Glossary term: 天頂
Description: 天頂定義為觀測者正上方的一點,因此這個點隨著觀測者位置的變化而變化。例如,對位於倫敦、北京與開普敦的觀測者來說,他們的天頂是各不相同的。若用角度來度量,則天頂與觀測者的地平線成90度。天頂角定義為天體與天頂之間的角距離。位於天頂的天體的天頂角為0度,而位於地平線上的天體的天頂角為90度。與天頂相對的一點,即觀測者的正下方,稱為觀測者的天底。如果地球是一個完美的球體,那麼觀測者的天頂和天底之間的連線就會穿過地心,但實際上地球只是近似於球體,因此地心與這條連線通常有一定的距離。
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".