{"id":766,"date":"2011-12-16T10:22:00","date_gmt":"2011-12-16T09:22:00","guid":{"rendered":"https:\/\/kids.esa.int\/young_star_rebels_against_parent_cloud\/"},"modified":"2026-10-08T00:32:02","modified_gmt":"2026-10-07T22:32:02","slug":"young_star_rebels_against_parent_cloud","status":"publish","type":"post","link":"https:\/\/kids.esa.int\/da\/young_star_rebels_against_parent_cloud\/","title":{"rendered":"Ung stjerne g\u00f8r opr\u00f8r mod for\u00e6ldrenes cloud"},"content":{"rendered":"
\n

Hubble-rumteleskopet har taget dette fantastiske billede af en k\u00e6mpe gassky, der oplyses af en lysst\u00e6rk, ung stjerne. Billedet viser, hvor voldsomme de sidste faser af stjernedannelsesprocessen kan v\u00e6re, idet det unge himmellegeme ryster omgivelserne igennem.<\/p>\n<\/div>\n

En vild ung stjerne ved navn S106 IR befinder sig inde i skyen af brintgas og udst\u00f8der materiale med h\u00f8j hastighed, hvilket forstyrrer gassen og st\u00f8vet omkring den. Stjernen har en masse, der er omkring 15 gange st\u00f8rre end Solens, og befinder sig i de sidste faser af sin dannelse. Den vil snart falde til ro, n\u00e5r den tr\u00e6der ind i hovedsekvensen, den voksne fase af et stjerneliv.<\/p>\n

Forel\u00f8big forbliver S106 IR inden for sin modersky, men den g\u00f8r opr\u00f8r mod den. Det materiale, der str\u00f8mmer ud fra stjernen, giver ikke blot skyen sin timeglasform, men g\u00f8r ogs\u00e5 brintgassen i den meget varm og urolig. De komplicerede m\u00f8nstre, den danner, kan tydeligt ses p\u00e5 dette Hubble-billede.<\/p>\n

Den unge stjerne opvarmer ogs\u00e5 den omgivende gas, s\u00e5 den n\u00e5r temperaturer p\u00e5 10 000 grader Celsius! Stjernens str\u00e5ling f\u00e5r gassen til at lyse, hvilket ses som det bl\u00e5 omr\u00e5de p\u00e5 dette billede.<\/p>\n

Mellem disse omr\u00e5der med gl\u00f8dende gas ligger et k\u00f8ligere, t\u00e6t st\u00f8vb\u00e5nd, der fremst\u00e5r r\u00f8dt. Dette m\u00f8rke materiale skjuler den unge stjerne n\u00e6sten fuldst\u00e6ndigt for synet, men man kan stadig se den titte frem gennem st\u00f8vb\u00e5ndets bredeste del.<\/p>","protected":false},"excerpt":{"rendered":"

The Hubble space telescope has captured this amazing image of a giant gas cloud lit up by a bright young star. The image shows how violent the end stages of […]<\/p>\n","protected":false},"author":5,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"esa_banner_image":"https:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/images\/2011\/12\/hubble_view_of_star-forming_region_s1062\/18248289-2-eng-GB\/Hubble_view_of_star-forming_region_S106.jpg","esa_banner_description":"","esa_banner_credit":"NASA\/ESA","esa_banner_licence":"ESA Standard Licence","esa_banner_detail_url":"https:\/\/www.esa.int\/ESA_Multimedia\/Images\/2011\/12\/Hubble_view_of_star-forming_region_S1062","esa_external_url":"","esa_external_new_window":false,"_jetpack_feature_clip_id":0,"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_post_was_ever_published":true},"categories":[10,11,21],"tags":[],"panel":[],"language":[],"age":[],"duration":[],"resource_type":[],"audience":[],"wf_post_folders":[],"class_list":["post-766","post","type-post","status-publish","format-standard","hentry","category-learn","category-our-universe","category-stars-and-galaxies"],"jetpack_sharing_enabled":true,"jetpack_featured_media_url":"","_links":{"self":[{"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/posts\/766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/comments?post=766"}],"version-history":[{"count":1,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/posts\/766\/revisions"}],"predecessor-version":[{"id":1909,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/posts\/766\/revisions\/1909"}],"wp:attachment":[{"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/media?parent=766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/categories?post=766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/tags?post=766"},{"taxonomy":"panel","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/panel?post=766"},{"taxonomy":"language","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/language?post=766"},{"taxonomy":"age","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/age?post=766"},{"taxonomy":"duration","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/duration?post=766"},{"taxonomy":"resource_type","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/resource_type?post=766"},{"taxonomy":"audience","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/audience?post=766"},{"taxonomy":"wf_post_folders","embeddable":true,"href":"https:\/\/kids.esa.int\/da\/wp-json\/wp\/v2\/wf_post_folders?post=766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}