Glossary term: 彗尾
Description: 當彗星靠近太陽時,太陽輻射會加熱彗星表面。表面的冰變成氣體("升華"),同時帶走岩石和塵埃物質。由此產生的混合物在彗核周圍形成一團雲,這就是彗發。一般來說,彗星會有兩條尾巴:噴射出的塵埃粒子形成彗尾,彗尾呈典型的彎曲狀。它由從表面釋放出來的塵埃粒子組成,這些塵埃粒子沿著彗星的軌道繞太陽運行。塵埃尾的長度可達數百萬公里或更長。它們反射太陽光,如果條件合適,肉眼能觀測到的彗星大部分都是由它們的白色漫射形狀組成的。
相當一部分氣體被太陽風--太陽發出的帶電粒子--吹走並電離。這些離子形成了彗星的離子尾,通常呈藍色。離子尾總是直指太陽。如果彗星本身正在遠離太陽,離子尾就會在彗星之前。
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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
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Credit: Dietmar Gutermuth/IAU OAE
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons
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Credit: E.Kolmhofer, H. Raab; Johannes Kepler Observatory, Linz, Austria credit link
License: CC-BY-SA-3.0 Creative Commons Attribution-ShareAlike 3.0 Unported icons