Step 1: Write the conservation of mechanical energy equation.
At the earth's surface, the projectile has kinetic energy and gravitational potential energy.
At the maximum height, the projectile momentarily comes to rest, so kinetic energy becomes zero.
Using conservation of energy,
\[
\frac12 mV^2-\frac{GMm}{R}
=
-\frac{GMm}{R+h}
\]
where,
\[
V=\alpha V_E
\]
\[
h=800 \, km
\]
\[
R=6400 \, km
\]
Step 2: Use the escape velocity relation.
Escape velocity is given by
\[
V_E=\sqrt{\frac{2GM}{R}}
\]
Squaring both sides,
\[
V_E^2=\frac{2GM}{R}
\]
Substitute \(V=\alpha V_E\) into the energy equation,
\[
\frac12 m\alpha^2V_E^2-\frac{GMm}{R}
=
-\frac{GMm}{R+h}
\]
Now replace \(V_E^2\) by \(\dfrac{2GM}{R}\),
\[
\frac12 m\alpha^2\left(\frac{2GM}{R}\right)-\frac{GMm}{R}
=
-\frac{GMm}{R+h}
\]
\[
\frac{GMm}{R}\alpha^2-\frac{GMm}{R}
=
-\frac{GMm}{R+h}
\]
Step 3: Simplify the equation.
Divide throughout by \(GMm\),
\[
\frac{\alpha^2}{R}-\frac1R
=
-\frac1{R+h}
\]
\[
\frac{\alpha^2-1}{R}
=
-\frac1{R+h}
\]
Multiply both sides by \(R\),
\[
\alpha^2-1
=
-\frac{R}{R+h}
\]
\[
\alpha^2
=
1-\frac{R}{R+h}
\]
\[
\alpha^2
=
\frac{h}{R+h}
\]
Step 4: Substitute the numerical values.
\[
\alpha^2
=
\frac{800}{6400+800}
\]
\[
=
\frac{800}{7200}
\]
\[
=
\frac19
\]
Taking square root,
\[
\alpha=\frac13
\]
Step 5: Final conclusion.
Hence, the value of the constant is
\[
\boxed{\frac13}
\]