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Glossary term: 軌道

Description: 軌道是在一個系統中運動的天體圍繞該系統質心的軌跡,由系統中天體之間相互施加的萬有引力引起。在太陽系等系統中,中心天體的質量遠大於其他天體,質心位於質量最大的天體(在太陽系中為太陽)內部或其附近。在雙星系統中,恆星軌道的質心通常位於兩顆恆星之間。

軌道的形狀通常呈橢圓形,系統的質心位於橢圓的一個焦點上。軌道的大小和形狀由橢圓的半長軸和離心率決定。離心率越大的軌道橢圓度越高。太陽系中大多數行星軌道的離心率都非常接近零,例如金星(0.007)和地球(0.017)。而離心率較大的例外有水星(0.206)和矮行星冥王星(0.244)。

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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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Related Media


木星和圍繞它運行的四顆伽利略衛星中的兩顆(可見亮點)。

木星的自轉,作者 Vishal Sharma,印度

Caption: 2021 年國際天文學聯合會 (IAU) 天文教育辦公室 (OAE) 天體攝影比賽,伽利略衛星類第三名:《木星的自轉》,作者 Vishal Sharma,來自印度。 這幅延時攝影作品精美地展示了木星的自轉,以及畫面右側經過的兩顆伽利略衛星。木星自轉一圈只需不到 10 個小時,我們可以看到大紅斑從左向右移動。在這短短的時間內,兩顆衛星明顯沿著它們的軌道前進了一段距離。這張照片是 2020 年在印度北部拍攝的。
Credit: Vishal Sharma/IAU OAE

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons


木星是一個明亮的圓盤,由四顆伽利略衛星環繞運行,在圖中是四個亮點。

木衛影片2,Nicolas Hurez,Paul-Antoine Matrangolo,和Carl Pennypacker,美國

Caption: 2021 年國際天文學聯合會 OAE 天體攝影比賽伽利略衛星類第二名。 這組照片展示了四顆伽利略衛星圍繞木星運行的軌道。從中幾乎可以看到最內側的衛星木衛一艾奧的兩個完整軌道,其他衛星(木衛二歐羅巴和木衛三加尼美得,尤其是木衛四卡利斯托)距離較遠,運行速度明顯較慢。這些圖像是在2018年由Las Cumbres全球天文臺在地球上不同地點拍攝的,因此可以在大約半個星期內連續拍攝一系列圖像,白天也沒有間隙。在天空晴朗的條件下,連續幾個夜晚,也可以用雙筒望遠鏡觀測到伽利略衛星的運動(最好將手肘穩穩地放在地面上)。
Credit: Nicolas Hurez,Paul-Antoine Matrangolo 和 Carl Pennypacker/IAU OAE

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons


有著彩色水平雲帶的木星。木衛一的陰影在左上方顯示為一個黑色圓圈。

木星、木衛一及其陰影,作者:Ralf Burkart,德國

Caption: 2021 年國際天文學聯合會 OAE 天體攝影比賽伽利略衛星類第一名。 這幅木星的延時攝影是於2017 年從德國拍攝的,作品精美地展示了伽利略衛星之一木衛一在木星前的凌星現象。由於這只是衛星在行星上投下影子,因此相當於從更遠的地方觀測地球上的月食。雖然衛星的影子從一開始就清晰可見,但在木星美麗的大氣帶背景下,第一次觀看視頻時可能很難發現衛星本身。反復觀看可以欣賞到這一奇妙的快速運動和旋轉過程。
Credit: Ralf Burkart/IAU OAE

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons


β Pictoris b 從右下方移向圖像中心,22 個月後再次出現在左上方

β Pictoris b的軌道

Caption: 這組圖像展示了太陽系外行星(系外行星)β Pictoris b 的軌道運動。這顆行星是每幅圖中的亮點。行星的主星被隱藏在每幅圖中間的黑圈後面。這樣做是為了去掉更亮的主星,否則主星的光會掩蓋行星的光。行星軌道側面對著我們。從這個角度觀察軌道,會讓人覺得行星是沿著一條直線運動的。 2015年2月至2016年11月期間,β Pictoris b似乎越來越靠近它的主星。之後,這顆行星離恆星如此之近,以至於近兩年都沒有人看到它,之後它又再次出現在恆星的另一側。
Credit: ESO/拉格朗日/SPHERE合作組織 credit link

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons

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