{"id":23668,"date":"2021-03-18T09:00:13","date_gmt":"2021-03-18T13:00:13","guid":{"rendered":"https:\/\/hobbyspace.com\/Blog\/?p=23668"},"modified":"2021-03-25T11:53:10","modified_gmt":"2021-03-25T15:53:10","slug":"23668","status":"publish","type":"post","link":"https:\/\/hobbyspace.com\/Blog\/?p=23668","title":{"rendered":"ESO: Powerful stratospheric winds on Jupiter measured with ground based array"},"content":{"rendered":"<p>A new report from<a href=\"https:\/\/www.eso.org\/public\/news\/eso2104\/?lang\"> ESO (European Southern Observatory)<\/a>:<\/p>\n<p style=\"text-align: center;\"><strong><a href=\"https:\/\/www.eso.org\/public\/news\/eso2104\/?lang\">Powerful stratospheric winds measured on Jupiter for the first time<\/a><\/strong><\/p>\n<figure id=\"attachment_23669\" aria-describedby=\"caption-attachment-23669\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/www.eso.org\/public\/images\/eso2104a\/\"><img loading=\"lazy\" decoding=\"async\" data-attachment-id=\"23669\" data-permalink=\"https:\/\/hobbyspace.com\/Blog\/?attachment_id=23669\" data-orig-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso2104a1.jpg\" data-orig-size=\"700,438\" data-comments-opened=\"1\" data-image-meta=\"{&quot;aperture&quot;:&quot;0&quot;,&quot;credit&quot;:&quot;ESO\/L. Cal\\u00e7ada \\u0026amp; NASA\/JPL-Calte&quot;,&quot;camera&quot;:&quot;&quot;,&quot;caption&quot;:&quot;This image shows an artist\\u2019s impression of winds in Jupiter\\u2019s stratosphere near the planet\\u2019s south pole, with the blue lines representing wind speeds. These lines are superimposed on a real image of Jupiter, taken by the JunoCam imager aboard NASA\\u2019s Juno spacecraft. Jupiter\\u2019s famous bands of clouds are located in the lower atmosphere, where winds have previously been measured. But tracking winds right above this atmospheric layer, in the stratosphere, is much harder since no clouds exist there. By analysing the aftermath of a comet collision from the 1990s and using the ALMA telescope, in which ESO is a partner, researchers have been able to reveal incredibly powerful stratospheric winds, with speeds of up to 1450 kilometres an hour, near Jupiter\\u2019s poles.&quot;,&quot;created_timestamp&quot;:&quot;1616076000&quot;,&quot;copyright&quot;:&quot;&quot;,&quot;focal_length&quot;:&quot;0&quot;,&quot;iso&quot;:&quot;0&quot;,&quot;shutter_speed&quot;:&quot;0&quot;,&quot;title&quot;:&quot;Representation of stratospheric winds near Jupiter\\u2019s south pol&quot;,&quot;orientation&quot;:&quot;0&quot;}\" data-image-title=\"Representation of stratospheric winds near Jupiter\u2019s south pol\" data-image-description=\"\" data-image-caption=\"&lt;p&gt;This image shows an artist\u2019s impression of winds in Jupiter\u2019s stratosphere near the planet\u2019s south pole, with the blue lines representing wind speeds. These lines are superimposed on a real image of Jupiter, taken by the JunoCam imager aboard NASA\u2019s Juno spacecraft. Jupiter\u2019s famous bands of clouds are located in the lower atmosphere, where winds have previously been measured. But tracking winds right above this atmospheric layer, in the stratosphere, is much harder since no clouds exist there. By analysing the aftermath of a comet collision from the 1990s and using the ALMA telescope, in which ESO is a partner, researchers have been able to reveal incredibly powerful stratospheric winds, with speeds of up to 1450 kilometres an hour, near Jupiter\u2019s poles.&lt;\/p&gt;\n\" data-large-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso2104a1.jpg\" class=\"size-medium wp-image-23669\" src=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso2104a1-500x313.jpg\" alt=\"\" width=\"500\" height=\"313\" srcset=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso2104a1-500x313.jpg 500w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso2104a1.jpg 700w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-23669\" class=\"wp-caption-text\">This image shows an artist\u2019s impression of winds in Jupiter\u2019s stratosphere near the planet\u2019s south pole, with the blue lines representing wind speeds. These lines are superimposed on a real image of Jupiter, taken by the JunoCam imager aboard NASA\u2019s Juno