{"id":293395,"date":"2025-09-30T02:00:00","date_gmt":"2025-09-29T16:00:00","guid":{"rendered":"http:\/\/www.vibewire.com.au\/?guid=b194799278ded3385e04105382492f2f"},"modified":"2025-09-30T02:00:00","modified_gmt":"2025-09-29T16:00:00","slug":"hubble-surveys-cloudy-cluster-2","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=293395","title":{"rendered":"Hubble Surveys Cloudy Cluster"},"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-none \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg\"><img fetchpriority=\"high\" decoding=\"async\" width=\"2048\" height=\"1254\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?w=2048\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Stars in a star cluster shine brightly blue, with four-pointed diffraction spikes radiating from them. The center shows a small, crowded group of stars while a larger group is partially visible on the right side of the image. The nebula is mostly thick, smoky clouds of gas, lit up in blue tones by the stars. Clumps of dust hover before and around the stars; they are mostly dark but lit around their edges where the starlight erodes them.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"eager\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg 2831w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=300,184 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=768,470 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=1024,627 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=1536,941 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=2048,1254 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=400,245 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=600,368 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=900,551 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=1200,735 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/09\/hubble-lmc-n44c-potw2536a.jpg?resize=2000,1225 2000w\" sizes=\"auto, (max-width: 2048px) 100vw, 2048px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-credits\">ESA\/Hubble &amp; NASA, C. Murray, J. Ma\u00edz Apell\u00e1niz<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>This NASA\/ESA&nbsp;<a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/\" rel=\"noopener\">Hubble Space Telescope<\/a>&nbsp;image released on Sept. 12, 2025, features a cloudy starscape from an impressive star cluster. This scene is in the Large Magellanic Cloud, a dwarf galaxy situated about 160,000 light-years away in the constellations Dorado and Mensa. With a mass equal to 10\u201320% of the mass of the Milky Way, the Large Magellanic Cloud is the largest of the dozens of small galaxies that orbit our galaxy.<\/p>\n<p>The Large Magellanic Cloud is home to several massive stellar nurseries where gas clouds, like those strewn across this image, coalesce into new stars. Today\u2019s image depicts a portion of the galaxy\u2019s second-largest star-forming region, which is called N11. (The most massive and prolific star-forming region in the Large Magellanic Cloud, the&nbsp;<a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/science\/explore-the-night-sky\/hubble-caldwell-catalog\/caldwell-103\/\" rel=\"noopener\">Tarantula Nebula<\/a>, is a frequent target for Hubble.) We see bright, young stars lighting up the gas clouds and sculpting clumps of dust with powerful ultraviolet radiation.<\/p>\n<p>This image marries observations made roughly 20 years apart, a testament to Hubble\u2019s longevity. The first set of observations, which were carried out in 2002\u20132003, capitalized on the exquisite sensitivity and resolution of the then-newly-installed&nbsp;<a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/observatory\/design\/advanced-camera-for-surveys\/\" rel=\"noopener\">Advanced Camera for Surveys<\/a>. Astronomers turned Hubble toward the N11 star cluster to do something that had never been done before at the time: catalog all the stars in a young cluster with masses between 10% of the Sun\u2019s mass and 100 times the Sun\u2019s mass.<\/p>\n<p>The second set of observations came from Hubble\u2019s newest camera, the&nbsp;<a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/observatory\/design\/wide-field-camera-3\/\" rel=\"noopener\">Wide Field Camera 3<\/a>. These images focused on the dusty clouds that permeate the cluster, providing us with a new perspective on cosmic dust.<\/p>\n<p><a  href=\"https:\/\/facebook.com\/NASAHubble\" rel=\"noreferrer noopener\">@NASAHubble<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This NASA\/ESA\u00a0Hubble Space Telescope\u00a0image released on Sept. 12, 2025, features a cloudy starscape from an impressive star cluster. This scene is in the Large Magellanic Cloud, a dwarf galaxy situated about 160,000 light-years away in the constellations Dorado and Mensa. With a mass equal to 10\u201320% of the mass of the Milky Way, the Large [\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,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[15776],"tags":[],"class_list":["post-293395","post","type-post","status-publish","format-standard","hentry","category-star-clusters"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/293395","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/13"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=293395"}],"version-history":[{"count":3,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/293395\/revisions"}],"predecessor-version":[{"id":294039,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/293395\/revisions\/294039"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=293395"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=293395"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=293395"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}