Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

Example Red Shift Problem

红移问题示例

Suppose you abserve a galaxy for which the bluegreen line of hydrogen is red shifted to the red end of the visible spectrum at 700 nm. What is the recession speed of the galaxy?

假设你观测到一个星系,其氢的蓝绿色谱线红移到可见光谱的红色端,波长为700 nm。该星系的退行速度是多少?

The bluegreen line of the hydrogen spectrum is the n=4 to n=2 transition for which the photon energy and wavelength are:

氢谱中的蓝绿色线对应的是从n=4跃迁到n=2的跃迁,其光子的能级和波长为:

The main difficulty I have with this kind of problem is getting the sign wrong on one of the quantities or inverting a term. So, starting from the beginning, the observed wavelength is lengthened by a receding source according to

我遇到这类问题的主要困难在于一个量的符号弄错或某个项的倒置。因此,从头开始,根据远离源的多普勒效应,观测到的波长会被拉长:

but the observer sees the period of the light as time-dilated, so the observed wavelength is

但观察者看到光的周期被时间膨胀,因此观测到的波长是

So the galaxy is seen to be receding at 0.349c. Note that in this approach, the velocity of recession is treated as a positive number. Problems occur from the fact that some approaches use a negative number for a receding velocity. The usual red shift treatment in astronomy books treat the recession velocity as positive and express the red shift in terms of a z-parameter. In those terms, this calculation becomes

因此,星系被观测到以0.349c的速度远离。需要注意的是,在这种处理方式中,远离速度被当作一个正数来处理。由于某些方法使用负数表示远离速度,因此会出现问题。在天文学教科书中的通常红移处理方式中,将远离速度视为正数,并用z参数来表达红移。在这种表述下,该计算变为

But in standard Doppler shift calculations, a receding velocity is treated as a negative quantity and with that presumption, the Doppler wavelength shift becomes

但在标准的多普勒频移计算中,退行速度被当作一个负量处理,因此多普勒波长移位变为

So care must be taken to keep the signs consistent.

必须注意保持符号的一致性。
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