spacecraft. Jupiter\u2019s famous bands of clouds are located in the lower atmosphere, where winds have previously been measured. But tracking winds right above this atmospheric layer, in the stratosphere, is much harder since no clouds exist there. By analysing the aftermath of a comet collision from the 1990s and using the ALMA telescope, in which ESO is a partner, researchers have been able to reveal incredibly powerful stratospheric winds, with speeds of up to 1450 kilometres an hour, near Jupiter\u2019s poles. <a href=\"https:\/\/www.eso.org\/public\/images\/eso2104a\/\">Credits: ESO<\/a><\/figcaption><\/figure>\n<p>Using the Atacama Large Millimeter\/submillimeter Array (ALMA), in which the European Southern Observatory (ESO) is a partner, a team of astronomers have directly measured winds in Jupiter\u2019s middle atmosphere for the first time. By analysing the aftermath of a comet collision from the 1990s, the researchers have revealed incredibly powerful winds, with speeds of up to 1450 kilometres an hour, near Jupiter\u2019s poles. They could represent what the team have described as a \u201c<em>unique meteorological beast in our Solar System<\/em>\u201d.<\/p>\n<p>Jupiter is famous for its distinctive red and white bands: swirling clouds of moving gas that astronomers traditionally use to track winds in Jupiter\u2019s lower atmosphere. Astronomers have also seen, near Jupiter&#8217;s poles, the vivid glows known as aurorae, which appear to be associated with strong winds in the planet\u2019s upper atmosphere. But until now, researchers had never been able to directly measure wind patterns in between these two atmospheric layers, in the stratosphere.<\/p>\n<p><span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" class=\"youtube-player\" width=\"1600\" height=\"900\" src=\"https:\/\/www.youtube.com\/embed\/JPtsAVAFryo?version=3&#038;rel=1&#038;showsearch=0&#038;showinfo=1&#038;iv_load_policy=1&#038;fs=1&#038;hl=en&#038;autohide=2&#038;wmode=transparent\" allowfullscreen=\"true\" style=\"border:0;\" sandbox=\"allow-scripts allow-same-origin allow-popups allow-presentation allow-popups-to-escape-sandbox\"><\/iframe><\/span><\/p>\n<p>Measuring wind speeds in Jupiter\u2019s stratosphere using cloud-tracking techniques is impossible because of the absence of clouds in this part of the atmosphere. However, astronomers were provided with an alternative measuring aid in the form of comet<a href=\"https:\/\/www.eso.org\/public\/images\/eso9410a\/\"> Shoemaker\u2013Levy 9<\/a>, which collided with the gas giant in spectacular fashion in 1994. This impact produced new molecules in Jupiter\u2019s stratosphere, where they have been moving with the winds ever since.<\/p>\n<p>A team of astronomers, led by Thibault Cavali\u00e9 of the Laboratoire d&#8217;Astrophysique de Bordeaux in France, have now tracked one of these molecules \u2014 hydrogen cyanide \u2014 to directly measure stratospheric &#8220;<em>jets<\/em>&#8221; on Jupiter. Scientists use the word &#8220;<em>jets<\/em>&#8221; to refer to narrow bands of wind in the atmosphere, like Earth\u2019s jet streams.<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;The most spectacular result is the presence of strong jets, with speeds of up to 400 metres per second, which are located under the aurorae near the poles,&#8221;\u00a0says Cavali\u00e9.<\/em><\/p>\n<figure id=\"attachment_23670\" aria-describedby=\"caption-attachment-23670\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/www.eso.org\/public\/images\/1994-sl9-irac-ii\/\"><img loading=\"lazy\" decoding=\"async\" data-attachment-id=\"23670\" data-permalink=\"https:\/\/hobbyspace.com\/Blog\/?attachment_id=23670\" data-orig-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/1994-sl9-irac-ii1.jpg\" data-orig-size=\"700,376\" data-comments-opened=\"1\" data-image-meta=\"{&quot;aperture&quot;:&quot;0&quot;,&quot;credit&quot;:&quot;ESO&quot;,&quot;camera&quot;:&quot;&quot;,&quot;caption&quot;:&quot;This image, taken with the MPG\/ESO 2.2-metre telescope and the IRAC instrument, shows comet Shoemaker\\u2013Levy 9 impacting Jupiter in July 1994.