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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

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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Caption: Second place in the IAU OAE Astrophotography Contest, category Star trails. Astronomy is one of the oldest (if not the oldest) of the sciences, and as such has connection to various cultures over millennia. This image in a way conveys this relationship by being contextualised in Stonehenge. There is much research into what astronomers call archeoastronomy sites, and how they connect to the sky (for example, seasons, phases of the moon and much more). Civilizations across time and from all over the world have their own views and interpretations of what they see in the sky, and this has been tied not only to culture but also to the people’s day-to-day and seasonal activities. The “concentric circles” which are often referred to as “star trails”, are the result of the apparent motion of the sky, which is in reality due to the rotation of the Earth on its axis. The small dot appearing towards the top center of the image is Polaris – The North or Pole Star. Polaris is only visible to observers in the Northern latitudes. The height of the Pole Star can be used to infer the observer’s actual latitude. Stonehenge is located at around 51° North. This image is taken from one of the most notable ancient sites in the world, brings us back in time, and makes us wonder about the stories told by the people that lived in that place many millennia ago.
Credit: Till Credner/IAU OAE

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Bright star trails for arcs around the center of the image behind the silhouette of a tree

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Caption: First place in the IAU OAE Astrophotography Contest, category Star trails. This star trail image shows the apparent movement of the stars in the night sky, which results from the Earth’s rotation around its polar axis. The trees in the foreground serve as an anchor as we turn with the Earth. The bright white semi-circle in the center of the image is the North (Pole) star – Polaris, which is located very close to the North Celestial Pole. One way to imagine that the Earth is at center of hollow crystal sphere, and the stars are embedded on this sphere, as the Earth spins on its axis, an observer on Earth sees the stars rising and setting, following an arc, because the horizon prevents the observer from the full arc for stars that are further away from the Celestial Pole. The North Celestial Pole (and its opposite the South Celestial Pole) is essentially formed by extending the line of the Earth’s axis. Capturing this image requires the photographer to take a long exposure with the camera on a tripod and pointing towards the Pole Star (North Hemisphere). In the Southern Hemisphere there is no star as close as Polaris is to the Celestial Pole, so the position of the South Celestial Pole is found using the South Cross and Pointer Stars (Alpha and Beta Centauri). Although overall the image has a slight blue tint, it does capture the varying colours of stars, it is easy to distinguish between the higher temperature blue stars and the lower temperature of the whitish stars, and even lower temperature reddish stars. The reason for this variation in colour is because higher temperature stars emit more in shorter wavelengths (bluer), compared to lower temperature stars which emit in longer wavelengths (redder).
Credit: Fabrizio Melandri/IAU OAE

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The ladle-shaped Big Dipper with the orange star Arcturus to its left. Right is the diffuse disk-shaped Andromeda galaxy

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Credit: Likai Lin/IAU OAE

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The Big Dipper, seven bright stars shaped like a ladle, viewed in 4 seasons, each time at a different angle

Big Dipper in Four Seasons

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Credit: Giorgia Hofer/IAU OAE

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北斗七星和新智彗星 C2020 F3

Caption: 這段延時攝影記錄了2020年7月拍攝的三幀畫面中標誌性的北斗七星的軌跡。影像在意大利的三個地點拍攝:拉瓦雷多三峰(Tre Cime di Lavaredo)奧隆佐迪卡多雷、裡特山(Monte Rite)奇比亞納迪卡多雷,以及拉佐牧場(Casera Razzo)維戈迪卡多雷。這場視覺奧德賽展示了北斗七星的迷人軌跡,並在夜空中繪製出天體畫卷。它不僅描繪了這個著名星群的軌跡,還捕捉到2020年7月照亮天空的罕見新智彗星 C/2020 F3 這一非凡的天文事件,為我們的夜空增添了光彩。
Credit: 喬爾賈·霍弗/國際天文學聯合會教育辦公室 (CC BY 4.0)

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北斗七星在天空中下沉,其柄部掃過的圓圈比星群的碗部更大。

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Credit: Fabrizio Melandri/IAU OAE (CC BY 4.0)

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一座傳統的中國建築。上方的星星圍繞北極星形成一個圓形圖案。

故宮星軌

Caption: 2022 年 3 月拍攝的這張照片中,北京故宮矗立在星軌編織的夜空芭蕾之下,見證著古老的天體之間的聯繫。紫禁城在設計時考慮到了宇宙的排列,呼應了北極星的方位,北極星又叫 Polaris,是長期以來指引航海者的天體之錨,象徵著天空的穩定。人們相信皇帝是北極星在人間的化身,是連接天地的橋梁。在這張用智能手機拍攝的和諧的一小時曝光照片中,星星的軌跡描繪了它們夜間穿越蒼穹的旅程,它們向北極星匯聚,體現了建築設計和天體軌跡的精確性。
Credit: Stephanie Ziyi Ye/IAU OAE (CC BY 4.0)

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Tags: History , Geography , Celestial navigation
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