{"id":5723,"date":"2012-02-22T09:58:29","date_gmt":"2012-02-22T07:58:29","guid":{"rendered":"http:\/\/www.islamidavet.com\/kutuphane\/\/?p=5723"},"modified":"2012-02-22T09:58:29","modified_gmt":"2012-02-22T07:58:29","slug":"uranus","status":"publish","type":"post","link":"https:\/\/www.islamidavet.com\/kutuphane\/uranus\/","title":{"rendered":"Uran\u00fcs"},"content":{"rendered":"<p> Uran\u00fcs, 2.872.460.000 km lik mesafe ile g\u00fcne\u015fe yak\u0131nl\u0131k s\u0131ras\u0131nda 7. gezegendir. 1781 y\u0131l\u0131nda Sir W. Herschel taraf\u0131ndan g\u00f6zlenmi\u015ftir. \u00c7ap\u0131 yakla\u015f\u0131k olarak 25600 km kadard\u0131r. 17 saat civar\u0131nda tamamlad\u0131\u011f\u0131 eksen periyodunu yuvarlanarak yapar. Bu nedenle kutuplardaki bas\u0131kl\u0131\u011f\u0131 y\u00fcksektir. G\u00fcne\u015fe olan uzakl\u0131\u011f\u0131 nedeni ile hakk\u0131nda pek fazla bilgi bulunmamakt\u0131r. Gezegenin yap\u0131s\u0131 ve atmosferi hakk\u0131ndaki bilgiler \u00e7o\u011funlukla tahminlere ve 1986 y\u0131l\u0131nda gezegenin yak\u0131nlar\u0131ndan ge\u00e7en Voyager 2 sondas\u0131ndan al\u0131nan bilgilere dayanmaktad\u0131r. Bu bilgiler \u0131\u015f\u0131\u011f\u0131nda; gezegenin, hidrojen bak\u0131m\u0131ndan zengin, metan ve helyum i\u00e7eren \u00e7ok yo\u011fun bir atmosfere sahip oldu\u011fu, y\u00fczey s\u0131cakl\u0131\u011f\u0131n\u0131n -221 C\u00ba civarlar\u0131nda oldu\u011fu, d\u00fcnyan\u0131nkinden daha b\u00fcy\u00fck bir ma\u011fnetik alana sahip oldu\u011fu ve kayal\u0131k bir \u00e7ekirde\u011finin bulundu\u011fu gibi tahminler ileri s\u00fcr\u00fclmektedir.<br \/>\n Uran\u00fcs&#8217;\u00fcn \u015fu ana kadar g\u00f6zlene bilinmi\u015f 17 uydusu bulunmaktad\u0131r. Bu uydulardan ikisi olan Titana ve Oberon gezegeni ilk g\u00f6zlemleme \u00fcnvan\u0131na da sahip olan Sir W. Herschel taraf\u0131ndan g\u00f6zlenmi\u015ftir. 1948 y\u0131l\u0131na kadar be\u015f b\u00fcy\u00fck ana uydusu g\u00f6zlenile bilinmi\u015fti. Fakat 1986&#8217;da Voyager 2 sondas\u0131 bu uydulara ek olarak 10 k\u00fc\u00e7\u00fck uydu daha bulmu\u015ftur. 31 Ekim 1997&#8217;de ise yar\u0131 \u00e7aplar\u0131 160 ve 80 km olan iki uydu daha g\u00f6zlenmi\u015ftir.<br \/>\n Gezegenin \u00e7evresinde 9 ince halka bulunmaktad\u0131r. Bu halkalar 10 Mart 1997 y\u0131l\u0131nda bir y\u0131ld\u0131z\u0131n gezegenin arkas\u0131nda kalmas\u0131 sonucunda yap\u0131lan g\u00f6zlemler ile ke\u015ffedilmi\u015ftir. Halkalar gezegenin merkezinden 42000 km sonra ba\u015flamaktad\u0131r ve en geni\u015fi bile kal\u0131nl\u0131\u011f\u0131 bile 10 Km&#8217;den fazla de\u011fildir. En i\u00e7ten d\u0131\u015fa do\u011fru halkalara 6, 5, 4, \u03b1, \u03b2, \u03b3, \u03b4, \u03b5 isimleri verilmi\u015ftir. S\u0131ras\u0131 ile bu halkalar\u0131n gezegenin merkezine olan uzakl\u0131klar\u0131 41980, 42360, 42663, 44844, 45799, 47323, 47746, 48423 ve 51000 km dir. En d\u0131\u015ftaki halka olan \u03b5 halkas\u0131 elips \u015feklindedir ve her iki ucunda yar\u0131\u00e7aplar\u0131 40-50 km olan iki uydu yer almaktad\u0131r.<\/p>\n<p> \u00d6zellikleri :<br \/>\n G\u00fcne\u015fe Olan Uzakl\u0131\u011f\u0131 2.872.460.000 km<br \/>\n Yar\u0131 \u00c7ap\u0131 25600 km<br \/>\n K\u00fctlesi 86,832 x 10 24 kg<br \/>\n Yo\u011funlu\u011fu 1270 kg\/m3<br \/>\n Atmosferik Bas\u0131n\u00e7 &#8212;-<br \/>\n S\u0131cakl\u0131\u011f\u0131 -221 C\u00ba<br \/>\n G\u00f6r\u00fcn\u00fcr Parlakl\u0131\u011f\u0131 5.8 m<br \/>\n G\u00fcne\u015f Etraf\u0131nda D\u00f6nme S\u00fcresi 84 y\u0131l<br \/>\n Kendi Ekseninde D\u00f6nme S\u00fcresi 17 saat<br \/>\n D\u00f6nme H\u0131z\u0131 6.81 km\/sn<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Uran\u00fcs, 2.872.460.000 km lik mesafe ile g\u00fcne\u015fe yak\u0131nl\u0131k s\u0131ras\u0131nda 7. gezegendir. 1781 y\u0131l\u0131nda Sir W. Herschel taraf\u0131ndan g\u00f6zlenmi\u015ftir. \u00c7ap\u0131 yakla\u015f\u0131k olarak 25600 km kadard\u0131r. 17 saat civar\u0131nda tamamlad\u0131\u011f\u0131 eksen periyodunu yuvarlanarak yapar. Bu nedenle kutuplardaki bas\u0131kl\u0131\u011f\u0131 y\u00fcksektir. G\u00fcne\u015fe olan uzakl\u0131\u011f\u0131 nedeni ile hakk\u0131nda pek fazla bilgi bulunmamakt\u0131r. Gezegenin yap\u0131s\u0131 ve atmosferi hakk\u0131ndaki bilgiler \u00e7o\u011funlukla tahminlere &hellip;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1407,1403],"tags":[2796,10309,3525],"class_list":["post-5723","post","type-post","status-publish","format-standard","hentry","category-fen-ve-teknoloji-odevleri","category-odevler","tag-atmosfer","tag-atmosferik-basinc","tag-uranus"],"_links":{"self":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/5723","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/comments?post=5723"}],"version-history":[{"count":0,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/5723\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/media?parent=5723"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/categories?post=5723"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/tags?post=5723"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}