&quot;,&quot;created_timestamp&quot;:&quot;1616076000&quot;,&quot;copyright&quot;:&quot;&quot;,&quot;focal_length&quot;:&quot;0&quot;,&quot;iso&quot;:&quot;0&quot;,&quot;shutter_speed&quot;:&quot;0&quot;,&quot;title&quot;:&quot;Comet Shoemaker\\u2013Levy 9 impacting Jupiter in 1994&quot;,&quot;orientation&quot;:&quot;0&quot;}\" data-image-title=\"Comet Shoemaker\u2013Levy 9 impacting Jupiter in 1994\" data-image-description=\"\" data-image-caption=\"&lt;p&gt;This image, taken with the MPG\/ESO 2.2-metre telescope and the IRAC instrument, shows comet Shoemaker\u2013Levy 9 impacting Jupiter in July 1994.&lt;\/p&gt;\n\" data-large-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/1994-sl9-irac-ii1.jpg\" class=\"size-medium wp-image-23670\" src=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/1994-sl9-irac-ii1-500x269.jpg\" alt=\"\" width=\"500\" height=\"269\" srcset=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/1994-sl9-irac-ii1-500x269.jpg 500w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/1994-sl9-irac-ii1.jpg 700w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-23670\" class=\"wp-caption-text\">This image, taken with the MPG\/ESO 2.2-metre telescope and the IRAC instrument, shows comet Shoemaker\u2013Levy 9 impacting Jupiter in July 1994. <a href=\"https:\/\/www.eso.org\/public\/images\/1994-sl9-irac-ii\/\">Credits: ESO<\/a><\/figcaption><\/figure>\n<p>These wind speeds, equivalent to about 1450 kilometres an hour, are more than twice the maximum storm speeds reached in Jupiter\u2019s Great Red Spot and over three times the wind speed measured on Earth\u2019s strongest tornadoes.<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;Our detection indicates that these jets could behave like a giant vortex with a diameter of up to four times that of Earth, and some 900 kilometres in height,&#8221;\u00a0explains co-author Bilal Benmahi, also of the Laboratoire d\u2019Astrophysique de Bordeaux. &#8220;A vortex of this size would be a unique meteorological beast in our Solar System,&#8221;\u00a0Cavali\u00e9 adds.<\/em><\/p>\n<p>Astronomers were aware of strong winds near Jupiter\u2019s poles, but much higher up in the atmosphere, hundreds of kilometres above the focus area of the new study, which is published today in Astronomy &amp; Astrophysics. Previous studies predicted that these upper-atmosphere winds would decrease in velocity and disappear well before reaching as deep as the stratosphere.<\/p>\n<p style=\"padding-left: 40px;\">&#8220;<em>The new ALMA data tell us the contrary,<\/em>&#8220;<\/p>\n<p>\u00a0says Cavali\u00e9, adding that finding these strong stratospheric winds near Jupiter\u2019s poles was a &#8220;<em>real surprise<\/em>&#8220;.<\/p>\n<p><span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" class=\"youtube-player\" width=\"1600\" height=\"900\" src=\"https:\/\/www.youtube.com\/embed\/CXvnappC-q0?version=3&#038;rel=1&#038;showsearch=0&#038;showinfo=1&#038;iv_load_policy=1&#038;fs=1&#038;hl=en&#038;autohide=2&#038;wmode=transparent\" allowfullscreen=\"true\" style=\"border:0;\" sandbox=\"allow-scripts allow-same-origin allow-popups allow-presentation allow-popups-to-escape-sandbox\"><\/iframe><\/span><\/p>\n<p>The team used 42 of ALMA\u2019s 66 high-precision antennas, located in the Atacama Desert in northern Chile, to analyse the hydrogen cyanide molecules that have been moving around in Jupiter\u2019s stratosphere since the impact of Shoemaker\u2013Levy 9. The ALMA data allowed them to measure the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Doppler_effect\">Doppler shift<\/a> \u2014 tiny changes in the frequency of the radiation emitted by the molecules \u2014 caused by the winds in this region of the planet.<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;By measuring this shift, we were able to deduce the speed of the winds much like one could deduce the speed of a passing train by the change in the frequency of the train whistle,&#8221;\u00a0<\/em><\/p>\n<p>explains study co-author Vincent Hue, a planetary scientist at the Southwest Research Institute in the US.<\/p>\n<p>In addition to the surprising polar winds, the team also used ALMA to confirm the existence of strong stratospheric winds around the planet\u2019s equator, by directly measuring their speed, also for the first time. The jets spotted in this part of the planet have average speeds of about 600 kilometres an hour.