  We present a dynamical cosmological solution that simultaneously accounts for
the early inflationary stage of the Universe and solves the supersymmetric
little hierarchy problem via the relaxion mechanism. First, we consider an
inflationary potential arising from the $D$-term of a new $U(1)$ gauge symmetry
with a Fayet--Iliopolous term, that is independent of the relaxion. A
technically natural, small $U(1)$ gauge coupling, $g\lesssim 10^{-8}$, allows
for a low Hubble scale of inflation, $H_I\lesssim 10^5$ GeV, which is shown to
be consistent with Planck data. This feature is then used to realize a
supersymmetric two-field relaxion mechanism, where the second field is
identified as the inflaton provided that $H_I\lesssim 10$ GeV. The inflaton
controls the relaxion barrier height allowing the relaxion to evolve in the
early Universe and scan the supersymmetric soft masses. After electroweak
symmetry is broken, the relaxion settles at a local supersymmetry-breaking
minimum with a range of $F$-term values that can naturally explain
supersymmetric soft mass scales up to $10^6$ GeV.
