Amerikan Uzay ve Havac\u0131l\u0131k Dairesi’nin (NASA) uzay teleskopu Kepler ile tespit edilen ‘G\u00fcne\u015f sistemi d\u0131\u015f\u0131ndaki’ bu gezegenlerden yaln\u0131zca \u00fc\u00e7\u00fcnde ya\u015fam ko\u015fullar\u0131 g\u00f6zlendi.<\/p>\n
Ya\u015fama uygun olma ihtimali olan gezegenlere Kepler 438b, Kepler 442b ve Kepler 440b isimleri verildi.<\/p>\n
Bu gezegenler aras\u0131nda da D\u00fcnya’ya en \u00e7ok benzeyenin de Kepler 438b oldu\u011fu belirtildi.<\/p>\n
Daha \u00f6nce ise Kepler 186f adl\u0131 gezegenin D\u00fcnya ile benzerlikleri en \u00e7ok olan gezegen oldu\u011funa inan\u0131l\u0131yordu.<\/p>\n
D\u00fcnya’dan y\u00fczde 12 oran\u0131nda daha geni\u015f olan Kepler 438b, Kepler 186b’den daha b\u00fcy\u00fck. Ayr\u0131ca y\u0131ld\u0131z\u0131na daha yak\u0131n mesafede d\u00f6nmesi nedeniyle, D\u00fcnya’ya k\u0131yasla y\u00fczde 40 daha fazla \u0131\u015f\u0131k al\u0131yor.<\/p>\n
ABD’nin California eyaletindeki ara\u015ft\u0131rma merkezi Seti’de g\u00f6revli Doktor Doug Caldwell’e g\u00f6re, 438b’nin y\u00fczeyi D\u00fcnya’n\u0131n y\u00fczeyinden daha s\u0131cak. Caldwell, k\u0131z\u0131l c\u00fcce g\u00fcne\u015fi etraf\u0131nda d\u00f6nen bu gezegenden bak\u0131ld\u0131\u011f\u0131nda g\u00f6ky\u00fcz\u00fcn\u00fcn, D\u00fcnya’ya k\u0131yasla daha k\u0131rm\u0131z\u0131 g\u00f6r\u00fcnebilece\u011fini s\u00f6yl\u00fcyor.<\/p>\n
475 \u0131\u015f\u0131k y\u0131l\u0131 uzakta<\/strong><\/p>\n Bilim insanlar\u0131na g\u00f6re bu gezegene dair daha ayr\u0131nt\u0131l\u0131 bilgi elde etmek g\u00fc\u00e7. Zira gezegen 475 \u0131\u015f\u0131k y\u0131l\u0131 uzakta ve gezegeni olu\u015fturan maddeler hakk\u0131nda hen\u00fcz bir bilgi yok.<\/p>\n Ara\u015ft\u0131rmac\u0131lar\u0131n tespit etti\u011fi sekiz gezegen, 500’den fazla gezegen \u00fczerinde yap\u0131lan ara\u015ft\u0131rmalar sonucu tespit edildi.<\/p>\n Ya\u015fam ko\u015fullar\u0131n\u0131n g\u00f6r\u00fclebildi\u011fi gezegenler kendi g\u00fcne\u015flerine, suyu muhafaza edebilecek kadar uzak, fakat suyun donmas\u0131na engel olacak kadar da yak\u0131n bir mesafede bulunuyor.<\/p>\n Bu tip gezegenlerin belirlenmesi de bilim insanlar\u0131n\u0131n ara\u015ft\u0131rmalar\u0131 sonucu yapt\u0131klar\u0131 tahminlere dayand\u0131r\u0131l\u0131yor.<\/p>\n BBC’ye konu\u015fan Doktor Caldwell, “Yapt\u0131\u011f\u0131m\u0131z Kepler ve di\u011fer \u00f6l\u00e7\u00fcmlere g\u00f6re, bu gezegenlerde bal\u0131klar\u0131n ya\u015fad\u0131\u011f\u0131 okyanuslar veya a\u011fa\u00e7lar\u0131n bulundu\u011fu topraklar olup olmad\u0131\u011f\u0131n\u0131 bilmiyoruz. Bildi\u011fimiz \u015feyler ise boyutlar\u0131 ve kendi y\u0131ld\u0131zlar\u0131ndan enerji almalar\u0131i” diyor.<\/p>\n Caldwel, gezegenlerin D\u00fcnya gibi kayal\u0131k olduklar\u0131n\u0131 ve ald\u0131klar\u0131 \u0131\u015f\u0131\u011f\u0131n da D\u00fcnya’n\u0131nkiyle k\u0131yaslanabilir oldu\u011fu yorumunu yap\u0131yor.<\/p>\n","protected":false},"excerpt":{"rendered":" Amerikan Uzay ve Havac\u0131l\u0131k Dairesi’nin (NASA) uzay teleskopu Kepler ile tespit edilen ‘G\u00fcne\u015f sistemi d\u0131\u015f\u0131ndaki’ bu gezegenlerden yaln\u0131zca \u00fc\u00e7\u00fcnde ya\u015fam ko\u015fullar\u0131 g\u00f6zlendi.<\/p>\n Ya\u015fama uygun olma ihtimali olan gezegenlere Kepler 438b, Kepler 442b ve Kepler 440b isimleri verildi.