{"id":131725,"date":"2024-11-30T09:50:46","date_gmt":"2024-11-30T02:50:46","guid":{"rendered":"https:\/\/hotvideos24.online\/?p=131725"},"modified":"2024-11-30T09:50:46","modified_gmt":"2024-11-30T02:50:46","slug":"mysterious-record-breaking-energy-burst-connected-to-dead-star-and-red-dwarf","status":"publish","type":"post","link":"https:\/\/hotvideos24.online\/?p=131725","title":{"rendered":"Mysterious, record-breaking energy burst connected to dead star and red dwarf"},"content":{"rendered":"<p> <script async src=\"https:\/\/pagead2.googlesyndication.com\/pagead\/js\/adsbygoogle.js?client=ca-pub-3711241968723425\"\r\n     crossorigin=\"anonymous\"><\/script>\r\n<ins class=\"adsbygoogle\"\r\n     style=\"display:block\"\r\n     data-ad-format=\"fluid\"\r\n     data-ad-layout-key=\"-fb+5w+4e-db+86\"\r\n     data-ad-client=\"ca-pub-3711241968723425\"\r\n     data-ad-slot=\"7910942971\"><\/ins>\r\n<script>\r\n     (adsbygoogle = window.adsbygoogle || []).push({});\r\n<\/script><br \/>\n<\/p>\n<div id=\"article-body\">\n<p>Astronomers have discovered a record-breaking burst of energy coming from deep space, tracing it to a binary system containing a tiny red dwarf star and a dead stellar remnant called a white dwarf.<\/p>\n<p>The team from the Curtin University node of the International Center for Radio Astronomy Research (ICRAR) discovered the pulse of bright energy in archival low-frequency data from the <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/neutral-hydrogen-dark-ages-of-universe.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/neutral-hydrogen-dark-ages-of-universe.html\">Murchison Widefield Array<\/a> (MWA). This radio wave pulse, designated GLEAM-X J0704-37, erupts every three hours, with these bursts lasting between 30 and 60 seconds. That makes this signal the longest-period example of a rare and extreme phenomenon called &#8220;<a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/weird-radio-pulsar-slow-rotator\" data-before-rewrite-localise=\"https:\/\/www.space.com\/weird-radio-pulsar-slow-rotator\">long-period radio transients<\/a>.&#8221;<\/p>\n<aside class=\"hawk-nest\" data-block-type=\"embed\" data-render-type=\"fte\" data-skip=\"dealsy\" data-widget-type=\"seasonal\"\/>\n<p>First discovered in 2006, astronomers have been puzzled by long-period radio transients for almost 20 years, unable to figure out how exactly they generate <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/what-is-the-electromagnetic-spectrum\" data-before-rewrite-localise=\"https:\/\/www.space.com\/11420-alien-planets-radio-aurora-exoplanets.htmlhttps:\/\/www.space.com\/what-is-the-electromagnetic-spectrum\">radio waves<\/a>. This research may have solved that mystery by identifying a probable source of these energy bursts.<\/p>\n<p>One reason the mystery has been so tricky is that previously discovered long-period radio transients sat within areas of <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/19915-milky-way-galaxy.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/19915-milky-way-galaxy.html\">the Milky Way<\/a> packed with stars. That has made it tough to hone in on what is actually generating these <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/fast-radio-bursts\" data-before-rewrite-localise=\"https:\/\/www.space.com\/fast-radio-bursts\">bursts of radio waves<\/a>.