  We give explicit constructions of static, non-supersymmetric $p$-brane (for
$p \leq d-4$, where $d$ is the space-time dimensionality and including $p=-1$
or D-instanton) solutions of type II supergravities in diverse dimensions. A
subclass of these are the static counterpart of the time dependent solutions
obtained in [hep-th/0309202]. Depending on the forms of the non-extremality
function $G(r)$ defined in the text, we discuss various possible solutions and
their region of validity. We show how one class of these solutions interpolate
between the $p$-brane--anti $p$-brane solutions and the usual BPS $p$-brane
solutions in $d=10$, while the other class, although have BPS limits, do not
have such an interpretation. We point out how the time dependent solutions
mentioned above can be obtained by a Wick rotation of one class of these static
solutions. We also discuss another type of solutions which might seem
non-supersymmetric, but we show by a coordinate transformation that they are
nothing but the near horizon limits of the various BPS $p$-branes already
known.
