Glossary term: 拱极星
Description: 在地球上的大多数地方,都能在地平线以上一定距离的天空中看到北天极或南天极。对于处于这样一个位置的观测者来说,随着时间的流逝,星星似乎在围绕着天极旋转:每颗恒星都在天空中划出一个圆圈,其中心是地轴指向的天极。在圆圈与观测者地平线相交的两点,即东点和西点,该恒星将分别升起和落下。对于距离天极足够近的恒星,其划出的圆圈将完全位于地平线之上。我们的观测者将永远看不到这些恒星升起或落下。这些永不落下的恒星被称为拱极星。
哪些恒星是拱极星取决于观测者的地理纬度和恒星的赤纬——后者是恒星所在位置与天赤道之间的夹角。在北半球,如果一颗恒星的赤纬大于90°减去观测者的地理纬度,那么它就是拱极星。在南半球,我们需要考虑到地理南纬和恒星的南赤纬都带有负号。考虑到这些负号,在南半球,如果一颗恒星的赤纬小于-90°减去观测者的地理纬度,那么它就是拱极星。
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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
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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