The Colors of The Moon (Doppler Effect)

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SUMMARY

The discussion focuses on the feasibility of detecting the Doppler effect of sunlight reflected by the Moon from Earth's surface. Key calculations reveal that the average lunar orbit is approximately 384,000 km, with the Moon's speed in this orbit being 1,022.7 m/s. The calculated velocity ratio (v/c) is 3.4E-6, leading to a wavelength difference of 2.2 picometers for the Balmer spectrum at n=3 (656 nm). Participants conclude that current technology may not be sufficient to detect such a minuscule effect.

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dom_quixote
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Hey guys!

I will pass an illustrated problem, below.
moonlight.JPG


- We know that the solar rays that reach the Moon and Earth are practically parallel;

- We know that the lunar orbit with respect to Earth lasts 27.322 days or 2,360,621 seconds;

- We know that the lunar orbit with respect to the Earth is elliptical;

- We know that 27.322 days the distance between the Moon and Earth varies between 362,600 km and 405,400 km.

In order to simplify our calculations, let us consider an average circular orbit:

[405,400,000 m + 362,600,000 m] / 2 = 384,000,000 m

The perimeter of the average lunar orbit is equal to:

2 * pi * 384,000,000 m = 2,412,743,158 m

The speed of the Moon relative to its average orbit is:

2,412,743,158 m / 2,360,621 s = 1,022.7 m/s

We ask:

Do we have enough technology to detect the Doppler effect of sunlight reflected by the Moon from the Earth's surface?
 
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From your numbers I calculate v/c = 3.4E-6. Balmer spectre of n=3 has wave length of 656 nm would undertake the wave length difference of 2.2 pico meter. I am not good at relevant technologies at all but suppose the effect is too tiny to detect.
 
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There are some narrow lines:
moonspec.jpg

NIST
 
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