<\/p>\n<p>&#8220;The long-period transients are very exciting, and for astronomers to understand what they are, we need an optical image,&#8221; Natasha Hurley-Walker, discovery team member and a researcher at Curtin University, <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.icrar.org\/binarytransient\/\" target=\"_blank\" data-url=\"https:\/\/www.icrar.org\/binarytransient\/\" referrerpolicy=\"no-referrer-when-downgrade\" data-hl-processed=\"none\" rel=\"noopener\">said in a statement<\/a>. &#8220;However, when you look toward them, there are so many stars lying in the way that it&#8217;s like <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/20482-2001-space-odyssey-infographic.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/20482-2001-space-odyssey-infographic.html\">2001: A Space Odyssey<\/a>. &#8216;My god, it\u2019s full of stars!'&#8221;<\/p>\n<p>However, the team had a stroke of luck when discovering GLEAM-X J0704-37. This remarkable long-period radio transient originated from 5,000 light-years away at the <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/31590-dark-matter-waves-milky-way-edge.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/31590-dark-matter-waves-milky-way-edge.html\">edge of the Milky Way<\/a>, which is more sparsely populated by stars.<\/p>\n<p>&#8220;Our new discovery lies far off the <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/470-puzzling-milky-companion.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/470-puzzling-milky-companion.html\">galactic plane,<\/a> so there are only a handful of stars nearby, and we&#8217;re now certain one-star system, in particular, is generating the radio waves,&#8221; Hurley-Walker added.<\/p>\n<div id=\"slice-container-newsletterForm-articleInbodyContent-RTMFDvp7DxTDjwdcPRDWeU\" class=\"slice-container newsletter-inbodyContent-slice newsletterForm-articleInbodyContent-RTMFDvp7DxTDjwdcPRDWeU slice-container-newsletterForm\">\n<div data-hydrate=\"true\" class=\"newsletter-form__wrapper newsletter-form__wrapper--inbodyContent\">\n<div class=\"newsletter-form__container\">\n<section class=\"newsletter-form__top-bar\"\/>\n<section class=\"newsletter-form__main-section\">\n<p class=\"newsletter-form__strapline\">Breaking space news, the latest updates on rocket launches, skywatching events and more!<\/p>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n<figure class=\"van-image-figure inline-layout\" data-bordeaux-image-check=\"\">\n<div class=\"image-full-width-wrapper\">\n<div class=\"image-widthsetter\" style=\"max-width:1920px;\">\n<p class=\"vanilla-image-block\" style=\"padding-top:56.25%;\"><picture><source type=\"image\/webp\" srcset=\"https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-320-80.png.webp 320w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-480-80.png.webp 480w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-650-80.png.webp 650w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-970-80.png.webp 970w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-1024-80.png.webp 1024w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-1200-80.png.webp 1200w\" sizes=\"(min-width: 1000px) 970px, calc(100vw - 40px)\"\/><img decoding=\"async\" alt=\"A large white sphere shining with blue light to the right of a smaller glowing orange sphere\" class=\"expandable\" srcset=\"https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-320-80.png 320w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-480-80.png 480w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-650-80.png 650w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-970-80.png 970w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-1024-80.png 1024w, https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4-1200-80.png 1200w\" sizes=\"(min-width: 1000px) 970px, calc(100vw - 40px)\" loading=\"lazy\" src=\"https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4.png\" data-pin-media=\"https:\/\/cdn.mos.cms.futurecdn.net\/8tqgzZYzBreEffvPFVQTS4.png\"\/><\/picture><\/p>\n<\/div>\n<\/div><figcaption itemprop=\"caption description\" class=\" inline-layout\"><span class=\"caption-text\">An illustration shows a white dwarf orbiting a small main sequence star in a binary system <\/span><span class=\"credit\" itemprop=\"copyrightHolder\">(Image credit: Robert Lea (created with Canva))<\/span><\/figcaption><\/figure>\n<p>The team used the <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/33565-meerkat-radio-telescope-first-light-new-galaxies.