Fig. 9From: Asteroid Ryugu before the Hayabusa2 encounterLeft: similar to Fig. 8, but for a case with sub-solar latitude of 30, i.e., a tilted spin axis. Left: the thermal inertia is 200 J m−2 s−1/2 K−1. Right: thermal inertia is 1000 J m−2 s−1/2 K−1Back to article page