1. Orbital and In Situ Observation of Transverse Aeolian Ridges at Zhurong Landing Site.
- Author
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Liu, Jia, Liu, Yang, Wan, Wenhui, Zhou, Xiang, Zhao, Zhenxing, Wu, Yuchun, Zhang, Chaolin, Wang, Xiyu, Wu, Xing, and Zou, Yongliao
- Subjects
SAND waves ,WIND pressure ,GEOMORPHOLOGY ,SULFATE minerals ,REMOTE sensing ,TAR - Abstract
A large amount of transverse aeolian ridges (TARs) bedforms exist in the Zhurong rover landing region. The acquisition of high‐resolution data from the orbiter and the rover from Tianwen‐1 mission provides an excellent opportunity to study the geological characteristics of TARs. The length, width, and density of a total of 8,274 TAR samples at the landing site were analyzed. The orientation of TARs at the landing region is dominated in the E‐W direction. Analysis of Mars Climate Station (MCS) data on the Zhurong rover shows that the present‐day wind direction is inconsistent with the wind forces that promoted the formation of TARs, suggesting that the formation of TARs is dependent on the ancient wind direction. With the help of the Zhurong MarSCoDe shortwave infrared (SWIR) spectrometer data, we investigate the composition of materials including TARs, soil, and rocks, and the results show that their spectra display similar distinct absorptions consistent with the presence of hydrated minerals such as hydrated sulfates. The cemented and dusty crust covering the TARs indicates that the TARs have not migrated for a period of time in the landing site area. Some of the TARs have been eroded into small sand ridges or ripples due to the change in the prevailing wind directions, which may indicate the climate change on Mars. Plain Language Summary: Using the high‐resolution remote sensing images from the orbiter and Zhurong rover of Tianwen‐1 mission, we identified a total of 8,274 aeolian bedforms at the landing site of the rover on the Utopia Planitia. These aeolian bedforms can be classified as transverse aeolian ridges (TARs) according to their morphology, size and other observational features. The detailed geometry such as the length, the width, the density, and orientation of these TARs were characterized and compared with Martian TARs measured in the previous studies. The TARs in the study area were found to have formed in an ancient wind regime. The TARs are covered with bright dust and their surfaces have been cemented. This suggests that these TARs have not moved for a long time. Some of the TARs have been eroded into small sand ripples. The cause of this may be related to the change in the direction of the ancient wind because the current wind direction derived from the Mars Climate Station (MCS) data on the Zhurong rover is found to be different from the ancient wind direction. Key Points: The geomorphology of transverse aeolian ridges (TARs) at Zhurong landing area are mapped and analyzed and the results show that they formed at an ancient wind regimeThe cemented and dusty crust covering the TARs indicate that the TARs have not migrated for a period of timeSome of the TARs have been eroded due to the change of the prevailing wind directions which may indicate the climate change on Mars [ABSTRACT FROM AUTHOR]
- Published
- 2023
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