Glossary term: 二至點
Description: 地軸並非垂直於地球圍繞太陽的軌道平面,而是與垂直方向呈23.4度的傾斜角。因此,在地球軌道的不同位置上,地軸與太陽視線之間的角度在一年內是不同的。這種現象的實際效果是,對於地球上的觀測者來說,太陽在一天中達到地平線上最高點的高度會隨時間而變化。北半球夏至,同時也是南半球的冬至,大約發生在6月21日,此時太陽在北半球的高度到達一年中的最高點,同時在南半球的高度則到達最低點。而南半球夏至,同時也是北半球的冬至,大約發生在12月21日,此時太陽在南半球的高度到達最高點,同時在北半球的高度則到達最低點。
Related Terms:
See this term in other languages
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".
If you notice a factual or translation error in this glossary term or definition then please get in touch.
Related Media
每月日落的地方
Credit: John Paul Pile/IAU OAE (CC BY 4.0)
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons
太陽的軌跡
Credit: Frank Niessen/IAU OAE (CC BY 4.0)
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons
日至和日分
Credit: 通奇·特澤爾/國際天文學聯合會教育辦公室 (CC BY 4.0)
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons
西落幅度
Credit: Marcella Giulia Pace/IAU OAE (CC BY 4.0)
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons