{"id":139469,"date":"2025-11-16T17:54:09","date_gmt":"2025-11-16T17:54:09","guid":{"rendered":"https:\/\/kamucalisani.net\/?p=139469"},"modified":"2025-11-16T17:54:09","modified_gmt":"2025-11-16T17:54:09","slug":"gunes-sistemi-bugune-kadar-dusunulenden-3-kat-daha-hizli-hareket-ediyor-olabilir","status":"publish","type":"post","link":"https:\/\/kamucalisani.net\/index.php\/2025\/11\/16\/gunes-sistemi-bugune-kadar-dusunulenden-3-kat-daha-hizli-hareket-ediyor-olabilir\/","title":{"rendered":"G\u00fcne\u015f Sistemi, bug\u00fcne kadar d\u00fc\u015f\u00fcn\u00fclenden 3 kat daha h\u0131zl\u0131 hareket ediyor olabilir"},"content":{"rendered":"<p><figure> <span> <img decoding=\"async\" src=\"https:\/\/kamucalisani.net\/wp-content\/uploads\/2025\/11\/gunes-sistemi-bugune-kadar-dusunulenden-3-kat-daha-hizli-hareket-ediyor-olabilir-0-FpgtnLuB.jpg\"\/> <\/span> Bug\u00fcne kadar kabul g\u00f6ren modellere g\u00f6re D\u00fcnya, G\u00fcne\u015f etraf\u0131nda y\u00fcksek h\u0131zlarla d\u00f6nerken, G\u00fcne\u015f Sistemi de galaksinin merkezine do\u011fru yakla\u015f\u0131k <strong>828.000 km\/s h\u0131zla<\/strong> ilerliyordu. Ancak y\u00fcr\u00fct\u00fclen yeni bir ara\u015ft\u0131rma, bu hareketin d\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fczden \u00e7ok daha h\u0131zl\u0131 olabilece\u011fini ortaya koyarak mevcut modelleri ciddi \u015fekilde sorgulat\u0131yor.\u00a0<strong>Bielefeld \u00dcniversitesi<\/strong>\u2019nde astrofizik\u00e7i <strong>Lukas B\u00f6hme<\/strong> \u00f6nc\u00fcl\u00fc\u011f\u00fcnde yap\u0131lan analiz, G\u00fcne\u015f Sistemi\u2019nin uzaydaki ger\u00e7ek h\u0131z\u0131n\u0131n<strong> bug\u00fcne kadar kabul edilenin \u00fc\u00e7 kat\u0131ndan fazla<\/strong> olabilece\u011fini g\u00f6steriyor. <\/figure>\n<p>Ara\u015ft\u0131rmac\u0131lar bu sonuca ula\u015fmak i\u00e7in, evrenin \u00e7ok uzak b\u00f6lgelerinde yer alan ve <strong>g\u00fc\u00e7l\u00fc radyo sinyalleri yayan galaksilerin g\u00f6ky\u00fcz\u00fcndeki da\u011f\u0131l\u0131m\u0131n\u0131 detayl\u0131 \u015fekilde analiz etti<\/strong>. Bu galaksiler, G\u00fcne\u015f Sistemi\u2019nin uzayda hangi y\u00f6ne do\u011fru hareket etti\u011fine dair \u00e7ok hafif bir iz b\u0131rak\u0131yor: E\u011fer belirli bir y\u00f6ne do\u011fru ilerliyorsak, o y\u00f6nde \u00e7ok az da olsa daha fazla radyo galaksisi g\u00f6r\u00fcl\u00fcyor. Ancak bu fark inan\u0131lmaz derecede k\u00fc\u00e7\u00fck oldu\u011fu i\u00e7in, normal teleskoplarla tespit edilmesi neredeyse imk\u00e2ns\u0131z. Bu nedenle ekip, yaln\u0131zca en hassas radyo teleskop a\u011flar\u0131n\u0131n verilerini kullanarak bu ince y\u00f6n de\u011fi\u015fimini \u00f6l\u00e7ebildi.<\/p>\n<p>Bu ama\u00e7 do\u011frultusunda ekip, Avrupa \u00e7ap\u0131nda dev bir radyo teleskop a\u011f\u0131 olan <strong>Low Frequency Array (LOFAR)<\/strong> g\u00f6zlemlerini, iki farkl\u0131 radyo g\u00f6zlemevi taraf\u0131ndan sa\u011flanan verilerle birle\u015ftirdi. G\u00fcne\u015f Sistemi&#8217;nin d\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fczden \u00e7ok daha h\u0131zl\u0131 ilerledi\u011fi de bu sayede tespit edildi. B\u00f6hme, \u201cYapt\u0131\u011f\u0131m\u0131z analiz, G\u00fcne\u015f Sistemi\u2019nin standart kozmoloji modellerinin \u00f6ng\u00f6rd\u00fc\u011f\u00fcnden \u00fc\u00e7 kat daha h\u0131zl\u0131 hareket etti\u011fini ortaya koyuyor. Bu bulgu, mevcut evren modellerimizin temel varsay\u0131mlar\u0131na do\u011frudan meydan okuyor.