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Fig. 9 | Progress in Earth and Planetary Science

Fig. 9

From: Asteroid Ryugu before the Hayabusa2 encounter

Fig. 9

Left: 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−1

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