{"id":7689,"date":"2023-12-21T10:00:00","date_gmt":"2023-12-21T08:00:00","guid":{"rendered":"https:\/\/uni-mag.gr\/?p=7689"},"modified":"2024-07-23T21:18:18","modified_gmt":"2024-07-23T18:18:18","slug":"heart-nebula","status":"publish","type":"post","link":"https:\/\/www.uni-mag.gr\/de\/heart-nebula\/","title":{"rendered":"DER HERZNEBEL"},"content":{"rendered":"\n<p class=\"has-text-align-left\">Der Emissionsnebel IC 1805, wegen seiner charakteristischen Form auch Herznebel genannt, liegt etwa 7.500 Lichtjahre entfernt im Sternbild Kassiopeia. Dieser Nebel wurde durch die Sternwinde und die ultraviolette Strahlung der jungen, riesigen, \u00fcberhitzten Sterne geformt, die im Sternhaufen Melotte 15 in seinem Zentrum enthalten sind.<\/p>\n\n<p class=\"has-text-align-left\">Weitere Informationen finden Sie auf der Website der Eugenides-Stiftung <a href=\"https:\/\/www.eef.edu.gr\/el\/nea\/to-nefeloma-tis-kardias\/?fbclid=IwAR0dI075j3tlwAD2MKAgYOfPTtQiaQU4HQ9Psj691UDCFuLLHrh6Gzha0o0\">https:\/\/www.eef.edu.gr\/el\/nea\/to-nefeloma-tis-kardias\/?fbclid=IwAR0dI075j3tlwAD2MKAgYOfPTtQiaQU4HQ9Psj691UDCFuLLHrh6Gzha0o0<\/a><\/p>\n<div class=\"wp-block-image\">\n<figure class=\"alignleft size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"1198\" height=\"800\" src=\"https:\/\/www.uni-mag.gr\/wp-content\/uploads\/2023\/12\/heart-nebula-web.png\" alt=\"\" class=\"wp-image-7569\" srcset=\"https:\/\/www.uni-mag.gr\/wp-content\/uploads\/2023\/12\/heart-nebula-web.png 1198w, https:\/\/www.uni-mag.gr\/wp-content\/uploads\/2023\/12\/heart-nebula-web-300x200.png 300w, https:\/\/www.uni-mag.gr\/wp-content\/uploads\/2023\/12\/heart-nebula-web-1024x684.png 1024w, https:\/\/www.uni-mag.gr\/wp-content\/uploads\/2023\/12\/heart-nebula-web-768x513.png 768w\" sizes=\"auto, (max-width: 1198px) 100vw, 1198px\" \/><figcaption class=\"wp-element-caption\">Herznebel IC 1805, aufgenommen mit einem Teleskop und einer wissenschaftlichen CCD-Kamera<\/figcaption><\/figure><\/div>","protected":false},"excerpt":{"rendered":"<p class=\"card-text\">Dieser Nebel wurde durch die Sternwinde und die ultraviolette Strahlung der jungen, riesigen und \u00fcberhitzten Sterne geformt, die im Sternhaufen Melotte 15 in seinem Zentrum enthalten sind. [&#8230;]<\/p>\n<p class=\"m-0\"><a class=\"btn btn-outline-secondary btn-read-more\" href=\"https:\/\/www.uni-mag.gr\/de\/heart-nebula\/\">Read More<\/a><\/p>\n","protected":false},"author":3,"featured_media":7571,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[765,1106],"tags":[1454,1325,1459,1460,1326,1461],"class_list":["post-7689","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-issues-de","category-issue-06-de","tag-heart-de","tag-heart-nebula-de","tag-ic-de","tag-ic-1805-de","tag-issue-06-de","tag-nebula-de"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>DER HERZNEBEL | UNI-MAG<\/title>\n<meta name=\"description\" content=\"Der Emissionsnebel IC 1805, wegen seiner charakteristischen Form auch Herznebel genannt, liegt etwa 7.500 Lichtjahre entfernt im 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