Step 1: Use the condition for coincidence of bright fringes.
In Young's double slit experiment, the position of the \(n^{\text{th}}\) bright fringe is given by
\[
y_n=\frac{n\lambda D}{d}
\]
For two wavelengths, bright fringes coincide when
\[
n_1\lambda_1=n_2\lambda_2
\]
Step 2: Substitute the given wavelengths.
Given,
\[
\lambda_1=3750\,\text{\AA}
\]
\[
\lambda_2=7500\,\text{\AA}
\]
Now,
\[
n_1\lambda_1=n_2\lambda_2
\]
\[
n_1(3750)=n_2(7500)
\]
\[
n_1=2n_2
\]
For the minimum non-zero distance from the central bright fringe, take the smallest positive integers:
\[
n_2=1
\]
\[
n_1=2
\]
So, the first coincidence occurs when the second bright fringe of wavelength \(3750\,\text{\AA}\) coincides with the first bright fringe of wavelength \(7500\,\text{\AA}\).
Step 3: Convert the given quantities into SI units.
The slit separation is
\[
d=3\,\text{mm}=3\times 10^{-3}\,\text{m}
\]
The screen distance is
\[
D=4\,\text{m}
\]
The longer wavelength is
\[
\lambda_2=7500\,\text{\AA}
\]
Since,
\[
1\,\text{\AA}=10^{-10}\,\text{m}
\]
we get
\[
\lambda_2=7500\times 10^{-10}\,\text{m}
\]
\[
\lambda_2=7.5\times 10^{-7}\,\text{m}
\]
Step 4: Find the distance of the first coincident bright fringe.
Using
\[
y=\frac{n_2\lambda_2D}{d}
\]
Since \(n_2=1\),
\[
y=\frac{(1)(7.5\times 10^{-7})(4)}
{3\times 10^{-3}}
\]
\[
y=\frac{30\times 10^{-7}}
{3\times 10^{-3}}
\]
\[
y=10\times 10^{-4}\,\text{m}
\]
\[
y=10^{-3}\,\text{m}
\]
\[
y=1\,\text{mm}
\]
Step 5: Final conclusion.
Therefore, the minimum distance from the common central bright fringe is
\[
\boxed{1\,\text{mm}}
\]