Index of Refraction of Outer/Interplanetary Space

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The discussion centers on the index of refraction in outer and interplanetary space, highlighting that while air is often treated as having the same index of refraction as a vacuum, it actually differs slightly due to wavelength dependence. It raises questions about the measurable index of refraction in interstellar and intergalactic space, noting that space is not a perfect vacuum and contains low-density plasma, which affects light speed based on frequency. This frequency dependence leads to observable phenomena, such as varying arrival times of pulsar signals, a concept known as "dispersion delay." Although it is suggested that the index of refraction for visible light in space could be evaluated, no significant measurements have been reported, indicating the effect may be too small to detect. The conversation emphasizes the importance of understanding these differences for astrophysical observations.
Jolb
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In electricity and magnetism, we typically assume that the relative permittivity (or dielectric constant) ε of air is equal to the "permittivity of free space" ε0, and likewise we assume that air has a relative permeability μ equal to the "permeability of free space" μ0. This is equivalent to assuming that air has the same index of refraction n as vacuum.

However, in reality, air has slightly different index of refraction from vacuum; the most obvious example is that there's some wavelength dependence in n that causes rainbows. Pretty much all substances have have an n that's different from that of the vacuum.

So my question is this: what is the index of refraction of the interplanetary space in our solar system, or in outer space (interstellar, intergalactic, etc.)? Since outer space and interplanetary space is not a pure vacuum, it must have a slightly different index of refraction... has this ever been measured? Is it observably different from the vacuum value?

Does quantum field theory predict any changes to the index of refraction of space when we go from a classical vacuum to a quantized electromagnetic field, given that the background radiation is about 3K?

In a nutshell, I want to know if there are any observable or theoretically predicted differences between the ideal vacuum's index of refraction and the index of refraction of real outer space.

Please include any references.
 
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There are definitely observable consequences to space not being a perfect vacuum. Because space is filled with a low density plasma, the index of refraction is a function of frequency. This means the speed of light in interstellar space is a function of frequency. This means that if I observe a transient source, like a pulsar, the arrival time of the pulses is different depending on the frequency. Radio astronomers use this effect to get information on the distance to radio sources and the density of the intervening interstellar medium. Try looking up "dispersion delay". Here's a good link:

http://www.cv.nrao.edu/course/astr534/Pulsars.html
 
Jolb said:
However, in reality, air has slightly different index of refraction from vacuum; the most obvious example is that there's some wavelength dependence in n that causes rainbows.
Rainbows come from the refraction in water, not in air.
References ;)


For visible light, it should be possible to evaluate the diffractive index, too. However, as I did not hear about a measurement yet (or do not remember it), the effect might be too small to observe.
 
UC Berkely, December 16, 2025 https://news.berkeley.edu/2025/12/16/whats-powering-these-mysterious-bright-blue-cosmic-flashes-astronomers-find-a-clue/ AT 2024wpp, a luminous fast blue optical transient, or LFBOT, is the bright blue spot at the upper right edge of its host galaxy, which is 1.1 billion light-years from Earth in (or near) a galaxy far, far away. Such objects are very bright (obiously) and very energetic. The article indicates that AT 2024wpp had a peak luminosity of 2-4 x...

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