{"id":3710,"date":"2024-09-11T09:01:37","date_gmt":"2024-09-11T07:01:37","guid":{"rendered":"http:\/\/brera.inaf.it\/?p=3710"},"modified":"2024-10-22T11:45:24","modified_gmt":"2024-10-22T09:45:24","slug":"astronomers-track-bubbles-on-stars-surface-in-most-detailed-video-yet-eso-press-release","status":"publish","type":"post","link":"https:\/\/brera.inaf.it\/en\/astronomers-track-bubbles-on-stars-surface-in-most-detailed-video-yet-eso-press-release\/","title":{"rendered":"Astronomers track bubbles on star\u2019s surface in most detailed video yet &#8211; ESO Press Release"},"content":{"rendered":"\n<p>For the first time, astronomers have captured images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface. The images of the star, R Doradus, were obtained with the Atacama Large Millimeter\/submillimeter Array (ALMA), a telescope co-owned by the European Southern Observatory (ESO), in July and August 2023. They show giant, hot bubbles of gas, 75 times the size of the Sun, appearing on the surface and sinking back into the star\u2019s interior faster than expected &#8211; <a href=\"https:\/\/www.eso.org\/public\/unitedkingdom\/news\/eso2412\/?lang\">Read on ESO website<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>For the first time, astronomers have captured images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface. The images of the star, R Doradus, were obtained with the Atacama Large Millimeter\/submillimeter Array (ALMA), a telescope co-owned by the European Southern Observatory (ESO), in July [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":4251,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[24,30],"tags":[],"class_list":["post-3710","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news-en","category-scientific-news"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",1280,720,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",150,84,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",300,169,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",768,432,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",1024,576,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",1280,720,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/09\/bolle-stella-2024.png",1280,720,false]},"post_excerpt_stackable":"<p>For the first time, astronomers have captured images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface. The images of the star, R Doradus, were obtained with the Atacama Large Millimeter\/submillimeter Array (ALMA), a telescope co-owned by the European Southern Observatory (ESO), in July and August 2023. They show giant, hot bubbles of gas, 75 times the size of the Sun, appearing on the surface and sinking back into the star\u2019s interior faster than expected &#8211; Read on ESO website<\/p>\n","category_list":"<a href=\"https:\/\/brera.inaf.it\/en\/category\/news-en\/\" rel=\"category tag\">News<\/a>, <a href=\"https:\/\/brera.inaf.it\/en\/category\/news-en\/scientific-news\/\" rel=\"category tag\">Scientific news<\/a>","author_info":{"name":"Maria Rosa Panzera","url":"https:\/\/brera.inaf.it\/en\/author\/maria-rosa-panzera\/"},"comments_num":"0 comments","_links":{"self":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/posts\/3710","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/comments?post=3710"}],"version-history":[{"count":1,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/posts\/3710\/revisions"}],"predecessor-version":[{"id":3711,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/posts\/3710\/revisions\/3711"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/4251"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=3710"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=3710"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=3710"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}