{"id":800961,"date":"2026-03-03T07:54:41","date_gmt":"2026-03-03T12:54:41","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=800961"},"modified":"2026-03-03T07:54:41","modified_gmt":"2026-03-03T12:54:41","slug":"one-of-the-biggest-stars-in-the-universe-might-be-ready-to-explode","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=800961","title":{"rendered":"One of the biggest stars in the universe might be ready to explode"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div xmlns:default=\"http:\/\/www.w3.org\/2000\/svg\">\n<figure id=\"attachment_537947\" aria-describedby=\"caption-attachment-537947\" style=\"width: 754px\" class=\"wp-caption alignnone\"><figcaption id=\"caption-attachment-537947\" class=\"wp-caption-text\">This is an artist\u2019s impression of the dying star WOH G64. It\u2019s more than 160,000 light-years away, in the Large Magellanic Cloud. It\u2019s one of the biggest stars in the universe, and it might be getting ready to explode. Image via ESO\/ L. Cal\u00e7ada.<\/figcaption><\/figure>\n<ul>\n<li><strong>Star WOH G64 is one of the largest known in the universe.<\/strong> It\u2019s more than 1,500 times the sun\u2019s radius.<\/li>\n<li><strong>In 2014, the star appeared to be transforming<\/strong> from a red supergiant into a rare yellow hypergiant. It shed its outer layers and began heating up.<\/li>\n<li><strong>The star might be getting ready to explode.<\/strong> Stars like this live fast and die young. The transformation might be driven by  a powerful pre-supernova \u201csuperwind.\u201d<\/li>\n<\/ul>\n<p>  <span>By Sara Webb, Swinburne University of Technology<\/span><\/p>\n<p><strong>You deserve a daily dose of good news.<\/strong>  For the latest in science and the night sky, click here to subscribe to our free daily newsletter.<\/p>\n<h3>One of the biggest stars in the universe might be getting ready to\u00a0explode<\/h3>\n<p>One of the largest known stars in the universe underwent a dramatic transformation in 2014, new research shows, and may be preparing to explode.<\/p>\n<p>A study led by Gonzalo Mu\u00f1oz-Sanchez at the National Observatory of Athens, published in <em>Nature Astronomy<\/em> on February 23, 2026, argues that the enormous star WOH G64 has transitioned from a red supergiant to a rare yellow hypergiant. \u2026 And it may be evidence of an impending supernova.<\/p>\n<p>The evidence suggests we may be witnessing, in real time, a massive star shedding its outer layers, shrinking as it heats up, and moving closer to the end of its short life.<\/p>\n<h3>A very special star<\/h3>\n<p>WOH G64 was first discovered in the 1970s as a star of interest in the Large Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. <\/p>\n<p>It turned out the star was not only extremely luminous, but also one of the biggest ever discovered. It\u2019s more than 1,500 times the radius of the sun. <\/p>\n<p>In 2024, WOH G64 was the first star beyond our galaxy ever photographed in detail, thanks to the Very Large Telescope Interferometer. The image showed a clear dusty cocoon around the central giant star, which confirmed it was losing mass as it aged. <\/p>\n<h3>From supergiant to hypergiant, big is big<\/h3>\n<p>WOH G64 is a young star in the grand scheme of the cosmos. It has an estimated age of less than 5 million years old. Unlike our sun (currently about 4.6 billion years old), WOH G64 is destined to live fast and die young. <\/p>\n<p>WOH G64 was born big, forming from a huge cloud of gas and dust collapsing until the pressure made it ignite. Like our sun, it would have burned hydrogen in its core by nuclear fusion. <\/p>\n<p>Later it would have expanded and burned helium, becoming what is called a red supergiant. <\/p>\n<p>Not all supergiants become hypergiants. It\u2019s been theorized that hypergiants form when very large stars quickly burn and evolve from burning hydrogen to burning helium. <\/p>\n<p>During this transition, these stars start to shed their outer layers, while their cores begin to shrink inward. Once a star becomes a hypergiant, it is destined for a quick death in the fiery explosion of a supernova.<\/p>\n<h3>What has caused this change seen in WOH G64?<\/h3>\n<p>So what happened to WOH G64 in 2014? The new study proposes that a large part of the original supergiant\u2019s surface was ejected away from the star. This may have been due to interactions with a companion star, which the authors have confirmed exists by looking at the spectrum of light from WOH G64.<\/p>\n<p>Another theory: the star is getting ready to explode. We know stars this big will inevitably go kaboom. But exactly when it will happen can be hard to determine in advance.<\/p>\n<p>One possible scenario is that the transition we\u2019re seeing is due to a pre-supernova \u201csuperwind\u201d phase. This is theorized to occur due to strong internal pulsations as the fuel in the core is spent quickly. <\/p>\n<h3>Only time will tell<\/h3>\n<p>Most stars live for tens of millions or even tens of billions of years. It was never a given we would witness and be able to document so much transformation in a star, let alone one outside our galaxy. <\/p>\n<p>If we are lucky, we will see the death of WOH G64 in our lifetimes \u2013 not only providing an incredible intergalactic spectacle but also helping scientists complete the puzzle of this fascinating star. <!-- Below is The Conversation's page counter tag. Please DO NOT REMOVE. --><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/counter.theconversation.com\/content\/276519\/count.gif?distributor=republish-lightbox-basic\" alt=\"The Conversation\" width=\"1\" height=\"1\" style=\"border: none !important; box-shadow: none !important; margin: 0 !important; max-height: 1px !important; max-width: 1px !important; min-height: 1px !important; min-width: 1px !important; opacity: 0 !important; outline: none !important; padding: 0 !important\" referrerpolicy=\"no-referrer-when-downgrade\"\/><!-- End of code. If you don't see any code above, please get new code from the Advanced tab after you click the republish button. The page counter does not collect any personal data. More info: https:\/\/theconversation.com\/republishing-guidelines --><\/p>\n<p><span>Sara Webb, Lecturer, Centre for Astrophysics and Supercomputing, Swinburne University of Technology<\/span><\/p>\n<p>This article is republished from The Conversation under a Creative Commons license. Read the original article.<\/p>\n<p>Bottom line: One of the biggest stars in the universe might be getting ready to explode. The star WOH G64 in a nearby galaxy showed a dramatic change in 2014.<\/p>\n<p>Source: The dramatic transition of the extreme red supergiant WOH G64 to a yellow hypergiant<\/p>\n<p>Read more: Star outside the Milky Way seen about to blow in closeup image<\/p>\n<\/div>\n<div>\n<div class=\"post-author\">\n<h4>EarthSky Voices<\/h4>\n<p>                    View Articles\n                  <\/p><\/div>\n<div class=\"post-tags\">\n<h6 data-udy-fe=\"text_7c58270d\">About the Author:<\/h6>\n<p>Members of the EarthSky community &#8211; including scientists, as well as science and nature writers from across the globe &#8211; weigh in on what&#8217;s important to them.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/earthsky.org\/space\/one-of-the-biggest-stars-in-the-universe-getting-ready-to-explode\/?rand=772280\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This is an artist\u2019s impression of the dying star WOH G64. It\u2019s more than 160,000 light-years away, in the Large Magellanic Cloud. It\u2019s one of the biggest stars in the&hellip; <\/p>\n","protected":false},"author":1,"featured_media":800962,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[46],"tags":[],"class_list":["post-800961","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-earth-sky"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/800961","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=800961"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/800961\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/800962"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=800961"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=800961"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=800961"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}