{"id":1365,"date":"2022-04-11T20:36:00","date_gmt":"2022-04-11T20:36:00","guid":{"rendered":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/?p=1365"},"modified":"2025-02-26T13:37:27","modified_gmt":"2025-02-26T13:37:27","slug":"neptune-is-cooler-than-we-thought-study-reveals-unexpected-changes-in-atmospheric-temperatures","status":"publish","type":"post","link":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/2022\/04\/11\/neptune-is-cooler-than-we-thought-study-reveals-unexpected-changes-in-atmospheric-temperatures\/","title":{"rendered":"Neptune is cooler than we thought: Study reveals unexpected changes in atmospheric temperatures"},"content":{"rendered":"\n

New research led by space scientists at the University of Leicester has revealed how temperatures in Neptune\u2019s atmosphere have unexpectedly fluctuated over the past two decades.<\/em><\/strong>

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Observed changes in Neptune\u2019s thermal-infrared brightness, a measure of temperature in Neptune\u2019s atmosphere. The plot shows the relative change in the thermal-infrared brightness from Neptune\u2019s stratosphere with time for all existing images taken by ground-based telescopes. Brighter images are interpreted as warmer. Corresponding thermal-infrared images (top) at wavelengths of ~12 \u00b5m show Neptune\u2019s appearance in 2006, 2009, 2018 (observed by the European Southern Observatory\u2019s Very Large Telescope\u2019s VISIR instrument), and 2020 (observed by Subaru\u2019s COMICS instrument). The south pole appears to have become dramatically warmer in just the past few years. Credit: Michael Roman\/NASA\/JPL\/Voyager-ISS\/Justin Cowart<\/figcaption><\/figure><\/div>\n\n\n\n

The study, published today (Monday) in\u00a0Planetary Science Journal<\/em>, used observations in thermal-infrared wavelengths beyond the visible light spectrum, effectively sensing heat emitted from the planet\u2019s atmosphere.

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An international team of researchers, including scientists from Leicester and NASA\u2019s Jet Propulsion Laboratory (JPL), combined all existing thermal infrared images of Neptune gathered from multiple observatories over almost two decades. These include the European Southern Observatory\u2019s Very Large Telescope and Gemini South telescope in Chile, together with the Subaru Telescope, Keck Telescope, and the Gemini North telescope, all in Hawai\u2019i, and spectra from NASA\u2019s Spitzer Space Telescope.

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By analysing the data, the researchers were able to reveal a more complete picture of trends in Neptune\u2019s temperatures than ever before.

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But to the researchers\u2019 surprise, these collective datasets show a decline in Neptune\u2019s thermal brightness since reliable thermal imaging began in 2003, indicating that globally-averaged temperatures in Neptune\u2019s stratosphere \u2013 the layer of the atmosphere just above its active weather layer \u2013 have dropped by roughly 8 degrees Celsius (14 degrees Fahrenheit) between 2003 and 2018.

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Dr Michael Roman, Postdoctoral Research Associate at the University of Leicester and lead author on the paper, said: \u201cThis change was unexpected. Since we have been observing Neptune during its early southern summer, we would expect temperatures to be slowly growing warmer, not colder.\u201d

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Neptune has an axial tilt, and so it experiences seasons, just like Earth. However, given its great distance from the Sun, Neptune takes over 165 years to complete an orbit around its host star, and so its seasons change slowly, lasting over 40 Earth-years each.

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Dr Glenn Orton, Senior Research Scientist at JPL and co-author on the study, noted:\u00a0\u201cOur data cover less than half of a Neptune season, so no one was expecting to see large and rapid changes.\u201d

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Neptune as seen in visible light (centre) and thermal-infrared wavelengths (right), in 2020. The centre image combines multiple images from the Hubble Space Telescope, while the thermal-infrared image on the right was taken from the Subaru Telescope on Maunakea, Hawai\u2019i. In the thermal-infrared, Neptune\u2019s warm south pole glows more brightly than ever seen before. Credit: Michael Roman\/NASA\/ESA\/STSci\/M.H. Wong\/L.A. Sromovsky\/P.M. Fry<\/figcaption><\/figure><\/div>\n\n\n\n



Yet, at Neptune\u2019s south pole, the data reveal a different and surprisingly dramatic change. A combination of observations from Gemini North in 2019 and Subaru in 2020 reveal that Neptune\u2019s polar stratosphere warmed by roughly 11\u02daC (~20\u02daF) between 2018 and 2020, reversing the previous globally-averaged cooling trend. Such polar warming has never been observed on Neptune before.

