{"id":50283,"date":"2025-07-02T18:15:59","date_gmt":"2025-07-02T16:15:59","guid":{"rendered":"https:\/\/www.h-its.org\/de\/?p=50283"},"modified":"2025-11-26T18:26:01","modified_gmt":"2025-11-26T17:26:01","slug":"doppelte-detonation","status":"publish","type":"post","link":"https:\/\/www.h-its.org\/de\/2025\/07\/02\/doppelte-detonation\/","title":{"rendered":"Doppelte Detonation: Tod eines wei\u00dfen Zwergs"},"content":{"rendered":"\n<p>Ein internationales Team unter Mitwirkung von HITS-Forschenden hat visuell bewiesen, dass ein Wei\u00dfer Zwergstern in einer doppelten Detonation explodierte und nicht, wie bisher angenommen, durch eine einzige. Mit dem Very Large Telescope (VLT) der ESO und dessen MUSE-Instrument nahmen sie ein Bild des Supernova-\u00dcberrestes SNR 0509 67.5 auf, der sich etwa 160.000 Lichtjahre entfernt in der Gro\u00dfen Magellanschen Wolke befindet.<\/p>\n\n\n<div class=\"wp-block-image\">\n<figure class=\"alignleft size-large is-resized\"><a href=\"https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a.jpg\" target=\"_blank\" rel=\" noreferrer noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"682\" src=\"https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-1024x682.jpg\" alt=\"This image, taken with ESO\u2019s Very Large Telescope (VLT), shows the supernova remnant SNR 0509-67.5. These are the expanding remains of a star that exploded hundreds of years ago in a double-detonation \u2013 the first photographic evidence that stars can die with two blasts. The data were captured with the Multi-Unit Spectroscopic Explorer (MUSE) instrument at the VLT. MUSE allows astronomers to map the distribution of different chemical elements, displayed here in different colours. Calcium is shown in blue, and it is arranged in two concentric shells. These two layers indicate that the now-dead star exploded with a double-detonation.\" class=\"wp-image-50284\" style=\"width:312px;height:auto\" srcset=\"https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-1024x682.jpg 1024w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-300x200.jpg 300w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-768x512.jpg 768w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-640x427.jpg 640w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-1200x800.jpg 1200w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-2x1.jpg 2w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-420x280.jpg 420w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a-610x407.jpg 610w, https:\/\/www.h-its.org\/de\/wp-content\/uploads\/sites\/2\/2025\/11\/eso2511a.jpg 1280w\" sizes=\"auto, (max-width: 639px) 98vw, (max-width: 1199px) 64vw, 770px\" \/><\/a><figcaption class=\"wp-element-caption\">VLT-Aufnahme einer Supernova mit doppelter Detonation (Bild: ESO)<\/figcaption><\/figure>\n<\/div>\n\n\n<p>Zum ersten Mal haben sie zwei konzentrische Kalziumschalen \u2013 einen \u00e4u\u00dferen und einen inneren Ring \u2013 beobachtet, die sie als \u00dcberreste der beiden Explosionen interpretieren: Zuerst entz\u00fcndete sich die Heliumh\u00fclle des Wei\u00dfen Zwergs, und kurz darauf detonierte der Kern.<\/p>\n\n\n\n<p>\u201eDie Explosionen von Wei\u00dfen Zwergen spielen in der Astronomie eine entscheidende Rolle\u201c, sagt <a href=\"https:\/\/www.unsw.edu.au\/hdr\/priyam-das\" target=\"_blank\" rel=\"noreferrer noopener\">Priyam Das<\/a>,(University of New South Wales Canberra, Australien), Erstautor der <a href=\"https:\/\/www.nature.com\/articles\/s41550-025-02589-5\" target=\"_blank\" rel=\"noreferrer noopener\">Studie<\/a> und ehemaliger HITS-Gastwissenschaftler. Ein Gro\u00dfteil unseres Wissens \u00fcber die Expansion des Universums basiert auf Supernovae vom Typ Ia, die auch die Hauptquelle f\u00fcr Eisen auf unserem Planeten sind, einschlie\u00dflich des Eisens in unserem Blut. Die Ergebnisse der Studie geben Aufschluss dar\u00fcber, wie einige dieser Supernovae auf andere Weise entstehen k\u00f6nnen.<\/p>\n\n\n\n<p>Ivo Seitenzahl, der als Gastwissenschaftler in der HITS-Gruppe \u201e<a href=\"https:\/\/www.h-its.org\/de\/forschung\/pso\/\">Physics of Stellar Objects<\/a>\u201c die Beobachtungen leitete, sieht in den Ergebnissen einen klaren Hinweis darauf, \u201edass Wei\u00dfe Zwerge schon lange vor Erreichen der ber\u00fchmten Chandrasekhar-Masse explodieren k\u00f6nnen und dass der Mechanismus der Doppeldetonation tats\u00e4chlich in der Natur vorkommt\u201c.<\/p>\n\n\n\n<p><em>Das, P., Seitenzahl, I.R., Ruiter, A.J.\u00a0et al.\u00a0Calcium in a supernova remnant as a fingerprint of a sub-Chandrasekhar-mass explosion.\u00a0In: Nat Astron\u00a0(2025). <\/em><a href=\"https:\/\/doi.org\/10.1038\/s41550-025-02589-5\" target=\"_blank\" rel=\"noreferrer noopener\"><em>https:\/\/doi.org\/10.1038\/s41550-025-02589-5<\/em><\/a><\/p>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Ein internationales Team unter Mitwirkung von HITS-Forschenden hat visuell bewiesen, dass ein Wei\u00dfer Zwergstern in einer doppelten Detonation explodierte und &#8230;<\/p>\n","protected":false},"author":58,"featured_media":50284,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":""},"categories":[1,92],"hits-research-group":[1279],"class_list":["post-50283","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-gruppen-news","category-wissenschaftsnews","hits-research-group-pso-de"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.2 - 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