{"id":766064,"date":"2026-06-28T04:10:09","date_gmt":"2026-06-28T04:10:09","guid":{"rendered":"https:\/\/www.newsbeep.com\/ca\/766064\/"},"modified":"2026-06-28T04:10:09","modified_gmt":"2026-06-28T04:10:09","slug":"a-rare-supernova-peeled-back-a-stars-layers-and-revealed-a-hidden-secret","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/ca\/766064\/","title":{"rendered":"A rare supernova peeled back a star\u2019s layers and revealed a hidden secret"},"content":{"rendered":"<p id=\"first\">Astronomers have glimpsed the inner structure of a dying star in a  rare kind of cosmic explosion called an \u201cextremely stripped supernova.\u201d<\/p>\n<p>In a paper <a href=\"https:\/\/doi.org\/10.1038\/s41586-025-09375-3\" rel=\"nofollow noopener\" target=\"_blank\">published in Nature<\/a>,  Steve Schulze of Northwestern University in the United States and  colleagues describe the supernova 2021yfj and a thick shell of gas  surrounding it.<\/p>\n<p>Their findings support our existing theories of what happens inside  massive stars at the end of their lives \u2013 and how they have shaped the  building blocks of the universe we see today.<\/p>\n<p>How stars make the elements<\/p>\n<p>Stars are powered by nuclear fusion \u2013 a process in which lighter  atoms are squished together into heavier ones, releasing energy.<\/p>\n<p>Fusion <a href=\"https:\/\/iopscience.iop.org\/article\/10.1086\/341728\" rel=\"nofollow noopener\" target=\"_blank\">happens in stages<\/a>  over the star\u2019s life. In a series of cycles, first hydrogen (the  lightest element) is fused into helium, followed by the formation of  heavier elements such as carbon. The most massive stars continue on to  neon, oxygen, silicon and finally iron.<\/p>\n<p>Each burning cycle is faster than the previous one. The hydrogen  cycle can last for millions of years, while the silicon cycle is over in  a matter of days.<\/p>\n<p>As the core of a massive star keeps burning, the gas outside the core  acquires a layered structure, where successive layers record the  composition of the progression of burning cycles.<\/p>\n<p>While all this is playing out in the star\u2019s core, the star is also  shedding gas from its surface, carried out into space by the stellar  wind. Each fusion cycle creates an expanding shell of gas containing a  different mix of elements.<\/p>\n<p>Core collapse<\/p>\n<p>What happens to a massive star <a href=\"https:\/\/www.google.com.au\/books\/edition\/Progress_in_Understanding_Iron_Peak_Elem\/6fHGwQEACAAJ?hl=en\" rel=\"nofollow noopener\" target=\"_blank\">when its core is full of iron<\/a>?  The great pressure and temperature will make the iron fuse, but unlike  the fusion of lighter elements, this process absorbs energy instead of  releasing it.<\/p>\n<p>The release of energy from fusion is what has been holding the star  up against the force of gravity \u2013 so now the iron core will collapse.  Depending on how big it is to start with, the collapsed core will become  a neutron star or a black hole.<\/p>\n<p>The process of collapse creates a \u201cbounce,\u201d which sends energy and  matter flying outwards. This is called a core-collapse supernova  explosion.<\/p>\n<p>The explosion lights up the layers of gas shed from the star earlier,  allowing us to see what they are made of. In all known supernovae until  now, this material was either the hydrogen, the helium or the carbon  layer, produced in the first two nuclear burning cycles.<\/p>\n<p>The inner layers (the neon, oxygen and silicon layers) are all  produced in a mere few hundred years before the star explodes, which  means they don\u2019t have time to travel out far from the star.<\/p>\n<p>An explosive mystery<\/p>\n<p>But that\u2019s what makes the new supernova SN2021yfj so interesting.  Schulze and colleagues found the material outside the star came from the  silicon layer, the last layer just above the iron core, which forms on a  timescale of a few months.<\/p>\n<p>The stellar wind must have expelled all the layers right down to the  silicon one before the explosion occurred. Astronomers don\u2019t understand  how a stellar wind could be powerful enough to do this.<\/p>\n<p>The most plausible scenario is a second star was involved. If another  star were orbiting the one that exploded, its gravity might have  rapidly pulled out the deep silicon layer.<\/p>\n<p>Exploding stars made the universe what it is today<\/p>\n<p>Whatever the explanation, this view deep inside the star has  confirmed our theories of the cycles of nuclear fusion inside massive  stars.<\/p>\n<p>Why is this important? Because stars are where all the elements come from.<\/p>\n<p>Carbon and nitrogen are manufactured primarily by lower mass stars, similar to our own Sun. Some <a href=\"https:\/\/theconversation.com\/cosmic-alchemy-colliding-neutron-stars-show-us-how-the-universe-creates-gold-86104\" rel=\"nofollow noopener\" target=\"_blank\">heavy elements such as gold<\/a> are manufactured in the exotic environments of colliding and merging neutron stars.<\/p>\n<p>However, oxygen and other elements such as neon, magnesium and sulfur mainly come from core-collapse supernovae.<\/p>\n<p>We are what we are because of the inner workings of stars. The  constant production of elements in stars causes the universe to change  continuously. Stars and planets formed later are very different from  those formed in earlier times.<\/p>\n<p>When the universe was younger it had much less in the way of  \u201cinteresting\u201d elements. Everything worked somewhat differently: stars  burned hotter and faster and planets may have formed less, differently,  or not at all.<\/p>\n<p>How much supernovae explode and just what they eject into  interstellar space is a critical question in figuring out why our  Universe and our world are the way they are.<img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.newsbeep.com\/ca\/wp-content\/uploads\/2025\/09\/1758532207_852_count.gif\" 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\"\/><\/p>\n","protected":false},"excerpt":{"rendered":"Astronomers have glimpsed the inner structure of a dying star in a rare kind of cosmic explosion called&hellip;\n","protected":false},"author":2,"featured_media":766065,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[272447,49,48,66],"class_list":["post-766064","post","type-post","status-publish","format-standard","has-post-thumbnail","category-science","tag-black-holes-astrophysics-extrasolar-planets-space-exploration-physics-nanotechnology-graphene-albert-einstein","tag-ca","tag-canada","tag-science"],"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/766064","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/comments?post=766064"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/766064\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media\/766065"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media?parent=766064"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/categories?post=766064"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/tags?post=766064"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}