\n<\/p>\n
Ara\u015ft\u0131rmac\u0131lar, s\u00f6z konusu diskin, y\u0131ld\u0131z\u0131n \u015fiddetli \u00f6l\u00fcm evresinden sa\u011f kurtulmay\u0131 ba\u015fard\u0131ktan sonra halkalar\u0131n i\u00e7ine g\u00f6m\u00fclen iki gezegen ya da daha k\u00fc\u00e7\u00fck kayal\u0131k cisim taraf\u0131ndan \u015fekillendirilmi\u015f olabilece\u011fini belirtti.<\/p>\n
\u00a0<\/p>\n
G\u00fcne\u015f’in k\u00fctlesinin yakla\u015f\u0131k y\u00fczde 47’sine sahip olan bu beyaz c\u00fcce, yakla\u015f\u0131k olarak D\u00fcnya’n\u0131nkiyle ayn\u0131 \u00e7apa s\u0131k\u0131\u015fm\u0131\u015f durumda bulunuyor.<\/p>\n
\u00a0<\/p>\n
Hayatta kalan gezegenimsi cisimlerin, daha b\u00fcy\u00fck ve a\u011f\u0131r bi\u00e7imde par\u00e7alanm\u0131\u015f gezegenlerin kal\u0131nt\u0131lar\u0131 olabilece\u011fi tahmin ediliyor.<\/p>\n
\u00a0<\/p>\n
Bu cisimlerden birinin c\u00fcce gezegen Pl\u00fcton b\u00fcy\u00fckl\u00fc\u011f\u00fcnde, di\u011ferinin ise ondan daha k\u00fc\u00e7\u00fck olabilece\u011fi de\u011ferlendiriliyor.<\/p>\n
\u00a0<\/p>\n
Nature Astronomy dergisinde yay\u0131mlanan \u00e7al\u0131\u015fman\u0131n yazarlar\u0131ndan, \u015eili’deki Universidad T\u00e9cnica Federico Santa Mar\u00eda’dan g\u00f6kbilimci Felipe Lagos-Vilches, Reuters ajans\u0131na verdi\u011fi deme\u00e7te, ke\u015ffin \u00f6nemini \u015fu s\u00f6zlerle anlatt\u0131:<\/p>\n
\u00a0<\/p>\n
“Bu ke\u015fif, bir gezegen sisteminin kal\u0131nt\u0131lar\u0131n\u0131n daha \u00f6nce d\u00fc\u015f\u00fcnd\u00fc\u011f\u00fcm\u00fczden \u00e7ok daha karma\u015f\u0131k bir yap\u0131ya sahip olabilece\u011fini g\u00f6steriyor ve gezegen niteli\u011findeki kayal\u0131k cisimlerin, bir y\u0131ld\u0131z\u0131n beyaz c\u00fcceye d\u00f6n\u00fc\u015f\u00fcm\u00fcnden sa\u011f \u00e7\u0131kabilece\u011fi fikrine ek destek sa\u011fl\u0131yor.”<\/p>\n<\/div>\n