{"id":191832,"date":"2025-03-28T04:13:38","date_gmt":"2025-03-27T18:13:38","guid":{"rendered":"http:\/\/www.vibewire.com.au\/?guid=dde7d9d2cc7ff05eae7184d1173e872e"},"modified":"2025-03-28T04:13:38","modified_gmt":"2025-03-27T18:13:38","slug":"understanding-cosmic-explosions-starburst-arrives-at-nasa-for-testing","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=191832","title":{"rendered":"Understanding Cosmic Explosions: StarBurst Arrives at NASA for Testing"},"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-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg\"><img fetchpriority=\"high\" decoding=\"async\" width=\"1403\" height=\"1052\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?w=1403\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Six people in white clean suits stand around a metal box holding Starburst, a wide-field gamma ray observatory.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg 1403w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=300,225 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=768,576 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=1024,768 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=400,300 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=600,450 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=900,675 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-3.jpg?resize=1200,900 1200w\" sizes=\"(max-width: 1403px) 100vw, 1403px\" loading=\"eager\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">From left to right, NASA Marshall engineers Carlos Diaz and John Luke Bili, U.S. Naval Research Laboratory mechanical engineer contractor Eloise Stump, and Marshall engineers Tomasz Liz, David Banks, and Elise Doan observe StarBurst in the cleanroom environment before it\u2019s unboxed from its shipping container. The cleanroom environment at Marshall is designed to minimize contamination and protect the observatory\u2019s sensitive instruments. <\/div>\n<div class=\"hds-credits\"><em>Image Credit: NASA \/Daniel Kocevski \u00a0<\/em><\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>StarBurst, a wide-field gamma ray observatory, arrived at <a href=\"https:\/\/www.nasa.gov\/marshall\/\">NASA\u2019s Marshall Space Flight Center<\/a> in Huntsville, Alabama, March 4 for environmental testing and final instrument integration. The instrument is designed to detect the initial emission of short <a href=\"https:\/\/science.nasa.gov\/universe\/gamma-ray-bursts-harvesting-knowledge-from-the-universes-most-powerful-explosions\/\" rel=\"noopener\">gamma-ray bursts<\/a>, a key electromagnetic indicator of neutron star mergers.<\/p>\n<p>\u201cGamma-ray bursts are among the most powerful explosions in the universe, and they serve as <a href=\"https:\/\/science.nasa.gov\/directorates\/smd\/astrophysics-division\/how-nasa-chases-and-investigates-bright-cosmic-blips\/\" rel=\"noopener\">cosmic beacons<\/a> that help us understand extreme physics, including black hole formation and the behavior of matter under extreme conditions,\u201d said Dr. Daniel Kocevski, principal investigator of the StarBurst mission at NASA Marshall.<\/p>\n<p>According to Kocevski, neutron star mergers are particularly exciting because they produce gamma-ray bursts and gravitational waves, meaning scientists can study these events using two different signals \u2013 light and ripples in space time.<\/p>\n<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-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"2048\" height=\"1537\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?w=2048\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg 2815w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=300,225 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=768,576 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=1024,768 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=1536,1152 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=2048,1537 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=400,300 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=600,450 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=900,675 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=1200,900 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/a-happy-pi.jpg?resize=2000,1501 2000w\" sizes=\"auto, (max-width: 2048px) 100vw, 2048px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Starburst Principal Investigator Dr. Daniel Kocevski, left, and Integration and Test Engineer Elise Doan, right, pose with the StarBurst instrument after it was unboxed in the cleanroom environment at NASA Marshall. The Naval Research Lab transferred the instrument to NASA in early March.<\/div>\n<div class=\"hds-credits\"><em>Image Credit: NASA\/Davy Haynes<\/em><\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>The merging of neutron stars forges heavy elements such as gold and platinum, revealing the origins of some of Earth\u2019s building blocks.<\/p>\n<p>\u201cBy studying these gamma-ray bursts and the neutron star mergers that produce them, we gain insights into fundamental physics, the origins of elements, and even the expansion of the universe,\u201d Kocevski said. \u201cNeutron star mergers and gamma-ray bursts are nature\u2019s laboratories for testing our understanding of the cosmos.\u201d<\/p>\n<p>StarBurst will undergo flight vibration and thermal vacuum testing at Marshall in the <a href=\"https:\/\/www.nasa.gov\/setmo\/facilities\/sunspot\/#:~:text=The%20Sunspot%20Thermal%20Vacuum%20Testing,space-borne%20craft%20and%20components.\">Sunspot Thermal Vacuum Testing Facility.<\/a> These tests ensure it can survive the rigors of launch and harsh environment of space.<\/p>\n<p>Final instrument integration will happen in the Stray Light Facility, which is a specialized environment to help identify and reduce unwanted light in certain areas of the optical systems.<\/p>\n<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-fit \"><a href=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"1403\" height=\"1052\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?w=1403\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg 1403w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=300,225 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=768,576 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=1024,768 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=400,300 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=600,450 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=900,675 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/03\/starburst-1.jpg?resize=1200,900 1200w\" sizes=\"auto, (max-width: 1403px) 100vw, 1403px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">The StarBurst Multimessenger Pioneer is a wide-field gamma-ray observatory designed to detect the initial emission of short gamma-ray bursts, important electromagnetic indicators of neutron star mergers. With an effective area over five times that of the Fermi Gamma-ray Burst Monitor and complete visibility of the unobscured sky, StarBurst will conduct sensitive observations. <\/div>\n<div class=\"hds-credits\">NASA\/Daniel Kocevski<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>StarBurst is a collaborative effort led by NASA\u2019s Marshall Space Flight Center, with partnerships with the U.S. Naval Research Laboratory, the University of Alabama Huntsville, the Universities Space Research Association, and the UTIAS Space Flight Laboratory. StarBurst was selected for development as part of the NASA Astrophysics Pioneers program, which supports lower-cost, smaller hardware missions to conduct compelling astrophysics science.<\/p>\n<p>To learn more about StarBurst visit:<\/p>\n<p class=\"has-text-align-center\"><a href=\"https:\/\/science.nasa.gov\/mission\/starburst\/\" rel=\"noopener\">https:\/\/science.nasa.gov\/mission\/starburst\/<\/a><\/p>\n<p><strong>Media Contact:<\/strong><\/p>\n<p>Lane Figueroa<br \/>Marshall Space Flight Center<br \/>Huntsville, Alabama<br \/>256.544.0034<br \/><a href=\"mailto:lane.e.figueroa@nasa.gov\">lane.e.figueroa@nasa.gov<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>StarBurst, a wide-field gamma ray observatory, arrived at NASA\u2019s Marshall Space Flight Center in Huntsville, Alabama, March 4 for environmental testing and final instrument integration. The instrument is designed to detect the initial emission of short gamma-ray bursts, a key electromagnetic indicator of neutron star mergers. \u201cGamma-ray bursts are among the most powerful explosions in [\u2026]<\/p>\n","protected":false},"author":24,"featured_media":1,"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":[16104,15672,16105,15673,15638],"tags":[],"class_list":["post-191832","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-gamma-rays","category-marshall-astrophysics","category-marshall-science-research-projects","category-marshall-space-flight-center","category-the-universe"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/191832","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\/24"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=191832"}],"version-history":[{"count":3,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/191832\/revisions"}],"predecessor-version":[{"id":191878,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/191832\/revisions\/191878"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=191832"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=191832"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=191832"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}