Distance Measurement in Astronomy天文学中的距离测量
Since all stars appear as points of light, even with the largest telescopes, and since geometrical distance measurement by parallax is possible only for the closest stars, an overlapping chain of distance measurement techniques has been developed. The distance indicators include: 由于所有恒星在最大的望远镜中仍表现为光点,而且只有最近的恒星才能通过视差进行几何距离测量,因此发展出一系列重叠的距离测量技术。距离指示器包括:
A supporting idea for distance measurement is that if a specific kind of light source is known to have a constant and dependable absolute luminosity, then the measured intensity at the detector can be used to calculate its distance. Light from a point source diminishes according to the purely geometrical inverse square law, so the number of photons into a standard area detector can be used as a distance measurement. This is often referred to as the "standard candle" approach. 距离测量的一个支持性想法是,如果某种特定类型的光源已知具有恒定且可靠的绝对亮度,那么在探测器上测量到的强度可以用来计算其距离。来自点光源的光按照纯粹的几何反平方定律减弱,因此可以将进入标准面积探测器的光子数量用作距离测量。这种方法通常被称为“标准烛光”方法。
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Index Distance units 索引距离单位 | ||||||||
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