Glossary term: 紅超巨星
Description: 紅超巨星是一種表面溫度相對較低,但半徑通常是太陽等主序星的幾百倍甚至幾千倍的恆星。較低的溫度使其表面呈現紅色,而較大的直徑則使恆星的亮度大大超過太陽。
紅超巨星的形成方式與紅巨星相同,但其前身恆星的質量要大得多。 這兩種類型的恆星最初都是主序星,也就是像太陽一樣通過核聚變在其內核中將氫燃燒成氦的恆星(不過紅超巨星的質量要比太陽大得多)。當這種恆星的氫燃料耗盡時,它就會開始將氦燃燒成更重的元素。這時,恆星會膨脹,其表面會在此過程中冷卻下來,隨著體積的增大,恆星會變得更加明亮。紅超巨星的剩餘壽命只有幾萬年。
獵戶座的參宿四和天蠍座的天兔座就是紅超巨星的例子。與紅巨星一樣,紅超巨星也容易發生脈動和質量損失。大多數(可能是全部)紅超巨星都會以超新星爆炸結束,噴出大量氣體,核心坍縮形成中子星或黑洞。
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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
This is an automated transliteration of the simplified Chinese translation of this term
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