<\/p>\n<p>The ALMA observations required to track stratospheric winds in both the poles and equator of Jupiter took less than 30 minutes of telescope time.<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;The high levels of detail we achieved in this short time really demonstrate the power of the ALMA observations,&#8221;\u00a0says Thomas Greathouse, a scientist at the Southwest Research Institute in the US and co-author of the study. &#8220;It is astounding to me to see the first direct measurement of these winds.&#8221;<\/em><\/p>\n<p>[ Cavali\u00e9 says, ]<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;These ALMA results open a new window for the study of Jupiter\u2019s auroral regions, which was really unexpected just a few months back,&#8221; [&#8230;]<\/em><\/p>\n<p>[ Greathouse adds, ]<\/p>\n<p style=\"padding-left: 40px;\"><em>&#8220;They also set the stage for similar yet more extensive measurements to be made by the JUICE mission and its Submillimetre Wave Instrument,&#8221; [&#8230;]<\/em><\/p>\n<p>referring to the European Space Agency\u2019s <em>JUpiter ICy moons Explorer<\/em>, which is expected to launch into space next year.<\/p>\n<p>ESO\u2019s ground-based Extremely Large Telescope (ELT), set to see first light later this decade, will also explore Jupiter. The telescope will be capable of making highly detailed observations of the planet\u2019s aurorae, giving us further insight into Jupiter\u2019s atmosphere.<\/p>\n<figure id=\"attachment_23671\" aria-describedby=\"caption-attachment-23671\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/www.eso.org\/public\/images\/eso0833a\/\"><img loading=\"lazy\" decoding=\"async\" data-attachment-id=\"23671\" data-permalink=\"https:\/\/hobbyspace.com\/Blog\/?attachment_id=23671\" data-orig-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1.jpg\" data-orig-size=\"700,700\" data-comments-opened=\"1\" data-image-meta=\"{&quot;aperture&quot;:&quot;0&quot;,&quot;credit&quot;:&quot;ESO\/F. Marchis, M. Wong, E. Marc&quot;,&quot;camera&quot;:&quot;&quot;,&quot;caption&quot;:&quot;Amazing image of Jupiter taken in infrared light on the night of 17 August 2008 with the Multi-Conjugate Adaptive Optics Demonstrator (MAD) prototype instrument mounted on ESO&#039;s Very Large Telescope. This false colour photo is the combination of a series of images taken over a time span of about 20 minutes, through three different filters (2, 2.14, and 2.16 microns). The image sharpening obtained is about 90 milli-arcseconds across the whole planetary disc, a real record on similar images taken from the ground. This corresponds to seeing details about 300 km wide on the surface of the giant planet. The great red spot is not visible in this image as it was on the other side of the planet during the observations. The observations were done at infrared wavelengths where absorption due to hydrogen and methane is strong. This explains why the colours are different from how we usually see Jupiter in visible-light. This absorption means that light can be reflected back only from high-altitude hazes, and not from deeper clouds. These hazes lie in the very stable upper part of Jupiter&#039;s troposphere, where pressures are between 0.15 and 0.3 bar. Mixing is weak within this stable region, so tiny haze particles can survive for days to years, depending on their size and fall speed. Additionally, near the planet&#039;s poles, a higher stratospheric haze (light blue regions) is generated by interactions with particles trapped in Jupiter&#039;s intense magnetic field.&quot;,&quot;created_timestamp&quot;:&quot;1222905600&quot;,&quot;copyright&quot;:&quot;&quot;,&quot;focal_length&quot;:&quot;0&quot;,&quot;iso&quot;:&quot;0&quot;,&quot;shutter_speed&quot;:&quot;0&quot;,&quot;title&quot;:&quot;Sharpening up Jupiter&quot;,&quot;orientation&quot;:&quot;0&quot;}\" data-image-title=\"Sharpening up Jupiter\" data-image-description=\"\" data-image-caption=\"&lt;p&gt;Amazing image of Jupiter taken in infrared light on the night of 17 August 2008 with the Multi-Conjugate Adaptive Optics Demonstrator (MAD) prototype instrument mounted on ESO&amp;#8217;s Very Large Telescope. This false colour photo is the combination of