Glossary term: 红超巨星
Description: 红超巨星是一种表面温度相对较低,但半径通常是太阳等主序星的几百倍甚至几千倍的恒星。较低的温度使其表面呈现红色,而较大的直径则使恒星的亮度大大超过太阳。
红超巨星的形成方式与红巨星相同,但其前身恒星的质量要大得多。 这两种类型的恒星最初都是主序星,也就是像太阳一样通过核聚变在其内核中将氢燃烧成氦的恒星(不过红超巨星的质量要比太阳大得多)。当这种恒星的氢燃料耗尽时,它就会开始将氦燃烧成更重的元素。这时,恒星会膨胀,其表面会在此过程中冷却下来,随着体积的增大,恒星会变得更加明亮。红超巨星的剩余寿命只有几万年。
猎户座的参宿四和天蝎座的天兔座就是红超巨星的例子。与红巨星一样,红超巨星也容易发生脉动和质量损失。大多数(可能是全部)红超巨星都会以超新星爆炸结束,喷出大量气体,核心坍缩形成中子星或黑洞。
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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
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