Shape, regolith size and thickness, SMFe^0 content, and spectral type of Tianwen-2 target asteroid (469219) Kamo'oalewa
Pengfei Zhang, Guozheng Zhang, Yongxiong Zhang, Marco Fenucci, Pierre Vernazza, Jin Zhao, Yunbo Niu, Xuejin Lu, Xing Wu, Honglei Lin, Edward Cloutis, Xiaoran Yan, Xiaoping Lu, Xiaobin Wang, Xiaoping Zhang, Yang Li

TL;DR
This study models Kamo'oalewa's shape, regolith properties, and spectral type using observational data and laboratory measurements, providing detailed physical and compositional insights relevant for sample return missions.
Contribution
It offers a comprehensive physical and spectral characterization of Kamo'oalewa, including shape, rotation, regolith, and composition, based on modeling and laboratory data.
Findings
Kamo'oalewa's size is approximately 68 x 46 x 39 meters.
Regolith grains smaller than 2 cm cover over 93.8% of its surface.
SMFe0 content in regolith is estimated at 0.29 ± 0.05 wt.%.
Abstract
China's Tianwen-2 spacecraft will return samples from the near-Earth asteroid (469219) Kamo'oalewa. We previously reported that Kamo'oalewa develops an LL-chondrite-compositional, highly space-weathered surface. This study aims to estimate Kamo'oalewa's shape, regolith grain size and thickness, sub-micrometer iron (SMFe0) content, and spectral type. Using the lightcurve data and the Cellinoid model, we modeled Kamo'oalewa's shape, rotation period, and pole orientation. We then estimated its global distribution of regolith critical size using the balance method of gravity, cohesive force, and centrifugal force. Furthermore, in the temperature range of 253.15 to 473.15 K, we measured the thermal parameters of laser-irradiated LL chondrite powder that best matches Kamo'oalewa's spectrum, estimating Kamo'oalewa's thermal inertia and skin depth (lower limit of regolith thickness). Using the…
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