If you look at the field of an infinite sheet of charge (with charge density $\sigma$), the field is:
$$ \vec E(x) = \frac{\sigma}{2\epsilon_0} \frac{\vec x}{|x|} $$
It's uniform. At a distance $x$ from the sheet, the total charge at radius $r\pm dr/2 $, with $r \gg x $, contributing to the field is:
$$ \rho = \sigma rdr$$
The transverse component of the field cancel, leaving a longitudinal component:
$$ E_x \propto E\times \frac x r $$
where:
$$ E \propto \frac{\rho}{r^2} \propto \frac {\sigma dr} r$$
So contributions from distant charge falls of as:
$$ dE(r) \propto \frac x {r^2} $$
So you for well behaved charge distributions, you can ignore contributions from $r \gg x $.
If if you get close enough to a surface ($x \ll R_c$) where $R_c$ is the smallest radius of curvature, it looks flat, and
$$ E = c_0 \times \frac{\sigma}{\epsilon_0} $$
For an infinite sheet: $c_0 = \frac 1 2$, and for a conducting sphere: $c_0 = 1$.