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The cause of these unexpected stratospheric temperature changes is currently unknown, and the results challenge scientists\u2019 understanding of Neptune\u2019s atmospheric variability.\u00a0

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Dr Roman continued: \u201cTemperature variations may be related to seasonal changes in Neptune\u2019s atmospheric chemistry, which can alter how effectively the atmosphere cools.

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\u201cBut random variability in weather patterns or even a response to the 11-year solar activity cycle may also have an effect.\u201d\u00a0\u00a0

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The 11-year solar cycle (marked by periodic variation in the Sun\u2019s activity and sunspots) has been previously suggested to affect Neptune\u2019s visible brightness, and the new study reveals a possible, but tentative, correlation between the solar activity, stratospheric temperatures, and the number of bright clouds seen on Neptune.

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Follow-up observations of the temperature and cloud patterns are needed to further assess any possible connection in the years ahead.

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Answers to these mysteries and more will come from the James Webb Space Telescope (JWST), which is set to observe both ice giants, Uranus and Neptune, later this year.

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Leigh Fletcher, Professor of Planetary Science at the University of Leicester, will lead such observations with allocated time of JWST\u2019s suite of instruments. Professor Fletcher, also a co-author on this study, said: \u201cThe exquisite sensitivity of the space telescope\u2019s mid-infrared instrument, MIRI, will provide unprecedented new maps of the chemistry and temperatures in Neptune\u2019s atmosphere, helping to better identify the nature of these recent changes.\u201d

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This study was funded by a European Research Council grant to the University of Leicester, known as GIANTCLIMES. This project has previously discovered long-term changes in atmospheric temperatures and clouds on the gas giants, Jupiter and Saturn, and it provided the first maps of the stratospheric temperatures of Uranus. GIANTCLIMES has paved the way for new discoveries on all four giant planets from JWST in the years to come.

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Additional co-authors on this work include Thomas Greathouse (Southwest Research Institute), Julianne Moses (Space Science Institute), Naomi Rowe-Gurney (Howard University \/ NASA Goddard Space Flight Center), Patrick Irwin (Oxford), Arrate Antu\u00f1ano (UPV\/EHU), James Sinclair (JPL), Yasumasa Kasaba (Tohoku University), Takuya Fujiyoshi (Subaru Telescope), Imke de Pater (UC Berkeley), and Heidi Hammel (Association of Universities for Research in Astronomy).\u00a0\u00a0

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\u2018Sub-Seasonal Variation in Neptune\u2019s Mid-Infrared Emission<\/a>\u2019 is published in\u00a0Planetary Science Journal<\/em>.

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Voyager 2 view of Neptune, captured in August 1989. Credit: NASA\/JPL-Caltech\/Kevin M. Gill<\/figcaption><\/figure><\/div>\n\n\n\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

New research led by space scientists at the University of Leicester has revealed how temperatures in Neptune\u2019s atmosphere have unexpectedly fluctuated over the past two decades. The study, published today (Monday) in\u00a0Planetary Science Journal, used observations in thermal-infrared wavelengths beyond the visible light spectrum, effectively sensing heat emitted from the planet\u2019s atmosphere. An international team […]<\/p>\n","protected":false},"author":256,"featured_media":1366,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[10],"tags":[],"class_list":["post-1365","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-planetary"],"_links":{"self":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1365","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=1365"}],"version-history":[{"count":1,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1365\/revisions"}],"predecessor-version":[{"id":1369,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1365\/revisions\/1369"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/media\/1366"}],"wp:attachment":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/media?parent=1365"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/categories?post=1365"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/tags?post=1365"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}