Glossary term: 拱極星
Description: 在地球上的大多數地方,都能在地平線以上一定距離的天空中看到北天極或南天極。對於處於這樣一個位置的觀測者來說,隨著時間的流逝,星星似乎在圍繞著天極旋轉:每顆恆星都在天空中劃出一個圓圈,其中心是地軸指向的天極。在圓圈與觀測者地平線相交的兩點,即東點和西點,該恆星將分別升起和落下。對於距離天極足夠近的恆星,其劃出的圓圈將完全位於地平線之上。我們的觀測者將永遠看不到這些恆星升起或落下。這些永不落下的恆星被稱為拱極星。
哪些恆星是拱極星取決於觀測者的地理緯度和恆星的赤緯——後者是恆星所在位置與天赤道之間的夾角。在北半球,如果一顆恆星的赤緯大於90°減去觀測者的地理緯度,那麼它就是拱極星。在南半球,我們需要考慮到地理南緯和恆星的南赤緯都帶有負號。考慮到這些負號,在南半球,如果一顆恆星的赤緯小於-90°減去觀測者的地理緯度,那麼它就是拱極星。
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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
This is an automated transliteration of the simplified Chinese translation of this term
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