{"id":587598,"date":"2026-10-29T02:33:10","date_gmt":"2026-10-28T15:33:10","guid":{"rendered":"http:\/\/www.vibewire.com.au\/?guid=e0acd7d4769f1ab5711ae06c65ecef05"},"modified":"2026-10-29T02:33:10","modified_gmt":"2026-10-28T15:33:10","slug":"webb-sees-turbulent-star-nursery","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=587598","title":{"rendered":"Webb Sees Turbulent Star Nursery"},"content":{"rendered":"<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg\"><img fetchpriority=\"high\" decoding=\"async\" width=\"2048\" height=\"1365\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?w=2048\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"A nebula made of clouds of gas and dust with stars forming within. In the center and out to the left it is filled with thin, wispy blue gas that forms delicate layers. Around this are thicker orange clouds with dark ridges. Thin red filaments of gas cross the center of the nebula. Glowing bubbles in the gas contain dense, very bright clusters of stars. In the edges, distant stars are visible as bright points on a dark background.\" style=\"transform: scale(1.2); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"eager\" parallax_attr=\"\" parallax_off=\"1\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg 9694w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=300,200 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=768,512 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=1024,683 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=1536,1024 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=2048,1365 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=400,267 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=600,400 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=900,600 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=1200,800 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/10\/55604475252-31d25bf2e0-o.jpg?resize=2000,1333 2000w\" sizes=\"auto, (max-width: 2048px) 100vw, 2048px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-credits\">ESA\/Webb, NASA &amp; CSA, E. Sabbi, M. Zamani (ESA\/Webb); Acknowledgement: M. H. \u00d6zsara\u00e7<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\">In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy.<\/p>\n<p class=\"wp-block-paragraph\">This region has a lower metallicity (proportion of elements that are heavier than helium and hydrogen) than the Milky Way, giving astronomers an opportunity to learn more about conditions found in the early universe and how stars formed under those conditions.<\/p>\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/esawebb.org\/images\/potm2610a\/\" rel=\"noopener\">Read more about N159.<\/a><\/p>\n<p class=\"wp-block-paragraph\"><em>Image credit: ESA\/Webb, NASA &amp; CSA, E. Sabbi, M. Zamani (ESA\/Webb); Acknowledgement: M. H. \u00d6zsara\u00e7<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy. This region has a lower metallicity [\u2026]<\/p>\n","protected":false},"author":13,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[],"tags":[],"class_list":["post-587598","post","type-post","status-publish","format-standard","hentry"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO Pro 5.0.4 - aioseo.com -->\n\t<meta name=\"description\" content=\"In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy. This region has a lower metallicity [\u2026]\" \/>\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<meta name=\"author\" content=\"Guest authors\"\/>\n\t<meta name=\"google-site-verification\" content=\"1EIWGZ5FoylKQrO3pqls-2hXlDXKIP1lffdWZCVV0V4\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.vibewire.com.au\/?p=587598\" \/>\n\t\t<meta name=\"generator\" content=\"All in One SEO Pro (AIOSEO) 5.0.4\" \/>\n\t\t<meta property=\"og:locale\" content=\"en_US\" \/>\n\t\t<meta property=\"og:site_name\" content=\"VibeWire Magazine - Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"Webb Sees Turbulent Star Nursery - VibeWire Magazine\" \/>\n\t\t<meta property=\"og:description\" content=\"In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. 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