Glossary term: 银河系
Description: 银河系是太阳系所在的星系。它由大约 1000-4000 亿颗恒星组成。太阳系距离银河系中心约 26600 光年。在夜空中,我们可以看到它像一条微弱的带子延伸至整个天空,其中心位于人马座。
银河系是一个相对较大的棒状螺旋星系,其中恒星的分布沿着厚度约为1000光年的盘面延伸到约10万光年处。银河系盘形成于 80 到 100 亿年前。
银河系盘的周围环绕着稀疏得多的恒星晕,其中包括球状星团。这些球状星团是银河系中最古老的天体,年龄约为 125 亿年。除了恒星,银河系还由星际介质的气体和尘埃以及暗物质组成。星际介质主要局限于星盘,而周围的暗物质晕则比恒星光环延伸得更远。
银河系中心有一个超大质量黑洞,其质量约为太阳的 400 万倍。银河系中心附近有一个星系核,其中大部分是较老的恒星,它们向一个方向伸长,形成一个棒状。
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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
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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