evelite

这种类型的橙黄色和橙色恒星相当稳定，人们相信要经过数百亿年的热核聚变过程，它们内核中的氢气储备才会燃烧殆尽。 稳定性和长生命周期，加上行星系的共同存在，标志着它们是进行殖民化和探索活动的可行性目标。

Yellow-orange and orange stars of this type are rather stable and believed to take tens of billions of years to burn through their core hydrogen reserves in a process of thermonuclear fusion. This stability and long life, combined with the common presence of planetary systems marks these as viable candidates for colonization and exploration efforts.