  The centaur 95P/(2060) Chiron is showing comet-like activity since its
discovery, but the mass-loss mechanisms triggering its activity remained
unexplained. Although the collision rates in the centaur region are expected to
be very low, and impacts are thought not to be responsible for the mass-loss,
since the recent indications that Chiron might possess a ring similar to
Chariklo's, and assuming that there is debris orbiting around, the impact
triggered mass-loss mechanism should not be excluded as a possible cause of its
activity. From time series observations collected on Calar Alto Observatory in
Spain between 2014 and 2016, we found that the photometric scatter in Chiron's
data is larger than a control star's scatter, indicating a possible
microactivity, possibly caused by debris falling back to Chiron's surface and
lifting small clouds of material. We also present rotational light curves, and
measurements of Chiron's absolute magnitudes, that are consistent with the
models supporting the presumption that Chiron possesses rings. By co-adding the
images acquired in 2015, we have detected a $ \sim $5 arcsec long tail, showing
a surface brightness of 25.3 mag(V)/arcsec$^{2}$.
