carbon n dwarf 碳矮星
At times, enough gas builds up for the dwarf to collapse, leading its carbon to fuse nearly instantly and the dwarf to explode in a Type I supernova, which can outshine a galaxy for a few months.
有时,足够的气体会积累起来导致这颗矮星发生坍缩,使得它的碳原子几乎能立即聚合,而爆炸成为I类超新星,它在几个月内的亮度能超过一个星系。
All that carbon and oxygen — byproducts of the helium fusion process — build up in its core. At that point the star will shed its outer layers and the core will form a White Dwarf.
所有氦聚变中的附产物碳和氧在它的核心逐渐积聚,这期间它将失掉较外层物质,核心最终枯萎成为白矮星。
And in 2004, they found that a white dwarf near the constellation Centaurus, BPM 37093, wasmade of crystallized carbon weighing 5 million trillion trillion pounds.
2004年,他们在半人马星座附近发现一颗白矮星,将其称之为“BPM 37093”。 这颗白矮星由晶化碳构成,重量为500万*1万亿*1万亿磅。
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