{"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\/sl\/young_star_rebels_against_parent_cloud\/","title":{"rendered":"Mlada zvezda se upira star\u0161evskemu oblaku"},"content":{"rendered":"
\n

Vesoljski teleskop Hubble je posnel to neverjetno sliko orja\u0161kega plinskega oblaka, ki ga osvetljuje svetla mlada zvezda. Slika prikazuje, kako burne so lahko zaklju\u010dne faze procesa nastajanja zvezd, saj mlado nebesno telo mo\u010dno pretresa svojo okolico.<\/p>\n<\/div>\n

V oblaku vodikovega plina se nahaja \u00bbporedna\u00ab mlada zvezda z imenom S106 IR, ki izvr\u017ee snov z visoko hitrostjo, kar povzro\u010da motnje v plinu in prahu okoli nje. Zvezda ima maso, ki je pribli\u017eno 15-krat ve\u010dja od Son\u010deve, in se nahaja v zaklju\u010dnih fazah svojega nastajanja. Kmalu se bo umirila, ko bo vstopila v glavno zaporedje, odraslo fazo zvezdnega \u017eivljenja.<\/p>\n

Zaenkrat S106 IR ostaja znotraj svojega mati\u010dnega oblaka, vendar se mu upira. Snov, ki se izlo\u010da iz zvezde, ne daje oblaku le obliko pe\u0161\u010dene ure, temve\u010d povzro\u010da tudi, da je vodikov plin v njem zelo vro\u010d in nemiren. Zapleteni vzorci, ki jih ustvarja, so jasno vidni na tej sliki teleskopa Hubble.<\/p>\n

Mlada zvezda segreva tudi okoli\u0161ki plin, tako da ta dose\u017ee temperature 10 000 stopinj Celzija! Zaradi sevanja zvezde plin zasveti, kar na tej sliki predstavlja modro obmo\u010dje.<\/p>\n

Ta obmo\u010dja \u017eare\u010dega plina lo\u010duje hladnej\u0161i, gost pas prahu, ki se zdi rde\u010d. Ta temna snov mlado zvezdo skoraj popolnoma zakriva, vendar jo je \u0161e vedno mogo\u010de videti, kako pokuka skozi naj\u0161ir\u0161i del prahovnega pasu.<\/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\/sl\/wp-json\/wp\/v2\/posts\/766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/comments?post=766"}],"version-history":[{"count":1,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/posts\/766\/revisions"}],"predecessor-version":[{"id":1909,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/posts\/766\/revisions\/1909"}],"wp:attachment":[{"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/media?parent=766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/categories?post=766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/tags?post=766"},{"taxonomy":"panel","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/panel?post=766"},{"taxonomy":"language","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/language?post=766"},{"taxonomy":"age","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/age?post=766"},{"taxonomy":"duration","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/duration?post=766"},{"taxonomy":"resource_type","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/resource_type?post=766"},{"taxonomy":"audience","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/audience?post=766"},{"taxonomy":"wf_post_folders","embeddable":true,"href":"https:\/\/kids.esa.int\/sl\/wp-json\/wp\/v2\/wf_post_folders?post=766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}