<\/p>\n Bu gezegenler aras\u0131nda da D\u00fcnya’ya en \u00e7ok benzeyenin de Kepler 438b oldu\u011fu belirtildi.<\/p>\n Daha \u00f6nce ise Kepler 186f adl\u0131 gezegenin D\u00fcnya ile benzerlikleri en \u00e7ok olan gezegen oldu\u011funa inan\u0131l\u0131yordu.<\/p>\n D\u00fcnya’dan y\u00fczde 12 oran\u0131nda daha geni\u015f olan Kepler 438b, Kepler 186b’den daha b\u00fcy\u00fck. Ayr\u0131ca y\u0131ld\u0131z\u0131na daha yak\u0131n mesafede d\u00f6nmesi nedeniyle, D\u00fcnya’ya k\u0131yasla y\u00fczde 40 daha fazla \u0131\u015f\u0131k al\u0131yor.<\/p>\n ABD’nin California eyaletindeki ara\u015ft\u0131rma merkezi Seti’de g\u00f6revli Doktor Doug Caldwell’e g\u00f6re, 438b’nin y\u00fczeyi D\u00fcnya’n\u0131n y\u00fczeyinden daha s\u0131cak. Caldwell, k\u0131z\u0131l c\u00fcce g\u00fcne\u015fi etraf\u0131nda d\u00f6nen bu gezegenden bak\u0131ld\u0131\u011f\u0131nda g\u00f6ky\u00fcz\u00fcn\u00fcn, D\u00fcnya’ya k\u0131yasla daha k\u0131rm\u0131z\u0131 g\u00f6r\u00fcnebilece\u011fini s\u00f6yl\u00fcyor.<\/p>\n 475 \u0131\u015f\u0131k y\u0131l\u0131 uzakta<\/strong><\/p>\n Bilim insanlar\u0131na g\u00f6re bu gezegene dair daha ayr\u0131nt\u0131l\u0131 bilgi elde etmek g\u00fc\u00e7. Zira gezegen 475 \u0131\u015f\u0131k y\u0131l\u0131 uzakta ve gezegeni olu\u015fturan maddeler hakk\u0131nda hen\u00fcz bir bilgi yok.<\/p>\n Ara\u015ft\u0131rmac\u0131lar\u0131n tespit etti\u011fi sekiz gezegen, 500’den fazla gezegen \u00fczerinde yap\u0131lan ara\u015ft\u0131rmalar sonucu tespit edildi.<\/p>\n Ya\u015fam ko\u015fullar\u0131n\u0131n g\u00f6r\u00fclebildi\u011fi gezegenler kendi g\u00fcne\u015flerine, suyu muhafaza edebilecek kadar uzak, fakat suyun donmas\u0131na engel olacak kadar da yak\u0131n bir mesafede bulunuyor.<\/p>\n Bu tip gezegenlerin belirlenmesi de bilim insanlar\u0131n\u0131n ara\u015ft\u0131rmalar\u0131 sonucu yapt\u0131klar\u0131 tahminlere dayand\u0131r\u0131l\u0131yor.<\/p>\n BBC’ye konu\u015fan Doktor Caldwell, “Yapt\u0131\u011f\u0131m\u0131z Kepler ve di\u011fer \u00f6l\u00e7\u00fcmlere g\u00f6re, bu gezegenlerde bal\u0131klar\u0131n ya\u015fad\u0131\u011f\u0131 okyanuslar veya a\u011fa\u00e7lar\u0131n bulundu\u011fu topraklar olup olmad\u0131\u011f\u0131n\u0131 bilmiyoruz. Bildi\u011fimiz \u015feyler ise boyutlar\u0131 ve kendi y\u0131ld\u0131zlar\u0131ndan enerji almalar\u0131i” diyor.<\/p>\n Caldwel, gezegenlerin D\u00fcnya gibi kayal\u0131k olduklar\u0131n\u0131 ve ald\u0131klar\u0131 \u0131\u015f\u0131\u011f\u0131n da D\u00fcnya’n\u0131nkiyle k\u0131yaslanabilir oldu\u011fu yorumunu yap\u0131yor.<\/p>\n","protected":false},"author":1,"featured_media":16685,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":[],"categories":[25],"tags":[],"_links":{"self":[{"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/posts\/16684"}],"collection":[{"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/comments?post=16684"}],"version-history":[{"count":0,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/posts\/16684\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/media\/16685"}],"wp:attachment":[{"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/media?parent=16684"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/categories?post=16684"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/gncz.net\/index.php\/wp-json\/wp\/v2\/tags?post=16684"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}