  We describe an induced inflation, which refers to a class of inflationary
models with a generalized non-minimal coupling $\xi g(\phi) R$ and a specific
scalar potential. The defining property of these models is that the scalar
field takes a vev in the vacuum and thus induces an effective Planck mass. We
study this model as a function of the coupling parameter $\xi$. At large $\xi$,
the predictions of the theory are known to have an attractor behavior,
converging to a universal result independent on the choice of the function
$g(\phi)$. We find that at small $\xi$, the theory approaches a second
attractor. The inflationary predictions of this class of theories continuously
interpolate between those of the Starobinsky model and the predictions of the
simplest chaotic inflation with a quadratic potential.
