<\/p>\n
\n\tAvrupa G\u00fcney G\u00f6zlemevinden yap\u0131lan a\u00e7\u0131klamaya g\u00f6re ara\u015ft\u0131rmac\u0131lar, D\u00fcnya’dan yakla\u015f\u0131k 620 \u0131\u015f\u0131k y\u0131l\u0131 uzakl\u0131kta herhangi bir y\u0131ld\u0131z\u0131n y\u00f6r\u00fcngesini izlemedi\u011fi ve uzayda serbest\u00e7e hareket etti\u011fi i\u00e7in “ba\u015f\u0131bo\u015f gezegen” kabul edilen bir g\u00f6k cismine y\u00f6nelik \u00e7al\u0131\u015fma y\u00fcr\u00fctt\u00fc.<\/p>\n
\n\tTeleskopla elde edilen verileri inceleyen ara\u015ft\u0131rmac\u0131lar, J\u00fcpiter’in 5 ila 10 kat\u0131 k\u00fctleye sahip “Cha 1107-7626” adl\u0131 gezegenin etraf\u0131ndaki gaz ve toz y\u0131\u011f\u0131nlar\u0131n\u0131 b\u00fcnyesinde toplad\u0131\u011f\u0131n\u0131 ve a\u011fustos itibar\u0131yla saniyede 6 milyar ton oran\u0131nda b\u00fcy\u00fcd\u00fc\u011f\u00fcn\u00fc g\u00f6zlemledi.<\/p>\n
\n\t“Ba\u015f\u0131bo\u015f gezegenin” bu b\u00fcy\u00fcme oran\u0131n\u0131n, herhangi bir gezegen t\u00fcr\u00fc i\u00e7in \u015fimdiye kadar kaydedilen en y\u00fcksek d\u00fczeyde oldu\u011fu belirtildi.<\/p>\n
\n\tAyr\u0131ca, gezegenin b\u00fcy\u00fcme oran\u0131n\u0131n sabit kalmad\u0131\u011f\u0131, k\u00fctle art\u0131\u015f\u0131ndaki h\u0131z\u0131n sadece birka\u00e7 ayl\u0131k s\u00fcre\u00e7te 8 kat\u0131na \u00e7\u0131kt\u0131\u011f\u0131 vurguland\u0131.<\/p>\n
\n\tAra\u015ft\u0131rmac\u0131lar, bulgular\u0131n ba\u015f\u0131bo\u015f gezegenlerin olu\u015fum evrelerine ili\u015fkin fikir verebilece\u011fini ifade etti.<\/p>\n
\n\t\u00c7al\u0131\u015fman\u0131n sonu\u00e7lar\u0131, “The Astrophysical Journal Letters” dergisinde yay\u0131mland\u0131.<\/p>\n
Avrupa G\u00fcney G\u00f6zlemevinden yap\u0131lan a\u00e7\u0131klamaya g\u00f6re ara\u015ft\u0131rmac\u0131lar, D\u00fcnya’dan yakla\u015f\u0131k 620 \u0131\u015f\u0131k y\u0131l\u0131 uzakl\u0131kta herhangi bir y\u0131ld\u0131z\u0131n y\u00f6r\u00fcngesini izlemedi\u011fi ve uzayda serbest\u00e7e hareket etti\u011fi i\u00e7in “ba\u015f\u0131bo\u015f gezegen” kabul edilen bir g\u00f6k cismine y\u00f6nelik \u00e7al\u0131\u015fma y\u00fcr\u00fctt\u00fc. Teleskopla elde edilen verileri inceleyen ara\u015ft\u0131rmac\u0131lar, J\u00fcpiter’in 5 ila 10 kat\u0131 k\u00fctleye sahip “Cha 1107-7626” adl\u0131 gezegenin etraf\u0131ndaki gaz ve toz<\/p>\n","protected":false},"author":1,"featured_media":94658,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[306],"tags":[],"class_list":["post-94657","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya"],"yoast_head":"\n