a series of images taken over a time span of about 20 minutes, through three different filters (2, 2.14, and 2.16 microns). The image sharpening obtained is about 90 milli-arcseconds across the whole planetary disc, a real record on similar images taken from the ground. This corresponds to seeing details about 300 km wide on the surface of the giant planet. The great red spot is not visible in this image as it was on the other side of the planet during the observations. The observations were done at infrared wavelengths where absorption due to hydrogen and methane is strong. This explains why the colours are different from how we usually see Jupiter in visible-light. This absorption means that light can be reflected back only from high-altitude hazes, and not from deeper clouds. These hazes lie in the very stable upper part of Jupiter&amp;#8217;s troposphere, where pressures are between 0.15 and 0.3 bar. Mixing is weak within this stable region, so tiny haze particles can survive for days to years, depending on their size and fall speed. Additionally, near the planet&amp;#8217;s poles, a higher stratospheric haze (light blue regions) is generated by interactions with particles trapped in Jupiter&amp;#8217;s intense magnetic field.&lt;\/p&gt;\n\" data-large-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1.jpg\" class=\"size-medium wp-image-23671\" src=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1-500x500.jpg\" alt=\"\" width=\"500\" height=\"500\" srcset=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1-500x500.jpg 500w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1-150x150.jpg 150w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/03\/eso0833a1.jpg 700w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-23671\" class=\"wp-caption-text\">Amazing image of Jupiter taken in infrared light on the night of 17 August 2008 with the Multi-Conjugate Adaptive Optics Demonstrator (MAD) prototype instrument mounted on ESO&#8217;s Very Large Telescope. This false colour photo is the combination of a series of images taken over a time span of about 20 minutes, through three different filters (2, 2.14, and 2.16 microns). The image sharpening obtained is about 90 milli-arcseconds across the whole planetary disc, a real record on similar images taken from the ground. This corresponds to seeing details about 300 km wide on the surface of the giant planet. The great red spot is not visible in this image as it was on the other side of the planet during the observations. The observations were done at infrared wavelengths where absorption due to hydrogen and methane is strong. This explains why the colours are different from how we usually see Jupiter in visible-light. This absorption means that light can be reflected back only from high-altitude hazes, and not from deeper clouds. These hazes lie in the very stable upper part of Jupiter&#8217;s troposphere, where pressures are between 0.15 and 0.3 bar. Mixing is weak within this stable region, so tiny haze particles can survive for days to years, depending on their size and fall speed. Additionally, near the planet&#8217;s poles, a higher stratospheric haze (light blue regions) is generated by interactions with particles trapped in Jupiter&#8217;s intense magnetic field. <a href=\"https:\/\/www.eso.org\/public\/images\/eso0833a\/\">Credits: ESO<\/a><\/figcaption><\/figure>\n<p><strong>Links<\/strong><\/p>\n<ul>\n<li><a href=\"https:\/\/www.eso.org\/public\/archives\/releases\/sciencepapers\/eso2104\/eso2104a.pdf\">Research paper<\/a><\/li>\n<li><a href=\"https:\/\/www.eso.org\/public\/images\/archive\/category\/alma\/\">Images of ALMA<\/a><\/li>\n<li><a href=\"http:\/\/eso.org\/sci\/publications\/announcements\/sciann17277.html\">For scientists: got a story? Pitch your research<\/a><\/li>\n<\/ul>\n<p style=\"text-align: center;\"><em>===<\/em><strong><em> Amazon Ads <\/em><\/strong><em>===<\/em><\/p>\n<p style=\"text-align: center;\"><strong><a href=\"https:\/\/www.amazon.com\/gp\/product\/1588346919\/ref=as_li_tl?ie=UTF8&amp;camp=1789&amp;creative=9325&amp;creativeASIN=1588346919&amp;linkCode=as2&amp;tag=hobbyspace&amp;linkId=f03c3ed8ae786328107b054c7548be90\" target=\"_blank\" rel=\"noopener\">Envisioning Exoplanets:<br \/>\nSearching for Life in the Galaxy<\/a><\/strong><img loading=\"lazy\" decoding=\"async\" style=\"border: none !important; margin: 0px !important;\" src=\"\/\/ir-na.amazon-adsystem.com\/e\/ir?t=hobbyspace&amp;l=am2&amp;o=1&amp;a=1588346919\" alt=\"\" width=\"1\" height=\"1\" border=\"0\" \/><\/p>\n<p style=\"text-align: center;\"><iframe style=\"width: 120px; height: 240px;\" src=\"\/\/ws-na.amazon-adsystem.com\/widgets\/q?ServiceVersion=20070822&amp;OneJS=1&amp;Operation=GetAdHtml&amp;MarketPlace=US&amp;source=ac&amp;ref=tf_til&amp;ad_type=product_link&amp;tracking_id=hobbyspace&amp;marketplace=amazon&amp;region=US&amp;placement=1588346919&amp;asins=1588346919&amp;linkId=4d8b47019f5b3324ce507a9ee3116e32&amp;show_border=true&amp;link_opens_in_new_window=true&amp;price_color=333333&amp;title_color=0066c0&amp;bg_color=ffffff\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\"><span style=\"display: inline-block; width: 0px; overflow: hidden; line-height: 0;\" data-mce-type=\"bookmark\" class=\"mce_SELRES_start\">\ufeff<\/span><\/iframe><\/p>\n<p style=\"text-align: center;\"><em>==<\/em><em>=<\/em><\/p>\n<p style=\"text-align: center;\"><strong><a href=\"https:\/\/www.amazon.com\/gp\/product\/B016VA9F30\/ref=as_li_tl?ie=UTF8&amp;camp=1789&amp;creative=9325&amp;creativeASIN=B016VA9F30&amp;linkCode=as2&amp;tag=hobbyspace&amp;linkId=2d48d4e250ad8af51a4807f6b5098f9d\" target=\"_blank\" rel=\"noopener noreferrer\">Xtronaut:<br \/>\nThe Game of Solar System Exploration<\/a><img loading=\"lazy\" decoding=\"async\" style=\"border: none !important; margin: 0px !important;\" src=\"\/\/ir-na.amazon-adsystem.com\/e\/ir?t=hobbyspace&amp;l=am2&amp;o=1&amp;a=B016VA9F30\" alt=\"\" width=\"1\" height=\"1\" border=\"0\" \/><\/strong><\/p>\n<p style=\"text-align: center;\"><iframe style=\"width: 120px; height: 240px;\" src=\"\/\/ws-na.amazon-adsystem.com\/widgets\/q?ServiceVersion=20070822&amp;OneJS=1&amp;Operation=GetAdHtml&amp;MarketPlace=US&amp;source=ac&amp;ref=tf_til&amp;ad_type=product_link&amp;tracking_id=hobbyspace&amp;marketplace=amazon&amp;region=US&amp;placement=B016VA9F30&amp;asins=B016VA9F30&amp;linkId=926ed1f3f0f85fe3cfa5778dd65a1145&amp;show_border=true&amp;link_opens_in_new_window=true&amp;price_color=333333&amp;title_color=0066c0&amp;bg_color=ffffff\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\"><\/iframe><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A new report from ESO (European Southern Observatory): Powerful stratospheric winds measured on Jupiter for the first time Using the Atacama Large Millimeter\/submillimeter Array (ALMA), in which the European Southern Observatory (ESO) is a partner, a team of astronomers have directly measured winds in Jupiter\u2019s middle atmosphere for the first time. By analysing the aftermath &hellip; <a href=\"https:\/\/hobbyspace.com\/Blog\/?p=23668\" class=\"more-link\">Continue reading <span class=\"screen-reader-text\">ESO: Powerful stratospheric winds on Jupiter measured with ground based array<\/span> <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jetpack_post_was_ever_published":false,"_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[12],"tags":[],"class_list":["post-23668","post","type-post","status-publish","format-standard","hentry","category-astronomy"],"jetpack_featured_media_url":"","jetpack_sharing_enabled":true,"jetpack_shortlink":"https:\/\/wp.me\/s34aWK-23668","jetpack-related-posts":[{"id":15691,"url":"https:\/\/hobbyspace.com\/Blog\/?p=15691","url_meta":{"origin":23668,"position":0},"title":"Juno: From Jupiter&#8217;s deep jet-streams to the equatorial twilight zone","author":"TopSpacer","date":"March 8, 2018","format":false,"excerpt":"A couple of items from the Juno mission at Jupiter: NASA Juno Findings - Jupiter\u2019s Jet-Streams Are Unearthly https:\/\/youtu.be\/hF0UjhPSS3A For hundreds of years, this gaseous giant planet appeared shrouded in colorful bands of clouds extending from dusk to dawn, referred to as zones and belts. The bands were thought to\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/03\/pia22336-161.