Selasa, 05 April 2011

solar systems : A New Theory of Solar System Formation

IntroductionOnce, in a far-away area of space and time, a system of three stars was formed. At the center, a massive star was companion to a more ordinary Sun. Another star existed on the outer edges of this Solar System.At an early stage in this evolutionary history, the large inner star erupted into a supernova, powerful enough to completely destroy the star, leaving only an iron core. As a result, catastrophic changes occurred in the system. From the resulting nebular material released into

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