1. Characterization of the Ryugu surface by means of the variability of the near-infrared spectral slope in NIRS3 data
- Author
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Masanao Abe, Moe Matsuoka, Yuto Takei, Andrea Longobardo, Mario D'Amore, T. Okada, Kohei Kitazato, Sei-ichiro Watanabe, Satoshi Tanaka, Koji Matsumoto, Driss Takir, Takanao Saiki, Naru Hirata, A. Zinzi, Yuichi Tsuda, Takahiro Hiroi, Ernesto Palomba, Fabrizio Dirri, A. Galiano, Yukio Yamamoto, Makiko Ohtake, Kei Shirai, Shuji Matsuura, Tomoki Nakamura, Makoto Yoshikawa, and Takahiro Iwata
- Subjects
geography ,geography.geographical_feature_category ,010504 meteorology & atmospheric sciences ,Near-infrared spectroscopy ,Mineralogy ,Astronomy and Astrophysics ,01 natural sciences ,Space weathering ,Standard deviation ,Parent body ,Impact crater ,Space and Planetary Science ,Asteroid ,Ridge ,0103 physical sciences ,Spectral slope ,010303 astronomy & astrophysics ,Ryugu Near-earth asteroid Hayabusa2 Space weathering NIR spectral slope ,Geology ,0105 earth and related environmental sciences - Abstract
The Near-Earth Asteroid 162173 Ryugu (1999 JU3) was investigated by the JAXA Hayabusa2 mission from June 2018 to November 2019. The data acquired by NIRS3 spectrometer revealed a dark surface with a positive near-infrared spectral slope. In this work we investigated the spectral slope variations across the Ryugu surface, providing information about physical/chemical properties of the surface. We analysed the calibrated, thermally and photometrically corrected NIRS3 data, and we evaluated the spectral slope between 1.9 μm and 2.5 μm, whose values extend from 0.11 to 0.28 and the mean value corresponds to 0.163±0.022. Starting from the mean value of slope and moving in step of 1 standard deviation (0.022), we defined 9 “slope families”, the Low-Red-Slope families (LR1, LR2 and LR3) and the High-Red-Sloped families (HR1, HR2, HR3, HR4, HR5, HR6). The mean values of some spectral parameters were estimated for each family, such as the reflectance factor at 1.9 μm, the spectral slope, the depth of bands at 2.7 μm and at 2.8 μm. A progressive spectral reddening, darkening and weakening/narrowing of OH bands is observed moving from the LR families to the HR families. We concluded that the spectral variability observed among families is the result of the thermal metamorphism experienced by Ryugu after the catastrophic disruption of its parent body and space weathering processes that occurred on airless bodies as Ryugu, such as impact cratering and solar wind irradiation. As a consequence, the HR1, LR1, LR2 and LR3 families, corresponding to equatorial ridge and crater rims, are the less altered regions on Ryugu surface, which experienced the minor alteration and OH devolatilization; the HR2, HR3, HR4, HR5 families, coincident with floors and walls of impact craters, are the most altered areas, result of the three processes occurring on Ryugu. The strong reddening of the HR6 family (coincident with Ejima Saxum) is likely due to the fine-sized material covering the large boulder.
- Published
- 2020