  The Seyfert 2 galaxy NGC 2992 has been monitored eight times by XMM-Newton in
2010 and then observed again in 2013, while in 2015 it was simultaneously
targeted by Swift and NuSTAR. XMM-Newton always caught the source in a faint
state (2-10 keV fluxes ranging from 0.3 to 1.6$\times10^{-11}$ erg cm$^{-2}$
s$^{-1}$) but NuSTAR showed an increase in the 2-10 keV flux up to
6$\times10^{-11}$ erg cm$^{-2}$ s$^{-1}$. We find possible evidence of an Ultra
Fast Outflow with velocity $v_1=0.21\pm0.01c$ (detected at about 99% confidence
level) in such a flux state. The UFO in NGC 2992 is consistent with being
ejected at a few tens of gravitational radii only at accretion rates greater
than 2% of the Eddington luminosity. The analysis of the low flux 2010/2013 XMM
data allowed us to determine that the Iron K$\alpha$ emission line complex in
this object is likely the sum of three distinct components: a constant, narrow
one due to reflection from cold, distant material (likely the molecular torus);
a narrow, but variable one which is more intense in brighter observations and a
broad relativistic one emitted in the innermost regions of the accretion disk,
which has been detected only in the 2003 XMM observation.
