EGU24-10193, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-10193
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

New insight into the surface composition of Zhurong landing area

Qing Zhang1,2, John Carter2,3, Mathieu Vincendon2, François Poulet2, Maxime Pineau3, Lin Guo1, Yuxuan Luo1, Dawei Liu1, Jean-Pierre Bibring2, Jianjun Liu1, and Chunlai Li1
Qing Zhang et al.
  • 1Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China (zhangq@nao.cas.cn; liujj@nao.cas.cn)
  • 2Institut d’Astrophysique Spatiale, CNRS, Paris-Saclay University, Orsay, France
  • 3Laboratoire d’Astrophysique de Marseille, CNRS, Aix-Marseille University, Marseille, France

The Zhurong rover conducted in-situ spectral investigations of southern Utopia Planitia, where orbital observations revealed the presence of spectrally featureless dust. However, in-situ reflectance spectra collected by the Short Wave Infrared (SWIR) spectrometer exhibit hydrated features for all observations along the traverse. These features have been interpreted as being associated with groundwater (Liu Y. et al., 2022) or ocean (Liu C. et al., 2022; Xiao et al., 2023) or atmospheric water (Zhao et al., 2023). Here, we combine the Multispectral Camera (MSCam) and SWIR data to characterize the spectra of landing site and provide some new insights into the surface composition diversity.

Multispectral images suggest that most of surfaces are consistent with the presence of dust whereas a few of rock surfaces exhibiting dark tones are compositionally distinct. The co-observational SWIR data can be used to further constrain the surface compositions. With Principal Component Analysis (PCA) and unmixing analysis of the SWIR data, we found that these dusty surfaces are ubiquitously characterized with faint 1900 and 2200 nm absorptions and the dark rock surfaces exhibit strong blue slopes in the NIR.

The hydrated dust features seem to contrast with previous knowledge, that the dust does not exhibit obvious NIR hydration features from orbital observations. Such discrepancies were also observed at Jezero crater, where the fine soils or dusty rocks exhibit a 1900 nm H2O absorption but without 2200 nm band (Mandon et al., 2023). Spectral variation may reflect distinct surface dust compositions between the Perseverance and Zhurong landing site, indicating different dust reservoirs or dust alteration processes. The surface dust of different sites may be mixtures of globally well-mixed fine materials and local/regional distinct hydrated phases. Another possibilities is that the dust underwent different post-deposition aqueous alteration.

The dark rock surfaces may represent less dust-coated surfaces. The strong blue slope features have been previously attributed to coatings on a dark substrate. Furthermore, the morphological properties show that these surfaces exhibit relatively fragile surface context, consistent with surface coatings or rinds.

How to cite: Zhang, Q., Carter, J., Vincendon, M., Poulet, F., Pineau, M., Guo, L., Luo, Y., Liu, D., Bibring, J.-P., Liu, J., and Li, C.: New insight into the surface composition of Zhurong landing area, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10193, https://doi.org/10.5194/egusphere-egu24-10193, 2024.