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/33565-meerkat-radio-telescope-first-light-new-galaxies.html\">MeerKAT telescope<\/a> in South Africa to pinpoint the origin of GLEAM-X J0704-37 to one specific star. The next step for the researchers was to uncover the nature of the GLEAM-X J0704-37 emitting star system.<\/p>\n<h2 id=\"red-dwarf-vs-white-dwarf-3\">Red dwarf vs. white dwarf<\/h2>\n<p>Turning to the Southern Astrophysical Research Telescope (SOAR) in Chile, the scientists were able to determine that one of the stars at the source of GLEAM-X J0704-37 is a low-mass <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/23772-red-dwarf-stars.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/23772-red-dwarf-stars.html\">red dwarf star<\/a>, also known as an &#8220;M-class,&#8221; or &#8220;M-dwarf,&#8221; star.<\/p>\n<p>This presented a dilemma for the team.<\/p>\n<p>&#8220;The M dwarfs are low-mass stars that have a mere fraction of the sun&#8217;s mass and luminosity. They constitute 70% of the stars in the Milky Way, but not one of them is visible to the naked eye,&#8221; Hurley-Walker explained. &#8220;An M dwarf alone couldn\u2019t generate the amount of energy we\u2019re seeing.&#8221;<\/p>\n<p>Returning to their data, the team found evidence suggesting that the red dwarf is in a binary system with another object. They determined that this companion body is likely to be a <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/23756-white-dwarf-stars.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/23756-white-dwarf-stars.html\">white dwarf<\/a>, the cooling stellar ember that is left over when a star with a mass around that of the sun dies.<\/p>\n<p>&#8220;Together, they power radio emission,&#8221; Hurley-Walker pointed out.<\/p>\n<div class=\"youtube-video youtube-facade\" data-timestamp=\"?start=30\" data-nosnippet=\"\">\n<div class=\"video-aspect-box\">\n<div class=\"watch-on-iframe-YdFi2qX9Hek\" data-yt-video-token=\"YdFi2qX9Hek\" title=\"Artist\u2019s impression video of the exotic binary star system AR Scorpii - YouTube\">\n<span class=\"youtube-video-title\">Artist\u2019s impression video of the exotic binary star system AR Scorpii &#8211; YouTube<\/span><br \/>\n<img decoding=\"async\" src=\"https:\/\/img.youtube.com\/vi\/YdFi2qX9Hek\/maxresdefault.jpg\" alt=\"Artist\u2019s impression video of the exotic binary star system AR Scorpii - YouTube\" data-aspect-ratio=\"16\/9\" loading=\"lazy\"\/>\n<\/div>\n<\/div>\n<p><svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" class=\"play-button\" viewbox=\"0 0 234.67 165.33\"><path fill=\"red\" d=\"M229.763 25.817c-2.699-10.162-10.65-18.165-20.748-20.881C190.716 0 117.333 0 117.333 0S43.951 0 25.651 4.936C15.553 7.652 7.6 15.655 4.903 25.817 0 44.236 0 82.667 0 82.667s0 38.429 4.903 56.85C7.6 149.68 15.553 157.681 25.65 160.4c18.3 4.934 91.682 4.934 91.682 4.934s73.383 0 91.682-4.934c10.098-2.718 18.049-10.72 20.748-20.882 4.904-18.421 4.904-56.85 4.904-56.85s0-38.431-4.904-56.85\"\/><path fill=\"#fff\" d=\"m93.333 117.559 61.333-34.89-61.333-34.894z\"\/><\/svg><br \/>\n<a