\u201d diyor.<\/p>\n<p><b>Ya G\u00fcne\u015f Sistemi D\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fczden Daha H\u0131zl\u0131 Hareket Ediyor ya da Radyo Galaksilere Dair Modeller Hatal\u0131<\/b><\/p>\n<p>Bu ara\u015ft\u0131rma sonras\u0131 mevcut modellerin g\u00fcncellenmesi gerekti\u011fi bir ger\u00e7ek. Ancak G\u00fcne\u015f Sistemi&#8217;nin hareket h\u0131z\u0131na dair kabulleri de\u011fi\u015ftirmek i\u00e7in bu ara\u015ft\u0131rma tek ba\u015f\u0131na yeterli de\u011fil. Bu bulgular\u0131n daha fazla veriyle desteklenmesi gerekiyor. \u00c7al\u0131\u015fman\u0131n ortak yazarlar\u0131ndan <strong>Prof. Dominik J. Schwarz<\/strong>\u2019a g\u00f6re bu bulgular iki ihtimali g\u00fcndeme getiriyor: Ya G\u00fcne\u015f Sistemi sand\u0131\u011f\u0131m\u0131zdan \u00e7ok daha h\u0131zl\u0131 hareket ediyor ve evrene dair temel kabullerimizde bir eksik var, ya da evrende radyo galaksilerinin da\u011f\u0131l\u0131m\u0131 d\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fcz kadar d\u00fczg\u00fcn de\u011fil. Bu iki se\u00e7enek de mevcut kozmoloji modellerinin yeniden g\u00f6zden ge\u00e7irilmesini gerektiriyor.<\/p>\n\n<p>Kaynak\u00a0 :\u00a0<span style=\"background-color: rgb(255, 249, 236); color: rgb(55, 58, 60); font-size: 14px;\">https:\/\/www.donanimhaber.com\/gunes-sistemi-dusunulenden-3-kat-daha-hizli-hareket-ediyor&#8211;198589<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Bug\u00fcne kadar kabul g\u00f6ren modellere g\u00f6re D\u00fcnya, G\u00fcne\u015f etraf\u0131nda y\u00fcksek h\u0131zlarla d\u00f6nerken, G\u00fcne\u015f Sistemi de galaksinin merkezine do\u011fru yakla\u015f\u0131k 828.000 km\/s h\u0131zla ilerliyordu. Ancak y\u00fcr\u00fct\u00fclen yeni bir ara\u015ft\u0131rma, bu hareketin d\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fczden \u00e7ok &#8230;<\/p>\n","protected":false},"author":1,"featured_media":139470,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[716,9379,2015,1823,5097],"class_list":["post-139469","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-teknoloji","tag-dogru","tag-gunes-sistemi","tag-hareket","tag-modelleri","tag-radyo"],"_links":{"self":[{"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/posts\/139469","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/comments?post=139469"}],"version-history":[{"count":1,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/posts\/139469\/revisions"}],"predecessor-version":[{"id":139472,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/posts\/139469\/revisions\/139472"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/media\/139470"}],"wp:attachment":[{"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/media?parent=139469"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/categories?post=139469"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kamucalisani.net\/index.php\/wp-json\/wp\/v2\/tags?post=139469"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}