Fig. 2From: Asteroid Ryugu before the Hayabusa2 encounterComposite lightcurve of Ryugu, as observed at the Very Large Telescope of the European Southern Observatory (ESO-VLT) on 12 Jul. 2016 by Perna et al. (2017). The rotational phase corresponds to a synodic period of 7.63Â h. The zero phase time corresponds to 57,581.0 MJDBack to article page