After 100,000 to one million years, depending on the original mass of the star, it ceases altogether, and the remnant star settles down as an extremely dense and hot white dwarf—a stellar ember crushed by gravity into a nearly crystalline orb about the si
After 100,000 to one million years, depending on the original mass of the star, it ceases altogether, and the remnant star settles down as an extremely dense and hot white dwarf—a stellar ember crushed by gravity into a nearly crystalline orb about the si
经过10~100万年（取决于恒星的原始质量），恒星风将骤然终止，而恒星的残留物会演变成极致密高热的白矮星：一种被重力挤压成地球般大小，近乎晶质球体的恒星遗骸。