Glossary term: 颜色
Description: 天体的颜色可以提供有关其物理特性的重要信息。即使用肉眼观察,你在天空中看到的偏蓝色的恒星(例如位于北斗七星“勺柄”末端的摇光星)也会比偏红色的恒星(例如位于猎户座肩部的参宿四星)热得多。为了量化颜色,天文学家通常使用可选的几种专用蓝色滤光片之一观测恒星的亮度,并将其与通过红色滤光片观测的亮度进行比较。通过比较不同的特定滤光片观测到的亮度,即可给出颜色的明确定义。目前有几种这样的定义处于应用中。其结果可用于统计分析。例如,颜色-星等图的两条轴线就分别是天体颜色与天体亮度。
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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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