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":16300,"url":"https:\/\/hobbyspace.com\/Blog\/?p=16300","url_meta":{"origin":23668,"position":1},"title":"Juno: The chaotic clouds of Jupiter","author":"TopSpacer","date":"June 28, 2018","format":false,"excerpt":"These processed images of Jupiter from the Juno probe never get old. Here is a new one: Chaotic Clouds of Jupiter This image captures swirling cloud belts and tumultuous vortices within Jupiter\u2019s northern hemisphere. NASA\u2019s Juno spacecraft took this color-enhanced image at 10:23 p.m. PDT on May 23, 2018 (1:23\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/06\/pia224241-1024x1024.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":15450,"url":"https:\/\/hobbyspace.com\/Blog\/?p=15450","url_meta":{"origin":23668,"position":2},"title":"Latest images from the Juno probe for the 10th perijove","author":"TopSpacer","date":"January 9, 2018","format":false,"excerpt":"The enhanced Juno images of Jupiter's clouds never get old. New ones\u00a0are now available from the tenth low pass (perijove) over the multi-colored clouds of the gas giant. High Above Jupiter\u2019s Clouds NASA\u2019s Juno spacecraft was a little more than one Earth diameter from Jupiter when it captured this mind-bending,\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/01\/pia219731-1024x1024.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":15855,"url":"https:\/\/hobbyspace.com\/Blog\/?p=15855","url_meta":{"origin":23668,"position":3},"title":"Juno video: An infrared tour of Jupiter&#8217;s North Pole","author":"TopSpacer","date":"April 12, 2018","format":false,"excerpt":"Latest findings from NASA's Juno probe orbiting Jupiter: NASA Juno Gives Infrared Tour of Jupiter\u2019s North Pole https:\/\/youtu.be\/By6sZ6RGCEQ In this animation the viewer is taken low over Jupiter\u2019s north pole to illustrate the 3-D aspects of the region\u2019s central cyclone and the eight cyclones that encircle it. The movie utilizes\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/img.youtube.com\/vi\/By6sZ6RGCEQ\/0.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":13775,"url":"https:\/\/hobbyspace.com\/Blog\/?p=13775","url_meta":{"origin":23668,"position":4},"title":"Help choose Juno&#8217;s next image targets on Jupiter","author":"TopSpacer","date":"January 20, 2017","format":false,"excerpt":"Help select spots on Jupiter for the Juno\u00a0spacecraft to image on its next pass close to the planet: Public to Choose Jupiter Picture Sites for NASA Juno\u00a0 Where should NASA's Juno spacecraft aim its camera during its next close pass of Jupiter on Feb. 2? You can now play a\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2017\/01\/PIA21377_hires1-1024x815.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":14123,"url":"https:\/\/hobbyspace.com\/Blog\/?p=14123","url_meta":{"origin":23668,"position":5},"title":"Juno: Citizen scientists turn Jupiter&#8217;s stormy clouds into dramatic artworks","author":"TopSpacer","date":"March 29, 2017","format":false,"excerpt":"The Juno spacecraft made its latest close flyby pass above the clouds of Jupiter: \u00a0Juno Spacecraft Completes Fifth Jupiter Flyby | Mission Juno At the time of closest approach (called perijove), Juno will be about 2,700 miles (4,400 kilometers) above the planet's cloud tops, traveling at a speed of about\u2026","rel":"","context":"In &quot;Gas giants Saturn, Jupiter, et al&quot;","block_context":{"text":"Gas giants Saturn, Jupiter, et al","link":"https:\/\/hobbyspace.com\/Blog\/?cat=87"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2017\/03\/pia213861-1024x931.jpg?resize=350%2C200","width":350,"height":200},"classes":[]}],"_links":{"self":[{"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/posts\/23668","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=23668"}],"version-history":[{"count":3,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/posts\/23668\/revisions"}],"predecessor-version":[{"id":23698,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=\/wp\/v2\/posts\/23668\/revisions\/23698"}],"wp:attachment":[{"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=23668"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=23668"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/hobbyspace.com\/Blog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=23668"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}