{"id":1698,"date":"2024-04-06T17:01:08","date_gmt":"2024-04-06T14:01:08","guid":{"rendered":"https:\/\/haberv8.thewpdemo.com\/nasa-yeni-olusan-gezegenlere-dair-kanitlar-buldu\/-1698.html"},"modified":"2024-04-06T17:01:08","modified_gmt":"2024-04-06T14:01:08","slug":"nasa-yeni-olusan-gezegenlere-dair-kanitlar-buldu","status":"publish","type":"post","link":"https:\/\/egetv.tr\/?p=1698","title":{"rendered":"NASA, yeni olu\u015fan gezegenlere dair kan\u0131tlar buldu"},"content":{"rendered":"<\/p>\n<p>\n                <span>AA <\/span>\n            <\/p>\n<p class=\"text\">NASA bilim insanlar\u0131, &#8220;SAO 206462&#8221;, &#8220;HL Tauri (HL Tau)&#8221;, ve &#8220;MWC 758&#8221; ad\u0131 verilen y\u0131ld\u0131zlar\u0131n y\u00f6r\u00fcngesindeki olas\u0131 \u00f6n gezegenlerin (protogezegen) tespiti i\u00e7in \u00e7al\u0131\u015fma ba\u015flatt\u0131.<\/p>\n<p class=\"text\">Bu kapsamda; JWST, Hubble Uzay Teleskobu ve Atacama B\u00fcy\u00fck Milimetre Dizisi (ALMA) taraf\u0131ndan toplanan veriler incelendi.<\/p>\n<p class=\"text\">Ara\u015ft\u0131rma Michigan \u00dcniversitesi, Arizona \u00dcniversitesi ve Victoria \u00dcniversitesinden bilim insanlar\u0131 liderli\u011findeki bir ekip taraf\u0131ndan yap\u0131ld\u0131.<\/p>\n<p class=\"text\">\u00c7al\u0131\u015fma, \u00f6n gezegen diskleri ile bu disklerin merkezinde yer alan y\u0131ld\u0131zlara daha yak\u0131n olan gaz zarflar\u0131 aras\u0131ndaki \u015fimdiye kadar g\u00f6r\u00fclmemi\u015f etkile\u015fimleri de ortaya \u00e7\u0131kard\u0131.<\/p>\n<p><strong>Kan\u0131tlar bulundu<\/strong><\/p>\n<p class=\"text\">Ekip \u00fcyesi ve Michigan \u00dcniversitesinden g\u00f6k bilimci Gabriele Cugno ve ekibi, hen\u00fcz G\u00fcne\u015f gibi \u00e7ekirde\u011finde hidrojenin helyuma d\u00f6n\u00fc\u015f\u00fcm f\u00fczyonunu tetikleyecek kadar yeterli k\u00fctleye sahip olmayan bir \u00f6n y\u0131ld\u0131z (protostar) &#8220;SAO 206462&#8243;nin y\u00f6r\u00fcngesindeki \u00f6n gezegen diskine ili\u015fkin JWST g\u00f6zleminde, bir gezegenin olu\u015fmakta oldu\u011funa dair kan\u0131tlar buldu.<\/p>\n<p><img decoding=\"async\" src=\"https:\/\/egetv.tr\/wp-content\/uploads\/2024\/04\/nasa-yeni-olusan-gezegenlere-dair-kanitlar-buldu-0.jpg\" \/><\/p>\n<p class=\"text\">SAO 206462&#8217;deki \u00f6n gezegen diskinin, Hubble, ALMA ve \u00c7ok B\u00fcy\u00fck Teleskop (VLT) taraf\u0131ndan da g\u00f6zlemlendi\u011fi ve diskin iki g\u00fc\u00e7l\u00fc sarmaldan olu\u015ftu\u011funun ortaya \u00e7\u0131kt\u0131\u011f\u0131 kaydedilen ara\u015ft\u0131rmada, ekibin Sat\u00fcrn veya J\u00fcpiter gibi \u00e7o\u011funlukla helyumdan olu\u015fan gaz devi bir gezegen g\u00f6rmeyi bekledi\u011fi, ancak buna dair bir g\u00f6zlem yap\u0131lamad\u0131\u011f\u0131 belirtildi.<\/p>\n<p class=\"text\">JWST&#8217;nin Yak\u0131n K\u0131z\u0131l\u00f6tesi Kameras\u0131&#8217;n\u0131 (NIRCam) kullanan ekip, olas\u0131 gezegenden gelen, y\u00fcksek h\u0131zlardaki maddelerin d\u00fc\u015fmesi sonucu ortaya \u00e7\u0131kan termal enerjiyi tespit etti.<\/p>\n<p class=\"text\">Bulgular, olas\u0131 gezegenin bir gaz devi olmas\u0131 halinde, merkezindeki SAO 206462&#8217;den D\u00fcnya ile G\u00fcne\u015f aras\u0131ndaki mesafenin yakla\u015f\u0131k 300 kat\u0131 kadar uzakta bulundu\u011funu, k\u00fctlesinin J\u00fcpiter&#8217;in en fazla 2,2 kat\u0131 ve \u00e7ok so\u011fuk olabilece\u011fini g\u00f6sterdi.<\/p>\n<p>        Haber Kayna\u011f\u0131: Anadolu Ajans\u0131 (AA)<\/p>\n","protected":false},"excerpt":{"rendered":"<p>AA NASA bilim insanlar\u0131, &#8220;SAO 206462&#8221;, &#8220;HL Tauri (HL Tau)&#8221;, ve &#8220;MWC 758&#8221; ad\u0131 verilen y\u0131ld\u0131zlar\u0131n y\u00f6r\u00fcngesindeki olas\u0131 \u00f6n gezegenlerin (protogezegen) tespiti i\u00e7in \u00e7al\u0131\u015fma ba\u015flatt\u0131. Bu kapsamda; JWST, Hubble Uzay Teleskobu ve Atacama B\u00fcy\u00fck Milimetre Dizisi (ALMA) taraf\u0131ndan toplanan veriler incelendi. Ara\u015ft\u0131rma Michigan \u00dcniversitesi, Arizona \u00dcniversitesi ve Victoria \u00dcniversitesinden bilim insanlar\u0131 liderli\u011findeki bir ekip taraf\u0131ndan [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1701,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[14],"tags":[32],"class_list":["post-1698","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-teknoloji","tag-teknoloji"],"views":1,"_links":{"self":[{"href":"https:\/\/egetv.tr\/index.php?rest_route=\/wp\/v2\/posts\/1698","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/egetv.tr\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/egetv.tr\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/egetv.tr\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/egetv.tr\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=1698"}],"version-history":[{"count":0,"href":"https:\/\/egetv.tr\/index.php?rest_route=\/wp\/v2\/posts\/1698\/revisions"}],"wp:attachment":[{"href":"https:\/\/egetv.tr\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1698"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/egetv.tr\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1698"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/egetv.tr\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1698"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}