| Autor: |
Deng, Qingyun, Zhong, Zhen, Ye, Mao, Zhang, Wensong, Qiu, Denggao, Zheng, Chong, Yan, Jianguo, Li, Fei, Barriot, Jean‐Pierre |
| Předmět: |
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| Zdroj: |
Journal of Geophysical Research. Planets; Jun2023, Vol. 128 Issue 6, p1-19, 19p |
| Abstrakt: |
Characterizing the thermophysical properties of the lithosphere is critical for studying its evolution. We determine the elastic thickness of the lithosphere by modeling mass‐related loads and lithospheric deflection and analyzing gravity and topography data. In impact basins region where a mantle plug is present, the correlation between topography and gravity can be low, and the admittance can change quickly, making it difficult to develop accurate models without considering mantle uplift. In this study, we developed a lithospheric loading model for large impact basins that take advantage of a high‐resolution crustal thickness model and does not require the assuming compensation. Since the mantle uplift formed by super‐isostatic adjustment following the impact, the elastic thickness obtained by fitting the observed data reflects the lithospheric temperature at the end of the super‐isostatic process. Sensitivity analysis suggests that modeling the impact‐induced load is critical to reproduce how the mascon is expressed in the correlation and admittance data. Our mantle loading model provides a better fit to the observed admittance spectrum compared to previous research. The larger elastic thicknesses obtained for the Hellas basin indicate a longer duration of mascon formation or a faster cooling of the lithosphere. Models that consider a denser upper crust and an elastic thickness of about 0 km fit the observed admittance of the Utopia basin. The elastic thickness of the Argyre and Isidis basins cannot be precisely inferred without additional constraints on the load ratio. Plain Language Summary: The lithosphere is defined as the outer rigid part of a planet, and its deformation due to applied masses (loading) can be calculated using the deflection equation. Topography and gravity data are used to measure this deformation and constrain the thickness of the elastic shell assumed to represent the lithosphere. However, this approach is difficult to apply to impact basins due to the complex loading process that follows the impact, such as the formation of a mass concentration (mascon) beneath the basin center. In this work, we modeled the mascons as mantle plugs and inferred their structures from a global crustal thickness model. The resulting mantle loading model is applied to large impact basins on Mars. The large elastic thickness inferred for the Hellas basin means the temperature of the lithosphere was low when the mascon formed, indicating that the lithosphere cooled quickly or mascon formation took a long time. The Utopia basin's nearly zero lithosphere thickness means the mascon formed in a relatively high‐temperature situation, causing the lithosphere to be too weak to support the mascon. Key Points: A mantle‐plug loading model based on crustal thickness helps understand the gravity and topography signals of large impact basins on MarsThe elastic thickness inferred for the Hellas basin indicates fast lithosphere cooling or long‐duration mascon formationThe elastic thickness inferred for the Utopia basin is near 0 km when considering a denser upper crust [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
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