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Glossary term: 彗核

Description: 彗核是彗星的核心。它是一個類似臟雪球的固體,由冰和岩石、塵埃顆粒組成。在遠離太陽的地方,彗核是彗星的唯一組成部分。靠近太陽時,彗核會被陽光加熱。這導致表面的冰升華。升華後的冰及其中的塵埃被噴射出來,以彗尾的形式圍繞著彗核,彗尾指向遠離太陽的方向。

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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

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".

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This comet nucleus looks like two large, bumpy lumps joined together. A small jet of material is being blown off the nucleus

Comet 67P/Churyumov-Gerasimenko

Caption: Comet 67P/Churyumov–Gerasimenko's nucleus is a "dirty snowball" made of a mixture of frozen materials and dust. It is shaped like two large lobes: one 4.1 km × 3.3 km × 1.8 km, the other 2.6 km × 2.3 km × 1.8 km. These lobes are connected by a small bridge. When a cometary nucleus such as this nears the Sun its frozen, icy material is heated, turning into gas. This, combined with the embedded dust, provide the material for the comet's characteristic coma and tail.
Credit: ESA/Rosetta/NAVCAM credit link

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