Here is another take making use of the symmetry, as hinted in the text.
The vacuum state is by definition symmetric with respect to any Lorentz transformation and translation. Let $U(\Lambda)$ be a unitary representation of the Lorentz transformation $\Lambda$ acting on the states, and let
$$T(a) \equiv \exp ( -i Pa) \equiv \exp (- i P_\mu a^\mu )$$
be the unitary spacetime translation operator. Then by Lorentz invariance we have
$$ \tag{A-1} |\Omega \rangle = U(\Lambda) |\Omega\rangle, $$
$$ \tag{A-2}\langle\Omega | = U(\Lambda)^{-1} \langle \Omega |,$$
and by translational invariance we have
$$ \tag{B-1} | \Omega \rangle = T(a) | \Omega \rangle, $$
$$ \tag{B-2} \langle \Omega | = \langle \Omega | T(a)^{-1}. $$
Moreover, $U(\Lambda)$ and $T(a)$ act on a scalar field $\varphi(x)$ as
$$ \tag{C-1} U(\Lambda)^{-1} \varphi(x) U(\Lambda) = \varphi(\Lambda^{-1}x), $$
$$ \tag{C-2} T(a)^{-1} \varphi(x) T(a) \equiv e^{iPa}\varphi(x) e^{-iPa} = \varphi(x-a). $$
Using these relations we have
$$ \tag{D-1} \langle \Omega | \varphi(x) | \Omega \rangle =
\langle \Omega | U(\Lambda)^{-1}\varphi(x)U(\Lambda) | \Omega \rangle = \langle \Omega | \varphi(\Lambda^{-1}x) \Omega \rangle, $$
$$ \tag{D-2} \langle \Omega | \varphi(x) | \Omega \rangle = \langle \Omega | \varphi(x+a) | \Omega \rangle, $$
for any Lorentz transformation (whose vector representation is) $\Lambda$ and for any 4-vector $a$.
In particular from (D-2) you can see that
$$ \tag{E} \langle \Omega | \varphi(x) | \Omega \rangle = c,$$
where $c$ does not depend on the space-time variable $x$. The answer of @lionelbrits explains why this constant can often be considered to be 0.
For a spinor field $\psi_\alpha(x)$ (or a vector field for that matter) you can use the same argument as above to obtain
$$ \tag{F} \langle \Omega | \psi_\alpha(x) | \Omega \rangle = \langle \Omega | \psi_\alpha(0) | \Omega \rangle \equiv c_\alpha,$$
but now you have to remember the non trivial action of the Lorentz group on a spinor field: you have
$$ \tag{G} U(\Lambda)^{-1} \psi_\alpha(x) U(\Lambda) = S(\Lambda)_\alpha^{\,\,\,\beta} \psi_\beta(\Lambda^{-1} x), $$
where $S(\Lambda)$ is the spinor representation of the Lorentz transformation.
Using (G) in (F) you obtain:
$$ \tag{H} c_\alpha
\equiv \langle \Omega | \psi_\alpha(0) | \Omega \rangle
= S(\Lambda)_\alpha^{\,\,\beta} \langle \Omega | \psi_\alpha(0) | \Omega \rangle
\equiv S(\Lambda)_\alpha^{\,\,\beta} c_\beta, $$
and due to the arbitrariness in the choice of the Lorentz transformation this implies that $c_\alpha=0$, i.e. remembering (F),
$$ \langle \Omega | \psi_\alpha(x) | \Omega \rangle = 0.$$