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Glossary term: 小行星

Description: 小行星是圍繞太陽或其他恆星或恆星遺跡運行的小天體。小行星是由不同成分組成的固態天體:其中一些富含碳,一些含有更多岩石物質(硅酸鹽),還有一些主要由金屬組成。

大多數小行星都是被引力束縛在一起的碎石堆,形狀凹凸不平。一些小行星擁有衛星——圍繞它們運行的其他小行星。

小行星比矮行星小(矮行星的質量足以讓引力把它們拉成近似圓形的形狀),而比流星體大;小行星的尺寸下限通常定為1到10米之間。如果太陽或其他恆星的加熱導致小天體散髮出氣體和塵埃,那麼這個天體就是彗星而不是小行星(儘管這種區別並不總是很明顯)。

在歷史上,小行星這個名稱用來稱呼任何圍繞太陽運行、但體積太小因而無法用望遠鏡分辨細節的天體。由於這些天體在望遠鏡中看起來像恆星一樣,因此小行星在西方被稱為“asteroids”,希臘語含義是“恆星狀的天體”。

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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


小行星艾達是灰色的,形狀像一個土豆,有很多淺坑。它的衛星達克提爾比它小 40 倍。

伊達和達克提爾

Caption: 這張伊達小行星及其衛星達克提爾的照片是伽利略太空探測器於 1993 年 8 月在距其 10,870 公里(6,755 英里)的距離上拍攝的。艾達小行星是火星和木星之間的主小行星帶中一顆隕石坑嚴重、形狀不規則的小行星。這張圖片證明,像伊達這樣大 56 千米的小行星也可以擁有自己的衛星。
Credit: NASA/JPL credit link

License: PD Public Domain icons

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