A little math:
full multi coating on an air-to-glass surface transmits ~99.5% of the light and reflects about 0.5%.
So, the transmission of FMC coatings in eyepieces of:
1 group (monocentric?)--99.0%
2 groups (Plössls, orthos, Kellners, Ramsden, Huygens, Brandon)--98.0%
3 groups (Masuyama, Erfle, etc.)--97.0%
4 groups (many widefields)--96.1%
5 groups (many widefields)--95.1%
6 groups (some hyperwides, some complex designs)--94.2%
7 groups (a few exotic designs)--93.2%
There is also a loss of about 1% per inch of glass, so some of the large complex designs may lose another 2-3%.
But, with some exceptions, and there are a few, almost every modern FMC eyepiece falls in the 90-98% transmission range.
There are some transmission figures that indicate sophisticated coatings with >99.5% transmission, but for purposes of this post, I'll ignore those.
So, what is the visible difference in terms of light transmission? about 8% max.
Note that 0.1 magnitude is a 9.6% difference, so the difference in transmission is smaller than 0.1 magnitude among all FMC eyepieces.
How does that stack up?
Well,
- nightly variations in sky darkness and transparency range, but almost always exceed 0.2 magnitudes or more.
- if we are talking about the visibility of DSOs, the difference of 0.1 magnitude is right at the limit of human vision, where we are likely talking about the difference between visible 20% of the time with averted vision and maybe 10% of the time with averted vision. We are definitely not talking about the difference between visible with direct vision and invisible to direct vision, a difference that would be significantly larger than 0.1 magnitude.
- A difference of 0.1 magnitude can barely be seen in a controlled lab experiment, and use of a telescope in the field is hardly a controlled lab environment.
Yet, we all have seen that some eyepieces go deeper than some others and reveal fainter features in DSOs.
Can we attribute that to light transmission in the eyepiece?
Perhaps partially. But other factors enter into the picture as well:
--sharpness of focus. A smaller spot size in the design might increase the per square arc-second light intensity.
--control of scattered light in the eyepiece. We see contrast, so reducing scattered light can improve contrast and make fainter things more visible.
--control of scattered light outside the eyepiece--in the scope, the environment. We all see more in the eyepiece when all peripheral light is blocked. The tops of some eyepieces do a better job at that than others.
--lens polish. Reducing scattered light at the lens surface, making coatings more effective.
--control of scattered light in the scope. One of the advantages to refractors, though reflectors can be optimized for this as well, but don't seem to be very often.
So when all the factors are added up, the difference from one eyepiece to another in terms of how faint it sees can be noticeable.
Light transmission, though, is only a minor part of that. Contrast is the major factor, and there is likely a % of that related to the psychology of use of a particular eyepiece.