dlgoff said:
For length units (meters in this case) you could show them this
Scale of the Universe presentation (From the largest down to the Planck scale). More of a wow factor though.
Thanks! Illustration, including a wow factor, is part of what makes introductory explanations effective. What I'm dwelling on though is whether one make an approach that starts from the central constant of the GR equation. the 8πG/c
4
That is reciprocal of a force and the large size of the force (by our standards) corresponds to how STIFF geometry is (by our standards) against being curved by matter.
So that force, call it F for the time being, is key to the relation between geometry and matter. You could paraphrase the GR equation by saying
(curvature) = (1/F) (matter density)
or simply swapping sides you could say
(matter density) = (F) (curvature)
F being big means it takes a LOT of matter density to make a small dent in the geometry (by our standards).
But from Nature's standpoint F is just the UNIT proportionality between energy density and curvature----or pressure and curvature (pressure and energy density have algebraically the same unit)
When I look at Wikipedia for, say, cosmology, I see
G_{\mu \nu} + \Lambda g_{\mu \nu}= {8\pi G\over c^4} T_{\mu \nu}
I'm wondering what notation to use for that force c
4/(8πG)
Should I call it F
planck or F
p or maybe Fbar, because like hbar it is 'reduced'?
When I type this into google
" hbar in (Newton meter second)"
I get "hbar = 1.05457173 × 10-34 Newton meter second"
So I could USE that universal force constant in order to parse the universal hbar constant and get stuff out of it. Any thoughts, cautions

, preferences, deprecations,... abhorrences?