{"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\/pl\/young_star_rebels_against_parent_cloud\/","title":{"rendered":"M\u0142oda gwiazda buntuje si\u0119 przeciwko chmurze rodzicielskiej"},"content":{"rendered":"
\n

Kosmiczny teleskop Hubble'a uchwyci\u0142 to niesamowite zdj\u0119cie gigantycznej chmury gazowej roz\u015bwietlanej przez jasn\u0105, m\u0142od\u0105 gwiazd\u0119. Zdj\u0119cie pokazuje, jak gwa\u0142towne mog\u0105 by\u0107 ko\u0144cowe etapy procesu powstawania gwiazd, gdy m\u0142ody obiekt wywiera ogromny wp\u0142yw na swoje otoczenie.<\/p>\n<\/div>\n

W chmurze wodoru znajduje si\u0119 niegrzeczna m\u0142oda gwiazda o nazwie S106 IR, kt\u00f3ra wyrzuca materi\u0119 z du\u017c\u0105 pr\u0119dko\u015bci\u0105, co powoduje zaburzenia w otaczaj\u0105cym j\u0105 gazie i pyle. Gwiazda ta ma mas\u0119 oko\u0142o 15 razy wi\u0119ksz\u0105 od S\u0142o\u0144ca i znajduje si\u0119 w ko\u0144cowej fazie swojego powstawania. Wkr\u00f3tce jej aktywno\u015b\u0107 ust\u0105pi, gdy wejdzie w sekwencj\u0119 g\u0142\u00f3wn\u0105, czyli doros\u0142\u0105 faz\u0119 \u017cycia gwiazdowego.<\/p>\n

Na razie S106 IR pozostaje w obr\u0119bie swojej macierzystej chmury, ale buntuje si\u0119 przeciwko niej. Materia\u0142 wydostaj\u0105cy si\u0119 z gwiazdy nie tylko nadaje chmurze kszta\u0142t klepsydry, ale tak\u017ce sprawia, \u017ce znajduj\u0105cy si\u0119 w niej wod\u00f3r jest bardzo gor\u0105cy i niespokojny. Skomplikowane wzory, kt\u00f3re tworzy, mo\u017cna wyra\u017anie dostrzec na tym zdj\u0119ciu z teleskopu Hubble\u2019a.<\/p>\n

M\u0142oda gwiazda ogrzewa r\u00f3wnie\u017c otaczaj\u0105cy j\u0105 gaz, powoduj\u0105c wzrost jego temperatury do 10 000 stopni Celsjusza! Promieniowanie gwiazdy sprawia, \u017ce gaz \u015bwieci \u2013 jest to niebieski obszar widoczny na tym zdj\u0119ciu.<\/p>\n

Te obszary \u015bwiec\u0105cego gazu oddziela od siebie ch\u0142odniejszy, g\u0119sty pas py\u0142u, kt\u00f3ry ma czerwony kolor. Ten ciemny materia\u0142 niemal ca\u0142kowicie zas\u0142ania m\u0142od\u0105 gwiazd\u0119, ale wci\u0105\u017c mo\u017cna j\u0105 dostrzec, jak wy\u0142ania si\u0119 z najszerszej cz\u0119\u015bci tego pasa py\u0142u.<\/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\/pl\/wp-json\/wp\/v2\/posts\/766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/comments?post=766"}],"version-history":[{"count":1,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/posts\/766\/revisions"}],"predecessor-version":[{"id":1909,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/posts\/766\/revisions\/1909"}],"wp:attachment":[{"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/media?parent=766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/categories?post=766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/tags?post=766"},{"taxonomy":"panel","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/panel?post=766"},{"taxonomy":"language","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/language?post=766"},{"taxonomy":"age","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/age?post=766"},{"taxonomy":"duration","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/duration?post=766"},{"taxonomy":"resource_type","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/resource_type?post=766"},{"taxonomy":"audience","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/audience?post=766"},{"taxonomy":"wf_post_folders","embeddable":true,"href":"https:\/\/kids.esa.int\/pl\/wp-json\/wp\/v2\/wf_post_folders?post=766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}