class=\"watch-on-youtube-YdFi2qX9Hek\" href=\"https:\/\/youtu.be\/YdFi2qX9Hek\" target=\"_blank\" data-url=\"https:\/\/youtu.be\/YdFi2qX9Hek\" referrerpolicy=\"no-referrer-when-downgrade\" data-hl-processed=\"none\" rel=\"noopener\">Watch On <svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" class=\"youtube-logo\" viewbox=\"0 0 507.9 113.39\"><g fill=\"#fff\"><path d=\"M64.792 80.99V32.396l42.082 24.297zm93.803-63.285a20.285 20.285 0 0 0-14.32-14.32C131.642 0 80.99 0 80.99 0S30.337 0 17.705 3.385a20.286 20.286 0 0 0-14.32 14.32C0 30.338 0 56.693 0 56.693S0 83.049 3.385 95.68A20.285 20.285 0 0 0 17.705 110c12.632 3.386 63.285 3.386 63.285 3.386s50.652 0 63.285-3.386a20.284 20.284 0 0 0 14.32-14.32c3.385-12.632 3.385-38.988 3.385-38.988s0-26.355-3.385-38.988m94.473 74.326c.887-2.314 1.332-6.098 1.332-11.35V58.556c0-5.097-.445-8.822-1.332-11.178-.888-2.355-2.452-3.533-4.69-3.533-2.163 0-3.69 1.178-4.577 3.533-.888 2.356-1.332 6.081-1.332 11.178V80.68c0 5.25.424 9.035 1.275 11.35.848 2.318 2.392 3.475 4.633 3.475 2.239 0 3.803-1.157 4.691-3.475zm-17.953 11.122c-3.207-2.16-5.486-5.52-6.835-10.079-1.352-4.554-2.027-10.617-2.027-18.185v-10.31c0-7.644.771-13.784 2.316-18.417 1.544-4.633 3.956-8.011 7.24-10.135 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9.383 1.197 4.247 1.796 10.117 1.796 17.607v12.163h-26.757m-284.953-1.33-18.187-65.68h15.869l6.37 29.77c1.623 7.339 2.82 13.594 3.591 18.766h.464c.54-3.706 1.738-9.922 3.591-18.65l6.603-29.886h15.869l-18.417 65.68v31.51h-15.754v-31.51M322.115 34.23v71.007h-12.511l-1.39-8.688h-.347c-3.399 6.564-8.496 9.845-15.291 9.845-4.71 0-8.185-1.543-10.425-4.633-2.24-3.087-3.359-7.915-3.359-14.48V34.23h15.985v52.126c0 3.168.348 5.426 1.043 6.776.695 1.353 1.853 2.027 3.475 2.027 1.39 0 2.722-.423 3.996-1.275 1.274-.849 2.22-1.928 2.838-3.241V34.229h15.986m81.995.001v71.007h-12.511l-1.391-8.688h-.345c-3.402 6.564-8.498 9.845-15.292 9.845-4.711 0-8.186-1.543-10.426-4.633-2.24-3.087-3.358-7.915-3.358-14.48V34.23h15.985v52.126c0 3.168.347 5.426 1.041 6.776.696 1.353 1.855 2.027 3.476 2.027 1.391 0 2.723-.423 3.996-1.275 1.275-.849 2.22-1.928 2.839-3.241V34.229h15.985\"\/><path d=\"M365.552 20.908h-15.87v84.329h-15.637v-84.33h-15.869V8.05h47.376v12.858m76.811 53.636c0 5.174-.215 9.229-.639 12.162-.424 2.937-1.139 5.021-2.143 6.255-1.004 1.236-2.357 1.854-4.053 1.854a7.404 7.404 0 0 1-3.65-.927c-1.12-.618-2.026-1.544-2.722-2.78V50.796c.54-1.93 1.467-3.513 2.78-4.749 1.313-1.234 2.74-1.853 4.285-1.853 1.623 0 2.876.637 3.766 1.91.886 1.275 1.505 3.418 1.853 6.43.348 3.011.523 7.297.523 12.857zm14.652-28.964c-.967-4.478-2.531-7.721-4.692-9.73-2.163-2.007-5.136-3.011-8.919-3.011-2.935 0-5.676.83-8.224 2.49a16.926 16.926 0 0 0-5.908 6.545h-.117l.001-37.416h-15.405v100.777h13.204l1.622-6.717h.347c1.235 2.393 3.088 4.285 5.56 5.675 2.47 1.39 5.213 2.085 8.225 2.085 5.404 0 9.382-2.491 11.931-7.471 2.548-4.982 3.823-12.76 3.823-23.341V64.23c0-7.953-.484-14.17-1.448-18.65\"\/><\/g><\/svg><\/a>\n<\/div>\n<p>Hurley-Walker and colleagues propose that strong magnetic fields in the system cause the emission of periodic blasts of energy similar to those seen from rapidly spinning neutron stars, or &#8220;pulsars.&#8221; Because the system from which GLEAM-X J0704-37 emerges is located high above the disk of the Milky Way, the researchers were able to rule out a highly magnetic neutron star, or &#8220;magnetar,&#8221; as the source of this long-period radio transient.<\/p>\n<p>The team is now hard at work scouring data to confirm the nature of this <a data-analytics-id=\"inline-link\" href=\"https:\/\/www.space.com\/22509-binary-stars.html\" data-before-rewrite-localise=\"https:\/\/www.space.com\/22509-binary-stars.html\">binary system<\/a> and explain exactly how it launched GLEAM-X J0704-37.