Glossary term: 视星等
Description: 视星等是观测者看到的天体亮度的量度。由于历史原因,星等表将较大的数字分配给较暗的天体。星等是一个对数刻度,5 个星等的差异相当于测量亮度的 100 倍。由于亮度可以用不同的波长和不同的技术测量,因此有许多震级标度。常用的 "视星等 "刻度是这样设定的:明亮的织女星的视星等为零。在这个星等表上,夜空中最亮的恒星天狼星的星等为-1.46,太阳和满月的星等分别为-26.7 和-12.7。负数表示这些天体看起来比织女星更亮。在非常暗的条件下,视力极好的人可以看到约 6 等的恒星。哈勃超深视场的视星等接近 31 等。这比 6 等暗大约 100 到 5 的幂,或者说比 6 等暗 10,000,000,000 倍。
视星等是用来衡量天体在观测者眼中亮度的一种度量。由于历史原因,星等标尺将较大的数字分配给较暗的天体。视星等是一个对数刻度,星等相差5个单位时,亮度相差100倍。因为亮度可以在不同波长和通过不同技术进行测量,所以有多种星等标尺。常见的“视星等”尺度设定明亮的织女星视星等为0。在该标尺上,夜空中最亮的恒星天狼星的视星等为-1.46,太阳和满月的视星等分别为-26.7和-12.7。负数表示这些天体比织女星更亮。在非常黑暗的条件下,视力极佳的人可以看到视星等约为6的恒星。而哈勃超深空的视星等接近31,这比视星等为6的恒星暗约100的五次方,即100亿倍。
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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
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