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Fig. 2 | Progress in Earth and Planetary Science

Fig. 2

From: Asteroid Ryugu before the Hayabusa2 encounter

Fig. 2

Composite 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 7.63 h. The zero phase time corresponds to 57,581.0 MJD

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