{"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\/nb\/young_star_rebels_against_parent_cloud\/","title":{"rendered":"Ung stjerne gj\u00f8r oppr\u00f8r mot moderskyen"},"content":{"rendered":"
\n

Hubble-romteleskopet har tatt dette fantastiske bildet av en gigantisk gassky som blir opplyst av en lys, ung stjerne. Bildet viser hvor voldsomme sluttfasene av stjernedannelsesprosessen kan v\u00e6re, der det unge himmellegemet ryster opp omgivelsene sine.<\/p>\n<\/div>\n

En urolig ung stjerne, kalt S106 IR, befinner seg inne i skyen av hydrogen og slynger ut materiale i h\u00f8y hastighet, noe som forstyrrer gassen og st\u00f8vet rundt seg. Stjernen har en masse som er omtrent 15 ganger st\u00f8rre enn Solens og befinner seg i de siste stadiene av sin dannelse. Den vil snart roe seg ned n\u00e5r den g\u00e5r inn i hovedsekvensen, den voksne fasen av et stjerneliv.<\/p>\n

Forel\u00f8pig holder S106 IR seg innenfor sin modersky, men den gj\u00f8r oppr\u00f8r mot den. Materialet som str\u00f8mmer ut fra stjernen gir ikke bare skyen sin timeglassform, men gj\u00f8r ogs\u00e5 hydrogenet i den sv\u00e6rt varmt og urolig. De kompliserte m\u00f8nstrene som dannes, kan tydelig ses p\u00e5 dette Hubble-bildet.<\/p>\n

Den unge stjernen varmer ogs\u00e5 opp gassen rundt seg, slik at den n\u00e5r temperaturer p\u00e5 10 000 grader Celsius! Str\u00e5lingen fra stjernen f\u00e5r gassen til \u00e5 gl\u00f8de, noe som vises som det bl\u00e5 omr\u00e5det p\u00e5 dette bildet.<\/p>\n

Mellom disse omr\u00e5dene med gl\u00f8dende gass ligger et kj\u00f8ligere, tykt st\u00f8vb\u00e5nd som fremst\u00e5r som r\u00f8dt. Dette m\u00f8rke materialet skjuler den unge stjernen nesten fullstendig, men man kan likevel se den titte frem gjennom den bredeste delen av st\u00f8vb\u00e5ndet.<\/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\/nb\/wp-json\/wp\/v2\/posts\/766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/comments?post=766"}],"version-history":[{"count":1,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/posts\/766\/revisions"}],"predecessor-version":[{"id":1909,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/posts\/766\/revisions\/1909"}],"wp:attachment":[{"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/media?parent=766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/categories?post=766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/tags?post=766"},{"taxonomy":"panel","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/panel?post=766"},{"taxonomy":"language","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/language?post=766"},{"taxonomy":"age","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/age?post=766"},{"taxonomy":"duration","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/duration?post=766"},{"taxonomy":"resource_type","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/resource_type?post=766"},{"taxonomy":"audience","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/audience?post=766"},{"taxonomy":"wf_post_folders","embeddable":true,"href":"https:\/\/kids.esa.int\/nb\/wp-json\/wp\/v2\/wf_post_folders?post=766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}