大多数科学家认为,当白矮星(年老恒星坍缩而成的残骸)超过质量极限,变得不稳定并爆发的时候,会产生Ia型超新星。
Most scientists agree a Type 1a supernova occurs when a White Dwarf star — a collapsed remnant of an elderly star — exceeds its weight limit, becomes unstable and explodes.
在这个极限点上,其中心压力将变得如此巨大,以至于爆发失控的核聚变,而恒星则爆炸成为热核爆炸型超新星。
At this point the pressure at its center will become so great that runaway fusion occurs and the star will detonate in a thermonuclear supernova.
在这个极限点上,其中心压力将变得如此巨大,以至于爆发失控的核聚变,而恒星则爆炸成为热核爆炸型超新星。
At this point the pressure at its center will become so great that runaway fusion occurs and the star will detonate in a thermonuclear supernova.
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