<\/p>\n<p>More generally, the fact that GLEAM-X J0704-37 has been active for the last 10 years, remaining undiscovered until now, suggests there are likely many more long-period radio transients lurking in archival data from a wide range of telescopes across the globe, including the MWA.<\/p>\n<p>&#8220;These long-period radio transients are new scientific discoveries, and the MWA has fundamentally enabled the discoveries,&#8221; MWA Director Steven Tingay, said in the statement. &#8220;The MWA has a 55-petabyte archive of observations that provide a decade-long record of our universe. It is like having the data storage equivalent of 55,000 high-end home computers \u2013 one of the biggest single collections of science data in the world.\u00a0<\/p>\n<p>&#8220;It is an absolute gold mine for discovering more phenomena in our universe, and the data are a playground for astronomers.&#8221;<\/p>\n<p>The team&#8217;s research was published on Nov. 26 in the <a data-analytics-id=\"inline-link\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ad890e\" target=\"_blank\" data-url=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ad890e\" referrerpolicy=\"no-referrer-when-downgrade\" data-hl-processed=\"none\" rel=\"noopener\">Astrophysical Journal Letters.<\/a><\/p>\n<\/div>\n<p><script async src=\"https:\/\/pagead2.googlesyndication.com\/pagead\/js\/adsbygoogle.js?client=ca-pub-3711241968723425\"\r\n     crossorigin=\"anonymous\"><\/script>\r\n<ins class=\"adsbygoogle\"\r\n     style=\"display:block\"\r\n     data-ad-format=\"fluid\"\r\n     data-ad-layout-key=\"-fb+5w+4e-db+86\"\r\n     data-ad-client=\"ca-pub-3711241968723425\"\r\n     data-ad-slot=\"7910942971\"><\/ins>\r\n<script>\r\n     (adsbygoogle = window.adsbygoogle || []).push({});\r\n<\/script><br \/>\n<br \/><div data-type=\"_mgwidget\" data-widget-id=\"1660802\">\r\n<\/div>\r\n<script>(function(w,q){w[q]=w[q]||[];w[q].push([\"_mgc.load\"])})(window,\"_mgq\");\r\n<\/script>\r\n<br \/>\n<br \/><a href=\"https:\/\/www.space.com\/record-breaking-mystery-energy-burst-gleam-xj0704-37\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Astronomers have discovered a record-breaking burst of energy coming from deep space, tracing it to a binary system containing a tiny red dwarf star and a dead stellar remnant called &hellip; <a href=\"https:\/\/hotvideos24.online\/?p=131725\" class=\"more-link\">Read More<\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8628],"tags":[],"class_list":["post-131725","post","type-post","status-publish","format-standard","hentry","category-science","entry"],"_links":{"self":[{"href":"https:\/\/hotvideos24.online\/index.php?rest_route=\/wp\/v2\/posts\/131725","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/hotvideos24.online\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/hotvideos24.online\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/hotvideos24.online\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/hotvideos24.online\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=131725"}],"version-history":[{"count":0,"href":"https:\/\/hotvideos24.online\/index.php?rest_route=\/wp\/v2\/posts\/131725\/revisions"}],"wp:attachment":[{"href":"https:\/\/hotvideos24.online\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=131725"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/hotvideos24.online\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=131725"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/hotvideos24.online\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=131725"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}