<br><br><\/p>\n\n\n\n<p>\u201cWith every Jupiter space mission, along with ground-based observations, over the past 50 years, we have consistently measured the equatorial temperatures as being much too hot.<br><br><\/p>\n\n\n\n<p>\u201cThis \u2018energy crisis\u2019 has been a long standing issue \u2013 do the models fail to properly model how heat flows from the aurora, or is there some other unknown heat source near the equator?<br><br><\/p>\n\n\n\n<p>\u201cThis paper describes how we have mapped this region in unprecedented detail and have shown that, at Jupiter, the equatorial heating is directly associated with auroral heating.\u201d<br><br><\/p>\n\n\n\n<p>Aurorae occur when charged particles are caught in a planet\u2019s magnetic field. These spiral along the field lines towards the planet\u2019s magnetic poles, striking atoms and molecules in the atmosphere to release light and energy.<br><br><\/p>\n\n\n\n<p>On Earth, this leads to the characteristic light show that forms the Aurora Borealis and Australis. At Jupiter, the material spewing from its volcanic moon, Io, leads to the most powerful aurora in the Solar System and enormous heating in the polar regions of the planet.<br><br><\/p>\n\n\n\n<p>Although the Jovian aurorae have long been a prime candidate for heating the planet\u2019s atmosphere, observations have previously been unable to confirm or deny this until now.<br><br><\/p>\n\n\n\n<p>Previous maps of the upper atmospheric temperature were formed using images consisting of only several pixels. This is not enough resolution to see how the temperature might be changed across the planet, providing few clues as to the origin of the extra heat.<br><br><\/p>\n\n\n\n<p>Researchers created five maps of the atmospheric temperature at different spatial resolutions, with the highest resolution map showing an average temperature measurement for squares two degrees longitude \u2018high\u2019 by two degrees latitude \u2018wide\u2019.<br><br><\/p>\n\n\n\n<p>The team scoured more than 10,000 individual data points, only mapping points with an uncertainty of less than five per cent.<br><br><\/p>\n\n\n\n<p>Models of the atmospheres of gas giants suggest that they work like a giant refrigerator, with heat energy drawn from the equator towards the pole, and deposited in the lower atmosphere in these pole regions.<br><br><\/p>\n\n\n\n<p>These new findings suggest that fast-changing aurorae may drive waves of energy against this poleward flow, allowing heat to reach the equator.<\/p>\n\n\n\n<p>Observations also showed a region of localised heating in the sub-auroral region that could be interpreted as a limited wave of heat propagating equatorward, which could be interpreted as evidence of the process driving heat transfer.<br><br><\/p>\n\n\n\n<p>Planetary research at the University of Leicester spans the breadth of Jovian system, from the planet\u2019s magnetosphere and atmosphere, out to its diverse collection of satellites.<br><br><\/p>\n\n\n\n<p>Leicester researchers are members of the Juno mission made up of a global team astronomers observing the giant planet, and are\u00a0<a href=\"https:\/\/le.ac.uk\/news\/2021\/may\/jwst-time-allocation\">leading Jupiter observations from the forthcoming James Webb Space Telescope<\/a>. Leicester also plays a leading role in science and instrumentation on the European Space Agency (ESA)\u2019s Jupiter Icy Moons Explorer (JUICE), due for launch in 2022.<br><br><\/p>\n\n\n\n<p>\u2018Global upper-atmospheric heating on Jupiter by the polar aurorae\u2019 is available in&nbsp;<em><a href=\"https:\/\/www.nature.com\/articles\/s41586-021-03706-w\">Nature<\/a><\/em>.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>New research published in\u00a0Nature\u00a0has revealed the solution to Jupiter\u2019s \u2018energy crisis\u2019, which has puzzled astronomers for decades. Space scientists at the University of Leicester worked with colleagues from the Japanese Space Agency (JAXA), Boston University, NASA\u2019s Goddard Space Flight Center and the National Institute of Information and Communications Technology (NICT) to reveal the mechanism behind [&hellip;]<\/p>\n","protected":false},"author":256,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[10],"tags":[],"class_list":["post-1103","post","type-post","status-publish","format-standard","hentry","category-planetary"],"_links":{"self":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1103","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/users\/256"}],"replies":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/comments?post=1103"}],"version-history":[{"count":1,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1103\/revisions"}],"predecessor-version":[{"id":1104,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1103\/revisions\/1104"}],"wp:attachment":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/media?parent=1103"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/categories?post=1103"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/tags?post=1103"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}