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彗翎

彗星尘埃尾的图,尘埃尾(或彗翎都是以气体为主的彗尾。NASA


鹿林彗星。左边的是彗翎,俗称为反尾;离子尾在右边。但有评论指出,因为上图没有显示反尾,对下图则存疑。
显示从地球上看,彗星可能呈现出与离子尾或尘埃尾方向相反的短尾,即彗翎(反尾)。

彗翎(也称逆向彗尾反尾)是从彗星彗发投射出来的明显的尖峰,它似乎朝向太阳,因此在几何上与另一个彗尾相反:离子尾尘埃尾。然而,这种现象是从地球上看到的视错觉。彗翎是由更大的尘埃颗粒组成,它们受太阳辐射压力的影响较小,并倾向于大致保持在彗星的轨道平面内,最终由于颗粒从彗星表面喷出的速度而沿彗星轨道形成盘状。当地球穿过彗星的轨道平面时,是由侧面看见这一盘面,并表现为特征性的尖峰[1]。尽管盘的另一面往往会消失在尘埃的尾部,但有时仍可以看到。因此,通常只有当地球穿过彗星的轨道平面时,才能在短时间内看到彗翎[2][3]

大多数彗星都没有发育到足以看到彗翎的程度,但值得注意的是,确实显示出彗翎的彗星包括1957年的阿兰德-罗兰彗星、1973年的柯侯德彗星[4]、1997年的海尔·波普彗星、和2013年的泛星彗星

相关条目

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注解

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  1. ^ Encyclopedia of science:antitail. [失效链接]
  2. ^ Rao, Joe. Newfound Comet Lulin to Grace Night Skies. SPACE.com. 6 February 2009 [2009-02-25]. (原始内容存档于26 February 2009). 
  3. ^ Tosar, Borja; Paolo Candy. What is an antitail. 3.bp.blogspot. [2009-02-25]. (原始内容存档于25 February 2009). 
  4. ^ Naugles, John E. Statement of John E. Naugle, Associate Administrator for Space Science, NASA: Comet Kohoutek Program. Committee on Science and Astronautics U.S. House of Representatives. Hearings Before the Subcommittee on Space Science and Applications (Washington DC). 7 March 1974, 25 (3): 401 [2021-11-10]. [drawing on page 403] the Skylab crewmen observed a brilliant spike or anti tail projecting toward the Sun from the head of Kohoutek [...] Dr Zdenek Sekanina concluded that the spike was not wholly due to a perspective or geometrical effect as has been assumed in previous comet studies. 

外部链接

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彗翎
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