Unit is - lux.
3 or 4 for night with no moon
about 50,000 for direct sunlight
The eye pupil will dilate or contract. About 7mm max to about 3 minimum. Objective lens divided by power gives exit pupil. So 56mm/20 = 2.8 mm.
Other stuff being - from Wikipedia
"The
Rayleigh criterion shows that the minimum angular spread that can be resolved by an image forming system is limited by
diffraction to the ratio of the
wavelength of the waves to the
aperture width. For this reason, high resolution imaging systems such as astronomical
telescopes, long distance
telephoto camera lenses and
radio telescopes have large apertures."
Small aperture width, more diffraction & image degradation. Light from a tiny little exit pupil of 2mm or smaller will easily fit into any eye pupil.
Diffraction - bending of light waves caused by the aperture becoming a secondary source (propagating) of light waves - light spreading, less intensity. making an increased dull fuzzy image or sometimes an image consisting of concentric rings.
And
Optical science guys use the term - "numerical aperture" or NA to describe a lens. A lens with a bigger NA has a bigger angle of acceptance, like a cone with a larger diameter as related to cone height or length. This results in more light being gathered in the pointy end of the cone providing better resolution.
Glass quality & coatings matter. Some 40 mm objective lens scopes are noticeably brighter than other 50mm objective lens scopes - both set at the same power.
Scopes with fat tubes like 30mm & 34mm will have internal lenses having larger NA's.
A nice 34/56 scope would be as good as it gets.
Whatever -never ever look at the sun directly with or without an optic.