Lightcurve and Phase Function Photometry of the OSIRIS-REx Target (101955) 1999 RQ36

Physics

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Scientific paper

We present visible wavelength photometry of the OSIRIS-REx target
asteroid (101955) 1999 RQ36. We find a rotation period of 4.2968
± 0.0017 hr and phase slope of 0.039 mag/deg. YORP induced
rotation rate changes should be detectable by OSIRIS-REx.

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