{"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\/ro\/young_star_rebels_against_parent_cloud\/","title":{"rendered":"T\u00e2n\u0103ra vedet\u0103 se revolt\u0103 \u00eempotriva \u201enorului\u201d p\u0103rintesc"},"content":{"rendered":"<div class=\"lede\">\n<p>Telescopul spa\u021bial Hubble a surprins aceast\u0103 imagine uimitoare a unui nor uria\u0219 de gaz iluminat de o stea t\u00e2n\u0103r\u0103 \u0219i str\u0103lucitoare. Imaginea ilustreaz\u0103 c\u00e2t de violente pot fi etapele finale ale procesului de formare a stelelor, obiectul t\u00e2n\u0103r provoc\u00e2nd tulbur\u0103ri \u00een mediul \u00eenconjur\u0103tor.<\/p>\n<\/div>\n<p>O stea t\u00e2n\u0103r\u0103 \u0219i neast\u00e2mp\u0103rat\u0103, numit\u0103 S106 IR, se afl\u0103 \u00een interiorul norului de hidrogen gazos \u0219i arunc\u0103 materie cu vitez\u0103 mare, ceea ce perturb\u0103 gazul \u0219i praful din jurul ei. Steaua are o mas\u0103 de aproximativ 15 ori mai mare dec\u00e2t cea a Soarelui \u0219i se afl\u0103 \u00een etapele finale ale form\u0103rii sale. \u00cen cur\u00e2nd se va lini\u0219ti, c\u00e2nd va intra \u00een secven\u021ba principal\u0103, etapa adult\u0103 a vie\u021bii stelare.<\/p>\n<p>Deocamdat\u0103, S106 IR r\u0103m\u00e2ne \u00een norul din care provine, dar se revolt\u0103 \u00eempotriva acestuia. Materialul care se desprinde din stea nu numai c\u0103 confer\u0103 norului forma de clepsidr\u0103, ci \u0219i face ca hidrogenul gazos din interiorul acestuia s\u0103 fie foarte fierbinte \u0219i agitat. Modelele complexe pe care le formeaz\u0103 pot fi observate clar \u00een aceast\u0103 imagine realizat\u0103 de telescopul Hubble.<\/p>\n<p>De asemenea, t\u00e2n\u0103ra stea \u00eenc\u0103lze\u0219te gazul din jur, f\u0103c\u00e2ndu-l s\u0103 ating\u0103 temperaturi de 10 000 de grade Celsius! Radia\u021bia stelei face ca gazul s\u0103 str\u0103luceasc\u0103, aceasta fiind zona albastr\u0103 din aceast\u0103 imagine.<\/p>\n<p>\u00centre aceste zone de gaz str\u0103lucitor se afl\u0103 o f\u00e2\u0219ie de praf mai rece \u0219i mai dens\u0103, care apare \u00een ro\u0219u. Acest material \u00eentunecat ascunde aproape complet steaua t\u00e2n\u0103r\u0103, dar aceasta poate fi totu\u0219i z\u0103rit\u0103 prin cea mai larg\u0103 parte a f\u00e2\u0219iei de praf.<\/p>","protected":false},"excerpt":{"rendered":"<p>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 [&hellip;]<\/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\/ro\/wp-json\/wp\/v2\/posts\/766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/comments?post=766"}],"version-history":[{"count":1,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/posts\/766\/revisions"}],"predecessor-version":[{"id":1909,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/posts\/766\/revisions\/1909"}],"wp:attachment":[{"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/media?parent=766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/categories?post=766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/tags?post=766"},{"taxonomy":"panel","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/panel?post=766"},{"taxonomy":"language","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/language?post=766"},{"taxonomy":"age","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/age?post=766"},{"taxonomy":"duration","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/duration?post=766"},{"taxonomy":"resource_type","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/resource_type?post=766"},{"taxonomy":"audience","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/audience?post=766"},{"taxonomy":"wf_post_folders","embeddable":true,"href":"https:\/\/kids.esa.int\/ro\/wp-json\/wp\/v2\/wf_post_folders?post=766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}